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<article article-type="research-article" dtd-version="2.3" xml:lang="EN" xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">
<front>
<journal-meta>
<journal-id journal-id-type="publisher-id">Front. Astron. Space Sci.</journal-id>
<journal-title>Frontiers in Astronomy and Space Sciences</journal-title>
<abbrev-journal-title abbrev-type="pubmed">Front. Astron. Space Sci.</abbrev-journal-title>
<issn pub-type="epub">2296-987X</issn>
<publisher>
<publisher-name>Frontiers Media S.A.</publisher-name>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="publisher-id">839794</article-id>
<article-id pub-id-type="doi">10.3389/fspas.2022.839794</article-id>
<article-categories>
<subj-group subj-group-type="heading">
<subject>Astronomy and Space Sciences</subject>
<subj-group>
<subject>Original Research</subject>
</subj-group>
</subj-group>
</article-categories>
<title-group>
<article-title>Jovian Planets and Lunar Nodal Cycles in the Earth&#x2019;s Climate Variability</article-title>
<alt-title alt-title-type="left-running-head">Yndestad</alt-title>
<alt-title alt-title-type="right-running-head">Solar Lunar Forced Climate Oscillation</alt-title>
</title-group>
<contrib-group>
<contrib contrib-type="author" corresp="yes">
<name>
<surname>Yndestad</surname>
<given-names>Harald</given-names>
</name>
<xref ref-type="corresp" rid="c001">&#x2a;</xref>
<uri xlink:href="https://loop.frontiersin.org/people/1536014/overview"/>
</contrib>
</contrib-group>
<aff>
<institution>Norwegian University of Science and Technology</institution>, <addr-line>Aalesund</addr-line>, <country>Norway</country>
</aff>
<author-notes>
<fn fn-type="edited-by">
<p>
<bold>Edited by:</bold> <ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/23249/overview">Nicola Scafetta</ext-link>, University of Naples Federico II, Italy</p>
</fn>
<fn fn-type="edited-by">
<p>
<bold>Reviewed by:</bold> <ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/1615679/overview">Stephen Puetz</ext-link>, Progressive Foundation, United States</p>
<p>
<ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/1632480/overview">Victor Manuel Velasco Herrera</ext-link>, National Autonomous University of Mexico, Mexico</p>
</fn>
<corresp id="c001">&#x2a;Correspondence: Harald Yndestad, <email>Harald.Yndestad@ntnu.no</email>
</corresp>
<fn fn-type="other">
<p>This article was submitted to Planetary Science, a section of the journal Frontiers in Astronomy and Space Sciences</p>
</fn>
</author-notes>
<pub-date pub-type="epub">
<day>10</day>
<month>05</month>
<year>2022</year>
</pub-date>
<pub-date pub-type="collection">
<year>2022</year>
</pub-date>
<volume>9</volume>
<elocation-id>839794</elocation-id>
<history>
<date date-type="received">
<day>20</day>
<month>12</month>
<year>2021</year>
</date>
<date date-type="accepted">
<day>11</day>
<month>04</month>
<year>2022</year>
</date>
</history>
<permissions>
<copyright-statement>Copyright &#xa9; 2022 Yndestad.</copyright-statement>
<copyright-year>2022</copyright-year>
<copyright-holder>Yndestad</copyright-holder>
<license xlink:href="http://creativecommons.org/licenses/by/4.0/">
<p>This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY). The use, distribution or reproduction in other forums is permitted, provided the original author(s) and the copyright owner(s) are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these terms.</p>
</license>
</permissions>
<abstract>
