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  <front>
    <journal-meta>
<journal-id journal-id-type="publisher">NPG</journal-id>
<journal-title-group>
<journal-title>Nonlinear Processes  in Geophysics</journal-title>
<abbrev-journal-title abbrev-type="publisher">NPG</abbrev-journal-title>
<abbrev-journal-title abbrev-type="nlm-ta">Nonlin. Processes Geophys.</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub">1607-7946</issn>
<publisher><publisher-name>Copernicus GmbH</publisher-name>
<publisher-loc>Göttingen, Germany</publisher-loc>
</publisher>
</journal-meta>

    <article-meta>
      <article-id pub-id-type="doi">10.5194/npg-22-513-2015</article-id><title-group><article-title>Systematic attribution of observed Southern Hemisphere circulation
trends to external forcing and internal variability</article-title>
      </title-group><?xmltex \runningtitle{Southern Hemisphere circulation trends}?><?xmltex \runningauthor{C.~L.~E.~Franzke et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Franzke</surname><given-names>C. L. E.</given-names></name>
          <email>christian.franzke@uni-hamburg.de</email>
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>O'Kane</surname><given-names>T. J.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Monselesan</surname><given-names>D. P.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Risbey</surname><given-names>J. S.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Horenko</surname><given-names>I. </given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>Meteorological Institute and Center for Earth System Research and Sustainability, University of Hamburg, Hamburg, Germany</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>CSIRO Oceans and Atmosphere, Hobart, Australia</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Università della Svizzera  Italiana, Lugano, Switzerland</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">C. L. E. Franzke (christian.franzke@uni-hamburg.de)</corresp></author-notes><pub-date><day>8</day><month>September</month><year>2015</year></pub-date>
      
      <volume>22</volume>
      <issue>5</issue>
      <fpage>513</fpage><lpage>525</lpage>
      <history>
        <date date-type="received"><day>19</day><month>March</month><year>2015</year></date>
           <date date-type="rev-request"><day>30</day><month>April</month><year>2015</year></date>
           <date date-type="rev-recd"><day>16</day><month>August</month><year>2015</year></date>
           <date date-type="accepted"><day>27</day><month>August</month><year>2015</year></date>
      </history>
      <permissions>
<license license-type="open-access">
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<self-uri xlink:href="https://npg.copernicus.org/articles/22/513/2015/npg-22-513-2015.pdf">The full text article is available as a PDF file from https://npg.copernicus.org/articles/22/513/2015/npg-22-513-2015.pdf</self-uri>


      <abstract>
    <p>A critical question in the global warming debate concerns the causes of the
observed trends of the Southern Hemisphere (SH) atmospheric circulation over
recent decades. Secular trends have been identified in the frequency of
occurrence of circulation regimes, namely the positive phase of the Southern
Annular Mode (SAM) and the hemispheric wave-3 pattern which is associated
with blocking. Previous studies into the causes of these secular trends have
either been purely model based, have not included observational forcing data
or have mixed external forcing with indices of internal climate variability
impeding a systematic and unbiased attribution of the causes of the secular
trends. Most model studies also focused mainly on the austral summer season.
However, the changes to the storm tracks have occurred in all seasons and
particularly in the austral winter and early spring when midlatitude
blocking is most active and stratospheric ozone should not play a role. Here
we systematically attribute the secular trends over the recent decades using
a non-stationary clustering method applied to both reanalysis and
observational forcing data from all seasons. While most previous studies
emphasized the importance of stratospheric ozone depletion in causing austral
summer SH circulation trends, we show observational evidence that
anthropogenic greenhouse gas concentrations have been the major driver of
these secular trends in the SAM and blocking when all seasons are considered.
Our results suggest that the recovery of the ozone hole might delay the
signal of global warming less strongly than previously thought and that
effects from all seasons are likely crucial in understanding the causes of
the secular trends.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

