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<article xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:oasis="http://docs.oasis-open.org/ns/oasis-exchange/table" xml:lang="en" dtd-version="3.0">
  <front>
    <journal-meta><journal-id journal-id-type="publisher">ESD</journal-id><journal-title-group>
    <journal-title>Earth System Dynamics</journal-title>
    <abbrev-journal-title abbrev-type="publisher">ESD</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Earth Syst. Dynam.</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">2190-4987</issn><publisher>
    <publisher-name>Copernicus Publications</publisher-name>
    <publisher-loc>Göttingen, Germany</publisher-loc>
  </publisher></journal-meta>
    <article-meta>
      <article-id pub-id-type="doi">10.5194/esd-10-257-2019</article-id><title-group><article-title>ESD Ideas: Propagation of high-frequency forcing<?xmltex \hack{\break}?> to ice age
dynamics</article-title><alt-title>Propagation of high-frequency forcing</alt-title>
      </title-group><?xmltex \runningtitle{Propagation of high-frequency forcing}?><?xmltex \runningauthor{M.~Y.~Verbitsky et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1 aff4 aff5">
          <name><surname>Verbitsky</surname><given-names>Mikhail Y.</given-names></name>
          <email>verbitskys@gmail.com</email>
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Crucifix</surname><given-names>Michel</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-3437-4911</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Volobuev</surname><given-names>Dmitry M.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-5407-3155</ext-link></contrib>
        <aff id="aff1"><label>1</label><institution>Gen5 Group, LLC, Newton, MA, USA</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>UCLouvain, Earth and Life Institute, Louvain-la-Neuve, Belgium</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>The Central Astronomical Observatory of the Russian Academy of
Sciences at Pulkovo,<?xmltex \hack{\break}?> Saint Petersburg, Russia</institution>
        </aff>
        <aff id="aff4"><label>a</label><institution>formerly at: Yale University, Department of Geology and Geophysics,<?xmltex \hack{\break}?>
New Haven, CT, USA</institution>
        </aff>
        <aff id="aff5"><label>*</label><institution>retired</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Mikhail Y. Verbitsky (verbitskys@gmail.com)</corresp></author-notes><pub-date><day>24</day><month>April</month><year>2019</year></pub-date>
      
      <volume>10</volume>
      <issue>2</issue>
      <fpage>257</fpage><lpage>260</lpage>
      <history>
        <date date-type="received"><day>17</day><month>October</month><year>2018</year></date>
           <date date-type="rev-request"><day>9</day><month>November</month><year>2018</year></date>
           <date date-type="rev-recd"><day>4</day><month>April</month><year>2019</year></date>
           <date date-type="accepted"><day>13</day><month>April</month><year>2019</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2019 Mikhail Y. Verbitsky et al.</copyright-statement>
        <copyright-year>2019</copyright-year>
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p></license></permissions><self-uri xlink:href="https://esd.copernicus.org/articles/10/257/2019/esd-10-257-2019.html">This article is available from https://esd.copernicus.org/articles/10/257/2019/esd-10-257-2019.html</self-uri><self-uri xlink:href="https://esd.copernicus.org/articles/10/257/2019/esd-10-257-2019.pdf">The full text article is available as a PDF file from https://esd.copernicus.org/articles/10/257/2019/esd-10-257-2019.pdf</self-uri>
      <abstract><title>Abstract</title>
    <p id="d1e132">Palaeoclimate records display a continuous background of
variability connecting centennial to 100 kyr periods. Hence, the dynamics at
the centennial, millennial, and astronomical timescales should not be
treated separately. Here, we show that the nonlinear character of ice sheet
dynamics, which was derived naturally from the ice-flow conservation laws,
provides the scaling constraints to explain the structure of the observed
spectrum of variability.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e144">Most theories of Quaternary climates consider that
glacial–interglacial cycles emerge from components of the climate system
interacting with each other and responding to the forcing generated by the
variations in summer insolation caused by climatic precession and the changes
in obliquity and in eccentricity. A common approach is to represent these
interactions and responses by ordinary differential equations. In a low-order
dynamical system, the state vector only includes a handful of variables,
which vary on roughly the same timescales as the forcing. Barry Saltzman
has long promoted this approach, and his models' state variables represented
the volume of continental ice sheets, deep ocean temperature, carbon dioxide
concentration, and in some models the lithospheric depression (e.g.,
Saltzman and Verbitsky, 1993). Similar models featuring other mechanisms
were published more recently (e.g., Omta et al., 2016). The purpose of these
models is to explain the temporal structure of ice age cycles, but the
spectrum of variability at centennial and millennial timescales is
generally ignored. This approach is commonly justified by a hypothesis of the separation of timescales, as formulated by Saltzman (1990). However, this
hypothesis is questionable. Indeed, the observational records display a
continuous background of variability connecting centennial to 100 kyr periods
(Huybers and Curry, 2006). For this reason, the dynamics at the centennial,
millennial, and astronomical timescales should not be considered
separately. Here, we address this concern and show that the ice dynamics are an effective vehicle for propagating high-frequency forcing upscale.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Methods</title>
      <p id="d1e155">To make this case, we use the dynamical model previously
presented in Verbitsky et al. (2018). This nonlinear dynamical system was
derived from scaled conservation equations of ice flow, combined with an
equation describing the evolution of a variable synthesizing the state of
rest of the climate, called “climate temperature”. The three variables are
thus the area of glaciation, ice sheet basal temperature, and climate
temperature. Without astronomical forcing, the system evolves to an
equilibrium. When the astronomical<?pagebreak page258?> forcing is present, the system exhibits
different modes of nonlinearity leading to different periods of ice age
rhythmicity. Specifically, when the ratio of positive climate feedback to
negative glaciation feedback (quantified by the <inline-formula><mml:math id="M1" display="inline"><mml:mi>V</mml:mi></mml:math></inline-formula> number) is about 0.75, the
system displays glacial–interglacial cycles of a period of roughly 100 kyr.