<p>This study utilizes time-series data devised to measure solar irradiation, sea surface temperatures, and temperatures in the lower atmosphere to gain a better understanding of how gravitational effects from the moon and Jovian planets (Jupiter, Saturn, Uranus, and Neptune) influence solar activity and climatic conditions on Earth. Then, standard statistical methods are used to determine the degree of correlation among these time series and construct a Jovian gravitational model. The study reveals a direct relationship between JSUN perihelion coincidences and TSI amplitude variations in cycles up to 4,450&#xa0;years. The forced solar accumulation of heat in oceans introduces a new phase relation between solar forced cycles and new climate variation. Earth&#x2019;s axis nutation cycles have coincidences with lunar nodal tide cycles and lunar forced sea surface temperature cycle periods up to 446&#xa0;years. Earth&#x2019;s temperature variation shows coincidence with constructive and destructive interference between lunar-forced and accumulated solar-forced temperature variations in oceans. Upcoming events have a computed modern temperature maximum in 2025 and a deep minimum in 2070. Interference between solar-forced temperature cycles of 333,2142, and 4,450&#xa0;years and a lunar-forced temperature cycle of 445&#xa0;years indicates that &#x201c;The Little Ice Age&#x201d; covers a total period of 820&#xa0;years from 1330 to 2150 A.D. and an upcoming temporary cold climate period from 2070 to 2150.</p>
</abstract>
<kwd-group>
<kwd>deep solar minima</kwd>
<kwd>climate variability</kwd>
<kwd>jovian planet variations</kwd>
<kwd>TSI variations</kwd>
<kwd>lunar nodal cycle spectrum</kwd>
<kwd>solar-lunar-forced climate variation</kwd>
</kwd-group>
</article-meta>
</front>
<body>
<sec id="s1">
<title>Introduction</title>
<p>Studies using climate models have observed global multidecadal variation originating from an unknown source (<xref ref-type="bibr" rid="B24">Mann et al., 2020</xref>). <xref ref-type="bibr" rid="B18">Kravtsov et al. (2018)</xref> found that current climate models fail to explain a substantial amount of global climate variation. The unexplained variation can be up to 0.3&#xb0;C. Multidecadal temperature variations on Earth may be deterministic or random; deterministic variations originating from known sources can be used to predict future variations, whereas random (nondeterministic) variations originating from unknown sources can only explain past events. Stationary cycles in time series are deterministic if the cycles have deterministic external sources. Deterministic variation from an external source may serve as a reference for climate variation. Some possible external sources of deterministic stationary climate cycles include stationary cycles in total solar irradiance (TSI) cycles, originating from planet cycles, and stationary lunar-forced temperature variations, originating from the Earth&#x2019;s axis nutation. When phase relations between the stationary cycles are known, it opens new possibilities for estimating past and future events.</p>
<p>Records have shown correlation between solar variations and global temperatures (<xref ref-type="bibr" rid="B38">Suess 1980</xref>). Cycles featuring solar variations, as identified from Greenland ice cores, have stimulated a discussion about the possible planetary modulation of solar irradiation in the solar system. <xref ref-type="bibr" rid="B15">Jose (1965)</xref> identified a correlation among planets, i.e., solar barycenter motion with a 179-year cycle. <xref ref-type="bibr" rid="B52">Zhenqiu and Zhisen (1980)</xref> analyzed planetary conjunctions and climate in China and estimated minimum temperatures for the years 1982, 2163 and 2344 A.D. Numerous other investigations have elucidated the relationships among planetary cycles, solar irradiance, and climate variations (<xref ref-type="bibr" rid="B9">Fairbridge and Sanders, 1987</xref>; <xref ref-type="bibr" rid="B13">Hoyt and Schatten 1993</xref>; <xref