      <?xmltex \hack{\newpage}?>
<sec id="Ch1.S1" sec-type="intro">
  <title>Introduction</title>
      <p>The SH climate and atmospheric circulation has undergone significant changes
over the last few decades. It is important to understand its causes and
anthropogenic contributions because this will not only help to constrain
future climate projections but is also essential to evaluate the ability of
the current generation of climate models to accurately simulate these
changes. Previous attempts at understanding the causes of SH climate change
focused on changes in the mean climate and its variance
<xref ref-type="bibr" rid="bib1.bibx2 bib1.bibx63 bib1.bibx60" id="paren.1"/> during austral summer. Here we
instead focus on changes in the frequency of occurrence of circulation
regimes <xref ref-type="bibr" rid="bib1.bibx44 bib1.bibx37" id="paren.2"/> in all seasons. Such circulation regimes
have a significant impact on surface weather and climate. For instance, the
frequency of occurrence of blocking strongly affects temperature and
precipitation <xref ref-type="bibr" rid="bib1.bibx51 bib1.bibx48" id="paren.3"/>. Furthermore, the secular trend
towards the increased occurrence of the positive SAM phase, linked in the
austral summer to stratospheric ozone
<xref ref-type="bibr" rid="bib1.bibx56 bib1.bibx47 bib1.bibx60 bib1.bibx49 bib1.bibx3" id="paren.4"/>, affects
Antarctic temperatures and sea ice extent <xref ref-type="bibr" rid="bib1.bibx64" id="paren.5"/>. It also has to
be noted that the way SAM is defined can impact on the outcomes of any study
using a SAM index <xref ref-type="bibr" rid="bib1.bibx27" id="paren.6"/>. Hence, we use here a method which does not
presuppose any particular spatial structure on the resultant regimes and the
particular form of the SAM we find is determined from the data.</p>
      <p>Over the recent decades (1980–present) large changes in the SH storm track
modes have occurred in all seasons including the austral winter, when
blocking is at its most active <xref ref-type="bibr" rid="bib1.bibx38" id="paren.7"/>. The austral winter storm
track changes manifest as reduced baroclinicity and a decrease in the July
zonal winds of about <inline-formula><mml:math display="inline"><mml:mo>≈</mml:mo></mml:math></inline-formula> 10 m s<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> in the subtropical jet
relative to the earlier period 1950–1980 <xref ref-type="bibr" rid="bib1.bibx20" id="paren.8"/>. The
changes in the storm track modes provide a dynamical mechanism for the
observed systematic linear downward trends in the annual number of SH
blocking events <xref ref-type="bibr" rid="bib1.bibx68 bib1.bibx44" id="paren.9"/>. Such events predominantly
occur in preferred locations about the Australian (110–210<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E),
eastern Pacific (260–315<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E) and Indian   (20–80<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E)
ocean sectors. These regions are associated with the ridges of the hemispheric
wave-3 pattern <xref ref-type="bibr" rid="bib1.bibx65 bib1.bibx62" id="paren.10"/>.</p>
      <p>A recent study <xref ref-type="bibr" rid="bib1.bibx44" id="paren.11"/> using non-stationary clustering has shown
that, consistent with reduced blocking activity post the late 1970s, the
wave-3 pattern has weakened while the corresponding zonal state (SAM) has
strengthened and moved poleward (positive phase). While an early study
hypothesized that global warming is likely to change the frequency of
occurrence of these circulation regimes but not their spatial patterns
<xref ref-type="bibr" rid="bib1.bibx12 bib1.bibx44" id="paren.12"/>. Furthermore, <xref ref-type="bibr" rid="bib1.bibx44" id="text.13"/> has shown that
the spatial character of the SH persistent climate regimes has changed
significantly over the reanalysis period 1948–2009. Here we extend our
earlier study of SH circulation regimes to show observational evidence that
when all seasons are considered these changes are mainly in response to
radiative forcing trends of anthropogenic CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> emissions and to a much
lesser degree to stratospheric ozone depletion. This is likely due to the
fact that ozone depletion plays a minor role outside of the austral summer
season.</p>
      <p>The main method of investigating the role of different forcings of the SH
secular trends has been through coupled climate models <xref ref-type="bibr" rid="bib1.bibx58" id="paren.14"/>. Modeling
studies <xref ref-type="bibr" rid="bib1.bibx2 bib1.bibx63 bib1.bibx56 bib1.bibx49 bib1.bibx3" id="paren.15"/> have
identified stratospheric ozone depletion as an important driver of the
observed austral summertime intensification of the SAM over the recent
decades. However, stratospheric ozone depletion is a highly seasonal effect
and can play no role in the austral winter–spring atmospheric circulation
dynamics. The SH storm tracks are equally active all year around
<xref ref-type="bibr" rid="bib1.bibx61" id="paren.16"/>. However, the austral wintertime is the season when the
observed changes to the storm track activity, namely reduced blocking and
baroclinicity of the subtropical jet <xref ref-type="bibr" rid="bib1.bibx20" id="paren.17"/>, have been
particularly evident and cannot be solely attributed to the ozone mass
deficit (OMD).</p>
      <p>Modeling studies of the effect of various individual and combined radiative
forcings on the SH circulation have largely compared trends in mean zonal
indices, mainly the SAM index, without consideration of related systematic
changes in the spatially coherent zonally asymmetric features of the
circulation <xref ref-type="bibr" rid="bib1.bibx44" id="paren.18"/>. Such studies often rely on ensemble averaging
of repeated forcing experiments to enhance the forcing signal while
simultaneously reducing intrinsic interannual- to decadal-scale variability.
The problem with this approach is the prohibitive computational cost of
coupled models, allowing only for relatively small ensemble sizes whose
models often have rather coarse resolutions and contain many biases.</p>
      <p>CMIP5 (Coupled Model Intercomparison Project Phase 5) models are known to poorly represent midlatitude blocking and to be
limited in their ability to capture important SH circulation responses such
as the response of the SAM to large volcanic eruptions
<xref ref-type="bibr" rid="bib1.bibx33 bib1.bibx25 bib1.bibx9" id="paren.19"/>. Furthermore, recent studies
showed that very high horizontal resolutions (grid spacing of about 16 km)
are necessary for climate models to accurately simulate the geographical
structure and probability distribution of blocking and regional weather
regimes <xref ref-type="bibr" rid="bib1.bibx14 bib1.bibx15" id="paren.20"/>.</p>
      <p>Given that the circulation changes are a key signature of the forcing for
attribution, the main aim of this paper is to complement model-based results
with observationally based studies and to try to separate natural variability
from the forced response. For example, the late 1970s climate shift occurred
coincident with the shift in phase of the Interdecadal Pacific Oscillation
(IPO), so separating the low frequency intrinsic ENSO (El Niño–Southern Oscillation) behavior from a
response to the constituent components of the radiative forcing is an
important problem.</p>
      <p>Here we argue that most studies (see <xref ref-type="bibr" rid="bib1.bibx60" id="text.21"/> for a review)
attributing secular trends in the SH circulation have exclusively focused on
changes in the mean zonal circulation and the trend toward positive SAM in
the summer months. This has been largely attributed to ozone because model
simulations with (without) ozone can (cannot) reproduce the magnitude of the
trend and because there is only a small trend towards the positive SAM in the
winter; thus, the conclusion is that ozone is the major driver of the secular
SAM trend. The mechanism proposed <xref ref-type="bibr" rid="bib1.bibx56" id="paren.22"/> is that stratospheric
cooling/heating allows the high latitude tropopause to rise in the summer
enabling a poleward movement of the westerlies and consequently the Hadley
cell. <xref ref-type="bibr" rid="bib1.bibx47" id="text.23"/> found that the only statistically significant
relationship between the position of the Hadley cell and the midlatitude jet
exists in the summer; however, in the winter no such relationship exists even
though the wintertime is when one expects such a relationship to be most
robust. Here we show results of a statistical analysis using zonally
asymmetric fields which not only represent the SAM pattern but also zonal
asymmetries, i.e., blocking, which has also undergone secular changes over the
last few decades.</p>
      <p>In Sect. 2 we present the data used in this study and in Sect. 3 we describe
the statistical method used for the non-stationary clustering. In Sect. 4 we
present the attribution results and also describe in detail our sensitivity
tests regarding the number of parameters to be estimated and demonstrate the
robustness of our results. We provide our conclusions in Sect. 5.</p>
</sec>
<sec id="Ch1.S2">
  <title>Data</title>
      <p>We use daily NCEP/NCAR (National Centers for
Environmental Prediction/National Center for Atmospheric Research) reanalysis data <xref ref-type="bibr" rid="bib1.bibx34" id="paren.24"/> covering the
period 1980–2007 for 500 hPa geopotential height and surface air
temperature. We consider only anomalies with respect to the climatological
mean where the mean seasonal cycle has been removed but not detrended. Note
that there is still an annual cycle in higher moments and in the frequency of
occurrence present in the time series. While there are still large biases in
the Antarctic region in the various reanalysis products
<xref ref-type="bibr" rid="bib1.bibx5 bib1.bibx6" id="paren.25"/>, we have shown in a similar study
<xref ref-type="bibr" rid="bib1.bibx45" id="paren.26"/> that by using the Japanese 55-year  Reanalysis (JRA-55)
conducted by the Japan Meteorological Agency (JMA) we found very similar
results. Hence, our results do not depend strongly on the used reanalysis
data set.</p>
      <p>As forcing data we use the Cape Grim CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> measurements <xref ref-type="bibr" rid="bib1.bibx57" id="paren.27"/>,
sulfate aerosols <xref ref-type="bibr" rid="bib1.bibx55" id="paren.28"/>, stratospheric aerosol optical thickness
<xref ref-type="bibr" rid="bib1.bibx4" id="paren.29"/> (available at
<uri>http://data.giss.nasa.gov/modelforce/strataer/</uri>), stratospheric ozone
mass deficit <xref ref-type="bibr" rid="bib1.bibx53" id="paren.30"/>, and the solar constant <xref ref-type="bibr" rid="bib1.bibx23" id="paren.31"/>.
Most of the forcing data is in monthly mean resolution. Since we are using
daily reanalysis data for the clustering, we expand the monthly forcing data
to daily resolution by using the monthly mean values for each day of the
respective month. Because stratospheric ozone depletion has a strong annual
cycle we carried out sensitivity analysis by lagging the ozone mass deficit
values by 1, 2 or 3 months and we also used a 365-day backward running mean.
The forcing time series are displayed in Fig. <xref ref-type="fig" rid="Ch1.F1"/>.</p>
      <p>As internal modes of climate variability, we use an ENSO 3.4 index, the
Madden–Julian Oscillation (MJO) index, the Indian Ocean Dipole (IOD) and the
eastern Indian Ocean Dipole mode indices and the annual cycle here defined as
sin(2 <inline-formula><mml:math display="inline"><mml:mo>⋅</mml:mo></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">π</mml:mi></mml:math></inline-formula>/365 <inline-formula><mml:math display="inline"><mml:mo>⋅</mml:mo></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula>). These indices describe tropical
sea surface temperature (SST) variability (ENSO, IOD) or an intrinsic mode of
tropical variability (MJO). We consider these to be intrinsic drivers of
midlatitude variability but recognize that they likely also respond to
changes in external radiative forcing such that a clear separation between
cause and effect is difficult. However, it is still important to elucidate
which role they play in the frequency changes of the regime patterns. We do
not consider Antarctic sea ice extent because of its marginal expansion and
because this slight expansion in extent is largely wind-driven
<xref ref-type="bibr" rid="bib1.bibx28" id="paren.32"/> and likely a response to the changes in the large-scale
circulation. Furthermore, the changes in sea ice extent and area have been
spatially heterogeneous, with increases in some areas like in the Ross Sea
and decreases in other areas like in the Bellingshausen/Amundsen seas
<xref ref-type="bibr" rid="bib1.bibx46" id="paren.33"/>. This is despite the trend towards the positive SAM;
thus, it is unlikely that sea ice extent would have a significant impact on
the secular circulation trends.</p>
</sec>
<sec id="Ch1.S3">
  <title>Non-stationary clustering</title>
      <p>We first give an intuitive description of the  clustering method used before
we explain it in much more detail in Sect. 3.1. That section can be skipped
by readers who are more interested in the clustering results.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1"><caption><p>Forcing time series: Cape Grim CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (dark blue),
sulfate aerosols (green), stratospheric aerosol optical thickness (red),
lagged OMD (blue), OMD (magenta) and solar constant (khaki). Time series are
normalized by subtracting the respective mean and dividing by the respective
standard deviation.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://npg.copernicus.org/articles/22/513/2015/npg-22-513-2015-f01.pdf"/>