In effect, the response doubles the obliquity period. For this mechanism to
operate, ice needs to survive through a first maximum of insolation and
then grow to a level at which it is vulnerable to an – even modest –
increase in insolation. In the Verbitsky et al. (2018) model with reference
parameters, the threshold corresponds to a glaciation area <inline-formula><mml:math id="M2" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula> of roughly
<inline-formula><mml:math id="M3" display="inline"><mml:mrow><mml:mn mathvariant="normal">20</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">6</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> km<inline-formula><mml:math id="M4" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula>.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1" specific-use="star"><?xmltex \currentcnt{1}?><label>Figure 1</label><caption><p id="d1e198"><bold>(a)</bold> The system response to pure 5 kyr sinusoid of variable
amplitude on a phase plane of glaciation area <inline-formula><mml:math id="M5" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula> (10<inline-formula><mml:math id="M6" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msup></mml:math></inline-formula> km<inline-formula><mml:math id="M7" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula>)
vs. climate temperature <inline-formula><mml:math id="M8" display="inline"><mml:mi mathvariant="italic">ω</mml:mi></mml:math></inline-formula> (<inline-formula><mml:math id="M9" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C); <inline-formula><mml:math id="M10" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>S</mml:mi></mml:mrow></mml:math></inline-formula> is the disruption potential; <bold>(b)</bold> the blue line represents the reference system
response to astronomical forcing (Verbitsky et al., 2018). Millennial forcing
is absent here. The brown line shows the system response when the orbital forcing
is combined with 5 kyr sinusoid of the 10-fold amplitude. The diagram is a
linear amplitude spectrum on a logarithmic scale; the vertical axis measures the
amplitude of glacial area variations,
log<inline-formula><mml:math id="M11" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msub></mml:math></inline-formula>[<inline-formula><mml:math id="M12" display="inline"><mml:mover accent="true"><mml:mi>S</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula>(10<inline-formula><mml:math id="M13" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msup></mml:math></inline-formula> km<inline-formula><mml:math id="M14" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula>)]; the horizontal axis is
log<inline-formula><mml:math id="M15" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msub></mml:math></inline-formula>[<inline-formula><mml:math id="M16" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(1 kyr<inline-formula><mml:math id="M17" 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>)]; <bold>(c)</bold> same as <bold>(a)</bold>
but millennial forcing is formed by seven sinusoids of the same amplitude
(<inline-formula><mml:math id="M18" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">2.5</mml:mn></mml:mrow></mml:math></inline-formula> of the insolation forcing amplitude) and periods of 3, 4, 5, 6,
7, 8, and 9 kyr. <bold>(d)</bold> Same as <bold>(b)</bold> for multi-period forcing of
<bold>(c)</bold>.</p></caption>
        <?xmltex \igopts{width=384.112205pt}?><graphic xlink:href="https://esd.copernicus.org/articles/10/257/2019/esd-10-257-2019-f01.png"/>

      </fig>

      <p id="d1e356">In the reference experiment presented in Verbitsky et al. (2018), the system is
driven, following standard practice, by mid-June insolation at 65<inline-formula><mml:math id="M19" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N
(Berger and Loutre, 1991). The output of three additional experiments is
shown here. In the first experiment, the mid-June insolation is replaced
with a sinusoid of 5 kyr period and variable amplitude (first, about the same
amplitude as of insolation forcing and then increased 10-fold). In the
second experiment, this 10-fold increased 5 kyr period sinusoid is combined
with mid-June insolation at 65<inline-formula><mml:math id="M20" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N. In the third experiment, the forcing
is represented by several sinusoids of smaller amplitudes (<inline-formula><mml:math id="M21" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">2.5</mml:mn></mml:mrow></mml:math></inline-formula> of the insolation forcing amplitude) and periods spread between 3 and
9 kyr. The results demonstrate the following.
