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  <front>
    <journal-meta>
<journal-id journal-id-type="publisher">ASCMO</journal-id>
<journal-title-group>
<journal-title>Advances in Statistical Climatology, Meteorology and Oceanography</journal-title>
<abbrev-journal-title abbrev-type="publisher">ASCMO</abbrev-journal-title>
<abbrev-journal-title abbrev-type="nlm-ta">Adv. Stat. Clim. Meteorol. Oceanogr.</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub">2364-3587</issn>
<publisher><publisher-name>Copernicus Publications</publisher-name>
<publisher-loc>Göttingen, Germany</publisher-loc>
</publisher>
</journal-meta>

    <article-meta>
      <article-id pub-id-type="doi">10.5194/ascmo-2-79-2016</article-id><title-group><article-title>Estimating changes in temperature extremes from millennial-scale climate simulations using generalized extreme value (GEV) distributions</article-title>
      </title-group><?xmltex \runningtitle{Temperature extremes in CCSM3}?><?xmltex \runningauthor{W.~K. Huang et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Huang</surname><given-names>Whitney K.</given-names></name>
          <email>huang251@purdue.edu</email>
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Stein</surname><given-names>Michael L.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>McInerney</surname><given-names>David J.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Sun</surname><given-names>Shanshan</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Moyer</surname><given-names>Elisabeth J.</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>Department of Statistics, Purdue University, West Lafayette, IN
47907, USA</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Department of Statistics, University of Chicago, Chicago, IL
60637, USA</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>School of Civil, Environmental and Mining Engineering,
University of Adelaide, Adelaide, <?xmltex \hack{\newline}?> South Australia, 5005, Australia</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Department of the Geophysical Sciences, University of Chicago,
Chicago, IL 60637, USA</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Whitney K. Huang  (huang251@purdue.edu)</corresp></author-notes><pub-date><day>1</day><month>July</month><year>2016</year></pub-date>
      
      <volume>2</volume>
      <issue>1</issue>
      <fpage>79</fpage><lpage>103</lpage>
      <history>
        <date date-type="received"><day>5</day><month>December</month><year>2015</year></date>
           <date date-type="rev-recd"><day>16</day><month>May</month><year>2016</year></date>
           <date date-type="accepted"><day>6</day><month>June</month><year>2016</year></date>
      </history>
      <permissions>
<license license-type="open-access">
<license-p>This work is licensed under a Creative Commons Attribution 3.0 Unported License. To view a copy of this license, visit <ext-link ext-link-type="uri" xlink:href="http://creativecommons.org/licenses/by/3.0/">http://creativecommons.org/licenses/by/3.0/</ext-link></license-p>
</license>
</permissions><self-uri xlink:href="https://ascmo.copernicus.org/articles/.html">This article is available from https://ascmo.copernicus.org/articles/.html</self-uri>
<self-uri xlink:href="https://ascmo.copernicus.org/articles/.pdf">The full text article is available as a PDF file from https://ascmo.copernicus.org/articles/.pdf</self-uri>


      <abstract>
    <p>Changes in extreme weather may produce some of the largest societal impacts
of anthropogenic climate change. However, it is intrinsically difficult to
estimate changes in extreme events from the short observational record. In
this work we use millennial runs from the Community Climate System Model
version 3 (CCSM3) in equilibrated pre-industrial and possible future (700 and
1400 ppm <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) conditions to examine both how extremes change in this
model and how well these changes can be estimated as a function of run
length. We estimate changes to distributions of future temperature extremes
(annual minima and annual maxima) in the contiguous United States by fitting
generalized extreme value (GEV) distributions. Using 1000-year pre-industrial
and future time series, we show that warm extremes largely change in
accordance with mean shifts in the distribution of summertime temperatures.
Cold extremes warm more than mean shifts in the distribution of wintertime
temperatures, but changes in GEV location parameters are generally well
explained by the combination of mean shifts and reduced wintertime
temperature variability. For cold extremes at inland locations, return levels
at long recurrence intervals show additional effects related to changes in
the spread and shape of GEV distributions. We then examine uncertainties that
result from using shorter model runs. In theory, the GEV distribution can
allow prediction of infrequent events using time series shorter than the
recurrence interval of those events. To investigate how well this approach
works in practice, we estimate 20-, 50-, and 100-year extreme events using
segments of varying lengths. We find that even using GEV distributions, time
series of comparable or shorter length than the return period of interest can
lead to very poor estimates. These results suggest caution when attempting to
use short observational time series or model runs to infer infrequent
extremes.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <title>Introduction</title>
      <p>As the Earth's mean climate changes under increased
concentrations of human-emitted greenhouse gases, the intensity and frequency
of extreme weather conditions may change as well (<xref ref-type="bibr" rid="bib1.bibx15" id="altparen.1"/>,
chap. 11: <xref ref-type="bibr" rid="bib1.bibx29" id="altparen.2"/>, and references therein). Extreme events, while
rare by definition, can have large impacts on both human society and
environmental systems: present-day weather damages are dominated by rare
events that happen only every several decades or less <xref ref-type="bibr" rid="bib1.bibx40" id="paren.3"/>, and
society's vulnerability to extreme events appears to be growing
<xref ref-type="bibr" rid="bib1.bibx35" id="paren.4"/>. In the United States, the frequency of climate and
weather events with damages greater than USD 1 billion appears to be increasing at around 5 % per year
<xref ref-type="bibr" rid="bib1.bibx49" id="paren.5"/>. It remains unclear to what extent long-term climate trends
contribute to that rise, but these factors have led to extensive efforts to
understand the relationship between long-term climate change driven by
greenhouse gas forcing and potential changes in climate extremes.</p>
      <p>Over the past 2 decades, numerous studies have sought to identify changes in
temperature extremes both in observations
<xref ref-type="bibr" rid="bib1.bibx15 bib1.bibx47 bib1.bibx42 bib1.bibx56 bib1.bibx37 bib1.bibx39" id="paren.6"/> and
in general circulation model (GCM) simulations of future climate
<xref ref-type="bibr" rid="bib1.bibx31 bib1.bibx53 bib1.bibx33 bib1.bibx52 bib1.bibx19 bib1.bibx34" id="paren.7"/>. A
number of studies find that extreme changes follow closely with changes in
means and standard deviations <xref ref-type="bibr" rid="bib1.bibx14 bib1.bibx42" id="paren.8"><named-content content-type="pre">e.g.,</named-content></xref>.
<xref ref-type="bibr" rid="bib1.bibx42" id="text.9"/>, for example, argue that changes in temperature extremes in
station data from Eurasia and the United States are largely explained by
changes in the mean and standard deviation of daily temperatures within the
relevant season (summer for warm extremes and winter for cold extremes).
Other studies may suggest more complex changes. <xref ref-type="bibr" rid="bib1.bibx3" id="text.10"/> use
quantile regression and clustering to show that the changes in the 5th
percentiles and the 95th percentiles of daily air temperature over central
Europe are not the same as changes in medians, although they do not
explicitly examine to what extent these differences can be explained by
changing standard deviations. <xref ref-type="bibr" rid="bib1.bibx2" id="text.11"/> find evidence that
accounting for changes in skewness in marginal distributions allows for a
more accurate representation of changes in cold extremes than can be obtained
from just considering changes in mean and standard deviation.</p>
      <p>Analysis of changes in extremes is complicated by the fact that there is no
unique definition of “extremes”. One common definition is as exceedance of
certain defined thresholds, with threshold values often defined based on past
climate distributions <xref ref-type="bibr" rid="bib1.bibx20 bib1.bibx1 bib1.bibx53" id="paren.12"><named-content content-type="pre">e.g.,</named-content></xref>.
Analyses then evaluate changes in the frequencies at which these thresholds
are surpassed. <xref ref-type="bibr" rid="bib1.bibx1" id="text.13"/>, for example, used percentile-based
thresholds for various climate metrics from 3 decades of global gridded
observations (1961–1990) and then considered changes in a subsequent period
(1991–2003). They found a significant increase in the occurrence of annual
warm nights (defined as the 90th percentile of daily minimum temperature
under the past climate) and a significant decrease in the occurrence of cold
nights (defined as the 10th percentile of daily minimum temperature under the
past climate). However, those studies do not characterize changes in the
shape of a distribution by making use of information on the magnitude of
exceedances above (or below) the defined threshold.</p>
      <p>An alternative and potentially more useful definition of “extremes” is
based on occurrences in the far tail of the distribution of the quantity of
interest. Extreme value theory (EVT)
<xref ref-type="bibr" rid="bib1.bibx18 bib1.bibx24 bib1.bibx7 bib1.bibx30" id="paren.14"/> provides a mathematical
framework for studying these far tails. One common approach making use of EVT
is based on “block extremes”, the maxima (minima) of some climate variable
over given blocks of time. In climate studies, blocks of 1 year are common
<xref ref-type="bibr" rid="bib1.bibx60" id="paren.15"><named-content content-type="pre">e.g.,</named-content></xref>, although <xref ref-type="bibr" rid="bib1.bibx42" id="text.16"/> use blocks of
45–50 days in order to get two blocks per season. Under some conditions, the
magnitudes of extremes over sufficiently long blocks approximately follow a
generalized extreme value (GEV) distribution (<xref ref-type="bibr" rid="bib1.bibx23" id="altparen.17"/>,
<xref ref-type="bibr" rid="bib1.bibx36" id="altparen.18"/>, and see chap. 1 of <xref ref-type="bibr" rid="bib1.bibx13" id="altparen.19"/>, for details).
In these cases, the tail behavior of the distribution can be described by a
functional form involving only three parameters: the location, scale, and
shape parameters of the GEV distribution. For example, the widely used
measure of extreme events, the <inline-formula><mml:math display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula>-year return level, can be expressed as a
function of the GEV parameters (see Sect. <xref ref-type="sec" rid="Ch1.S3"/> for further review).
Annual extremes are directly relevant to important societal impacts; for
example, the coldest temperature in a winter can affect the abundance of the
beetle population in the following spring <xref ref-type="bibr" rid="bib1.bibx48 bib1.bibx55 bib1.bibx59" id="paren.20"/>.
The behavior of annual extremes is difficult to discern from marginal
distributions of daily temperatures. Figure <xref ref-type="fig" rid="Ch1.F1"/> illustrates how
changes in block extremes can differ from changes in the underlying overall
distribution, using seasonal temperature minima from millennial-scale climate
model runs. Figure <xref ref-type="fig" rid="Ch1.F3"/> in Sect. <xref ref-type="sec" rid="Ch1.S3.SS2"/> illustrates
the effect on return levels of changing each individual GEV parameter.</p>
      <p>The major limitation of the block extremes approach is that it discards all
but the most extreme value within each block. In contrast, the peak over
threshold (POT) method uses all data above a specified threshold. The POT
method models exceedances over a (sufficiently high/low) threshold as a
generalized Pareto distribution (GPD)
<xref ref-type="bibr" rid="bib1.bibx43 bib1.bibx50 bib1.bibx12" id="paren.21"/>. Point process theory as applied
to exceedances over a threshold provides a unified way to derive both GEV and
GPD distributions <xref ref-type="bibr" rid="bib1.bibx45 bib1.bibx50" id="paren.22"/>. While the POT method allows
data on extremes to be used more efficiently, it requires choosing
appropriate thresholds and declustering temporally dependent extremes.
Threshold selection becomes complicated because temperature extremes show
strong seasonality and temporal dependence. Furthermore, the temporal
dependence in threshold exceedances means that it is not straightforward to
convert inferences from the POT approach into inferences on annual extremes.
We focus on the block extremes approach here because of its simplicity, its
ease of interpretation, and its common usage in climate science.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1"><caption><p>Wintertime (December–February) temperatures from a location in
Idaho from 1000-year CCSM3 model runs under pre-industrial and 700 ppm
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> levels. Bottom: marginal distributions of daily minimum
temperatures in winter. Top: distributions of winter seasonal minima. Note:
(1) in both climate states, the distributions of seasonal minima are skewed
to the right, whereas their marginal distributions are skewed to the left;
(2) in the future warmer climate state, variation in the marginal
distribution decreases but variation in the seasonal minima increases; and
(3) the median of the distribution of seasonal minima increases more than the
median of the marginal distribution. We use seasonal instead of annual minima
in this example so that the marginal and extreme distributions are based on
the same data. The analogous plot for summertime maxima at this location is
shown in Appendix Fig. <xref ref-type="fig" rid="App1.Ch1.F1"/>.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://ascmo.copernicus.org/articles/2/79/2016/ascmo-2-79-2016-f01.pdf"/>