ref-type="bibr" rid="B33">Satterley, A. K. 1996</xref>; <xref ref-type="bibr" rid="B4">Charv&#xe1;tov&#xe1; 2000</xref>; <xref ref-type="bibr" rid="B20">Liu et al., 2011</xref>; <xref ref-type="bibr" rid="B1">Abreu et al., 2012</xref>; <xref ref-type="bibr" rid="B36">Scafetta 2012</xref>, <xref ref-type="bibr" rid="B34">2016</xref>; <xref ref-type="bibr" rid="B26">McCracken et al., 2014</xref>; <xref ref-type="bibr" rid="B35">Scafetta et al., 2016</xref>: <xref ref-type="bibr" rid="B37">Steinhilber and Beer (2013)</xref>) studied solar irradiance over a cycle of 9400&#xa0;years and identified long cycles of 150, 208, 350, 500, 1000, 1450, and 2200&#xa0;years; the authors also computed a Dalton-type minimum at 2100 A.D. Wavelet spectrum analyses of time series of the TSI, sunspots and solar position have revealed close relations among the TSI variation, solar position oscillation and elliptical orbits of the Jovian planets (Jupiter, Saturn, Uranus, and Neptune) (<xref ref-type="bibr" rid="B48">Yndestad and Solheim 2017</xref>).</p>
<p>The oscillation of gravitational forces within the Earth-Moon-Sun system introduces a spectrum of tides that influence the redistribution of heat in the large-scale oceanic thermohaline system. Tidal forcing in the ocean&#x2019;s thermohaline system introduces vertical temperature mixing in the oceans, which influences sea surface temperatures and atmospheric climate. Studies have revealed that approximately 1&#xa0;TW (25&#x2013;30%) of the total dissipation of energy occurs in the deep oceans (<xref ref-type="bibr" rid="B8">Egbert and Ray 2000</xref>). The estimated mixing energy required to maintain large-scale thermohaline circulation is approximately 2&#xa0;TW. Therefore, half of this amount could be provided by tides. The relationship between the temperature variations of the Atlantic Ocean and lunar tides has been discussed for decades. In 1907, Otto Pettersson studied the relationship between herring catches and tides along the west coast of Sweden and concluded that the long-cycle (18- and 111-year) tidal cycles of climate variations were caused by vertical mixing (<xref ref-type="bibr" rid="B31">Pettersson 1905</xref>, <xref ref-type="bibr" rid="B29">1914</xref>, <xref ref-type="bibr" rid="B30">1915</xref>). Russian scientists <xref ref-type="bibr" rid="B23">Maksimov and Smirnov (1964</xref>, <xref ref-type="bibr" rid="B22">1967)</xref> and <xref ref-type="bibr" rid="B6">Currie (1981)</xref> identified an 18.6-year lunar nodal tide as a standing tide between the Earth&#x2019;s poles and equator. Since the 1960&#xa0;s, several studies have confirmed the 18.6-year cycle through spectrum analyses (<xref ref-type="bibr" rid="B16">Keeling and Whorf 1997</xref>; <xref ref-type="bibr" rid="B10">Gratiot et al., 2008</xref>; <xref ref-type="bibr" rid="B12">Hansen et al., 2015</xref>; <xref ref-type="bibr" rid="B11">Gustavo et al., 2018</xref>). Wavelet spectrum analyses of the water inflows from the North Atlantic into the Norwegian Sea and Barents Sea have identified that this 18.6-year lunar nodal tide introduces surface temperature cycles of 18.6/2, 18.6, 3&#x2a;18.6 and 4&#x2a;18.6 years (<xref ref-type="bibr" rid="B50">Yndestad et al., 2008</xref>). The same cycles have been identified in the North Atlantic Oscillation (NAO) index, the Arctic Sea ice extent (<xref ref-type="bibr" rid="B47">Yndestad 2021</xref>), the Arctic Ocean circulation, and the oscillations of the Earth&#x2019;s axis (<xref ref-type="bibr" rid="B49">Yndestad 2006</xref>). Nevertheless, the cycle- and phase-relations among planetary cycles, TSI variation, lunar-forced ocean temperature variation and global temperature variation are poorly understood. Using known cycle periods and cycle phase relations from Jovian planets and Earth&#xb4;s axis nutation, this study investigates solar forced temperature variations and lunar forced temperature variations in Earth temperature variation.</p>