<list list-type="custom"><list-item><label>a.</label>
      <p id="d1e389">When our system is forced by a pure 5 kyr sinusoid of small amplitude,
the system remains in the vicinity of its equilibrium point, with a glaciation
area of <inline-formula><mml:math id="M22" display="inline"><mml:mrow><mml:mn mathvariant="normal">15</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">6</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> km<inline-formula><mml:math id="M23" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> and a climate temperature of
<inline-formula><mml:math id="M24" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>2 <inline-formula><mml:math id="M25" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C (cf. Fig. 1a). When the amplitude of the sinusoid is
increased 10-fold, the effects of the negative phases of the forcing are no
longer symmetric to those of the positive phases because of the system's
nonlinearity. As a consequence, the system moves to a different phase-plane
domain, around <inline-formula><mml:math id="M26" display="inline"><mml:mrow><mml:mn mathvariant="normal">6</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">6</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> km<inline-formula><mml:math id="M27" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> of glaciation area, and a climate
temperature of 4.6 <inline-formula><mml:math id="M28" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C (Fig. 1a).</p></list-item><list-item><label>b.</label>
      <p id="d1e467">This shift of the time mean glaciation area and temperature has a dramatic
effect on ice age dynamics. When insolation forcing is combined with strong
millennial forcing, the latter moves the system into the domain where
obliquity period doubling no longer occurs because ice no longer grows to
the level needed to enable the strong positive deglaciation feedback.
Consequently, the 100 kyr variability almost vanishes – Fig. 1b. We term this suppression of ice age variability by millennial
variability “hijacking”. This result by itself invalidates the classical timescale
separation hypothesis: we see here that increased <italic>millennial</italic> variability causes the
<italic>ice age</italic> cycles to fade.</p></list-item><list-item><label>c.</label>
      <p id="d1e477">Millennial forcings can be aggregated: Several sinusoids of smaller
amplitudes and of different millennial periods create the same hijacking
effect as a single 5 kyr high-amplitude sinusoid, moving the system into the
phase-plane domain of higher temperatures and lower ice volume (Fig. 1c).</p></list-item><list-item><label>d.</label>
      <p id="d1e481">Acting alone, low-amplitude millennial sinusoids preserve their original
frequencies. However, several components may generate low-frequency
beatings, which are then demodulated by the system. Through this mechanism,
millennial forcing may induce responses at periods close to the orbital
periods, e.g., periods of precession and obliquity (Fig. 1d). For example,
the 41 kyr mode in Fig. 1d, which one might be tempted to attribute to obliquity,
is in fact the demodulation of the envelope generated by the interplay of
the 6  and 7 kyr forcing sinusoids: <inline-formula><mml:math id="M29" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">41</mml:mn><mml:mo>≈</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">6</mml:mn></mml:mrow></mml:math></inline-formula>–<inline-formula><mml:math id="M30" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">7</mml:mn></mml:mrow></mml:math></inline-formula>.</p></list-item></list></p>
      <p id="d1e517">It is possible to anticipate the disruptive effect of forcing at other
periods. Indeed, let us measure this disruption potential as the distance
<inline-formula><mml:math id="M31" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>S</mml:mi></mml:mrow></mml:math></inline-formula> (km<inline-formula><mml:math id="M32" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula>) on the phase plane between the system's equilibrium
point with zero forcing and the time mean ice sheet area expected given a
periodic forcing of amplitude <inline-formula><mml:math id="M33" display="inline"><mml:mi mathvariant="italic">ε</mml:mi></mml:math></inline-formula> and period <inline-formula><mml:math id="M34" display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula> (Fig. 1a, c). In
Verbitsky et al. (2018), we have shown that the dynamical properties of the
system are largely determined by the <inline-formula><mml:math id="M35" display="inline"><mml:mi>V</mml:mi></mml:math></inline-formula> number. We therefore may expect
<inline-formula><mml:math id="M36" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>S</mml:mi><mml:mo>=</mml:mo><mml:mi mathvariant="italic">φ</mml:mi><mml:mo>(</mml:mo><mml:mi>V</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="italic">ε</mml:mi><mml:mo>,</mml:mo><mml:mi>T</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>. Since <inline-formula><mml:math id="M37" display="inline"><mml:mi>V</mml:mi></mml:math></inline-formula> is dimensionless and
since the dimensions of <inline-formula><mml:math id="M38" display="inline"><mml:mi mathvariant="italic">ε</mml:mi></mml:math></inline-formula> (km kyr<inline-formula><mml:math id="M39" 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>) and <inline-formula><mml:math id="M40" display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula> (kyr) are independent (in our model, the forcing is