      </fig>

      <p>An important advantage of using any EVT-based approach for the study of
climate extremes is that it allows estimation of the probability of events
that are more rare than the “moderate extremes” analyzed in threshold
exceedance studies. The threshold exceedance study of <xref ref-type="bibr" rid="bib1.bibx1" id="text.23"/>,
for example, used a threshold equivalent to the 90th percentile
of temperature calculated over a 5-day sliding window, which corresponds to
events whose present mean recurrence interval is only 50 days. EVT allows
examination of rare events of much longer recurrence intervals, and in
principle even allows estimation of return levels longer than the observed
range of the available time series together with a measure of statistical
uncertainty. EVT has been widely applied in hydrology, for example, to
estimate 100-year floods using several decades of data
<xref ref-type="bibr" rid="bib1.bibx24 bib1.bibx30" id="paren.24"/>.</p>
      <p>In the past 2 decades, EVT has been applied in numerous studies to climate
variables, generally temperature and precipitation
<xref ref-type="bibr" rid="bib1.bibx60 bib1.bibx32 bib1.bibx33 bib1.bibx52 bib1.bibx19 bib1.bibx11 bib1.bibx34" id="paren.25"><named-content content-type="pre">including</named-content></xref>.
Studies have evaluated GEV distributions both in observational data and in
output from general circulation models (GCMs) and regional climate models
(RCMs). <xref ref-type="bibr" rid="bib1.bibx33 bib1.bibx34" id="text.26"/> evaluated GCM ensembles from the CMIP3
and CMIP5 archives under several projected emission scenarios. In both
studies, they found asymmetry in extreme changes, with high temperature
extremes in most regions following changes in the mean summer temperature,
while low temperature extremes warmed substantially more than mean winter
temperatures.</p>
      <p>Prior GEV studies are limited to some extent by two factors: the length and
non-stationarity of the analyzed time series. For observational studies,
existing data records are relatively short (often only several decades).
Model runs may be longer, but the model runs used in these studies typically
extend only around 100 years from the present. For some models and scenarios,
“initial condition ensembles” are available, i.e., multiple runs of the
same model and forcing scenario that differ only in their initial conditions.
Such ensembles obviously provide further information about extreme events,
but they generally include only a few model realizations. The length of the
time series has a large influence on the ability to detect changes in
extremes, and a record that is too short can lead to large uncertainty in
estimated return levels at long periods (see Sect. <xref ref-type="sec" rid="Ch1.S6"/>). Furthermore,
at present and for the foreseeable future, the Earth's climate is not in
equilibrium, but is evolving (transient), so the GEV model must be extended
to account for non-stationarity in climate extremes. The means of extension
are not trivial. The most commonly used nonstationary GEV model
<xref ref-type="bibr" rid="bib1.bibx32" id="paren.27"><named-content content-type="pre">e.g.,</named-content></xref> assumes that location and scale parameters change
linearly in time and the shape parameter is time-invariant. A more flexible
approach to modeling nonstationarity can be achieved by using generalized
additive temporal structure of the parameters for extreme value distributions
<xref ref-type="bibr" rid="bib1.bibx6 bib1.bibx58 bib1.bibx25" id="paren.28"/>. Given the limited information about
extreme events, it is a challenging and important problem to decide on an
appropriate degree of flexibility in a nonstationary model.</p>
      <p>In this study we avoid the limitations of short transient runs by using three
long (millennial) climate model runs in which climate is fully equilibrated.
Although numerical simulations of future climates provide only suggestions
for possible changes in climate variables, not direct evidence of changes,
they are important complements to observational studies. We use temperature
output from the widely used Community Climate System 3 (CCSM3) model
<xref ref-type="bibr" rid="bib1.bibx8 bib1.bibx57" id="paren.29"/> at three different <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> levels. For
each scenario, the climate model is run for a sufficiently long warmup period
to ensure the climate has fully responded to forcing changes, so that any
time series of block extremes effectively forms a stationary sequence.
Millennial stationary runs allow a more accurate determination of any changes
in GEV distributions than do the shorter runs of the CMIP archives. The long
model runs also allow us to assess, based on the max-stable property of GEV
distributions (see Sect. <xref ref-type="sec" rid="Ch1.S5"/> for details), the appropriateness of
the choice of annual blocks that have been traditionally used with shorter
(century-scale) climate model runs. Finally, millennial runs allow us to
evaluate empirically the sampling errors when estimating extreme return
levels in shorter model runs, because we can use estimates based on entire
long runs as “ground truth”.</p>
      <p>The paper is structured as follows: in Sect. <xref ref-type="sec" rid="Ch1.S2"/>, we describe the
climate model output used in this work; in Sect. <xref ref-type="sec" rid="Ch1.S3"/>, we provide a
background for the univariate extreme value theory we employ; in
Sect. <xref ref-type="sec" rid="Ch1.S4"/>, we describe the changes in extreme value distributions and
corresponding return levels, and compare them with changes in climate means.
In Sect. <xref ref-type="sec" rid="Ch1.S5"/>, we assess the assumption that annual blocks are
sufficiently long for the GEV approximation to be valid, and in
Sect. <xref ref-type="sec" rid="Ch1.S6"/> we assess the sensitivity of estimates of return levels to
the series length. We conclude with a discussion of the implications of these
results.</p>
</sec>
<sec id="Ch1.S2">
  <title>GCM output</title>
      <p>The GCM output used is part of an ensemble of climate simulations completed
by the Center for Robust Decision Making on Climate and Energy Policy (RDCEP)
<xref ref-type="bibr" rid="bib1.bibx5 bib1.bibx38" id="paren.30"><named-content content-type="pre">e.g.,</named-content></xref>, using the Community Climate System
Model version 3 (CCSM3) <xref ref-type="bibr" rid="bib1.bibx8" id="paren.31"/>, a fully coupled model with full
representation of the atmosphere (CAM3), land (CLM3), sea ice (CSIM5) and
ocean (POP 1.4.3) components. The model was run at the relatively coarse T31
spatial resolution (3.75<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 3.75<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> grid)
<xref ref-type="bibr" rid="bib1.bibx57" id="paren.32"/>, which made the lengthy runs used here possible. We use
here the last 1000 years of output from each of three multimillennial runs
with different atmospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> concentrations: 289 ppm
(pre-industrial), 700 ppm (3.4 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C increase in global mean
temperature (GMT)), and 1400 ppm (6.1 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C increase in GMT). In each
case, solar forcing, aerosol concentrations, and concentrations of greenhouse
gases other than <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> are kept at their pre-industrial values. The
final 1000 years of each model run are very nearly in equilibrium: net global
radiative imbalances at the surface and at the top-of-atmosphere (TOA) are
smaller than 0.1 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">W</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>. The annual extreme temperatures therefore
effectively form stationary time series. In this work, we consider annual
maxima (from 1 January to 31 December) of daily maximum temperature
(<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mtext>max</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>) and annual minima (from 1 July to 31 June) of daily
minimum temperature (<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mtext>min</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>) over the contiguous United States and
adjacent ocean regions (see Fig. <xref ref-type="fig" rid="Ch1.F2"/>).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2"><caption><p>Locations of centers of grid cells for model output used here. The
rainbow color scale for latitudes is used throughout this study. Idaho (ID),
California (CA), and Texas (TX) grid cells are used as examples in Figs. <xref ref-type="fig" rid="Ch1.F6"/>, <xref ref-type="fig" rid="Ch1.F10"/>, and
<xref ref-type="fig" rid="Ch1.F11"/>.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://ascmo.copernicus.org/articles/2/79/2016/ascmo-2-79-2016-f02.pdf"/>

      </fig>

<?xmltex \hack{\newpage}?>
</sec>
<sec id="Ch1.S3">
  <title>Statistical background</title>
      <p>The GEV distribution is widely applicable in the sciences because it arises,
at least approximately, in many cases of natural data. The simplest situation
where a GEV distribution can arise is in distributions of maxima taken from
sequences of <inline-formula><mml:math display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula> independent and identically distributed (i.i.d.) random
variables (<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>Y</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>,</mml:mo><mml:mi mathvariant="normal">⋯</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi>Y</mml:mi><mml:mi>n</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>), with “block length” <inline-formula><mml:math display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula> sufficiently
large. The extremal types theorem says that if the maxima <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi>n</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mo>max⁡</mml:mo><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mo>(</mml:mo><mml:msub><mml:mi>Y</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>,</mml:mo><mml:mi mathvariant="normal">⋯</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi>Y</mml:mi><mml:mi>n</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, after normalization (i.e.,
<inline-formula><mml:math display="inline"><mml:mstyle displaystyle="false"><mml:mfrac style="text"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi>n</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>b</mml:mi><mml:mi>b</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi>a</mml:mi><mml:mi>n</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>a</mml:mi><mml:mi>n</mml:mi></mml:msub><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>), converge in distribution as <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>n</mml:mi><mml:mo>→</mml:mo><mml:mi mathvariant="normal">∞</mml:mi></mml:mrow></mml:math></inline-formula> (see Appendix <xref ref-type="sec" rid="App1.Ch1.S2"/>), then they converge to a GEV
distribution <xref ref-type="bibr" rid="bib1.bibx18 bib1.bibx23" id="paren.33"/>.</p>
      <p>In this work, when studying high temperature extremes, the random variables
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>Y</mml:mi><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>,</mml:mo><mml:mi>i</mml:mi></mml:mrow></mml:msub><mml:mo>,</mml:mo><mml:mi mathvariant="normal">⋯</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi>Y</mml:mi><mml:mrow><mml:mi>n</mml:mi><mml:mo>,</mml:mo><mml:mi>i</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> are the daily maximum temperatures in year <inline-formula><mml:math display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>, and
the block length <inline-formula><mml:math display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula> is 365 days, so that <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mrow><mml:mi>n</mml:mi><mml:mo>,</mml:mo><mml:mi>i</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> is the maximum for year
<inline-formula><mml:math display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>. Of course time series of daily temperatures are neither independent
(they are somewhat autocorrelated) nor identically distributed (their
distributions vary within a year). There is however theoretical justification
for the use of GEV distributions in our case: it has been shown that the
independence assumption can be relaxed for weakly dependent stationary time
series <xref ref-type="bibr" rid="bib1.bibx36 bib1.bibx28" id="paren.34"/>, and <xref ref-type="bibr" rid="bib1.bibx17" id="text.35"/> extended the
theory to non-identically distributed observations with conditions on the
tail distributions (e.g., distributions share a common absolute maximum). In
this work, we explicitly assess whether inferred GEV distributions actually
provide an adequate description of the data set in question. The CCSM3
temperature time series studied here do seem to meet this condition:
quantile–quantile plots show that the GEV approximation fits reasonably well
for most locations in our study area (see Figs. <xref ref-type="fig" rid="App1.Ch1.F2"/>
and <xref ref-type="fig" rid="App1.Ch1.F3"/> in Appendix <xref ref-type="sec" rid="App1.Ch1.S3"/>). We therefore assume that
annual maxima and minima of daily temperatures in our model output can be
approximated by GEV distributions. We will revisit the assessment of the GEV
approximation in Sect. <xref ref-type="sec" rid="Ch1.S5"/> when we test whether our block length of 1
year is sufficient.</p>
<sec id="Ch1.S3.SS1">
  <title>GEV distributions</title>
      <p>We give here a brief review of EVT for block maxima. For further background,
<xref ref-type="bibr" rid="bib1.bibx13" id="text.36"/> and <xref ref-type="bibr" rid="bib1.bibx45 bib1.bibx46" id="text.37"/> give systematic theoretical
accounts and <xref ref-type="bibr" rid="bib1.bibx7" id="text.38"/> and <xref ref-type="bibr" rid="bib1.bibx4" id="text.39"/> provide statistical
treatments. The GEV distribution function, described in terms of its three
parameters <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">μ</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>, and <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">ξ</mml:mi></mml:math></inline-formula>, is