      </fig>

      <p>Many studies have provided evidence that the atmospheric circulation can be
efficiently described by a few persistent cluster states
<xref ref-type="bibr" rid="bib1.bibx10 bib1.bibx35 bib1.bibx12 bib1.bibx29 bib1.bibx39 bib1.bibx17 bib1.bibx18 bib1.bibx19 bib1.bibx44 bib1.bibx52" id="paren.34"/>.
Conventional clustering methods such as <italic>k</italic>-means partition phase space using
heuristic algorithms, for example using empirical orthogonal functions
(EOFs), into an a priori arbitrarily determined <italic>k</italic> set  of cluster
centroids whose points within each cluster are close but where each centroid
is in some sense far apart from each other <xref ref-type="bibr" rid="bib1.bibx15" id="paren.35"/>. Similarly,
self organizing maps <xref ref-type="bibr" rid="bib1.bibx32" id="paren.36"><named-content content-type="pre">SOMs;</named-content></xref> are typically based on
minimizing the geometric (Euclidean) distance between the observational data
and some specified set of recurrent patterns but without consideration of the
persistency of those states and mostly without considering the dynamics and
differences in dynamics within these states <xref ref-type="bibr" rid="bib1.bibx41" id="paren.37"/>.
Furthermore, classical clustering methods do not consider differences in the
dynamics of the cluster states <xref ref-type="bibr" rid="bib1.bibx11" id="paren.38"/>. Recently,
<xref ref-type="bibr" rid="bib1.bibx37" id="text.39"/> applied SOMs to reanalyzed daily zonal-mean zonal wind data
for the austral summer period employing four SOM patterns with the DJF (December–January–February) global
mean temperature taken as an indicator of the response to GHG (greenhouse gas) forcing. They
attribute the main response to ozone by correlating the third SOM DJF
zonal-mean zonal wind pattern with the November Antarctic ozone index. One of
the central problems in applying these methods to historical geophysical data
is related to the robustness, meaning that increasing the <inline-formula><mml:math display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula> away from
<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>k</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> increases the total number of parameters – thereby increasing the risk
of overfitting. Concepts from information theory like the  Akaike information
criterion (AIC) <xref ref-type="bibr" rid="bib1.bibx8" id="paren.40"/> are usually deployed to find the optimal
number of clusters <inline-formula><mml:math display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula> that allows avoiding overfitting.</p>
      <p>Our approach considers the
hemispheric response of not only the zonal annular mode but also systematic
changes in wave 3 and blocking. We also use reanalyzed data but consider all
possible combinations of the observed radiative forcings and relevant indices
of internal variability. Moreover, we make no a priori assumptions on
the number of states and employ an approach that considers persistency,
changes in the dynamics and that is able to ascertain causation between the
time series and the external forcings.</p>
      <p>Specifically, we use the non-stationary clustering method FEM-BV-VARX (finite
element method of time series analysis with bounded variation and vector autoregressive factor
of model
parameters; <xref ref-type="bibr" rid="bib1.bibx30 bib1.bibx44 bib1.bibx52 bib1.bibx24" id="altparen.41"/>) to
systematically attribute circulation trends to observed external forcings. In
this study we assume that the large-scale circulation can be effectively
decomposed into a small set of distinct patterns or regime states. On each
day the atmosphere is only in one of these patterns, where it might stay for
some time before it switches to one of the other regime states. If we order
the regime states from 1 to <inline-formula><mml:math display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula>, we get a  daily index denoting in which state the atmosphere is in on that particular day;
this index is referred to in the literature as the Viterbi path
<xref ref-type="bibr" rid="bib1.bibx66 bib1.bibx17" id="paren.42"/>. We then construct a statistical model which
simultaneously estimates the geographical structure of these patterns and the
evolution of the switching between the patterns. We do this by minimizing the
distance between the observed atmospheric circulation and the regime states
(see next subsection for a more detailed description of this procedure).
Furthermore, we also allow external factors, like CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, ozone, or ENSO, to
influence the evolution of the regime states. This is again done by
minimizing the distance. This also enables us to evaluate different forcing
combinations. By using different forcing combinations and looking for the
statistical model with the minimum distance, we can systematically find the
forcings which are most likely responsible for the observed evolution of the
regime states.</p>
<sec id="Ch1.S3.SS1">
  <title>Overview of the FEM-BV methodology </title>
      <p>The FEM-BV-VARX approach is a general variational framework that is reduced to
the well-known methods of linear regression, autoregressive models, <inline-formula><mml:math display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula> means
and hidden Markov approaches when more restrictive assumptions are made on
the nature of the underlying data-generating process
<xref ref-type="bibr" rid="bib1.bibx36 bib1.bibx7 bib1.bibx53 bib1.bibx40" id="paren.43"/>. Furthermore, as VARX is
a tool for inferring the Granger causality <xref ref-type="bibr" rid="bib1.bibx26" id="paren.44"/> (causation
between time series variables in terms of predictability and not
correlation), FEM-BV-VARX is a more general approach which allows  going
beyond the standard stationarity assumption of the usual methods currently
used for inferring cause–response relationships, e.g., in ecology
<xref ref-type="bibr" rid="bib1.bibx59" id="paren.45"/>, economics <xref ref-type="bibr" rid="bib1.bibx26" id="paren.46"/> and climate science
<xref ref-type="bibr" rid="bib1.bibx43 bib1.bibx67" id="paren.47"/>. The non-stationary FEM-BV-VARX framework
contains the standard stationary VARX and the concept of standard
Granger causality as a particular special case and allows for a systematic
comparison of causality relations inferred with and without the stationarity
assumption for a given set of observational data. See <xref ref-type="bibr" rid="bib1.bibx24" id="text.48"/> for
more details explaining the relation of the FEM-BV framework to standard
stationary approaches of data-driven causality inference.</p>
      <p>The approach we are following here is that we perform FEM-BV-VARX fits to all
possible combinations of the external forcings. Then we apply a standard
information theoretic criterion: the  AIC
<xref ref-type="bibr" rid="bib1.bibx1 bib1.bibx30 bib1.bibx44 bib1.bibx52" id="paren.49"/>, which is a measure of
the relative goodness of fit of a model to data. That means  that AIC can be
used to assess the goodness of fit relative to the number of fitted
parameters or external factors used, allowing us to find the model that is least
overfitting and best fitting the analyzed data <xref ref-type="bibr" rid="bib1.bibx8" id="paren.50"/>. This
standard procedure can tell us which forcing combination is best able to
explain the secular circulation trends given by the FEM-BV-VARX model.</p>
      <p>The presence of unresolved external covariates (which are not
statistically independent or identically distributed) may result in the
non-stationarity and non-homogeneity of the resulting data-driven statistical
models and may be manifested in the presence of secular trends and/or in
regime-transition behavior. By covariate we not only mean external forcings
but also unresolved physical processes and scales (e.g., due to EOF
truncation). This may then introduce problems when applying the standard
stationary approaches common to machine learning and statistics
<xref ref-type="bibr" rid="bib1.bibx31" id="paren.51"/>. In the context of this paper, this issue plays a very
important role when analyzing atmospheric data since many of the
potentially relevant covariates might not be available explicitly in the set
of covariates that we have chosen for testing. Therefore, when deploying
statistical time series analysis methods, they should be capable of dealing
with non-stationarity and non-homogeneity issues that emerge in the models as
a result of these systematically missing (and potentially important) external
influences.</p>
      <p>Combining the concepts and ideas from pure and applied mathematics (such as
the FEM  from numeric  of partial differential equations,
regularization in infinitely dimensional spaces from the theory of ill-posed
problems, stochastic calculus and theory of stochastic processes, information
criteria from information theory, and embedding theorems from the theory of
dynamical systems), Horenko and colleagues developed a family of
non-stationary, non-homogeneous and non-parametric time series analysis
methods. This family of time series analysis techniques, which is reviewed
concisely by <xref ref-type="bibr" rid="bib1.bibx40" id="text.52"/>, allows for systematic time-dependent model
identification when assumptions of temporal stationarity or spatial
homogeneity of some underlying statistics are not justifiable. The main idea
is based on regularized variational minimization of a scalar-valued
functional describing the error
<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>g</mml:mi><mml:mfenced close=")" open="("><mml:mi>x</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>,</mml:mo><mml:mi>u</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>,</mml:mo><mml:mi mathvariant="italic">θ</mml:mi><mml:mfenced close=")" open="("><mml:mi>t</mml:mi></mml:mfenced></mml:mfenced></mml:mrow></mml:math></inline-formula> of some model for a given
observation <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>x</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> subject to available external impacts/covariates <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>u</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>
and characterized by the time-dependent set of model parameters <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="italic">θ</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>

                <disp-formula id="Ch1.E1" content-type="numbered"><mml:math display="block"><mml:mrow><mml:mi mathvariant="bold">L</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="normal">Θ</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">Γ</mml:mi><mml:mo>)</mml:mo></mml:mrow><mml:mo>=</mml:mo><mml:mrow><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mrow><mml:mi>k</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi>K</mml:mi></mml:munderover><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mrow><mml:mi>t</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi>T</mml:mi></mml:msub></mml:mrow></mml:munderover><mml:msub><mml:mi mathvariant="italic">γ</mml:mi><mml:mi>k</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mi>g</mml:mi><mml:mfenced open="(" close=")"><mml:mi>x</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>,</mml:mo><mml:mi>u</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="normal">Θ</mml:mi><mml:mi>k</mml:mi></mml:msub></mml:mfenced><mml:mo>→</mml:mo><mml:msub><mml:mo>min⁡</mml:mo><mml:mrow><mml:mi mathvariant="normal">Γ</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">Θ</mml:mi></mml:mrow></mml:msub><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

          subject to the constraints on <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">Γ</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mfenced close=")" open="("><mml:msub><mml:mi mathvariant="italic">γ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>,</mml:mo><mml:mi mathvariant="normal">…</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="italic">γ</mml:mi><mml:mi>K</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mfenced></mml:mrow></mml:math></inline-formula>:

                <disp-formula specific-use="align" content-type="numbered"><mml:math display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E2"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mrow><mml:mi>k</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi>K</mml:mi></mml:munderover><mml:msub><mml:mi mathvariant="italic">γ</mml:mi><mml:mi>k</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mn mathvariant="normal">1</mml:mn><mml:mspace width="1em" linebreak="nobreak"/><mml:mo>∀</mml:mo><mml:mi>t</mml:mi><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:msub><mml:mi>N</mml:mi><mml:mi>T</mml:mi></mml:msub><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:msub><mml:mi mathvariant="italic">γ</mml:mi><mml:mi>k</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>≥</mml:mo><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mn mathvariant="normal">0</mml:mn><mml:mspace width="1em" linebreak="nobreak"/><mml:mo>∀</mml:mo><mml:mi>t</mml:mi><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:msub><mml:mi>N</mml:mi><mml:mi>T</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:mo>∀</mml:mo><mml:mi>k</mml:mi><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>K</mml:mi><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>|</mml:mo><mml:msub><mml:mi mathvariant="italic">γ</mml:mi><mml:mi>k</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mo>⋅</mml:mo><mml:mo>)</mml:mo><mml:msub><mml:mo>|</mml:mo><mml:mrow><mml:mi>B</mml:mi><mml:mi>V</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mrow><mml:mi>t</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi>T</mml:mi></mml:msub></mml:mrow></mml:munderover><mml:mo>|</mml:mo><mml:msub><mml:mi mathvariant="italic">γ</mml:mi><mml:mi>k</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>+</mml:mo><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>)</mml:mo><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="italic">γ</mml:mi><mml:mi>k</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>|</mml:mo><mml:mo>≤</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">C</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:mspace width="1em" linebreak="nobreak"/><mml:mo>∀</mml:mo><mml:mi>k</mml:mi><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>K</mml:mi><mml:mo>,</mml:mo></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">θ</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:msubsup><mml:mo>∑</mml:mo><mml:mrow><mml:mi>k</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi>K</mml:mi></mml:msubsup><mml:msub><mml:mi mathvariant="italic">γ</mml:mi><mml:mi>k</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:msub><mml:mi mathvariant="normal">Θ</mml:mi><mml:mi>k</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, thereby allowing  the
problem of statistical data analysis beyond the usual stationarity assumption
to be reformulated and algorithmically solved as a clustering problem with
<inline-formula><mml:math display="inline"><mml:mi>K</mml:mi></mml:math></inline-formula> clusters, distance kernel <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>g</mml:mi><mml:mfenced open="(" close=")"><mml:mi>x</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>,</mml:mo><mml:mi>u</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>,</mml:mo><mml:mi mathvariant="italic">θ</mml:mi><mml:mfenced open="(" close=")"><mml:mi>t</mml:mi></mml:mfenced></mml:mfenced></mml:mrow></mml:math></inline-formula>
and a regularization parameter <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">C</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, controlling the number of transition
between different clusters in time (special case <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">C</mml:mi></mml:msub><mml:mo>≡</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:mi>K</mml:mi><mml:mo>≡</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> corresponds to the homogeneous and stationary statistical problem).
Imposed regularization confines the bounded variation (BV) of the
regime-switching process <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">γ</mml:mi><mml:mi>k</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> in time, thereby making the temporal
change of inferred model parameters <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="italic">θ</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> more or less persistent.
Changing the constraining variable <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">C</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, one can test the whole range of
possible statistical models, going from <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">C</mml:mi></mml:msub><mml:mo>≡</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula> (stationary/well-posed)
to <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">C</mml:mi></mml:msub><mml:mo>≡</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mi>T</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (completely non-stationary/very ill-posed problems). The
above variational problem is non-convex since the parameters <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Θ</mml:mi><mml:mi>k</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> are
not known a priori and have to be inferred simultaneously with the
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">γ</mml:mi><mml:mi>k</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>.</p>
      <p>Many classical methods of data analysis and machine learning (e.g.,
multilinear statistical regression, <inline-formula><mml:math display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula>-means
clustering, Gaussian mixture
models (GMMs) and hidden Markov models (HMMs) <xref ref-type="bibr" rid="bib1.bibx39 bib1.bibx17" id="altparen.53"/>)
can be derived as special cases of this FEM-BV methodology. For example, HMMs are
obtained additionally assuming that <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Γ</mml:mi></mml:math></inline-formula> is an output of a homogeneous
Markov chain and setting <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">C</mml:mi></mml:msub><mml:mo>≡</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mi>T</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. For more detailed information
please see Sect. 2h “Relation to classical methods of unsupervised
learning” in <xref ref-type="bibr" rid="bib1.bibx40" id="text.54"/>. It is an important feature of the deployed
methodology, since it allows us to test different standards or more advanced
methods in the context of the same theoretical and algorithmic
FEM-BV framework.</p>
      <p>In the FEM-BV methodology, finite element methods are employed in the
numerical representation of indicator functions <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">γ</mml:mi><mml:mi>k</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> for the time
domain of applicability of different models from a common model class. Model
class is defined by the choice of the particular analytical form of the error
function <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>g</mml:mi><mml:mfenced close=")" open="("><mml:mi>x</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>,</mml:mo><mml:mi>u</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>,</mml:mo><mml:mi mathvariant="italic">θ</mml:mi><mml:mfenced open="(" close=")"><mml:mi>t</mml:mi><mml:mo>,</mml:mo><mml:mi>j</mml:mi></mml:mfenced></mml:mfenced></mml:mrow></mml:math></inline-formula>; the explicit
VARX-form deployed in this paper is given below. As shown above, these
indicators are regularized using a bounded variation criterion, hence  the
acronym FEM-BV. The choice of the model class depends on the type of data
and a specific form of error function <inline-formula><mml:math display="inline"><mml:mi>g</mml:mi></mml:math></inline-formula> considered. Here we have
implemented vector autoregressive models with external influences (VARX),
which are defined as <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>x</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mi mathvariant="italic">μ</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>+</mml:mo><mml:msubsup><mml:mo>∑</mml:mo><mml:mrow><mml:mi>i</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi mathvariant="normal">MEM</mml:mi></mml:msubsup><mml:msub><mml:mi>A</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:msub><mml:mi>x</mml:mi><mml:mrow><mml:mi>t</mml:mi><mml:mo>-</mml:mo><mml:mi>i</mml:mi><mml:mi mathvariant="italic">τ</mml:mi></mml:mrow></mml:msub><mml:mo>+</mml:mo><mml:mi>B</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mfenced open="(" close=")"><mml:mi>u</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mfenced><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="italic">ϵ</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, parameters being
<inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="italic">θ</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mfenced open="(" close=")"><mml:mi mathvariant="italic">μ</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>,</mml:mo><mml:msub><mml:mi>A</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>,</mml:mo><mml:mi mathvariant="normal">…</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi>A</mml:mi><mml:mi mathvariant="normal">MEM</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>,</mml:mo><mml:mi>B</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mfenced></mml:mrow></mml:math></inline-formula>,  and
the model error functional defined as <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>g</mml:mi><mml:mfenced open="(" close=")"><mml:mi>x</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>,</mml:mo><mml:mi>u</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="normal">Θ</mml:mi><mml:mi>k</mml:mi></mml:msub></mml:mfenced><mml:mo>=</mml:mo><mml:mo>‖</mml:mo><mml:mo>|</mml:mo><mml:msub><mml:mi>x</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msup><mml:mi mathvariant="italic">μ</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>k</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:msup><mml:mo>+</mml:mo><mml:msubsup><mml:mo>∑</mml:mo><mml:mrow><mml:mi>i</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi mathvariant="normal">MEM</mml:mi></mml:msubsup><mml:msubsup><mml:mi>A</mml:mi><mml:mi>i</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>k</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:msubsup><mml:msub><mml:mi>x</mml:mi><mml:mrow><mml:mi>t</mml:mi><mml:mo>-</mml:mo><mml:mi>i</mml:mi><mml:mi mathvariant="italic">τ</mml:mi></mml:mrow></mml:msub><mml:mo>+</mml:mo><mml:msup><mml:mi>B</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>k</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:msup><mml:mi mathvariant="italic">ϕ</mml:mi><mml:mfenced open="(" close=")"><mml:mi>u</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mfenced><mml:mo>‖</mml:mo><mml:msubsup><mml:mo>|</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup></mml:mrow></mml:math></inline-formula>  <xref ref-type="bibr" rid="bib1.bibx40 bib1.bibx30" id="paren.55"><named-content content-type="pre">for more details please see</named-content></xref>.</p>
      <p>The algebraic structure of the above problem allows us to deploy efficient
numerical algorithms  based on the iterative application of linear and/or
quadratic programming problems (optimizing for fixed <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Θ</mml:mi></mml:math></inline-formula>) followed by
stationary/convex inference of <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Θ</mml:mi></mml:math></inline-formula> for a fixed <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Γ</mml:mi></mml:math></inline-formula>. This procedure
is repeated iteratively, until the change in <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="bold">L</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="normal">Θ</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">Γ</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is
less than some small a priori-determined threshold, resulting in monotonic
minimization of <inline-formula><mml:math display="inline"><mml:mi mathvariant="bold">L</mml:mi></mml:math></inline-formula>. Here we have used the adaptive finite element method
from the numerics of partial differential equations (PDEs)
<xref ref-type="bibr" rid="bib1.bibx30 bib1.bibx31" id="paren.56"/> for numerical minimization of the
FEM-BV problems (Eqs. <xref ref-type="disp-formula" rid="Ch1.E1"/>, <xref ref-type="disp-formula" rid="Ch1.E2"/>).</p>
      <p>The number of different spatiotemporal <inline-formula><mml:math display="inline"><mml:mi>K</mml:mi></mml:math></inline-formula> regimes/clusters – the model
parameters to be chosen within these regimes, such as memory depth and number
of EOFs, and the indicator functions <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">γ</mml:mi><mml:mi>k</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mo>⋅</mml:mo><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> signaling activation
of the respective models – are all determined simultaneously in a global
optimization procedure. This yields a judicious compromise between low
residuals, reproducing the data of a training set on the one hand, and the
demand for the smallest-possible overall number of free parameters of the
complete model on the other. The optimization is based on a new
non-parametric modified AIC and may thus be
interpreted as a constructive implementation of “Occam's razor” for data
analysis problems. Thereby, the resulting FEM-BV-framework is essentially
free of parameters that should be defined and tuned by the user. The only
parameter that  needs to be set externally is the overall number of
optimization repetitions with different randomly chosen initial values of
<inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Γ</mml:mi></mml:math></inline-formula> or <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Θ</mml:mi></mml:math></inline-formula> for parameter optimization (in the following referred to
as the <italic>number of annealing steps</italic>). Increasing this number reduces
the probability of getting trapped in one of the local minima of <inline-formula><mml:math display="inline"><mml:mi mathvariant="bold">L</mml:mi></mml:math></inline-formula>
(for <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">C</mml:mi></mml:msub><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>), simultaneously linearly increasing the amount of computations.
Therefore, the <italic>number of annealing steps</italic> should be chosen carefully,
depending on the available computational resources and the size of the data
to be analyzed.</p>
</sec>
<sec id="Ch1.S3.SS2">
  <title>Application of FEM-BV-VARX to atmospheric reanalysis and observed
forcing data</title>
      <p>We have chosen to examine a time series of 500 hPa geopotential height
anomalies (seasonal cycle subtracted) projected on the 20 leading  EOFs  and with <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>u</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>   taken as
32 combinations of forcings (to be described in more detail below). Deploying
the FEM-BV-VARX method, comprehensive sensitivity tests were carried out for
the cluster parameters involving memory depth MEM and the number of
annealing steps. Although the resulting optimal choice of forcing
combinations has converged after 16 annealing steps, the model affiliation
sequence already remained unchanged after 4 annealing steps. The results
presented in the manuscript are for 64 annealing steps. The optimal memory
depth <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">τ</mml:mi></mml:math></inline-formula> was 2 days; however, the degree of memory tested ranged from 0 to
5 days. Daily forcing agents was spline interpolated with no lag apart from
OMD. Every possible combination of forcing agents was considered including
the observed OMD lagged by 0, 30, 60 and 90 days as well as a variant with a lag average of 365 days span (here we artificially introduce persistency into
the OMD time series). The optimal external radiative forcing agent was found
ultimately to correspond to the Cape Grim CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> time series.</p>
      <p>In order to choose the optimal model <inline-formula><mml:math display="inline"><mml:mi>M</mml:mi></mml:math></inline-formula> we first used the AIC:

                <disp-formula id="Ch1.E3" content-type="numbered"><mml:math display="block"><mml:mrow><mml:mi mathvariant="normal">AIC</mml:mi><mml:mo>(</mml:mo><mml:mi>M</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mi>log⁡</mml:mi><mml:mo>(</mml:mo><mml:mi>L</mml:mi><mml:mo>(</mml:mo><mml:mi>M</mml:mi><mml:mo>)</mml:mo><mml:mo>)</mml:mo><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mi>M</mml:mi><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>

          Application of the AIC is equivalent to assuming that the scalar-valued
squared model errors are <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">χ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>-distributed and that the vector-valued
FEM-BV-VARX model errors are Gaussian, i.e., dependent on the residuals having
a log-normal distribution. We tested this assumption  using a non-parametric
information-theoretic algorithm from <xref ref-type="bibr" rid="bib1.bibx40" id="text.57"/> and found that for
all of the model errors <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ϵ</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> the most optimal parametric family was
indeed the log-normal distribution.</p>
      <p>Additionally, the log-normal distribution was fitted to the model errors, the
respective log-likelihoods computed and used to calculate the AIC for the
non-stationary models. The most informative non-stationary model that emerged
using the AIC criteria (with posterior probability almost equal to one in
each case) was the model with Cape Grim CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and memory of 3 days.
Comparable results were found using Akaike information criteria corrected
(AICc) and the Bayesian information criteria (BIC). The two latter criteria
also take the size of the statistics into account and are derived under very
different mathematical assumptions than the AIC. This further confirmed our
results, demonstrating that they are not induced by the implicit assumptions
necessary for the information criteria applicability.</p>
      <p>In our study we have included only a selected number of several external
forcings. One might argue now that we have neglected some additional forcing
(e.g., sea ice extent or the strength of the Antarctic Circumpolar Current)
which might be responsible for the observed secular trend. However, if we
include something like sea ice extent into the set of forcings and
get a result showing that sea ice extent is more statistically
significant, then this would not contradict this study simply because the
variable <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">γ</mml:mi></mml:math></inline-formula> (describing the switching process and describing the bias
coming from all the unresolved covariates in our study) would be different
from the one that we obtained in this study. From our study we can guarantee
that in a given set of explicit covariates we found the one covariate that is
most important (in the Granger-causality sense)   and – taking into account
the presence of the unresolved covariates – this covariate is CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
<xref ref-type="bibr" rid="bib1.bibx40 bib1.bibx16" id="paren.58"/>. All of the other eventually important
covariates are in the regime-switching process that we have also
identified but were not explicitly represented in our results.</p>
</sec>
</sec>
<sec id="Ch1.S4">
  <title>Attribution results</title>
      <p>A previous study with the FEM-BV-VARX method <xref ref-type="bibr" rid="bib1.bibx44" id="paren.59"/> revealed the
existence of statistically significant persistent circulation regimes
corresponding to the positive phase of the SAM and a hemispheric wave-3
blocking pattern (Fig. <xref ref-type="fig" rid="Ch1.F2"/>). That study also found evidence for
significant secular trends in all seasons and, when the full reanalysis
period 1948–2010 was considered, that a distinct regime transition occurred
around 1980 towards a preference for the positive SAM phase; here shown in
Fig. <xref ref-type="fig" rid="Ch1.F3"/> in terms of time of residence in either a wave-3 blocked or
zonal (positive SAM) state. The increasingly frequent and persistent positive
SAM pattern is accompanied by a corresponding decrease in the frequency and
persistence of the wave-3 hemispheric pattern, which features blocking in the
Australian sector in particular. The increasing frequency of occurrence of
the zonal state and the corresponding decreasing frequency of occurrence of
the wave-3 blocking state are consistent with the study of <xref ref-type="bibr" rid="bib1.bibx44" id="text.60"/>
and are, thus, statistically significant. Furthermore, this behavior occurs
throughout all four seasons and, thus, is very robust. However, the changes
occur  slower in the summer season. While in all other seasons the wave-3
blocking state   occurred   more often than the zonal state up to about
1980; this transition has been much slower in the summer season and starting
in 2000 both states occur about equally frequent in the summer season. There
has been a much more distinct regime transition during the other three seasons
(Fig. <xref ref-type="fig" rid="Ch1.F3"/>).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2"><caption><p>Composites of 500 hPa geopotential height anomalies
(in m) over 1979–2010: <bold>(a)</bold> state 1 (blocking) and
<bold>(b)</bold> state 2 (positive SAM); and composites of surface air
temperature (in <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C) <bold>(c)</bold> state 1 (blocking),
<bold>(d)</bold> state 2 (positive SAM). Only persistent states
which last at least 5 days have been used.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://npg.copernicus.org/articles/22/513/2015/npg-22-513-2015-f02.png"/>