introduced as a component of ice sheet mass balance and therefore
<inline-formula><mml:math id="M41" display="inline"><mml:mi mathvariant="italic">ε</mml:mi></mml:math></inline-formula> has the same dimension as ice ablation rate; km kyr<inline-formula><mml:math id="M42" 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>),
the <inline-formula><mml:math id="M43" display="inline"><mml:mi mathvariant="italic">π</mml:mi></mml:math></inline-formula> theorem (Buckingham, 1914) tells us that <inline-formula><mml:math id="M44" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>S</mml:mi><mml:mo>/</mml:mo><mml:mo>(</mml:mo><mml:msup><mml:mi mathvariant="italic">ε</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:msup><mml:mi>T</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mi mathvariant="normal">Φ</mml:mi><mml:mo>(</mml:mo><mml:mi>V</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>. We determined experimentally that
<inline-formula><mml:math id="M45" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>S</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula> if <inline-formula><mml:math id="M46" display="inline"><mml:mrow><mml:mi>V</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula> and that <inline-formula><mml:math id="M47" display="inline"><mml:mrow><mml:mi mathvariant="normal">Φ</mml:mi><mml:mo>(</mml:mo><mml:mi>V</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> can be approximated as a linear
function. The scaling argument finally brings us to
          <disp-formula id="Ch1.E1" content-type="numbered"><label>1</label><mml:math id="M48" display="block"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>S</mml:mi><mml:mo>≈</mml:mo><mml:mo>-</mml:mo><mml:mi mathvariant="italic">μ</mml:mi><mml:mi>V</mml:mi><mml:msup><mml:mi mathvariant="italic">ε</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:msup><mml:mi>T</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:mi mathvariant="italic">μ</mml:mi><mml:mi>V</mml:mi><mml:msup><mml:mi mathvariant="italic">ε</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:msup><mml:mi>f</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
        where <inline-formula><mml:math id="M49" display="inline"><mml:mrow><mml:mi>f</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mi>T</mml:mi></mml:mrow></mml:math></inline-formula> is the frequency, and <inline-formula><mml:math id="M50" display="inline"><mml:mi mathvariant="italic">μ</mml:mi></mml:math></inline-formula> is a constant that has to be
determined experimentally. We thus see that <inline-formula><mml:math id="M51" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>S</mml:mi><mml:mo>∼</mml:mo><mml:msup><mml:mi>f</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>. The
<inline-formula><mml:math id="M52" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>2 frequency slope of <inline-formula><mml:math id="M53" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>S</mml:mi></mml:mrow></mml:math></inline-formula> has been confirmed in additional
numerical experiments (not shown here) for forcing periods between 2 and
20 kyr. The 5 kyr period sinusoids and multiple sinusoids of periods spread
between 3 and 9 kyr are arbitrary choices used to illustrate the
hijacking and beating effects. The phenomena can be replicated with other
modes of millennial activity such as, for example, 6.5, 2.5, 0.9, and 0.5 kyr
periods identified by Dima and Lohmann (2009). For example, we confirmed
that, as it is implied by Eq. (1), the hijacking effect of a 6.5 kyr
sinusoid is the same as that of a 5 kyr sinusoid if the ratio of the corresponding
amplitudes is 0.77.</p>
      <p id="d1e839">Similar scaling arguments can be applied to the amplitude of the <inline-formula><mml:math id="M54" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula> variable,
i.e., the amplitude of the glacial area over a glacial cycle. This amplitude
<inline-formula><mml:math id="M55" display="inline"><mml:mover accent="true"><mml:mi>S</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula> has the same dimension as <inline-formula><mml:math id="M56" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>S</mml:mi></mml:mrow></mml:math></inline-formula>; i.e., <inline-formula><mml:math id="M57" display="inline"><mml:mrow><mml:mover accent="true"><mml:mi>S</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>=</mml:mo><mml:mi mathvariant="italic">ψ</mml:mi><mml:mo>(</mml:mo><mml:mi>V</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="italic">ε</mml:mi><mml:mo>,</mml:mo><mml:mi>T</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M58" display="inline"><mml:mrow><mml:mover accent="true"><mml:mi>S</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>∼</mml:mo><mml:msup><mml:mi mathvariant="italic">ε</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:msup><mml:mi>T</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>,
where <inline-formula><mml:math id="M59" display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula> is the period of the system response. Depending on the value of the
<inline-formula><mml:math id="M60" display="inline"><mml:mi>V</mml:mi></mml:math></inline-formula> number, the system response may feature periods of external forcing or multiples of forcing periods or combinations of these. Accordingly, Fig. 1d shows a <inline-formula><mml:math id="M61" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1.9 slope<?pagebreak page259?> in the orbital frequency domain (though, again,
all peaks in this domain are, in fact, created by the millennial forcing) and