                <disp-formula id="Ch1.E1" content-type="numbered"><mml:math display="block"><mml:mrow><mml:msub><mml:mi>G</mml:mi><mml:mrow><mml:mi mathvariant="italic">μ</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="italic">σ</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="italic">ξ</mml:mi></mml:mrow></mml:msub><mml:mo>(</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mfenced close="" open="{"><mml:mtable class="array" columnalign="left left"><mml:mtr><mml:mtd><mml:mrow><mml:mi>exp⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mo>-</mml:mo><mml:msubsup><mml:mfenced open="{" close="}"><mml:mn mathvariant="normal">1</mml:mn><mml:mo>+</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi mathvariant="italic">ξ</mml:mi><mml:mo>(</mml:mo><mml:mi>y</mml:mi><mml:mo>-</mml:mo><mml:mi mathvariant="italic">μ</mml:mi><mml:mo>)</mml:mo></mml:mrow><mml:mi mathvariant="italic">σ</mml:mi></mml:mfrac></mml:mstyle></mml:mfenced><mml:mo>+</mml:mo><mml:mfrac><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi mathvariant="italic">ξ</mml:mi></mml:mfrac></mml:msubsup></mml:mfenced></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mi mathvariant="italic">ξ</mml:mi><mml:mo>≠</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd/></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:mi>exp⁡</mml:mi><mml:mfenced close=")" open="("><mml:mo>-</mml:mo><mml:mi>exp⁡</mml:mi><mml:mfenced close="}" open="{"><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>-</mml:mo><mml:mo>(</mml:mo><mml:mi>y</mml:mi><mml:mo>-</mml:mo><mml:mi mathvariant="italic">μ</mml:mi><mml:mo>)</mml:mo></mml:mrow><mml:mi mathvariant="italic">σ</mml:mi></mml:mfrac></mml:mstyle></mml:mfenced></mml:mfenced></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mi mathvariant="italic">ξ</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:mfenced></mml:mrow></mml:math></disp-formula>

          where <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>u</mml:mi><mml:mo>+</mml:mo></mml:msub><mml:mo>=</mml:mo><mml:mo>max⁡</mml:mo><mml:mo>(</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mo>,</mml:mo><mml:mi>u</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>. <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">μ</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula> are location and scale
parameters, respectively, and the shape parameter <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">ξ</mml:mi></mml:math></inline-formula> determines the tail
behavior of the density. When <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">ξ</mml:mi></mml:math></inline-formula> is zero, the distribution is an
<italic>exponentially tailed</italic> Gumbel distribution; <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="italic">ξ</mml:mi><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula> yields the
<italic>heavy-tailed</italic> Fréchet distribution; and <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="italic">ξ</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula> yields the
<italic>bounded-tailed</italic> reversed Weibull distribution, in which the
distribution has an absolute maximum of <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="italic">μ</mml:mi><mml:mo>-</mml:mo><mml:mi mathvariant="italic">σ</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="italic">ξ</mml:mi></mml:mrow></mml:math></inline-formula>. Distributions of
temperature extremes typically have <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="italic">ξ</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx22 bib1.bibx21" id="paren.40"><named-content content-type="pre">e.g.,</named-content></xref>.</p>
      <p>To study low temperature extremes, we must consider minima rather than
maxima. Equation (<xref ref-type="sec" rid="Ch1.S3.SS1"/>) can be used to study minima simply by
considering the maximum of <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:msub><mml:mi>Y</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>,</mml:mo><mml:mi mathvariant="normal">…</mml:mi><mml:mo>,</mml:mo><mml:mo>-</mml:mo><mml:msub><mml:mi>Y</mml:mi><mml:mi>n</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, where <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>Y</mml:mi><mml:mi>j</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> represents the
daily minimum temperature on day <inline-formula><mml:math display="inline"><mml:mi>j</mml:mi></mml:math></inline-formula>. However, if one lets <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>(</mml:mo><mml:mi mathvariant="italic">μ</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="italic">σ</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="italic">ξ</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>
be the parameters for the corresponding GEV distribution of the maximum of
the negative temperature, then increasing <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">μ</mml:mi></mml:math></inline-formula> would correspond to
decreasing temperature, which we find potentially confusing. We therefore
adopt the convention that when considering temperature minima, for the
corresponding GEV distribution, we write

                <disp-formula id="Ch1.E2" content-type="numbered"><mml:math display="block"><mml:mrow><mml:msub><mml:mi>G</mml:mi><mml:mrow><mml:mi mathvariant="italic">μ</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="italic">σ</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="italic">ξ</mml:mi></mml:mrow></mml:msub><mml:mo>(</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mfenced close="" open="{"><mml:mtable class="array" columnalign="left left"><mml:mtr><mml:mtd><mml:mrow><mml:mi>exp⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mo>-</mml:mo><mml:msubsup><mml:mfenced close="}" open="{"><mml:mn mathvariant="normal">1</mml:mn><mml:mo>+</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi mathvariant="italic">ξ</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="italic">μ</mml:mi><mml:mo>-</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo></mml:mrow><mml:mi mathvariant="italic">σ</mml:mi></mml:mfrac></mml:mstyle></mml:mfenced><mml:mo>+</mml:mo><mml:mfrac><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi mathvariant="italic">ξ</mml:mi></mml:mfrac></mml:msubsup></mml:mfenced></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mi mathvariant="italic">ξ</mml:mi><mml:mo>≠</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd/></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:mi>exp⁡</mml:mi><mml:mfenced close=")" open="("><mml:mo>-</mml:mo><mml:mi>exp⁡</mml:mi><mml:mfenced close="}" open="{"><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>-</mml:mo><mml:mo>(</mml:mo><mml:mi mathvariant="italic">μ</mml:mi><mml:mo>-</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo></mml:mrow><mml:mi mathvariant="italic">σ</mml:mi></mml:mfrac></mml:mstyle></mml:mfenced></mml:mfenced></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mi mathvariant="italic">ξ</mml:mi><mml:mo>=</mml:mo><mml:mn>0.</mml:mn></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:mfenced></mml:mrow></mml:math></disp-formula>

          With this definition, a larger <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">μ</mml:mi></mml:math></inline-formula> corresponds to warmer temperature
minima. In the remainder of this work, we assume that for annual maxima, the
relevant GEV distribution is Eq. (<xref ref-type="sec" rid="Ch1.S3.SS1"/>), and for annual minima, the
relevant distribution is Eq. (<xref ref-type="disp-formula" rid="Ch1.E2"/>).</p>
</sec>
<sec id="Ch1.S3.SS2">
  <title>Relationship between GEV distributions and return levels</title>
      <p>In the analysis that follows, we also describe extremes by their return
levels, a widely used measure of extreme events. For warm temperature
extremes, the <inline-formula><mml:math display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula>-year return level is the (block maximum) temperature
exceeded on average once per <inline-formula><mml:math display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula> years. Note that the concept of return
levels implicitly assumes stationary conditions. Return levels in a data set
whose extremes follow a GEV distribution can be written in terms of the GEV
parameters. Letting <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mi>r</mml:mi></mml:mrow></mml:math></inline-formula>, the <inline-formula><mml:math display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula>-year return level <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>y</mml:mi><mml:mi>p</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the <inline-formula><mml:math display="inline"><mml:mrow><mml:mn>100</mml:mn><mml:mo>×</mml:mo><mml:mo>(</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:mi>p</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>th quantile of the underlying GEV distribution, which can be
determined by solving the equation <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>G</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi>y</mml:mi><mml:mi>p</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:mi>p</mml:mi></mml:mrow></mml:math></inline-formula> (for <inline-formula><mml:math display="inline"><mml:mrow><mml:mn mathvariant="normal">0</mml:mn><mml:mo>&lt;</mml:mo><mml:mi>p</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula>) to obtain
            <disp-formula id="Ch1.E3" content-type="numbered"><mml:math display="block"><mml:mrow><mml:msub><mml:mi>y</mml:mi><mml:mi>p</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mfenced open="{" close=""><mml:mtable class="array" columnalign="left left"><mml:mtr><mml:mtd><mml:mrow><mml:mi mathvariant="italic">μ</mml:mi><mml:mo>-</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="italic">ξ</mml:mi></mml:mfrac></mml:mstyle><mml:mfenced close="}" open="{"><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:msup><mml:mfenced close=")" open="("><mml:mo>-</mml:mo><mml:mi>log⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:mi>p</mml:mi></mml:mfenced></mml:mfenced><mml:mrow><mml:mo>-</mml:mo><mml:mi mathvariant="italic">ξ</mml:mi></mml:mrow></mml:msup></mml:mfenced></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mi mathvariant="italic">ξ</mml:mi><mml:mo>≠</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:mi mathvariant="italic">μ</mml:mi><mml:mo>-</mml:mo><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>log⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mo>-</mml:mo><mml:mi>log⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:mi>p</mml:mi></mml:mfenced></mml:mfenced></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mi mathvariant="italic">ξ</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:mfenced></mml:mrow></mml:math></disp-formula>
          where the “log” denotes the natural logarithm. A similar result holds for
temperature minima.<fn id="Ch1.Footn1"><p>Note that Eq. (<xref ref-type="disp-formula" rid="Ch1.E3"/>) implicitly
assumes block lengths of 1 year and must be changed for different block
lengths: the definition of <inline-formula><mml:math display="inline"><mml:mi>p</mml:mi></mml:math></inline-formula> becomes <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>=</mml:mo><mml:mi>b</mml:mi><mml:mo>/</mml:mo><mml:mi>r</mml:mi></mml:mrow></mml:math></inline-formula>, where <inline-formula><mml:math display="inline"><mml:mi>b</mml:mi></mml:math></inline-formula> is the block length
in years. The differences in <inline-formula><mml:math display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula>-year return levels defined by different
block lengths are largest for the shortest return periods (largest <inline-formula><mml:math display="inline"><mml:mi>p</mml:mi></mml:math></inline-formula>) and
become negligible for multi-decadal return periods (<inline-formula><mml:math display="inline"><mml:mi>p</mml:mi></mml:math></inline-formula> close to 0).</p></fn></p>
      <p>In the warmer climate conditions that result from higher atmospheric
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, the GEV distributions of temperature extremes may change,
altering return levels. Changes in the different GEV parameters affect return
levels in different ways. In Fig. <xref ref-type="fig" rid="Ch1.F3"/>, we illustrate the
consequences on both distributions and return levels of changing each GEV
parameter. Changing the location parameter <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">μ</mml:mi></mml:math></inline-formula> simply shifts the
distribution of extremes by the change <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi mathvariant="italic">μ</mml:mi></mml:mrow></mml:math></inline-formula> and changes return levels
uniformly at all return periods by the same amount
(Fig. <xref ref-type="fig" rid="Ch1.F3"/>, top row). Changing the scale parameter <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>
broadens or narrows the distribution of extremes, so that for warm extremes,
increasing <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula> increases return levels for long return periods and
decreases them for short return periods (Fig. <xref ref-type="fig" rid="Ch1.F3"/>, middle
row). Changing the shape parameter <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">ξ</mml:mi></mml:math></inline-formula> alters the “heaviness” of the
tails, but does so asymmetrically, with the greatest extremes most strongly
affected (the high temperature tail for maxima, and the low temperature tail
for minima). The resultant changes in return levels are then highly nonlinear
with return period. Moderate changes in <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">ξ</mml:mi></mml:math></inline-formula> have a negligible effect on
return levels for periods less than 10 years, but strongly affect the
“extreme extremes” at long return periods.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><caption><p>Illustration of the effect on return levels of changing individual
GEV parameters. We show consequences for both warm (red, left columns) and
cold (blue, right columns) extremes. Columns 1 and 3 show GEV distributions
for baseline (solid) and future (dashed) climates. Columns 2 and 4 show
resulting changes in return levels for different return periods. Note that
1000-year periods are on the right for warm and left for cold extremes, to
conform with percentiles. Location and shape parameters used here are chosen
as representative of our model results, with larger effects in cold extremes
than warm extremes, while shape parameters are identical in both cases. Top
row: changing the location parameter shifts return levels uniformly across
return periods. Middle row: increasing the scale parameter produces effects
dependent on return period. All return levels increase (decrease for cold
extremes), but more so for longer return periods. Bottom row: increasing
the shape parameter produces dramatic increases in return levels at very long
return periods.</p></caption>
          <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://ascmo.copernicus.org/articles/2/79/2016/ascmo-2-79-2016-f03.pdf"/>