</sec>
<sec sec-type="materials|methods" id="s2">
<title>Materials and Methods</title>
<sec id="s2-1">
<title>Theory</title>
<p>This study investigates the relation between cycle periods, cycle phase and cycle amplitude in a chain of events, from the Jovian planets and the Earth&#x2019;s nutation, to climate variations. Cycle properties and notations are explained in the Nomenclature section.</p>
</sec>
<sec id="s2-2">
<title>Jovian Planet Oscillations</title>
<p>The Jovian planets, Jupiter, Saturn, Uranus, and Neptune (JSUN), have elliptic orbital cycles in time-variant distances from the Sun. The elliptic orbital cycles have maximum speeds and minimum distances from the Sun when the orbital phase position is at perihelion and minimum speeds and maximum distances at aphelion. The JSUN elliptic orbital cycles represent an oscillating spectrum, Sjsun (Tjsun, (&#x3b8;jsun (t-t<sub>per</sub>)). The Jovian planets have cycle periods (in years) Tjsun &#x3d; (Tju, Tsa, Tur, Tne) &#x3d; (11.862, 29.447, 84.02, 164.79) (yr.), and &#x3b8;jsun (t-t<sub>per</sub>) represents references to perihelion coincidences. JSUN planets have perihelion position phase coincidences, &#x3b8;jsun (t &#x3d; t<sub>per</sub>), at the year t<sub>per</sub> &#x3d; (t<sub>per-ju</sub>, t<sub>per-sa</sub>, t<sub>per-ur</sub>, t<sub>per-ne</sub>) &#x3d; (1714.69, 1709.00, 1714.32, 1711.88) (yr). (Astronomical Almanac, USNO, Governmental Printing Office). The mean perihelion coincidence occurs in 1712 A.D. JSUN elliptic orbital cycles have aphelion coincidences in the following years: t<sub>aph</sub> &#x3d; ((t<sub>per-ju</sub>-187.5Tju), (t<sub>per-sa</sub>-75.5Tsa), (t<sub>per-ur</sub> -26.5Tur), (t<sub>per-ne</sub>-13.5Tne)) &#x3d; (-509.43, -514.25, -512.21, -512.79) (yr.). The mean aphelion coincidence occurs in 512.17 B.C. The mean envelope time period of JSUN cycle phase coincidences is 4449.28&#xa0;years. The 4450-year envelope period has phase shifts at Ajsun-en(t) &#x3d; ((-0, -1624.49), (aper, &#x2212;512), (&#x2b;0, 600), (per, 1712), (&#x2212;0, 2825)).</p>
</sec>
<sec id="s2-3">
<title>Solar Position Oscillations</title>
<p>The Sun moves in a closed orbit around the barycenter of the solar system. The solar system oscillation is caused by the mutual gravity dynamics between the planet system oscillation and the solar position oscillation (SPO). The SPO has oscillations in the <italic>x, y,</italic> and <italic>z</italic> directions; they are represented by data series <italic>SPOx, SPOy,</italic> and <italic>SPOz,</italic> respectively. A wavelet spectrum analysis of SPO time-series in the (x, y, z)-direction revealed a coincidence between JSUN mean perihelion coincidences in 1712 A.D. (<xref ref-type="bibr" rid="B48">Yndestad and Solheim 2017</xref>). The coincidence between SPOs and JSUN cycles at the perihelion may be represented as a linear spectrum transform of JSUN cycle periods to SPO oscillations and solar dynamo oscillations. The total solar irradiation spectrum, Stsi, may be represented as a spectrum transformation from JSUN oscillation TSI oscillations.</p>
</sec>
<sec id="s2-4">
<title>Total Solar Irradiation Oscillation</title>
<p>Total solar irradiation (TSI) oscillations are represented as a spectrum: Stsi (Ttsi, &#x3b8;tsi (t-t<sub>tsi</sub>)), where Ttsi represents TSI cycle periods and &#x3b8;tsi (t &#x3d; t<sub>tsi</sub>) represents the years when TSI periods have a maximum amplitude. TSI amplitude variations, Atsi(t), experience minima when the Jovian planet cycles, Tjsun, experience perihelion coincidences at &#x3b8;jsun (t &#x3d; t<sub>per</sub>) (<xref ref-type="bibr" rid="B48">Yndestad and Solheim 2017</xref>). The total solar irradiation spectrum, Stsi (Ttsi, (&#x3b8;tsi (t-t<sub>tsi</sub>)), may be computed as a linear spectrum transformation of the JSUN cycle periods into a TSI cycle spectrum by the simplified model:<disp-formula id="e1">