a <inline-formula><mml:math id="M62" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>2 slope for the millennial domain. We regard this result as a
remarkable test in favor of the above hypothesis; i.e., <inline-formula><mml:math id="M63" display="inline"><mml:mrow><mml:mover accent="true"><mml:mi>S</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>=</mml:mo><mml:mi mathvariant="italic">ψ</mml:mi><mml:mo>(</mml:mo><mml:mi>V</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="italic">ε</mml:mi><mml:mo>,</mml:mo><mml:mi>T</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>. Different aspects of glacial geometry such as area
(<inline-formula><mml:math id="M64" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula>), ice thickness (<inline-formula><mml:math id="M65" display="inline"><mml:mrow><mml:mi>H</mml:mi><mml:mo>∼</mml:mo><mml:msup><mml:mi>S</mml:mi><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">4</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>; Verbitsky, et al., 2018), glaciation
horizontal span (<inline-formula><mml:math id="M66" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:msup><mml:mi>S</mml:mi><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, or ice volume (<inline-formula><mml:math id="M67" display="inline"><mml:mrow><mml:mi>H</mml:mi><mml:mi>S</mml:mi><mml:mo>∼</mml:mo><mml:msup><mml:mi>S</mml:mi><mml:mrow><mml:mn mathvariant="normal">5</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">4</mml:mn></mml:mrow></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> may
play a role in shaping climate conditions at a specific geographical point.
Thus, corresponding power spectra of empirical records may have frequency
slopes ranging from <inline-formula><mml:math id="M68" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>5 (<inline-formula><mml:math id="M69" display="inline"><mml:mrow><mml:msup><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mo>)</mml:mo><mml:mo>⋅</mml:mo><mml:mn mathvariant="normal">5</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">4</mml:mn><mml:mo>⋅</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>) to <inline-formula><mml:math id="M70" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1 (<inline-formula><mml:math id="M71" display="inline"><mml:mrow><mml:msup><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mo>)</mml:mo><mml:mo>⋅</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">4</mml:mn><mml:mo>⋅</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>).</p>
      <p id="d1e1126">For multi-period forcing in a frequency domain <inline-formula><mml:math id="M72" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>f</mml:mi></mml:mrow></mml:math></inline-formula>, the aggregate
hijacking potential <inline-formula><mml:math id="M73" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>S</mml:mi><mml:mi mathvariant="normal">A</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> can be estimated as

              <disp-formula id="Ch1.E2" content-type="numbered"><label>2</label><mml:math id="M74" display="block"><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>S</mml:mi><mml:mi mathvariant="normal">A</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">1</mml:mn><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>f</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo movablelimits="false">∫</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>S</mml:mi><mml:mi mathvariant="normal">d</mml:mi><mml:mi>f</mml:mi><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:mi mathvariant="italic">μ</mml:mi><mml:mi>V</mml:mi><mml:mi mathvariant="normal">Δ</mml:mi><mml:msup><mml:mi>f</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mo movablelimits="false">∫</mml:mo><mml:mi mathvariant="italic">ε</mml:mi><mml:msup><mml:mfenced close=")" open="("><mml:mi>f</mml:mi></mml:mfenced><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:msup><mml:mi>f</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup><mml:mi mathvariant="normal">d</mml:mi><mml:mi>f</mml:mi><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula></p>
      <p id="d1e1230">Accordingly, since amplitudes of high-frequency variability, <inline-formula><mml:math id="M75" display="inline"><mml:mrow><mml:mi mathvariant="italic">ε</mml:mi><mml:mo>(</mml:mo><mml:mi>f</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, may compensate for the frequency damping (<inline-formula><mml:math id="M76" display="inline"><mml:mrow><mml:msup><mml:mi>f</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, centennial,
decennial, and perhaps even annual variations potentially may contaminate the
spectrum throughout the millennial and multi-millennial range and perturb
ice age dynamics via two physical mechanisms: (a) centennial and millennial
oscillations shift the mean state of the system, and (b) the sensitivity of
ice sheets to the astronomical forcing depends on the system state.</p>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Discussion</title>
      <p id="d1e1271">To our knowledge, only Le Treut and Ghil (1983) have previously adopted a
deterministic framework to model a background spectrum connecting millennial
to astronomical timescales. Unfortunately, their model did not generate
credible ice age time series. The more common route for<?pagebreak page260?> simulating the
centennial and millennial spectrum is to introduce a stochastic forcing
(e.g., Wunsch, 2003; Ditlevsen and Crucifix, 2017). Such stochastic forcing may in