        </fig>

</sec>
</sec>
<sec id="Ch1.S4">
  <title>Results</title>
      <p>By fitting the annual maxima and minima to a GEV distribution (see Appendix <xref ref-type="sec" rid="App1.Ch1.S4"/> for details), we can identify changes in the distribution
of extremes in possible future warmer climates, and evaluate how the
characteristics of those changes alter return levels of extreme events. We
show results here for all three model runs (pre-industrial, 700  and 1400 ppm <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>).</p>
<sec id="Ch1.S4.SS1">
  <title>GEV parameters in pre-industrial and future climates</title>
      <p>We show in Fig. <xref ref-type="fig" rid="Ch1.F4"/> the estimated CCSM3 GEV parameters for
warm and cold temperature extremes over the North American region. We show
maps of GEV parameter values for the pre-industrial climate (left column),
and maps of changes between pre-industrial and 700 ppm <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (middle
column) and between 700 and 1400 ppm <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (right column). The fitted
GEV parameters of the pre-industrial run show spatially coherent patterns,
with both latitudinal gradients and land–ocean contrast that are consistent
with expectations. The location parameters for warm extremes are highest
where summers are warmest, in the desert southwest and the inland
northeast/Midwest. Similarly, for cold extremes, <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">μ</mml:mi></mml:math></inline-formula>s are lowest where
winters are coldest: their pattern shows a strong latitudinal gradient but
moderated along the coasts. The scale parameter, which affects the spread of
the distribution of extremes, is largest in the continental interior and very
small over the ocean, as expected. The shape parameter, which affects the far
tail of the distribution of extremes, is negative nearly everywhere, as is
usually the case for surface temperatures.</p>
      <p>Under warmer future climate conditions, we have strong reasons to expect
positive shifts in location parameters: extremes should shift to warmer
values for both warm and cold extremes. There are, however, no simple
physical arguments that guide expectations for changes in the scale and shape
parameters. The 1000-year model runs used here allow us to accurately
estimate changes in all three parameters under this model.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><caption><p>The estimated CCSM3 GEV parameters and their changes in possible
future climate conditions. Left: fitted GEV parameters (location <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">μ</mml:mi></mml:math></inline-formula>,
scale <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>, and shape <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">ξ</mml:mi></mml:math></inline-formula>) for annual extremes for the baseline model
run at pre-industrial CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration. The top three panels are for warm
extremes and the bottom ones are for cold extremes. Negative <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">ξ</mml:mi></mml:math></inline-formula> is
expected for temperature distributions. Middle: changes in parameters
(<inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi mathvariant="italic">μ</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>log⁡</mml:mi><mml:mi mathvariant="italic">σ</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi mathvariant="italic">ξ</mml:mi></mml:mrow></mml:math></inline-formula>) after a warming of global
mean temperature by 3.4 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C (by raising atmospheric <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> to
700 ppm). Right: changes in parameters after an additional 2.7 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C
warming (by raising <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> from 700 to 1400 ppm). The symbols <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mo>+</mml:mo></mml:mrow></mml:math></inline-formula> or
<inline-formula><mml:math display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mo>-</mml:mo></mml:mrow></mml:math></inline-formula> mean the bootstrapped <inline-formula><mml:math display="inline"><mml:mi>p</mml:mi></mml:math></inline-formula> value for testing whether the parameter is
different in the scenarios is <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn>0.02</mml:mn></mml:mrow></mml:math></inline-formula>; <inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> or <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> mean the <inline-formula><mml:math display="inline"><mml:mi>p</mml:mi></mml:math></inline-formula> value is
between <inline-formula><mml:math display="inline"><mml:mn>0.02</mml:mn></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mn>0.10</mml:mn></mml:math></inline-formula>.</p></caption>
          <?xmltex \igopts{width=455.244094pt}?><graphic xlink:href="https://ascmo.copernicus.org/articles/2/79/2016/ascmo-2-79-2016-f04.pdf"/>

        </fig>

      <?xmltex \floatpos{p}?><fig id="Ch1.F5" specific-use="star"><caption><p>Assessment of whether <italic>changes</italic> in the location parameter of
extremes are linked to changes in mean <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>(</mml:mo><mml:mi>m</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> and standard deviation (<inline-formula><mml:math display="inline"><mml:mi>s</mml:mi></mml:math></inline-formula>) of
the corresponding seasonal distributions. Left: ratio of differences
between GEV location parameter and seasonal mean compared to ratio of
within-season standard deviations, for the transition from pre-industrial
(climate state 1) to 700 ppm <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (climate state 2). Right: same
results with climate state 1 corresponding to 700 ppm and state 2 to
1400 ppm. Scatterplots show these terms for all locations in study area, for
warm extremes in upper panels and for cold extremes in lower panels. Plots
show that <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>m</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is very well approximated by
<inline-formula><mml:math display="inline"><mml:mrow><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>m</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>)</mml:mo><mml:msub><mml:mi>s</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi>s</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, where <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>s</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi>s</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is the ratio of within-season
standard deviations.</p></caption>
          <?xmltex \igopts{width=312.980315pt}?><graphic xlink:href="https://ascmo.copernicus.org/articles/2/79/2016/ascmo-2-79-2016-f05.pdf"/>

        </fig>

      <?xmltex \floatpos{p}?><fig id="Ch1.F6" specific-use="star"><caption><p>Illustration of the changes in return levels and their relationship
with the changes in seasonal means. The histograms are for the 1000 annual
maxima (warm extremes) and minima (cold extremes) for the pre-industrial
(289 ppm, blue) and future (700 ppm, red). Smooth curves are corresponding
estimated GEV distributions. Return level plots show changes in estimated
return levels (dark curve) and uncertainty from the bootstrap procedure
(lighter curves). The corresponding changes in seasonal means are marked with
a cross (change in mean summertime daily maximum for warm extremes and mean
wintertime daily minimum for cold extremes).</p></caption>
          <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://ascmo.copernicus.org/articles/2/79/2016/ascmo-2-79-2016-f06.pdf"/>

        </fig>

      <p>Changes in the location parameters for both warm and cold extremes are, as
expected, positive everywhere in the study region
(Fig. <xref ref-type="fig" rid="Ch1.F4"/>, first and fourth rows) as climate warms. As
previously found in other studies of climate model output <xref ref-type="bibr" rid="bib1.bibx33 bib1.bibx34" id="paren.41"/> and observations <xref ref-type="bibr" rid="bib1.bibx37" id="paren.42"/>, the changes are unequal, with a
larger amount of warming in cold extremes than in warm extremes. For warm
extremes, location parameter changes are fairly uniform spatially and similar
to changes in summer mean temperatures (see Fig. <xref ref-type="fig" rid="App1.Ch1.F8"/> in
Appendix <xref ref-type="sec" rid="App1.Ch1.S5"/>). For cold extremes, location parameter
changes show a strong latitudinal gradient, similar to the pattern in
seasonal mean changes but with greater magnitude. That is, changes in cold
extremes exceed changes in winter means (Fig. <xref ref-type="fig" rid="App1.Ch1.F9"/> in
Appendix <xref ref-type="sec" rid="App1.Ch1.S5"/>). This asymmetry is readily explained by the
asymmetric changes in the seasonal temperature distributions. In simulated
warmer climate conditions, temperature variability (the standard deviation of
the distribution) is relatively unchanged in summer but strongly reduced in
winter, especially at higher latitudes <xref ref-type="bibr" rid="bib1.bibx26" id="paren.43"><named-content content-type="pre">e.g.,</named-content></xref>.
Figure <xref ref-type="fig" rid="Ch1.F5"/> shows that for both warm and cold extremes,
changes in the location parameter are well explained by changes in means and
standard deviations of seasonal temperature distributions.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7" specific-use="star"><caption><p>Estimated changes in warm extremes return levels for possible future
climate conditions in our CCSM3 runs. Top: 700 ppm <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> vs.
289 ppm <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> climate conditions; bottom: 1400 ppm <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> vs.
700 ppm <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> climate conditions. Each panel shows results from the
six grid cells in a longitude band, while each color represents a latitude
band. Estimated changes in return levels are plotted as solid lines in their
corresponding colors. Estimates obtained from block bootstrapped samples by
resampling years are plotted as lighter and thinner curves to form envelopes
representing the associated uncertainties. The corresponding summertime mean
changes for inland and ocean grid cells are marked by cross and filled box
symbols, respectively.</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://ascmo.copernicus.org/articles/2/79/2016/ascmo-2-79-2016-f07.png"/>

        </fig>

      <?xmltex \floatpos{p}?><fig id="Ch1.F8" specific-use="star"><caption><p>As in Fig. <xref ref-type="fig" rid="Ch1.F7"/> but for annual temperature
minima. Crosses and boxes now give wintertime mean changes. Note that the
return period axis is now flipped so that longer return periods are on the
left. In general, cold extremes warm more than do winter means, especially at
high latitudes.</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://ascmo.copernicus.org/articles/2/79/2016/ascmo-2-79-2016-f08.png"/>