<mml:math id="m1">
<mml:mrow>
<mml:mtext>Stsi</mml:mtext>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mtext>Ttsi</mml:mtext>
<mml:mo>,</mml:mo>
<mml:mi mathvariant="normal">&#x3b8;</mml:mi>
<mml:mtext>tsi</mml:mtext>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mtext>t</mml:mtext>
<mml:mo>&#x2212;</mml:mo>
<mml:msub>
<mml:mtext>t</mml:mtext>
<mml:mrow>
<mml:mtext>tsi</mml:mtext>
</mml:mrow>
</mml:msub>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
<mml:mo>&#x3d;</mml:mo>
<mml:mtext>Hsol</mml:mtext>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mtext>Tsol</mml:mtext>
<mml:mo>,</mml:mo>
<mml:mtext>&#x3b8;sol</mml:mtext>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:msub>
<mml:mtext>t</mml:mtext>
<mml:mrow>
<mml:mtext>sol</mml:mtext>
</mml:mrow>
</mml:msub>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
<mml:mtext>Sjsun</mml:mtext>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mtext>Tjsun</mml:mtext>
<mml:mo>,</mml:mo>
<mml:mi mathvariant="normal">&#x3b8;</mml:mi>
<mml:mtext>jsun</mml:mtext>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mtext>t</mml:mtext>
<mml:mo>&#x2212;</mml:mo>
<mml:msub>
<mml:mtext>t</mml:mtext>
<mml:mrow>
<mml:mtext>per</mml:mtext>
</mml:mrow>
</mml:msub>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
<mml:mo>,</mml:mo>
</mml:mrow>
</mml:math>
<label>(1)</label>
</disp-formula>where Hsol (Tsol, &#x3b8;sol (t<sub>sol</sub>) represents the Sun&#xb4;s transformation of JSUN cycles and phase-relation periods into a TSI spectrum Stsi (Ttsi, &#x3b8;tsi (t-t<sub>tsi</sub>)). In this transformation, the cycle period transform Tsol &#x3d; 1 and the phase lag t<sub>sol</sub> &#x3d; 0 (yr.). The transformed spectrum has cycle periods Ttsi &#x3d; Tsol&#x002A;Tjsun &#x3d; Tjsun, and cycle phase shifts &#x3b8;tsi (t<sub>tsi</sub>) &#x3d; &#x3b8;jsun (t<sub>per</sub>) &#x2b; &#x3b8;sol (t<sub>sol</sub>) &#x3d; &#x3b8;jsun (t<sub>per</sub>). The 4450-year TSI envelope period has phase shifts in the years: Atsi-en(t) &#x3d; ((-0, -1624.49), (max, -512), (&#x2b;0, 600), (min, 1712), (&#x2212;0, 2825)).</p>
</sec>
<sec id="s2-5">
<title>Solar Forced Sea Temperature Oscillations</title>
<p>The solar-forced sea surface temperature (SST) in Earth&#x2019;s oceans is represented by a spectrum Ssst (Tsst, &#x3b8;sst (t-t<sub>sst</sub>)), where Tsst represents the solar-forced SST cycle periods and the phase state, &#x3b8;sst (t<sub>0-sst</sub>), represents the years when Tsst cycle periods have amplitude maxima. The accumulation of TSI forced heat cycle periods in Earth&#x2019;s oceans is expected to have a cycle phase lag of &#x3c0;/2 (rad), or Ttsi/4, from the Sun&#xb4;s JSUN cycle periods. The solar forced sea temperature spectrum is computed by the simplified model:<disp-formula id="e2">
<mml:math id="m2">
<mml:mrow>
<mml:mtext>Ssst</mml:mtext>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mtext>Tsst</mml:mtext>
<mml:mo>,</mml:mo>
<mml:mtext>&#x3b8;sst</mml:mtext>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mtext>t</mml:mtext>
<mml:mo>&#x2212;</mml:mo>
<mml:msub>
<mml:mtext>t</mml:mtext>
<mml:mrow>
<mml:mtext>sst</mml:mtext>
</mml:mrow>
</mml:msub>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
<mml:mo>&#x3d;</mml:mo>
<mml:mtext>Hsea</mml:mtext>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mtext>Tsea</mml:mtext>
<mml:mo>,</mml:mo>
<mml:mi mathvariant="normal">&#x3b8;</mml:mi>