principle be justified by the existence of chaotic or turbulent motion in the
atmosphere–ocean continuum. However, whether such forcing is large enough to
integrate all the way up to timescales of several tens of thousands of years
is speculative. The deterministic theory proposed here presents the advantage
of using the nonlinear character of ice sheet dynamics, which was derived
naturally from the conservation laws and therefore provides a clear physical
interpretation of the nonlinear origin of the cascade. Our approach is thus
remarkably parsimonious because it requires no more physics than the minimum
needed to explain ice ages plus the existence of centennial or millennium
modes of motions. The latter may very plausibly arise as modes of ocean
motion (Dijkstra and Ghil, 2005; Peltier and Vettoretti, 2014). Of course,
stochastic forcing may still be added, and its cumulated effects would then
be estimated by Eq. (2).</p>
      <p id="d1e1274">In summary, using a deterministic nonlinear dynamical model of the global
climate, we demonstrated that astronomical timescale variability cannot be
considered separately from millennial phenomena and that the ice dynamics are an effective vehicle for propagating high-frequency forcing into the orbital
timescale. This may imply that the knowledge of millennial and centennial
variability is needed to fully understand and replicate ice age history. As
we have seen, <italic>increased </italic> millennial variability <italic>decreases </italic>
the length of the ice age cycles. However, the reverse is also true. This
state of affairs generates a new hypothesis for the middle Pleistocene
transition: a decrease in millennial variability may have caused the
lengthening of ice ages. The millennial variability can legitimately be
modeled as a deterministic mode, which would allow us to come up with a
specific explanation of how this variability may influence ice age dynamics.
Hence our completely deterministic approach makes a physically justified
alternative to a popular notion that the background spectrum is merely
linearly integrated noise.</p>
</sec>

      
      </body>
    <back><notes notes-type="codedataavailability"><title>Code and data availability</title>

      <p id="d1e1287">The MatLab R2015b code and data to calculate the model
response to astronomical and millennial forcing (Verbitsky et al., 2019) are
available at <ext-link xlink:href="https://doi.org/10.5281/zenodo.2628310" ext-link-type="DOI">10.5281/zenodo.2628310</ext-link> (last access: 4 April 2019).</p>
  </notes><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e1296">MYV conceived the research and developed the
model. MYV and MC wrote the paper. DMV developed the numerical scheme and
MatLab code.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e1303">The authors declare that they have no conflict of
interest.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e1309">Michel Crucifix is funded by the Belgian National Fund of Scientific
Research. Dmitry M. Volobuev is funded in part by the Russian Foundation for
Basic Research, grant 19-02-00088-a. We are grateful to our reviewers
Gerrit Lohmann and Niklas Boers for their helpful comments.</p></ack><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e1314">This paper was edited by Anders Levermann and reviewed by Gerrit Lohmann and Niklas Boers.</p>
  </notes><ref-list>
    <title>References</title>

      <ref id="bib1.bib1"><label>1</label><mixed-citation>
Berger, A. and Loutre, M. F.: Insolation values for the climate of the last
10 million years, Quaternary Sci. Rev., 10, 297–317, 1991.</mixed-citation></ref>
      <ref id="bib1.bib2"><label>2</label><mixed-citation>
Buckingham, E.: On physically similar systems; illustrations of the use of
dimensional equations, Phys. Rev., 4, 345–376, 1914.</mixed-citation></ref>
      <ref id="bib1.bib3"><label>3</label><mixed-citation>Dijkstra, H. A. and Ghil, M.: Low-frequency variability of the large-scale
ocean circulation: A dynamical systems approach, Rev. Geophys., 43,
RG3002, <ext-link xlink:href="https://doi.org/10.1029/2002RG000122" ext-link-type="DOI">10.1029/2002RG000122</ext-link>,
2005.</mixed-citation></ref>
      <ref id="bib1.bib4"><label>4</label><mixed-citation>
Ditlevsen, P. and Crucifix, M.: On the importance of centennial variability
for ice ages, Past Global Changes Magazine, 25, 152–153, 2017.</mixed-citation></ref>
      <ref id="bib1.bib5"><label>5</label><mixed-citation>Dima, M. and Lohmann, G.: Conceptual model for millennial climate
variability: a possible combined solar-thermohaline circulation origin for
the <inline-formula><mml:math id="M77" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 1,500-year cycle, Clim. Dynam., 32, 301–311,
2009.</mixed-citation></ref>
      <ref id="bib1.bib6"><label>6</label><mixed-citation>Huybers, P. and Curry, W.: Links between annual, Milankovitch and continuum
temperature variability, Nature, 441, 329–332, <ext-link xlink:href="https://doi.org/10.1038/nature04745" ext-link-type="DOI">10.1038/nature04745</ext-link>, 2006.</mixed-citation></ref>
      <ref id="bib1.bib7"><label>7</label><mixed-citation>Le Treut, H. and Ghil, M.: Orbital forcing, climatic interactions and
glaciation cycles, J. Geophys. Res., 88, 5167–5190,
<ext-link xlink:href="https://doi.org/10.1029/JC088iC09p05167" ext-link-type="DOI">10.1029/JC088iC09p05167</ext-link>, 1983.</mixed-citation></ref>
      <ref id="bib1.bib8"><label>8</label><mixed-citation>Omta, A. W., Kooi, B. W., Voorn, G. A. K., Rickaby, R. E. M., and Follows, M.