        </fig>

<?xmltex \floatpos{p}?><table-wrap id="Ch1.T1" specific-use="star"><caption><p>GEV parameter estimates of warm and cold extremes for pre-industrial
climate state and the estimated changes from pre-industrial to 700 ppm
climate state at ID, CA, and TX locations.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="13">
     <oasis:colspec colnum="1" colname="col1" align="center"/>
     <oasis:colspec colnum="2" colname="col2" align="center"/>
     <oasis:colspec colnum="3" colname="col3" align="center"/>
     <oasis:colspec colnum="4" colname="col4" align="center"/>
     <oasis:colspec colnum="5" colname="col5" align="left"/>
     <oasis:colspec colnum="6" colname="col6" align="left"/>
     <oasis:colspec colnum="7" colname="col7" align="left"/>
     <oasis:colspec colnum="8" colname="col8" align="center"/>
     <oasis:colspec colnum="9" colname="col9" align="center"/>
     <oasis:colspec colnum="10" colname="col10" align="center"/>
     <oasis:colspec colnum="11" colname="col11" align="left"/>
     <oasis:colspec colnum="12" colname="col12" align="left"/>
     <oasis:colspec colnum="13" colname="col13" align="left"/>
     <oasis:thead>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry namest="col2" nameend="col7">Warm extremes </oasis:entry>  
         <oasis:entry namest="col8" nameend="col13">Cold extremes </oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry namest="col2" nameend="col4">289 ppm </oasis:entry>  
         <oasis:entry namest="col5" nameend="col7" align="center">700–289 ppm </oasis:entry>  
         <oasis:entry namest="col8" nameend="col10">289 ppm </oasis:entry>  
         <oasis:entry namest="col11" nameend="col13" align="center">700–289 ppm </oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2"><inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mi mathvariant="italic">μ</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col3"><inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mi mathvariant="italic">σ</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col4"><inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mi mathvariant="italic">ξ</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col5"><inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mover accent="true"><mml:mi mathvariant="italic">μ</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover></mml:mrow></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col6"><inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mover accent="true"><mml:mi mathvariant="italic">σ</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover></mml:mrow></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col7"><inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mover accent="true"><mml:mi mathvariant="italic">ξ</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover></mml:mrow></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col8"><inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mi mathvariant="italic">μ</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col9"><inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mi mathvariant="italic">σ</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col10"><inline-formula><mml:math display="inline"><mml:mover accent="true"><mml:mi mathvariant="italic">ξ</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col11"><inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mover accent="true"><mml:mi mathvariant="italic">μ</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover></mml:mrow></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col12"><inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mover accent="true"><mml:mi mathvariant="italic">σ</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover></mml:mrow></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col13"><inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mover accent="true"><mml:mi mathvariant="italic">ξ</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>  
         <oasis:entry colname="col1">ID</oasis:entry>  
         <oasis:entry colname="col2">26.4</oasis:entry>  
         <oasis:entry colname="col3">2.1</oasis:entry>  
         <oasis:entry colname="col4"><inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.32</oasis:entry>  
         <oasis:entry colname="col5"><inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>3.3<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>∗</mml:mo><mml:mo>∗</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col6"><inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.03</oasis:entry>  
         <oasis:entry colname="col7"><inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>0.05<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∗</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col8"><inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>41.9</oasis:entry>  
         <oasis:entry colname="col9">7.2</oasis:entry>  
         <oasis:entry colname="col10"><inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.37</oasis:entry>  
         <oasis:entry colname="col11"><inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>11.0<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>∗</mml:mo><mml:mo>∗</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col12"><inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>0.7<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>∗</mml:mo><mml:mo>∗</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col13"><inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>0.03</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">CA</oasis:entry>  
         <oasis:entry colname="col2">27.5</oasis:entry>  
         <oasis:entry colname="col3">0.8</oasis:entry>  
         <oasis:entry colname="col4"><inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.15</oasis:entry>  
         <oasis:entry colname="col5"><inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2.9<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>∗</mml:mo><mml:mo>∗</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col6"><inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>0.02</oasis:entry>  
         <oasis:entry colname="col7"><inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>0.01</oasis:entry>  
         <oasis:entry colname="col8"><inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1.5</oasis:entry>  
         <oasis:entry colname="col9">2.9</oasis:entry>  
         <oasis:entry colname="col10"><inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.14</oasis:entry>  
         <oasis:entry colname="col11"><inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>4.2<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>∗</mml:mo><mml:mo>∗</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col12"><inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.3<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>∗</mml:mo><mml:mo>∗</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col13"><inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>0.04<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∗</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">TX</oasis:entry>  
         <oasis:entry colname="col2">34.4</oasis:entry>  
         <oasis:entry colname="col3">1.7</oasis:entry>  
         <oasis:entry colname="col4"><inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.21</oasis:entry>  
         <oasis:entry colname="col5"><inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2.9<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>∗</mml:mo><mml:mo>∗</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col6"><inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>0.25<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>∗</mml:mo><mml:mo>∗</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col7"><inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.01</oasis:entry>  
         <oasis:entry colname="col8"><inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>6.9</oasis:entry>  
         <oasis:entry colname="col9">4.1</oasis:entry>  
         <oasis:entry colname="col10"><inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.10</oasis:entry>  
         <oasis:entry colname="col11"><inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>4.8<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>∗</mml:mo><mml:mo>∗</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col12"><inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1.1<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>∗</mml:mo><mml:mo>∗</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col13"><inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>0.05</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table><table-wrap-foot><p><inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∗</mml:mo></mml:msup></mml:math></inline-formula> means the bootstrapped <inline-formula><mml:math display="inline"><mml:mi>p</mml:mi></mml:math></inline-formula> value for testing whether
the parameter is different is between 0.02 and 0.1; <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>∗</mml:mo><mml:mo>∗</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula> means the
<inline-formula><mml:math display="inline"><mml:mi>p</mml:mi></mml:math></inline-formula> value is less than 0.02.</p></table-wrap-foot></table-wrap>

      <p>For both warm and cold extremes, scale parameters show changes that are
geographically complicated but statistically significant relative to
pre-industrial values over much of the region (see
Fig. <xref ref-type="fig" rid="Ch1.F4"/>). For warm extremes, scale parameters show little
change over much of the study area but modest increases over the eastern US,
up to 20 % larger than pre-industrial values. Scale parameters change
more strongly for cold extremes, with a strong latitudinal gradient over
land. The change from pre-industrial to 700 ppm CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> leads to
statistically significant decreases in scale parameters at lower latitudes
but statistically significant increases at higher latitudes. Scale parameters
for cold extremes additionally show clear nonlinear effects (see
Fig. <xref ref-type="fig" rid="Ch1.F4"/>, fifth row, middle and right panels): scale
parameters increase at high-latitude locations in the transition from
pre-industrial conditions to 700 ppm, but then decrease at these same
locations in the transition from 700 to 1400 ppm, partially negating the
earlier increases. Shape parameters show few statistically significant
changes for warm extremes but significant positive shifts for cold extremes
in some areas. When considering the full change in climate states from
pre-industrial to 1400 ppm CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, changes in the shape parameter for cold
extremes are in general significant at most inland locations, indicating that
linear transformations are not adequate for explaining all changes in
extremes (see Fig. <xref ref-type="fig" rid="App1.Ch1.F10"/>).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9" specific-use="star"><caption><p>A statistical diagnostic of the assumption that annual blocks are
sufficiently long for the GEV approximation. Differences (10- vs. 1-year
blocks) in estimated shape parameters are plotted for warm (left) and cold
(right) extremes against longitude. Estimates are shown for the
pre-industrial climate state, for all model grid cell locations in the study
area, with the same color and symbol scheme as in previous figures.
Subscripts in notation denote the block length; e.g., <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mover accent="true"><mml:mi mathvariant="italic">ξ</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover><mml:mtext>10</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>
means 10-year blocks. Circled points are those locations where differences in
estimates of the shape parameter changes are significant at the 0.05 level
based on their bootstrapped <inline-formula><mml:math display="inline"><mml:mi>p</mml:mi></mml:math></inline-formula> values.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://ascmo.copernicus.org/articles/2/79/2016/ascmo-2-79-2016-f09.pdf"/>

        </fig>

</sec>
<sec id="Ch1.S4.SS2">
  <title>Changes in return levels</title>
      <p>As discussed in Sect. <xref ref-type="sec" rid="Ch1.S3.SS2"/>, it can be helpful to describe changes in
tail behavior in terms of changes in return levels. We showed in
Fig. <xref ref-type="fig" rid="Ch1.F3"/> how hypothetical changes in individual GEV
parameters affect return levels at different return periods. Here we present
examples of changes in the actual fitted GEV distributions of model output,
and show how these produce changes in return levels. We use as examples three
model locations (individual grid cells), located in Idaho (ID), California
(CA), and Texas (TX) (see Fig. <xref ref-type="fig" rid="Ch1.F2"/> for locations), that illustrate
the behavior discussed in Sect. <xref ref-type="sec" rid="Ch1.S4.SS1"/>. For warm extremes in all three
locations (Fig. <xref ref-type="fig" rid="Ch1.F6"/>, left columns), the changes in return
levels are roughly constant for all return periods (except for ID at return
periods approaching 1000 years), meaning the dominant change is simply a
shift in the distribution of extremes, i.e., a change in location parameter.
The shifts are close (within 1 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C) to the shifts in mean seasonal
temperatures, as discussed previously. For cold extremes
(Fig. <xref ref-type="fig" rid="Ch1.F6"/>, right columns), in the inland locations of TX
and ID the shifts in extremes are much larger than in the seasonal means and
the scale and shape factors play a significant role, producing return level
changes that can vary with return period (though differently in different
locations). Of the examples shown here, scale and shape parameters play the
least significant role in the one coastal location (CA), as would be
expected.</p>
      <p>The different changes in warm and cold extremes shown in the example
locations of Fig. 6 are characteristic of the whole contiguous United States.
In CCSM3 model output, throughout the region, annual maximum return level
changes follow changes in summer means, but annual minimum return level
changes exceed winter means, with stronger influence of the scale and shape
parameters. Figures <xref ref-type="fig" rid="Ch1.F7"/> and <xref ref-type="fig" rid="Ch1.F8"/> show
the changes in return levels across return periods from 10 to 1000 years, for
annual maxima and minima, respectively. For warm extremes, changes in return
levels are relatively flat in both ocean and inland locations, implying that
the dominant effect is a change in the location parameter. Exceptions include
a small part of the central Midwest corn belt region and the far northeast,
which show increases in return levels with return periods. The sharply rising
“extreme extremes” in a few Midwest locations are due to the combined
increases in both the scale and the shape parameter; these effects grow still
further in the transition to a 1400 ppm climate
(Fig. <xref ref-type="fig" rid="Ch1.F7"/>, lower panel). For cold extremes
(Fig. <xref ref-type="fig" rid="Ch1.F8"/>), return level changes for ocean locations are
flat, but inland locations tend to show striking effects due to changes in
scale and shape parameters. Effects differ by latitude: at low latitudes,
return levels tend to increase with longer return periods, sometimes
dramatically so, whereas at high latitudes, the pattern generally reverses,
so that the most extreme cold temperatures tend to increase less than
modestly extreme cold temperatures. This distinction is particularly apparent
in the transition from pre-industrial to 700 ppm CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F10" specific-use="star"><caption><p>The relationship between sample errors for return levels and data
lengths for warm extremes. Estimates of changes (from pre-industrial to
700 ppm <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) in return levels (20-, 50-, 100-year return periods)
obtained by using different length segments (20 and 50 years, shown as blue
and red histograms), as compared to the “ground-truth” changes obtained
with the full 1000-year runs (dashed lines). We show warm extremes for the
same three grid cells shown in previous figures, located in Idaho,
California, and Texas. Pre-industrial return levels for these locations (for
20-, 50-, and 100-year periods) are ID: 30.4, 31.1, and 31.5 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C; CA:
29.4, 29.8, and 30.1 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C; and TX: 38.1, 38.9, and
39.4 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C.</p></caption>
          <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://ascmo.copernicus.org/articles/2/79/2016/ascmo-2-79-2016-f10.pdf"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F11" specific-use="star"><caption><p>Same as Fig. <xref ref-type="fig" rid="Ch1.F10"/> but for cold extremes.
Pre-industrial return levels for these locations are ID: <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>54.9, <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>56.8,
and <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>57.8 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C; CA: <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>8.5, <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>10.1, and <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>11.2 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C; and
TX: <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>17.2, <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>19.9, and <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>21.8 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C. Especially unreliable
estimates of changes in return levels were obtained for one pair of 20-year
segments in TX (denoted by <inline-formula><mml:math display="inline"><mml:mo>∗</mml:mo></mml:math></inline-formula>). This error is mainly due to a poorly
estimated shape parameter: for this pair of 20-year segments, the estimated
shape increased from <inline-formula><mml:math display="inline"><mml:mn>0.10</mml:mn></mml:math></inline-formula> to <inline-formula><mml:math display="inline"><mml:mn>0.60</mml:mn></mml:math></inline-formula> (the estimates given by PWM are <inline-formula><mml:math display="inline"><mml:mn>0.12</mml:mn></mml:math></inline-formula>
and <inline-formula><mml:math display="inline"><mml:mn>0.11</mml:mn></mml:math></inline-formula>), while the “true” values (based on 1000-year runs) were <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.10
and <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.05 for the pre-industrial and 700 ppm scenarios,
respectively.</p></caption>
          <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://ascmo.copernicus.org/articles/2/79/2016/ascmo-2-79-2016-f11.pdf"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F12"><caption><p>Assessment of sampling errors in estimates of return level changes
using comparable data lengths for all model grid cells in the study area.
Values shown are the estimated return level change minus the “ground-truth”
change determined from the entire 1000-year segment (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mtext>RL</mml:mtext><mml:mo>-</mml:mo><mml:mover accent="true"><mml:mi mathvariant="normal">Δ</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover><mml:mtext>RL</mml:mtext></mml:mrow></mml:math></inline-formula>), plotted against the “ground-truth”
change (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mtext>RL</mml:mtext></mml:mrow></mml:math></inline-formula>). Left: distribution (displayed as a boxplot) of
estimates of changes in 20-year return levels made using 20-year segments.
Right: the same for 50-year return levels and 50-year segments. Top and
bottom rows show warm and cold extremes. Gray reference lines are the <inline-formula><mml:math display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>:</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula>
lines (i.e., sampling error <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> return level change).</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://ascmo.copernicus.org/articles/2/79/2016/ascmo-2-79-2016-f12.pdf"/>