      </fig>

      <p>Our FEM-BV-VARX analysis finds strong evidence that anthropogenic greenhouse
gas concentrations have caused the secular trends in the SAM and hemispheric
wave-3 pattern. The clustering analysis with CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> forcing has the smallest
AIC value, AIC<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">min</mml:mi></mml:msub></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>63 053 (which corresponds to a Akaike
weight of about 1). This denotes the most parsimonious explanation of the
observational data among all of the other fitted explanatory statistical
models with all possible combinations of considered forcings. Hence,
providing the best compromise between the quality of fit to the data and a
low number of parameters. The absolute value of the AIC is less meaningful,
only its relative size compared with the other tested models is useful. The
next best forcing combinations relative to the optimal choice are the solar
constant (Akaike weight of 2.3550 <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:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) and stratospheric
aerosol (Akaike weight of 1.8217 <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:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>).</p>
      <p>The Akaike weight value <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>w</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mi>exp⁡</mml:mi><mml:mo>(</mml:mo><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">AIC</mml:mi><mml:mo>min⁡</mml:mo></mml:msub><mml:mo>-</mml:mo><mml:mi mathvariant="normal">AIC</mml:mi><mml:mo>(</mml:mo><mml:mi>i</mml:mi><mml:mo>)</mml:mo><mml:mo>)</mml:mo><mml:mo>/</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>
provides a measure for how much better the best FEM-BV-VARX fit explains the
data relative to the other FEM-BV-VARX models; this quantity can also be
interpreted as the posterior model probability <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>w</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and, thus, as how less likely
the FEM-BV-VARX model <inline-formula><mml:math display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula> is to explain  the data relative to the best-fit
model. The Akaike weight value (or posterior model probability)
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>w</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mi>exp⁡</mml:mi><mml:mo>(</mml:mo><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">AIC</mml:mi><mml:mo>min⁡</mml:mo></mml:msub><mml:mo>-</mml:mo><mml:mi mathvariant="normal">AIC</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="normal">OMD</mml:mi><mml:mo>)</mml:mo><mml:mo>)</mml:mo><mml:mo>/</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 3.1083 <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:mrow><mml:mo>-</mml:mo><mml:mn>18</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>
reveals statistically overwhelming support of CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> compared to
stratospheric OMD in explaining the secular trend in the cluster frequency of
occurrence. The corresponding Akaike weights reveal that the CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> forcing
is significantly better than all other possible used combinations in
explaining the observed trends.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3"><caption><p>Percentage of time in either the hemispheric
wave-3 state (black dashed) or the zonal state (blue dashed) for the NCEP
reanalysis 500 hPa geopotential height field for all seasons and annually. The
dashed lines are a LOESS fit to the time-averaged data where the solid lines
indicate the values and averaging periods of the data.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://npg.copernicus.org/articles/22/513/2015/npg-22-513-2015-f03.pdf"/>

      </fig>

      <p>We tested the sensitivity of our results using different information criteria
like the  BIC  <xref ref-type="bibr" rid="bib1.bibx8" id="paren.61"/> and the AIC
corrected for finite sample size (AICc) <xref ref-type="bibr" rid="bib1.bibx8" id="paren.62"/> and obtained very
similar results in that CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> was always the forcing which best explained
the secular trends. The next best fit varies according to the FEM-BV-VARX
setup but it typically includes stratospheric ozone depletion and
stratospheric sulfate aerosols. While our results are unclear as to the
relative importance of stratospheric ozone depletion over the other leading
forcings, we find strong evidence for the role of CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> in contributing to
the secular trends.</p>
      <p>Figure <xref ref-type="fig" rid="Ch1.F2"/> also shows the geographical structure of the two cluster
states in terms of 500 hPa geopotential height and surface air temperature
(SAT) (note that the upper atmospheric regime states are very similar to the
ones in <xref ref-type="bibr" rid="bib1.bibx44" id="text.63"/> which did not include external forcings in their
analysis.). The wave-3 blocked state (state 1) is associated at the surface
with a cold anomaly over the Antarctic Peninsula and a warm anomaly over the
Ross Ice Shelf and the coast of Antarctica's Victoria land as well as with SAT
over South America in SAT. The zonal positive SAM state (state 2) is associated at
the surface with a warm anomaly over East Antarctica and Australia and a cold
anomaly along the coast of Antarctica's Wilkes Land. The cluster states have
very different surface temperature signatures. With the strong trend towards
the SAM state in recent decades, it is interesting to ask whether the pattern
of surface temperature trends over the Antarctic region reflect the SAM state
surface signature. Figure <xref ref-type="fig" rid="Ch1.F4"/> shows the trend in surface air
temperature over the same period (1979–2010) calculated from yearly averaged
Had4Krig version 2.0.0 <xref ref-type="bibr" rid="bib1.bibx13" id="paren.64"/> data. Because large trends are
evident in both blocking (wave 3) and SAM in all seasons (Fig. <xref ref-type="fig" rid="Ch1.F3"/>), we
have used annual mean data to calculate the SAT trends. The remarkable
agreement between the SAM state surface temperature anomaly pattern
(Fig. <xref ref-type="fig" rid="Ch1.F2"/>d) and the Had4Krig SAT trend pattern over Antarctica is
further evidence of the weakening of the wave-3 state and the shift towards
the positive SAM state.</p>
      <p>Our results are in contrast to earlier studies which found that ozone
depletion is up to 9 times more important than anthropogenic CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
concentrations <xref ref-type="bibr" rid="bib1.bibx53 bib1.bibx56 bib1.bibx37" id="paren.65"/>. One possible explanation
for this difference is that the earlier studies mainly examined the austral
summer season focusing on the response of the linear trend in the zonal mean
circulation towards the positive SAM phase and the poleward shift of the
Hadley cell <xref ref-type="bibr" rid="bib1.bibx56 bib1.bibx47 bib1.bibx49" id="paren.66"/>. Our study focuses on
attributing systematic changes in the circulation over the latter half of the
NCEP reanalysis period employing a data-driven methodology that can infer
causation (as explained above, FEM-BV-VARX is a non-stationary extension of
the Granger causality inference and can describe the standard Granger
causality as a particular stationary case). Moreover, we are not simply
considering changes to the zonal SAM index in the austral summer in isolation
but are explicitly attributing changes to the entire SH circulation including
coherent features to all possible combinations of the relevant radiative
forcings. Previous studies mainly analyzed changes in the mean state and not
in the frequency of occurrence or changes in structure. This might also
partly explain why our findings differ from previous studies.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4"><caption><p>Surface air temperature trend (K decade<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) over
the period 1979–2010 calculated from the yearly averaged Had4Krig version
2.0.0 data set.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://npg.copernicus.org/articles/22/513/2015/npg-22-513-2015-f04.pdf"/>

      </fig>

      <p>To increase the confidence in our results, we systematically examined the
sensitivity of our results to the treatment of the ozone data. Considering
a 365-day-averaged and  time-lagged seasonally varying OMD leads to more
robust results because we account for the strong annual cycle of
stratospheric ozone and its delayed impact on the tropospheric circulation.
Ozone has a strong seasonal component with OMD known to impact the
tropospheric circulation (from the observational record) in December–January.
Thus, we repeated our analysis using lagged (by 0, 1, 2 and 3 months), seasonally
varying and 365-running-mean OMD data. While we did find some sensitivity to
lag interval, our results were qualitatively unchanged.</p>
<sec id="Ch1.S4.SS1">
  <title>Sensitivity to the number of model parameters</title>
      <p><xref ref-type="bibr" rid="bib1.bibx44" id="text.67"/> showed that, in order to accurately capture the dynamics
and amplitude of Southern Hemisphere midlatitude atmospheric blocking regime
transitions, any dimension reduction of the 500 hPa atmospheric reanalysis
data required including a minimum of 9 but more generally the leading
20 PCs (principle components).
Retaining these dominant modes makes the VARX model 20-dimensional with the
resulting FEM-BV-VARX, where each dimension communicates with every other
dimension, leading to quadratic growth in the number of VARX parameters in
the matrix <bold>A</bold>
and of dimension <inline-formula><mml:math display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula>. This also applies to the stationary VARX
model of the form

                <disp-formula id="Ch1.E4" content-type="numbered"><mml:math display="block"><mml:mrow><mml:msub><mml:mi>x</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mi mathvariant="italic">μ</mml:mi><mml:mo>+</mml:mo><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mrow><mml:mi>i</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi mathvariant="normal">MEM</mml:mi></mml:munderover><mml:msub><mml:mi>A</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:msub><mml:mi>x</mml:mi><mml:mrow><mml:mi>t</mml:mi><mml:mo>-</mml:mo><mml:mi>i</mml:mi><mml:mi mathvariant="italic">τ</mml:mi></mml:mrow></mml:msub><mml:mo>+</mml:mo><mml:mi>B</mml:mi><mml:msub><mml:mi>u</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="italic">ϵ</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow></mml:math></disp-formula>