J.: Inherent characteristics of sawtooth cycles can explain different
glacial periodicities, Clim. Dynam., 46, 557–569,
<ext-link xlink:href="https://doi.org/10.1007/s00382-015-2598-x" ext-link-type="DOI">10.1007/s00382-015-2598-x</ext-link>, 2016.</mixed-citation></ref>
      <ref id="bib1.bib9"><label>9</label><mixed-citation>Peltier, R. W. and Vettoretti, G.: Dansgaard-Oeschger oscillations predicted
in a comprehensive model of glacial climate: A “kicked” salt oscillator in
the Atlantic, Geophys. Res. Lett., 41, 7306–7313,
<ext-link xlink:href="https://doi.org/10.1002/2014GL061413" ext-link-type="DOI">10.1002/2014GL061413</ext-link>, 2014.</mixed-citation></ref>
      <ref id="bib1.bib10"><label>10</label><mixed-citation>
Saltzman, B.: Three basic problems of paleoclimatic modeling: A personal
perspective and review, Clim. Dynam., 5, 67–78, 1990.</mixed-citation></ref>
      <ref id="bib1.bib11"><label>11</label><mixed-citation>
Saltzman, B. and Verbitsky, M. Y.: Multiple instabilities and modes of
glacial rhythmicity in the Plio-Pleistocene: a general theory of late
Cenozoic climatic change, Clim. Dynam., 9, 1–15, 1993.</mixed-citation></ref>
      <ref id="bib1.bib12"><label>12</label><mixed-citation>Verbitsky, M. Y., Crucifix, M., and Volobuev, D. M.: A theory of Pleistocene
glacial rhythmicity, Earth Syst. Dynam., 9, 1025–1043,
<ext-link xlink:href="https://doi.org/10.5194/esd-9-1025-2018" ext-link-type="DOI">10.5194/esd-9-1025-2018</ext-link>, 2018.</mixed-citation></ref>
      <ref id="bib1.bib13"><label>13</label><mixed-citation>Verbitsky, M. Y., Crucifix, M., and Volobuev, D. M.: Supplementary code and
data to paper “ESD Ideas: Propagation of high-frequency forcing to ice age
dynamics” (Version 1.0), Zenodo, available at:
<ext-link xlink:href="https://doi.org/10.5281/zenodo.2628310" ext-link-type="DOI">10.5281/zenodo.2628310</ext-link>, last access: 4 April 2019.</mixed-citation></ref>
      <ref id="bib1.bib14"><label>14</label><mixed-citation>
Wunsch, C.: The spectral description of climate change including the 100 ky
energy, Clim. Dynam., 20, 353–363,  2003.</mixed-citation></ref>

  </ref-list></back>
    <!--<article-title-html>ESD Ideas: Propagation of high-frequency forcing to ice age dynamics</article-title-html>
<abstract-html><p>Palaeoclimate records display a continuous background of
variability connecting centennial to 100&thinsp;kyr periods. Hence, the dynamics at
the centennial, millennial, and astronomical timescales should not be
treated separately. Here, we show that the nonlinear character of ice sheet
dynamics, which was derived naturally from the ice-flow conservation laws,
provides the scaling constraints to explain the structure of the observed
spectrum of variability.</p></abstract-html>
<ref-html id="bib1.bib1"><label>1</label><mixed-citation>
Berger, A. and Loutre, M. F.: Insolation values for the climate of the last
10 million years, Quaternary Sci. Rev., 10, 297–317, 1991.
</mixed-citation></ref-html>
<ref-html id="bib1.bib2"><label>2</label><mixed-citation>
Buckingham, E.: On physically similar systems; illustrations of the use of
dimensional equations, Phys. Rev., 4, 345–376, 1914.