        </fig>

</sec>
</sec>
<sec id="Ch1.S5">
  <title>Sensitivity analysis: GEV block size</title>
      <p>In this analysis, as in many climate applications of EVT, we have assumed
that an annual block is long enough that the GEV distribution is
approximately valid. Our long time series allow us to explicitly evaluate
this assumption. The evaluation relies on the fact that the GEV distribution
has the property of “max-stability”. In the context of distributions of
block maxima (<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi>n</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>), max-stability means that the distribution after
normalization is identical for any block size larger than <inline-formula><mml:math display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula>.</p>
      <p>In our case, if an annual block is long enough that the GEV distribution is
approximately valid for a given time series, then the shape parameter
estimate <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mover accent="true"><mml:mi mathvariant="italic">ξ</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover><mml:mi>n</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> obtained with annual blocks should be approximately
the same as that obtained with a larger block size <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi>n</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mover accent="true"><mml:mi mathvariant="italic">ξ</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover><mml:mrow><mml:msup><mml:mi>n</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>).
The validity of the GEV approximation using annual extremes can therefore be
assessed by checking the consistency of estimated shape parameters using
longer block sizes (i.e., multiple years).</p>
      <p>We refit GEV distributions for each grid cell in our study region with block
maxima/minima sizes of 2, 5 and 10 years, and compare shape parameters. We
find that for annual maxima, the differences in <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">ξ</mml:mi></mml:math></inline-formula> with block size are
distributed around zero, suggesting that an annual block size may be
sufficient (Fig. <xref ref-type="fig" rid="Ch1.F9"/>, left panel). For annual minima, we see
effects of block size depending on latitude: longer blocks produce larger
<inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">ξ</mml:mi></mml:math></inline-formula> at high latitudes, where changes in extremes are largest
(Fig. <xref ref-type="fig" rid="Ch1.F9"/>, right panel). These results suggest that 1 year may
not be sufficiently long for the GEV approximation to be accurate. These
results also suggest that quantile–quantile plots (see Fig. <xref ref-type="fig" rid="App1.Ch1.F3"/>
in Appendix <xref ref-type="sec" rid="App1.Ch1.S3"/>) may not be sufficient to check for the
appropriateness of the GEV distribution for the purpose of predicting events
with a longer return period than the data length. We observe however that
annual blocks may be long enough for the study of the <italic>changes</italic> in
extremes, since changes in return levels are fairly consistent with block
length (see Figs. <xref ref-type="fig" rid="App1.Ch1.F4"/> and <xref ref-type="fig" rid="App1.Ch1.F5"/>).</p>
</sec>
<sec id="Ch1.S6">
  <title>Sensitivity analysis: data length on return level estimation</title>
      <p>The 1000-year model runs used in this work provide fairly accurate estimates
of changes in return levels even for long return periods. Estimated
uncertainties in return level changes – the bootstrapped envelopes in
Fig. <xref ref-type="fig" rid="Ch1.F8"/> – are generally within 20 % of the
estimated changes even for 100-year return periods. This data set therefore
allows us to study empirically how well GEV methods work when applied to
model output at the shorter lengths (decades to centuries) more commonly used
in climate studies.</p>
      <p>To assess how uncertainties increase with shorter model runs, we divide the
pre-industrial and 700 ppm time series into segments of 20 or 50 years and
refit the GEV parameters for each pair of segments (so, for example, pairing
the first 20 years of the pre-industrial run with the first 20 years of the
700 ppm run). The resulting distributions of estimates of changes in return
levels for warm and cold extremes are shown in
Figs. <xref ref-type="fig" rid="Ch1.F10"/> and <xref ref-type="fig" rid="Ch1.F11"/>.</p>
      <p>The results show that sampling error can be large, as expected, when using
climate simulations of length comparable to the return periods of interest.
In both warm and cold extremes, the distribution of estimates of return level
changes derived from short model segments are centered around their “true”
values but with large spread (Figs. <xref ref-type="fig" rid="Ch1.F10"/>
and <xref ref-type="fig" rid="Ch1.F11"/>). In these examples, the sampling errors are
comparable to their “true” changes in return level when 20-year segments
are used. Unsurprisingly, spreads are largest when using short model segments
to predict long return periods. For example, for the Idaho test location,
when changes in annual minimum 100-year return levels are estimated using
20-year segments (Fig. <xref ref-type="fig" rid="Ch1.F11"/>, lower left panel), those
estimates can differ by <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula>10 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C, while the “true” change is
only 8.4 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C. Uncertainties can be affected by the choice of
estimation method. <xref ref-type="bibr" rid="bib1.bibx27" id="text.44"/> suggest that estimation based on the
method of probability weighted moments (PWMs) has better small sample
properties than maximum likelihood, as we use here. Figure <xref ref-type="fig" rid="App1.Ch1.F6"/>
shows that results are generally very similar for the two methods, although a
PWM does avoid the few cases of highly unrealistic estimates seen in
Fig. <xref ref-type="fig" rid="Ch1.F11"/> in the TX example location.</p>
      <p>The example locations shown in Figs. <xref ref-type="fig" rid="Ch1.F10"/> and <xref ref-type="fig" rid="Ch1.F11"/> are representative of land locations in the entire
study area. In Fig. <xref ref-type="fig" rid="Ch1.F12"/>, we show the spread in estimates for
all model grid cells. We show two cases: estimating changes in 20-year
returns (both warm and cold extremes) with 20-year segments and changes in
50-year returns with 50-year segments. The length of the model segment is
especially important for temperature extremes, because their distribution has
a bounded tail. For inland locations, the spread in estimates is comparable
to the true change for the 20-year case but somewhat lower for the 50-year
case. Ocean locations show much smaller sampling error, presumably because
changes in extremes are produced predominantly by shifts in the location
parameter and not the scale or shape parameters, which are more difficult to
estimate. The locations with the largest uncertainties are indeed those with
the largest changes in shape parameter: a few Midwest locations for warm
extremes and some locations in Mexico for cold extremes.</p>
      <p>It is important to note that spatial modeling approaches may be able to
reduce estimation variability. (See further discussion in the following
section.) When not using such approaches, this assessment suggests that when
using single model runs or observational data, sampling error may be quite
large when the length of the series is comparable to the return period of
interest.</p>
</sec>
<sec id="Ch1.S7" sec-type="conclusions">
  <title>Discussion</title>
      <p>In this study, we have used extreme value theory to study changing
temperature extremes in model projections of future climate states. Following
prior work, we assume the GEV model provides a reasonable approximation for
the distribution of annual temperature extremes (see Figs. <xref ref-type="fig" rid="App1.Ch1.F2"/>
and <xref ref-type="fig" rid="App1.Ch1.F3"/>) and that changing temperature extremes can therefore
be studied by estimating changes in GEV parameters and resulting implied
changes in return levels. We use millennial-scale equilibrated simulations of
pre-industrial and 700 and 1400 ppm <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> concentrations (producing
changes in global mean temperature of 3.4 and 6.1 <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C) to explore both
the physics of climate model projections and the utility of statistical
approaches based on GEV distributions in different contexts.</p>
      <p>For our model runs, the results suggest that for the contiguous United
States, much of the behavior of temperature extremes in higher CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> climate
states appears to be a straightforward consequence of changes in the mean and
standard deviation of the underlying temperature distributions. Annual warm
extremes generally shift simply in accordance with mean shifts in summer
temperatures. Annual cold extremes warm more strongly than do winter mean
temperatures, but largely do so as expected given decreased variability in
wintertime temperatures. In both cases, the changes in the location parameter
of annual extremes appear well explained by shifts in overall seasonal
temperature means and standard deviations (Fig. <xref ref-type="fig" rid="Ch1.F5"/>). In
most inland locations in the winter, changes in the scale and shape
parameters can provide an additional complication, producing substantial
differences in return level changes at longer return periods
(Fig. <xref ref-type="fig" rid="Ch1.F8"/>). Note that these results are from a single
climate model, and there is no guarantee that any model will capture all
aspects of changes in extremes well <xref ref-type="bibr" rid="bib1.bibx41" id="paren.45"><named-content content-type="pre">e.g.,</named-content></xref>. Model studies
are, however, important given the difficulty in evaluating changes in
extremes from the short observational record.</p>
      <p>The millennial-scale model runs used here allow us to assess the validity of
the use of annual block sizes in studies of GEV distributions of temperature
extremes. Our results suggest that annual blocks are sufficiently long for
representing warm extremes, but may be insufficient for cold extremes,
especially for inland locations at high latitudes. In these locations,
altering the block length alters the shape parameter of the estimated GEV
distribution (Fig. <xref ref-type="fig" rid="Ch1.F9"/>). In general, increasing block size
reduces biases, but can increase sampling error in estimates if the time
series is limited. The choice of block size therefore requires consideration
of inherent trade-offs.</p>
      <p>Millennial-scale model runs also enable detailed investigation of the
relationship between data length and GEV sampling error. Previous studies
have suggested that extrapolation should be carried out with caution
<xref ref-type="bibr" rid="bib1.bibx33" id="paren.46"><named-content content-type="pre">e.g.,</named-content></xref>. Our long runs allow us to better quantify
estimation uncertainties resulting from short model runs. We find that over
inland locations, estimation uncertainty is indeed large when using series
length is comparable to the return period of interest
(Fig. <xref ref-type="fig" rid="Ch1.F12"/>). Ocean locations show much smaller sampling errors,
in large part because temperature variability is much lower over oceans than
over land. When using very short series (e.g., 20 years), lack of data
mandates care in choosing the appropriate estimation procedure
<xref ref-type="bibr" rid="bib1.bibx27 bib1.bibx22" id="paren.47"/>. Our 1000-year model runs allow us to
concretely demonstrate the large uncertainties in estimates of changes in
extremes that result when time series length is comparable to the return
period of interest.</p>
      <p>The computational demands of millennial-scale climate simulations restrict us
here to examining a single climate model run at fairly coarse resolution. A
single model should not be taken as robust guidance on how temperature
extremes may change in future climate conditions. However, few modeling
groups have performed runs of comparable length, and the multi-model data in
public archives are not ideal for estimating changes in extremes: run lengths
are much shorter (<inline-formula><mml:math display="inline"><mml:mo>≈</mml:mo></mml:math></inline-formula> 100 years), the number of realizations of any
scenario is small, and climate conditions in the simulations are evolving
rather than stationary. Estimating GEV distributions that are changing over
time is also more challenging than in the equilibrium setting, making the
limitations of short model runs even more pertinent. If understanding changes
in extremes in a changing climate is a research priority, larger ensembles of
model runs would be helpful.</p>
      <p>In the absence of large ensembles, one could potentially overcome some of the
challenges of limited data by exploiting the spatial structure of temperature
extremes (see Fig. <xref ref-type="fig" rid="Ch1.F4"/>) to “borrow strength over space”.
Numerous prior studies do explicitly model the spatial structure of a climate
variable of interest, e.g., <xref ref-type="bibr" rid="bib1.bibx10" id="text.48"/>, <xref ref-type="bibr" rid="bib1.bibx9" id="text.49"/>,
<xref ref-type="bibr" rid="bib1.bibx11" id="text.50"/>, and <xref ref-type="bibr" rid="bib1.bibx54" id="text.51"/>. However, spatial modeling is not
ideal: it may introduce bias, it greatly complicates the computation, and
spatial structure in GEV parameters can be difficult to distinguish from
spatial dependence in observed extremes. We do not use these approaches in
this work since the millennial-scale model runs allow us to estimate the GEV
parameters and their changes accurately by fitting them to each model grid
cell separately. However, where only shorter time series (decades to
centuries) are available, such as in analyses of observations, appropriate
spatial modeling may be essential to reduce estimation uncertainty.</p>
      <p><?xmltex \hack{\newpage}?>Extreme value theory (EVT) has become popular for studying climate extremes,
but our results here suggest that one should be aware of the underlying
assumptions, the corresponding implications, and the potential limitations
when applying it. EVT using block extremes can potentially allow
characterization of tail behavior that differs from that of the underlying
distribution, but it involves a corresponding penalty, as fitting a
distribution of block extremes necessarily involves throwing out most of
one's data. For short time series, care must be taken to ensure that the
drawbacks do not outweigh the benefits. In the climate model output studied
here, for example, shifts in the location parameter for both warm and cold
extremes are well explained by changes in the mean and standard deviation of
the underlying temperature distribution. The millennial time series used here
allow us to also identify significant changes in the scale parameter,
especially for cold extremes, but with shorter time series, sampling errors
can be too large for estimated return levels to be of much practical value.
Long model runs such as those used here therefore provide an important tool
for the study of climate extremes, helping both in clarifying the contexts in
which EVT should best be used and in devising approaches for working with
shorter time series.</p><?xmltex \hack{\clearpage}?>
</sec>