          where <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>x</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> has the dimension <inline-formula><mml:math display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>u</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> has the dimension <inline-formula><mml:math display="inline"><mml:mi>m</mml:mi></mml:math></inline-formula> and
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ϵ</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is independent and identically distributed. Here the total number of model parameters will be
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">param</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mi>n</mml:mi><mml:mo>+</mml:mo><mml:mi mathvariant="normal">MEM</mml:mi><mml:mo>⋅</mml:mo><mml:msup><mml:mi>n</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>+</mml:mo><mml:mi>n</mml:mi><mml:mo>⋅</mml:mo><mml:mi>m</mml:mi></mml:mrow></mml:math></inline-formula>. With <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>n</mml:mi><mml:mo>=</mml:mo><mml:mn>20</mml:mn></mml:mrow></mml:math></inline-formula> and MEM <inline-formula><mml:math display="inline"><mml:mo>≥</mml:mo></mml:math></inline-formula> 2 resulting in
many thousands of free model parameters. Since the length of the
available observational data is limited, a classical ill-posed problem
is manifested in the overfitting of the data. This is the case even for the
standard stationary data sets. BIC and AIC implicitly see this problem,
attributing these models to much higher values of the information criteria
than they would for more informative and well-posed models. A more complete
discussion can be found in <xref ref-type="bibr" rid="bib1.bibx40" id="text.68"/>.</p>
      <p>In order to try and address this problem, and given that we have ascertained
that a minimum of 20 PCs should be retained, we have considered additional
sensitivity experiments in which we diagonalize the matrix <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold">A</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. Since the
only coupling between the different dimensions of <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>x</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is induced by the
off-diagonal elements of <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold">A</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, diagonalizing is equivalent to a separate
identification of the <inline-formula><mml:math display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula> following problems with respect to
<inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="italic">μ</mml:mi><mml:mo>(</mml:mo><mml:mi>j</mml:mi><mml:mo>)</mml:mo><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="bold">A</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>j</mml:mi><mml:mo>,</mml:mo><mml:mi>j</mml:mi><mml:mo>)</mml:mo><mml:mo>,</mml:mo><mml:mi>B</mml:mi><mml:mo>(</mml:mo><mml:mi>j</mml:mi><mml:mo>,</mml:mo><mml:mo>:</mml:mo><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>; i.e.,

                <disp-formula specific-use="align" content-type="numbered"><mml:math display="block"><mml:mtable displaystyle="true"><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>∀</mml:mo><mml:mi>j</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>,</mml:mo><mml:mi>n</mml:mi><mml:mo>:</mml:mo><mml:msub><mml:mi>x</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>j</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mi mathvariant="italic">μ</mml:mi><mml:mo>(</mml:mo><mml:mi>j</mml:mi><mml:mo>)</mml:mo><mml:mo>+</mml:mo><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mrow><mml:mi>i</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi mathvariant="normal">MEM</mml:mi></mml:munderover><mml:msub><mml:mi mathvariant="bold">A</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>j</mml:mi><mml:mo>,</mml:mo><mml:mi>j</mml:mi><mml:mo>)</mml:mo><mml:msub><mml:mi>x</mml:mi><mml:mrow><mml:mi>t</mml:mi><mml:mo>-</mml:mo><mml:mi>i</mml:mi><mml:mi mathvariant="italic">τ</mml:mi></mml:mrow></mml:msub><mml:mo>(</mml:mo><mml:mi>j</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mlabeledtr id="Ch1.E5"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><mml:mo>+</mml:mo><mml:mi>B</mml:mi><mml:mo>(</mml:mo><mml:mi>j</mml:mi><mml:mo>,</mml:mo><mml:mo>:</mml:mo><mml:mo>)</mml:mo><mml:mo>⋅</mml:mo><mml:msub><mml:mi>u</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="italic">ϵ</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

            It is straightforward to see that the total number of parameters in such a
case will be growing linearly with <inline-formula><mml:math display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula> as <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">param</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mi>n</mml:mi><mml:mo>⋅</mml:mo><mml:mo>(</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>+</mml:mo><mml:mi mathvariant="normal">MEM</mml:mi><mml:mo>+</mml:mo><mml:mi>m</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> (multiplied by <inline-formula><mml:math display="inline"><mml:mi>K</mml:mi></mml:math></inline-formula> if considering non-stationary models
where <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>K</mml:mi><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula>). In sensitivity experiments with <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold">A</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>j</mml:mi><mml:mo>,</mml:mo><mml:mi>j</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> and for memory
depths <inline-formula><mml:math display="inline"><mml:mo>≥</mml:mo></mml:math></inline-formula> 2, Cape Grim CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> was again found to be optimal and the results
were insensitive to annealing steps <inline-formula><mml:math display="inline"><mml:mo>≥</mml:mo></mml:math></inline-formula> 4. In descending order, and for the
diagonalized experiments, the leading five combinations were found to be (1) Cape
Grim CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, (2) Cape Grim CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and ozone, (3) optical thickness, (4)
sulfate aerosols,  (5) stratospheric ozone, and where a memory depth of 2
days was found to be optimal.</p>
      <p>We further note that even such a diagonally restricted VARX model is
much more general than when applying multilinear regression:

                <disp-formula id="Ch1.E6" content-type="numbered"><mml:math display="block"><mml:mrow><mml:msub><mml:mi>x</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mi mathvariant="italic">μ</mml:mi><mml:mo>+</mml:mo><mml:mi>B</mml:mi><mml:msub><mml:mi>u</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="italic">ϵ</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