</mixed-citation></ref-html>
<ref-html id="bib1.bib3"><label>3</label><mixed-citation>
Dijkstra, H. A. and Ghil, M.: Low-frequency variability of the large-scale
ocean circulation: A dynamical systems approach, Rev. Geophys., 43,
RG3002, <a href="https://doi.org/10.1029/2002RG000122" target="_blank">https://doi.org/10.1029/2002RG000122</a>,
2005.
</mixed-citation></ref-html>
<ref-html id="bib1.bib4"><label>4</label><mixed-citation>
Ditlevsen, P. and Crucifix, M.: On the importance of centennial variability
for ice ages, Past Global Changes Magazine, 25, 152–153, 2017.
</mixed-citation></ref-html>
<ref-html id="bib1.bib5"><label>5</label><mixed-citation>
Dima, M. and Lohmann, G.: Conceptual model for millennial climate
variability: a possible combined solar-thermohaline circulation origin for
the  ∼ &thinsp;1,500-year cycle, Clim. Dynam., 32, 301–311,
2009.
</mixed-citation></ref-html>
<ref-html id="bib1.bib6"><label>6</label><mixed-citation>
Huybers, P. and Curry, W.: Links between annual, Milankovitch and continuum
temperature variability, Nature, 441, 329–332, <a href="https://doi.org/10.1038/nature04745" target="_blank">https://doi.org/10.1038/nature04745</a>, 2006.
</mixed-citation></ref-html>
<ref-html id="bib1.bib7"><label>7</label><mixed-citation>
Le Treut, H. and Ghil, M.: Orbital forcing, climatic interactions and
glaciation cycles, J. Geophys. Res., 88, 5167–5190,
<a href="https://doi.org/10.1029/JC088iC09p05167" target="_blank">https://doi.org/10.1029/JC088iC09p05167</a>, 1983.
</mixed-citation></ref-html>
<ref-html id="bib1.bib8"><label>8</label><mixed-citation>
Omta, A. W., Kooi, B. W., Voorn, G. A. K., Rickaby, R. E. M., and Follows, M.
J.: Inherent characteristics of sawtooth cycles can explain different
glacial periodicities, Clim. Dynam., 46, 557–569,
<a href="https://doi.org/10.1007/s00382-015-2598-x" target="_blank">https://doi.org/10.1007/s00382-015-2598-x</a>, 2016.
</mixed-citation></ref-html>
<ref-html id="bib1.bib9"><label>9</label><mixed-citation>
Peltier, R. W. and Vettoretti, G.: Dansgaard-Oeschger oscillations predicted
in a comprehensive model of glacial climate: A “kicked” salt oscillator in
the Atlantic, Geophys. Res. Lett., 41, 7306–7313,
<a href="https://doi.org/10.1002/2014GL061413" target="_blank">https://doi.org/10.1002/2014GL061413</a>, 2014.
</mixed-citation></ref-html>
<ref-html id="bib1.bib10"><label>10</label><mixed-citation>
Saltzman, B.: Three basic problems of paleoclimatic modeling: A personal
perspective and review, Clim. Dynam., 5, 67–78, 1990.
</mixed-citation></ref-html>
<ref-html id="bib1.bib11"><label>11</label><mixed-citation>
Saltzman, B. and Verbitsky, M. Y.: Multiple instabilities and modes of
glacial rhythmicity in the Plio-Pleistocene: a general theory of late
Cenozoic climatic change, Clim. Dynam., 9, 1–15, 1993.
</mixed-citation></ref-html>
<ref-html id="bib1.bib12"><label>12</label><mixed-citation>
Verbitsky, M. Y., Crucifix, M., and Volobuev, D. M.: A theory of Pleistocene
glacial rhythmicity, Earth Syst. Dynam., 9, 1025–1043,
<a href="https://doi.org/10.5194/esd-9-1025-2018" target="_blank">https://doi.org/10.5194/esd-9-1025-2018</a>, 2018.
</mixed-citation></ref-html>
<ref-html id="bib1.bib13"><label>13</label><mixed-citation>
Verbitsky, M. Y., Crucifix, M., and Volobuev, D. M.: Supplementary code and
data to paper “ESD Ideas: Propagation of high-frequency forcing to ice age
dynamics” (Version 1.0), Zenodo, available at:
<a href="https://doi.org/10.5281/zenodo.2628310" target="_blank">https://doi.org/10.5281/zenodo.2628310</a>, last access: 4 April 2019.
</mixed-citation></ref-html>
<ref-html id="bib1.bib14"><label>14</label><mixed-citation>
Wunsch, C.: The spectral description of climate change including the 100&thinsp;ky
energy, Clim. Dynam., 20, 353–363,  2003.
</mixed-citation></ref-html>--></article>