      
      </body>
    <back><app-group>

<app id="App1.Ch1.S1">
  <title>Comparison of distribution of extremes with overall distribution: summer</title>
      <p>We show the comparison of the overall distribution and the distribution of
extremes, as in Fig. <xref ref-type="fig" rid="Ch1.F1"/> but here for summer rather than winter.</p>

      <?xmltex \floatpos{h!}?><fig id="App1.Ch1.F1"><caption><p>As in Fig. <xref ref-type="fig" rid="Ch1.F1"/> but for summer warm extremes. Bottom:
overall distribution of summer (JJA) daily maximum temperature
(<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mtext>max</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>) in a northern Idaho location, for baseline and 700 ppm
CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> climate states. Top: distributions of seasonal maxima of summer
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mtext>max</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>. Note that the median shift of the overall distribution is
now slightly larger than that of the distribution of extremes; the opposite
was true for winter cold extremes.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://ascmo.copernicus.org/articles/2/79/2016/ascmo-2-79-2016-f13.pdf"/>

      </fig>

</app>

<app id="App1.Ch1.S2">
  <title>Extremal types theorem</title>
      <p>In this appendix, we briefly describe the fundamental result in extreme value
theory that justifies the use of GEV models for block maxima. Let <inline-formula><mml:math display="inline"><mml:mrow><mml:mo mathvariant="italic">{</mml:mo><mml:msub><mml:mi>Y</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo mathvariant="italic">}</mml:mo></mml:mrow></mml:math></inline-formula>
be a sequence of independent and identically distributed random variables
with cumulative distribution function <inline-formula><mml:math display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula> and let <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi>n</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mo>max⁡</mml:mo><mml:mo mathvariant="italic">{</mml:mo><mml:msub><mml:mi>Y</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>,</mml:mo><mml:mi mathvariant="normal">⋯</mml:mi><mml:mo>.</mml:mo><mml:msub><mml:mi>Y</mml:mi><mml:mi>n</mml:mi></mml:msub><mml:mo mathvariant="italic">}</mml:mo></mml:mrow></mml:math></inline-formula>. When <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>n</mml:mi><mml:mo>→</mml:mo><mml:mi mathvariant="normal">∞</mml:mi></mml:mrow></mml:math></inline-formula>, the sequence of random variables
<inline-formula><mml:math display="inline"><mml:mrow><mml:mfenced open="{" close="}"><mml:msub><mml:mi>M</mml:mi><mml:mi>n</mml:mi></mml:msub></mml:mfenced></mml:mrow></mml:math></inline-formula> converges to a single point <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>y</mml:mi><mml:mi>F</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mo>sup⁡</mml:mo><mml:mo mathvariant="italic">{</mml:mo><mml:mi>y</mml:mi><mml:mo>:</mml:mo><mml:mi>F</mml:mi><mml:mo>(</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo mathvariant="italic">}</mml:mo></mml:mrow></mml:math></inline-formula>,
where <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>y</mml:mi><mml:mi>F</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> may be infinite. In order to have a useful description of the
distribution of <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi>n</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> when <inline-formula><mml:math display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula> is sufficiently large, normalization is
needed; that is, we are seeking a limiting distribution for
<inline-formula><mml:math display="inline"><mml:mstyle displaystyle="false"><mml:mfrac style="text"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi>n</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>b</mml:mi><mml:mi>n</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi>a</mml:mi><mml:mi>n</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle></mml:math></inline-formula>. It turns out that if there exist constants
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>a</mml:mi><mml:mi>n</mml:mi></mml:msub><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>b</mml:mi><mml:mi>n</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and a non-degenerate distribution function <inline-formula><mml:math display="inline"><mml:mi>G</mml:mi></mml:math></inline-formula> such
that

              <disp-formula id="App1.Ch1.Ex1"><mml:math display="block"><mml:mrow><mml:mi mathvariant="double-struck">P</mml:mi><mml:mfenced close=")" open="("><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi>n</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>b</mml:mi><mml:mi>n</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi>a</mml:mi><mml:mi>n</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>≤</mml:mo><mml:mi>y</mml:mi></mml:mfenced><mml:mover><mml:mo movablelimits="false">→</mml:mo><mml:mi>d</mml:mi></mml:mover><mml:mi>G</mml:mi><mml:mo>(</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

        then <inline-formula><mml:math display="inline"><mml:mi>G</mml:mi></mml:math></inline-formula> must be of the same type (two random variables <inline-formula><mml:math display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula>
and <inline-formula><mml:math display="inline"><mml:mi>Y</mml:mi></mml:math></inline-formula> are of the same type if <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>a</mml:mi><mml:mi>X</mml:mi><mml:mo>+</mml:mo><mml:mi>b</mml:mi></mml:mrow></mml:math></inline-formula> has the same distribution as <inline-formula><mml:math display="inline"><mml:mi>Y</mml:mi></mml:math></inline-formula>) as
one of the three extreme value classes below:

              <disp-formula specific-use="align"><mml:math display="block"><mml:mtable displaystyle="true"><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mi mathvariant="normal">Gumbel</mml:mi><mml:mo>:</mml:mo><mml:mi>G</mml:mi><mml:mo>(</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mi mathvariant="normal">exp</mml:mi><mml:mo>(</mml:mo><mml:mo>-</mml:mo><mml:mi mathvariant="normal">exp</mml:mi><mml:mo>(</mml:mo><mml:mo>-</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo><mml:mo>)</mml:mo><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mo>-</mml:mo><mml:mi mathvariant="normal">∞</mml:mi><mml:mo>&lt;</mml:mo><mml:mi>y</mml:mi><mml:mo>&lt;</mml:mo><mml:mi mathvariant="normal">∞</mml:mi><mml:mo>;</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mi mathvariant="normal">Fr</mml:mi><mml:mtext>é</mml:mtext><mml:mi mathvariant="normal">chet</mml:mi><mml:mo>:</mml:mo><mml:mi>G</mml:mi><mml:mo>(</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mfenced close="" open="{"><mml:mtable class="array" columnalign="left"><mml:mtr><mml:mtd><mml:mrow><mml:mn mathvariant="normal">0</mml:mn><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi>y</mml:mi><mml:mo>≤</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:mi mathvariant="normal">exp</mml:mi><mml:mo>(</mml:mo><mml:mo>-</mml:mo><mml:msup><mml:mi>y</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mi mathvariant="italic">α</mml:mi></mml:mrow></mml:msup><mml:mo>)</mml:mo><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi>y</mml:mi><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mo>,</mml:mo><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi mathvariant="italic">α</mml:mi><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mo>;</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:mfenced></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mi mathvariant="normal">reversed</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi mathvariant="normal">Weibull</mml:mi><mml:mo>:</mml:mo><mml:mi>G</mml:mi><mml:mo>(</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mfenced close="" open="{"><mml:mtable class="array" columnalign="left"><mml:mtr><mml:mtd><mml:mrow><mml:mi mathvariant="normal">exp</mml:mi><mml:mo>(</mml:mo><mml:mo>-</mml:mo><mml:mo>(</mml:mo><mml:mo>-</mml:mo><mml:mi>y</mml:mi><mml:msup><mml:mo>)</mml:mo><mml:mi mathvariant="italic">α</mml:mi></mml:msup><mml:mo>)</mml:mo><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi>y</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mo>,</mml:mo><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi mathvariant="italic">α</mml:mi><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mspace linebreak="nobreak" width="0.33em"/><mml:mi>y</mml:mi><mml:mo>≥</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mo>;</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:mfenced></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula>

          where <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="italic">α</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mi mathvariant="italic">ξ</mml:mi></mml:mrow></mml:math></inline-formula> for Fréchet and <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="italic">α</mml:mi><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mi mathvariant="italic">ξ</mml:mi></mml:mrow></mml:math></inline-formula> for reversed
Weibull; see Eqs. (<xref ref-type="disp-formula" rid="Ch1.E1"/>) and (<xref ref-type="disp-formula" rid="Ch1.E2"/>). Conversely, any
distribution function of the same type as one of these extreme value classes
can appear as such a limit. The GEV distribution in Eq. (<xref ref-type="disp-formula" rid="Ch1.E1"/>) provides
a unifying representation of these three types of distributions.</p>
</app>

<app id="App1.Ch1.S3">
  <title>GEV diagnostics: Q–Q plots and effect of block size on estimated changes in return levels</title>
<sec id="App1.Ch1.S3.SS1">
  <title>Q–Q plots</title>
      <p>We assess the goodness of fit of GEV distributions used to model temperature
extremes with quantile–quantile plots. That is, we plot the quantiles of our
fitted GEV distributions against those of the empirical distribution of
annual maxima and minima. Figures show good agreement for both warm and cold
extremes (Figs. <xref ref-type="fig" rid="App1.Ch1.F2"/> and <xref ref-type="fig" rid="App1.Ch1.F3"/>).</p>
</sec>
<sec id="App1.Ch1.S3.SS2">
  <title>Effect of block size on estimated changes in return levels</title>

      <?xmltex \floatpos{p}?><fig id="App1.Ch1.F2" specific-use="star"><caption><p>The Q–Q plots for the fitted GEVs of warm extremes in the model run
simulating pre-industrial conditions. For clarity we display only every other
row and column of the grid cells shown in Fig. <xref ref-type="fig" rid="Ch1.F2"/>.</p></caption>
          <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://ascmo.copernicus.org/articles/2/79/2016/ascmo-2-79-2016-f14.pdf"/>

        </fig>

      <?xmltex \floatpos{p}?><fig id="App1.Ch1.F3" specific-use="star"><caption><p>As in Fig. <xref ref-type="fig" rid="App1.Ch1.F2"/> but for cold extremes.</p></caption>
          <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://ascmo.copernicus.org/articles/2/79/2016/ascmo-2-79-2016-f15.pdf"/>

        </fig>

      <p>In Sect. <xref ref-type="sec" rid="Ch1.S5"/>, we showed that, based on the max-stable property of GEV,
annual blocks may not be sufficiently long for GEV distribution to be valid
for the purpose of extrapolating more extreme events (i.e., return periods
are longer than the data length). Here we investigate whether annual blocks
are appropriate to study the <italic>changes</italic> in return levels by comparing
the results obtained from annual blocks vs. decadal blocks
(Figs. <xref ref-type="fig" rid="App1.Ch1.F4"/> and <xref ref-type="fig" rid="App1.Ch1.F5"/>). To infer return levels
for annual extremes from decadal extremes, we need to make the additional
assumption that annual extremes are independent across years.</p>