          which is a special case of VARX for <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>K</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold">A</mml:mi><mml:mi>j</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mo>∀</mml:mo><mml:mi>j</mml:mi></mml:mrow></mml:math></inline-formula>. Thus, even
with the diagonality restriction, this analysis is more general than the
stationary multilinear regression approaches, e.g., employed by
<xref ref-type="bibr" rid="bib1.bibx53" id="text.69"/>.</p>
      <p>One might further seek to reduce the number of parameters such that the
problem is not ill posed. While reducing the number of EOFs is a possible
approach even a reduction from 20 to 9 EOFs (the absolute minimum number of
modes required to capture the Southern Hemisphere  wave-3 blocking state) will
not sufficiently reduce the number of parameters such that the FEM-BV-VARX
with full <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>A</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> matrix is well posed. Also in the Southern Hemisphere
blocking is quite transient and, as shown in Fig. 11 of
<xref ref-type="bibr" rid="bib1.bibx70" id="text.70"/>, the difference between equilibrium zonal and blocked
states in terms of hemispheric zonal wind speeds averaged over a midlatitude
zonal band is only 3 ms<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> at 500 mb as compared to the Northern
Hemisphere which is 30 ms<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> an order of magnitude larger.</p>
      <p>One strategy that was comprehensively tested was  the sensitivity to
persistency over a large range of values as <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">C</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> from Eqs. (1) and (2) is changed
from <inline-formula><mml:math display="inline"><mml:mn mathvariant="normal">0</mml:mn></mml:math></inline-formula> to <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi>T</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. However, due to the transient nature of the Southern
Hemisphere atmospheric circulation, the residuals (model errors) for the
multiple-state model are not significantly smaller than for the one-state
model. By including the number of transitions in the definition of
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">param</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> it is immediately obvious that the one-state model is
always preferred in such cases and taking <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">C</mml:mi></mml:msub><mml:mo>→</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mi>T</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> we simply
converge on the one-state solution.</p>
      <p>Clearly time-series analysis where persistency of the respective metastable
states is weak represents a serious challenge. One approach we explored
assumes that – for fixed time-series <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>x</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, number of metastable states <inline-formula><mml:math display="inline"><mml:mi>K</mml:mi></mml:math></inline-formula>,
and persistency <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">C</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, as well as for fixed local VARX parameters
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">θ</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mo>(</mml:mo><mml:msup><mml:mi mathvariant="italic">μ</mml:mi><mml:mi>i</mml:mi></mml:msup><mml:mo>,</mml:mo><mml:msubsup><mml:mi mathvariant="bold">A</mml:mi><mml:mn mathvariant="normal">1</mml:mn><mml:mi>i</mml:mi></mml:msubsup><mml:mo>,</mml:mo><mml:mi mathvariant="normal">…</mml:mi><mml:mo>,</mml:mo><mml:msubsup><mml:mi mathvariant="bold">A</mml:mi><mml:mi mathvariant="normal">MEM</mml:mi><mml:mi>i</mml:mi></mml:msubsup><mml:mo>,</mml:mo><mml:msup><mml:mi>B</mml:mi><mml:mi>i</mml:mi></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> – we can
straightforwardly compute the respective Viterbi path solving the linear
programming step of the FEM-BV procedure (see Step 2 of the FEM-BV algorithm
description on p. 23 of <xref ref-type="bibr" rid="bib1.bibx30" id="altparen.71"/>). Since it is a linear
minimization problem with convex constraints, it has a unique solution. That
is, one can uniquely recover the distinct Viterbi path,
<inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">Γ</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mfenced close=")" open="("><mml:msub><mml:mi mathvariant="italic">γ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>,</mml:mo><mml:mi mathvariant="normal">…</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="italic">γ</mml:mi><mml:mi>k</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mfenced></mml:mrow></mml:math></inline-formula>, knowing only the full
data series <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>x</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and preserving only <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi mathvariant="normal">param</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mo>(</mml:mo><mml:mi>K</mml:mi><mml:mo>⋅</mml:mo><mml:mo>(</mml:mo><mml:mi>n</mml:mi><mml:mo>+</mml:mo><mml:mi mathvariant="normal">MEM</mml:mi><mml:mo>⋅</mml:mo><mml:msup><mml:mi>n</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>+</mml:mo><mml:mi>n</mml:mi><mml:mo>⋅</mml:mo><mml:mi>m</mml:mi><mml:mo>)</mml:mo><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> parameters while preserving the
value of persistency <inline-formula><mml:math display="inline"><mml:mi>C</mml:mi></mml:math></inline-formula>. Having computed the Viterbi path, one can also
compute the distinct values of the model errors <inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mover accent="true"><mml:mi mathvariant="italic">ϵ</mml:mi><mml:mo mathvariant="normal">̃</mml:mo></mml:mover><mml:mi>t</mml:mi><mml:mi>i</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> as
<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mover accent="true"><mml:mi mathvariant="italic">ϵ</mml:mi><mml:mo mathvariant="normal">̃</mml:mo></mml:mover><mml:mi>t</mml:mi><mml:mi>i</mml:mi></mml:msubsup><mml:mo>=</mml:mo><mml:mi mathvariant="italic">γ</mml:mi><mml:mo>(</mml:mo><mml:mi>i</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>⋅</mml:mo><mml:mo>(</mml:mo><mml:msub><mml:mi>x</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msup><mml:mi mathvariant="italic">μ</mml:mi><mml:mi>i</mml:mi></mml:msup><mml:mo>-</mml:mo><mml:msubsup><mml:mo>∑</mml:mo><mml:mrow><mml:mi>j</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi mathvariant="normal">MEM</mml:mi></mml:msubsup><mml:msubsup><mml:mi mathvariant="bold">A</mml:mi><mml:mi>j</mml:mi><mml:mi>i</mml:mi></mml:msubsup><mml:msub><mml:mi>x</mml:mi><mml:mrow><mml:mi>t</mml:mi><mml:mo>-</mml:mo><mml:mi>j</mml:mi><mml:mi mathvariant="italic">τ</mml:mi></mml:mrow></mml:msub><mml:mo>-</mml:mo><mml:msup><mml:mi>B</mml:mi><mml:mi>i</mml:mi></mml:msup><mml:msub><mml:mi>u</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>.</p>
      <p>The sensitivity experiments we describe effectively bound the problem of
overfitting inherent in analyzing atmospheric observational data.
Importantly, we achieve the same results for diagonalization (well-posed,
with no cross terms) and for the full FEM-BV-VARX (ill conditioned, with all
cross terms).</p>
</sec>
<sec id="Ch1.S4.SS2">
  <title>Internal climate variability</title>
      <p>Next we examined whether intrinsic climate variability statistically
significantly affected the regime behavior. We find that the combination of
ENSO and the first component of the multivariate MJO index (MJO1) provide the
major intrinsic driver of the observed atmospheric regime behavior. The next
best combinations are MJO1, MJO1 together with the eastern Indian Ocean Dipole
index and the annual cycle together with MJO1.</p>
      <p>The low frequency variability of ENSO is highly correlated to the IPO and, as
pointed out earlier, the IPO shifted phase in the late 1970s coinciding with
the transition to reduced blocking. Thus, it is natural to expect ENSO to be a
major component of internal variability driving changes in the wave 3. The
first component of the MJO index corresponds to enhanced convection over the
maritime continent (Indonesia, Philippines and Papua New Guinea) close to the
tropical warm pool <xref ref-type="bibr" rid="bib1.bibx69" id="paren.72"/>. This provides evidence for a tropical
origin of SH mid- and high-latitude climate variability on interannual to
decadal timescales. Since SST changes occur on longer timescales, this
might open the opportunity for making skillful long-range predictions on
seasonal to decadal timescales. However, the external CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> forcing still
explains the observed secular trends best; thus, the intrinsic climate
indices taken alone are not able to statistically explain the secular trends.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5"><caption><p>Smoothed (365-day backward running mean) Viterbi path of
blocking (black line), SAM (red line) state, and stratospheric aerosol
optical thickness (blue line).</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://npg.copernicus.org/articles/22/513/2015/npg-22-513-2015-f05.png"/>

        </fig>

      <p>We also find evidence that the Mt. Pinatubo volcanic eruption in 1991, as
measured by stratospheric aerosol optical thickness, could have triggered a
dramatic sudden increase in the regime frequency of occurrence in its
immediate aftermath. Figure <xref ref-type="fig" rid="Ch1.F5"/> shows that the eruption of Mt.
Pinatubo is followed by a sudden drop in the frequency of occurrence (1-year
running mean) of the positive phase of the SAM and a corresponding increase
in blocking. In the long term this only delayed the secular increase in the
SAM. From Fig. <xref ref-type="fig" rid="Ch1.F5"/> we infer also that the response timescale to the
eruption is about 3–4 years. In contrast, the 1982 eruption of El Chichón
did not cause a drop of the frequency of occurrence of the positive SAM
phase. This result is consistent with the EOF analysis of ERA-40 reanalysis data
where a significant shift to negative stratospheric and surface SAM was
observed only after the Fuego and Mt. Pinatubo eruptions
<xref ref-type="bibr" rid="bib1.bibx33 bib1.bibx25" id="paren.73"/>. Importantly, CMIP5 models have been shown
to be unable to reproduce a realistic dynamical response by the annular mode
to even large intermittent volcanic signals like Mt. Pinatubo, suggesting
that the extratropical circulations of current CMIP5 models are not able to
simulate the response to short-lived abrupt perturbations in stratospheric
forcing <xref ref-type="bibr" rid="bib1.bibx33 bib1.bibx25 bib1.bibx9" id="paren.74"/>.</p>
</sec>
</sec>
<sec id="Ch1.S5" sec-type="conclusions">
  <title>Conclusions</title>
      <p>Our examination of reanalysis data together with observed forcing data
reveals that greenhouse gas emissions are an important driver of SH
circulation changes over the last few decades. Recent studies have suggested
that stratospheric ozone depletion is many times more dominant than CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> in
driving systematic changes in the SH midlatitude circulation. However, our
results highlight that for understanding the anthropogenic impact on SH
circulation changes the delayed influence of stratospheric ozone depletion is
relevant  but not the dominant mechanism. Previous studies mainly focused on
the austral summer and the zonal response (SAM). Our results from analyzing data
from the whole year suggest that other seasons and the changes in coherent
features (wave-3 blocking), including implications for anomalous surface
warming of the high latitudes, need to be incorporated in order to more
completely understand and attribute SH circulation changes. Such studies are
particularly needed for evaluating and improving climate models. Temperature
trends in the Antarctic region are spatially heterogeneous. The pattern of
these trends reflects the surface signature of the shift toward a more zonal
SAM circulation regime at the expense of the blocking regime.</p>
      <p>Our observationally based results are also confirmed by numerical modeling
studies <xref ref-type="bibr" rid="bib1.bibx42 bib1.bibx21 bib1.bibx22" id="paren.75"/>. Atmospheric general
circulation model simulations forced by observed SST fields
<xref ref-type="bibr" rid="bib1.bibx50" id="paren.76"/> and CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations but with climatological O<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>
have been able to reproduce the observed SH circulation changes although the
magnitude is underestimated by about 40–50 %
<xref ref-type="bibr" rid="bib1.bibx21 bib1.bibx22" id="paren.77"/>. This provides support from a numerical
climate model for the observational data analysis presented in this
manuscript.</p>
      <p>Our finding that anthropogenic CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> is the dominant driver whereas
stratospheric ozone depletion makes a somewhat lesser contribution to the SH
circulation changes over recent decades has important implications for future
SH climate change. In particular, it may be that the recovery of ozone has
less relevance to changes in Southern Hemisphere extratropical circulation
than projected in many modeling studies <xref ref-type="bibr" rid="bib1.bibx3 bib1.bibx54" id="paren.78"/>. Our
findings regarding the sudden but short-lived increase in blocking and
negative SAM after the Mt. Pinatubo eruption highlights the potential of
the climate system to abruptly change in response to large transient
perturbations in stratospheric forcing while emphasizing the dominant role of
systematic changes in anthropogenic CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> on the climate.</p>
</sec>

      
      </body>
    <back><ack><title>Acknowledgements</title><p>We thank one anonymous reviewer and S. Vannitsem for constructive reviews.
C. L. E. Franzke is supported by the German Research Foundation (DFG) through
the cluster of excellence CliSAP (EXC177). T. J. O'Kane is supported by the
Australian Research Council Future Fellow program. T. J. O'Kane, J. S. Risbey
and D. P. Monselesan are supported by the Australian Climate Change Science
Program. I. Horenko is partly supported by the DFG (Mercator Fellowship
in the CRC 1114 Scaling cascades in complex systems) and the Swiss
National Science Foundation (SNF, grant 156398).<?xmltex \hack{\\\\}?> Edietd by: S. Vannitsem</p></ack><ref-list>
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