      <?xmltex \floatpos{p}?><fig id="App1.Ch1.F4" specific-use="star"><caption><p>As in Fig. <xref ref-type="fig" rid="Ch1.F7"/> (upper panel) but here comparing
the estimated changes obtained from using annual maxima (solid lines) vs.
decadal maxima (dashed lines). The results imply that annual blocks may be
long enough to study the changes in warm extremes, since changes in return
levels are fairly consistent with those using block sizes of
10 years.</p></caption>
          <?xmltex \igopts{width=412.564961pt}?><graphic xlink:href="https://ascmo.copernicus.org/articles/2/79/2016/ascmo-2-79-2016-f16.png"/>

        </fig>

      <?xmltex \floatpos{p}?><fig id="App1.Ch1.F5" specific-use="star"><caption><p>As in Fig. <xref ref-type="fig" rid="Ch1.F8"/> (upper panel) but here comparing
the estimated changes obtained from using annual minima (solid lines) vs.
decadal minima (dashed lines). The results imply that annual blocks may be
long enough to study the changes in cold extremes.</p></caption>
          <?xmltex \igopts{width=412.564961pt}?><graphic xlink:href="https://ascmo.copernicus.org/articles/2/79/2016/ascmo-2-79-2016-f17.pdf"/>

        </fig>

<?xmltex \hack{\clearpage}?>
</sec>
</app>

<app id="App1.Ch1.S4">
  <title>Model fitting procedures</title>
      <p>In this work we fit the parameters of the extreme value distributions for the
annual maxima/minima of each grid cell using maximum likelihood. For the
numerical optimization to find these estimates, we use the <monospace>gev.fit</monospace>
function in the <monospace>ismev</monospace> R package <xref ref-type="bibr" rid="bib1.bibx51" id="paren.52"/>. Return levels are
obtained by plugging the estimated GEV parameters into
Eq. (<xref ref-type="disp-formula" rid="Ch1.E3"/>). When fitting GEV
distributions from 20- and 50-year segments of model runs, we also compare
estimates obtained by maximum likelihood (ML) to those obtained with an
alternative fitting procedure, probability weighted moments (PWM). (See
<xref ref-type="bibr" rid="bib1.bibx27" id="text.53"/> for details on PWM.) The two fitting methods generally
produce very similar estimates on 20-year segments in three example
locations, but PWM does avoid occasional highly unreliable estimates seen in
one location (TX) for cold extremes (Fig. <xref ref-type="fig" rid="App1.Ch1.F6"/>).</p><?xmltex \hack{\vskip 7mm}?><?xmltex \floatpos{h!}?><fig id="App1.Ch1.F6"><caption><p>Boxplots of estimated changes in 20-, 50-, and 100-year return
levels obtained with two estimation procedures, PWM (blue) and ML (red), for
three example locations. Results are generally similar, but PWM does avoid
extreme outliers produced by ML for cold extremes in one location (TX).</p></caption>
        <?xmltex \hack{\hsize\textwidth}?>
        <?xmltex \igopts{width=412.564961pt}?><graphic xlink:href="https://ascmo.copernicus.org/articles/2/79/2016/ascmo-2-79-2016-f18.pdf"/>

      </fig>

      <p><?xmltex \hack{\newpage}?>We assess the uncertainties for GEV parameters and return levels by using
bootstrap resampling. Both simple nonparametric bootstrap <xref ref-type="bibr" rid="bib1.bibx16" id="paren.54"/>
and circular block bootstrap <xref ref-type="bibr" rid="bib1.bibx44" id="paren.55"/> were applied to annual
extremes. Specifically, let <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>m</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mo>,</mml:mo><mml:mi>j</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> be the annual extreme for year <inline-formula><mml:math display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula> and
site <inline-formula><mml:math display="inline"><mml:mi>j</mml:mi></mml:math></inline-formula> and  <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">m</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mo mathvariant="italic">{</mml:mo><mml:msub><mml:mi>m</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mo>,</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msub><mml:mo>,</mml:mo><mml:mi mathvariant="normal">⋯</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi>m</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mo>,</mml:mo><mml:mi>k</mml:mi></mml:mrow></mml:msub><mml:mo mathvariant="italic">}</mml:mo></mml:mrow></mml:math></inline-formula> where <inline-formula><mml:math display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula> is the total
number of sites. <inline-formula><mml:math display="inline"><mml:mrow><mml:mo mathvariant="italic">{</mml:mo><mml:msub><mml:mi mathvariant="bold-italic">m</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:msubsup><mml:mo mathvariant="italic">}</mml:mo><mml:mrow><mml:mi>i</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi>n</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> is split into <inline-formula><mml:math display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula>
(<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>n</mml:mi><mml:mo>=</mml:mo><mml:mn>1000</mml:mn></mml:mrow></mml:math></inline-formula> years in this study) overlapping temporal blocks of length <inline-formula><mml:math display="inline"><mml:mi>b</mml:mi></mml:math></inline-formula> (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>b</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>,</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mo>,</mml:mo><mml:mn mathvariant="normal">5</mml:mn><mml:mo>,</mml:mo><mml:mn>10</mml:mn></mml:mrow></mml:math></inline-formula> years): years <inline-formula><mml:math display="inline"><mml:mn mathvariant="normal">1</mml:mn></mml:math></inline-formula> to <inline-formula><mml:math display="inline"><mml:mi>b</mml:mi></mml:math></inline-formula> will be block <inline-formula><mml:math display="inline"><mml:mn mathvariant="normal">1</mml:mn></mml:math></inline-formula> (i.e.,
<inline-formula><mml:math display="inline"><mml:mrow><mml:mo mathvariant="italic">{</mml:mo><mml:msub><mml:mi mathvariant="bold-italic">m</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:msubsup><mml:mo mathvariant="italic">}</mml:mo><mml:mrow><mml:mi>i</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi>b</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula>), years <inline-formula><mml:math display="inline"><mml:mn mathvariant="normal">2</mml:mn></mml:math></inline-formula> to <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>b</mml:mi><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> will be block <inline-formula><mml:math display="inline"><mml:mn mathvariant="normal">2</mml:mn></mml:math></inline-formula> and
block <inline-formula><mml:math display="inline"><mml:mn>1000</mml:mn></mml:math></inline-formula> is years <inline-formula><mml:math display="inline"><mml:mrow><mml:mn>1000</mml:mn><mml:mo>,</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>,</mml:mo><mml:mi mathvariant="normal">⋯</mml:mi><mml:mo>,</mml:mo><mml:mi>b</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula>. From these <inline-formula><mml:math display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula> blocks, <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>n</mml:mi><mml:mo>/</mml:mo><mml:mi>b</mml:mi></mml:mrow></mml:math></inline-formula>
blocks are drawn at random with replacement. Then aligning these <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>n</mml:mi><mml:mo>/</mml:mo><mml:mi>b</mml:mi></mml:mrow></mml:math></inline-formula> blocks
will give the bootstrap observations. This approach allows us to provide
plausible uncertainties for our estimates without having to model spatial
dependencies or temporal dependencies for annual extremes within blocks.
Standard errors for different block sizes show little difference, suggesting
that extremes from one year to the next are nearly independent
(Fig. <xref ref-type="fig" rid="App1.Ch1.F7"/>).</p>

      <?xmltex \floatpos{p}?><fig id="App1.Ch1.F7" specific-use="star"><caption><p>Assessment of estimation uncertainty to return levels using
different block sizes for block bootstrap. The scatterplot shows block
bootstrapped standard errors by resampling years (<inline-formula><mml:math display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula> axis) and decades
(<inline-formula><mml:math display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> axis) of 2-year (left), 10-year, and 100-year (right) return levels.</p></caption>
        <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://ascmo.copernicus.org/articles/2/79/2016/ascmo-2-79-2016-f19.pdf"/>

      </fig>

<?xmltex \hack{\clearpage}?>
</app>

<app id="App1.Ch1.S5">
  <title>Relationships between changes in mean and changes in extremes</title>
      <p>Here we explore the relationship of changes in the location parameter of
extremes with changes in the corresponding seasonal means
(Figs. <xref ref-type="fig" rid="App1.Ch1.F8"/> and <xref ref-type="fig" rid="App1.Ch1.F9"/>). We find that
the changes in the location parameter of warm extremes generally follow the
mean changes during summer (see Fig. <xref ref-type="fig" rid="App1.Ch1.F8"/>). Changes in
the location parameter of cold extremes, however, are usually larger. For
most inland locations, changes in cold extremes are amplified by more than
50 % relative to changes in the average winter <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mtext>min</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>
(Fig. <xref ref-type="fig" rid="App1.Ch1.F9"/>). The greater shift in cold extremes is
largely explained by the decrease in wintertime variability
(Fig. <xref ref-type="fig" rid="Ch1.F5"/>).</p>

      <?xmltex \floatpos{h!}?><fig id="App1.Ch1.F8"><caption><p>An investigation of the relationship of changes in the location
parameter of warm extremes (i.e., <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi mathvariant="italic">μ</mml:mi></mml:mrow></mml:math></inline-formula>) with changes in summer means
(<inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>m</mml:mi></mml:mrow></mml:math></inline-formula>). Top: the ratio of changes in the location parameter of
extremes to changes in means for the climate state from pre-industrial to
700 ppm. Bottom: the ratio for climate states 700 and 1400 ppm. Red
(blue) grid cell location indicates that the shift of the GEV distribution is
larger (smaller) than the shift of the overall distribution. Numbers on the
top are the estimated ratios (i.e., <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mover accent="true"><mml:mi mathvariant="italic">μ</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>m</mml:mi></mml:mrow></mml:math></inline-formula>) and numbers
in parentheses are the bootstrapped standard errors for <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi mathvariant="italic">μ</mml:mi></mml:mrow></mml:math></inline-formula>. These
ratios are generally near 1 in the contiguous United
States.</p></caption>
        <?xmltex \hack{\hsize\textwidth}?>
        <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://ascmo.copernicus.org/articles/2/79/2016/ascmo-2-79-2016-f20.pdf"/>

      </fig>

      <?xmltex \floatpos{p}?><fig id="App1.Ch1.F9" specific-use="star"><caption><p>As in Fig. <xref ref-type="fig" rid="App1.Ch1.F8"/> but for changes in the location
parameter of cold extremes to changes in winter means. These ratios are
substantially greater than 1 nearly everywhere in the contiguous United
States.</p></caption>
        <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://ascmo.copernicus.org/articles/2/79/2016/ascmo-2-79-2016-f21.pdf"/>

      </fig>

<?xmltex \hack{\clearpage}?>
</app>

<app id="App1.Ch1.S6">
  <?xmltex \opttitle{Changes in the shape parameter from pre-industrial to 1400\,ppm}?><title>Changes in the shape parameter from pre-industrial to 1400 ppm</title>
      <p>Here we present changes in the estimated shape parameter of extremes in the
transition from pre-industrial to 1400 ppm climate states.</p>

      <?xmltex \floatpos{h!}?><fig id="App1.Ch1.F10"><caption><p>Changes in the estimated CCSM3 GEV shape parameter in the transition
from pre-industrial to 1400 ppm climate states. Top: warm extremes.
Bottom: cold extremes. Changes in the shape parameter are in general
significant for inland cold extremes.</p></caption>
        <?xmltex \hack{\hsize\textwidth}?>
        <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://ascmo.copernicus.org/articles/2/79/2016/ascmo-2-79-2016-f22.pdf"/>

      </fig>

<?xmltex \hack{\clearpage}?>
</app>
  </app-group><ack><title>Acknowledgements</title><p>This work was conducted as part of the
<uri>https://www.statmos.washington.edu</uri> Research Network for Statistical
Methods for Atmospheric and Oceanic Sciences (STATMOS), supported by NSF
award nos. 1106862, 1106974, and 1107046, and the
<uri>http://www.rdcep.org/</uri>Center for Robust Decision Making on Climate and
Energy Policy (RDCEP), supported by the NSF Decision Making Under
Uncertainty program award no. 0951576.<?xmltex \hack{\newline}?><?xmltex \hack{\newline}?> Edited
by: R. Donner<?xmltex \hack{\newline}?> Reviewed by: two anonymous referees</p></ack><ref-list>
    <title>References</title>

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<abstract-html><p class="p">Changes in extreme weather may produce some of the largest societal impacts
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