<mml:mtext>sea</mml:mtext>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:msub>
<mml:mtext>t</mml:mtext>
<mml:mrow>
<mml:mtext>sea</mml:mtext>
</mml:mrow>
</mml:msub>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
<mml:mtext>Stsi</mml:mtext>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mtext>Ttso</mml:mtext>
<mml:mo>,</mml:mo>
<mml:mi mathvariant="normal">&#x3b8;</mml:mi>
<mml:mtext>tsi</mml:mtext>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mtext>t</mml:mtext>
<mml:mo>&#x2212;</mml:mo>
<mml:msub>
<mml:mtext>t</mml:mtext>
<mml:mrow>
<mml:mtext>tsi</mml:mtext>
</mml:mrow>
</mml:msub>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
<mml:mo>,</mml:mo>
</mml:mrow>
</mml:math>
<label>(2)</label>
</disp-formula>where Hsea (Tsea, &#x3b8;sea (t<sub>sea</sub>) represents the sea surface transformation of TSI cycles and phase-relation periods into an SST spectrum Ssst (Tsst, &#x3b8;sst (t-t<sub>sst</sub>)), where Tsol &#x3d; 1 and t<sub>sea</sub> &#x3d; Tjsun/4. The transformed spectrum has cycle periods Tsst &#x3d; Tsol<sup>&#x2217;</sup>Ttsi &#x3d; Tsol&#x002A;Tjsun &#x3d; Tjsun, and cycle phase shifts &#x3b8;sst (t<sub>sst</sub>) &#x3d; &#x3b8;jsun (t<sub>tsi</sub> &#x2b; t<sub>sea</sub>) &#x3d; &#x3b8;jsun (t<sub>per</sub> &#x2b; Tjsun/4). The new 4450-year SST envelope period has phase shifts in the years: Asst-en(t) &#x3d; ((min, -1624.49), (-0, -512), (max, 600), (-0, 1712), (min, 2825)). Solar-forced SST variations have a maximum speed in the negative direction when solar-forced irradiation has a minimum in 1712.</p>
</sec>
<sec id="s2-6">
<title>Lunar Forced Sea Temperature Oscillations</title>
<p>The Earth axis tilt (obliquity of the ecliptic) is approximately 23&#xb0;27&#x2032;. Mutual gravity among the Earth-Moon-Sun oscillations introduces a nutation in Earth&#x2019;s axial tilt and precession. The Earth nutation has amplitude variations of approximately 9.2&#xa0;s of arc in a cycle period of 18.6134&#xa0;years. The amplitude variation influences the cross-point between the Moon&#x2019;s plane cycle and the ecliptic plane to the Sun in a lunar nodal cycle of Tln &#x3d; 18.61&#xa0;years. The Earth&#x2019;s axis nutation spectrum, Sln (Tln, &#x3b8;ln (t-t<sub>ln</sub>)), has harmonic periods Tln &#x3d; (1, 2, 3, 4, &#x2026; )18.61 (yr.) and reached a major standstill maximum in the year t<sub>ln</sub> &#x3d; 1932.3. The nutation spectrum, Sln (Tln, &#x3b8;ln (t-t<sub>ln</sub>)), introduces a global lunar nodal tide spectrum, Slnt (Tlnt, &#x3b8;lnt (t-t<sub>lnt</sub>)), as a standing wave in oceans. The global lunar nodal tide introduces vertical mixing and lunar forced sea surface temperature (LST) variations. The lunar forced sea temperature spectrum is computed by the simplified model:<disp-formula id="e3">
<mml:math id="m3">
<mml:mrow>
<mml:mtext>Slst</mml:mtext>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mtext>Tlst</mml:mtext>
<mml:mo>,</mml:mo>
<mml:mi mathvariant="normal">&#x3b8;</mml:mi>
<mml:mtext>lst</mml:mtext>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mtext>t</mml:mtext>
<mml:mo>&#x2212;</mml:mo>
<mml:msub>
<mml:mtext>t</mml:mtext>
<mml:mrow>
<mml:mtext>lst</mml:mtext>
</mml:mrow>
</mml:msub>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
<mml:mo>&#x3d;</mml:mo>
<mml:mtext>Hoce</mml:mtext>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mtext>Toce</mml:mtext>
<mml:mo>,</mml:mo>
<mml:mi mathvariant="normal">&#x3b8;</mml:mi>
<mml:mtext>osc</mml:mtext>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:msub>
<mml:mtext>t</mml:mtext>
<mml:mrow>
<mml:mtext>oce</mml:mtext>
</mml:mrow>
</mml:msub>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
<mml:mtext>S</mml:mtext>
<mml:mi>ln</mml:mi>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mtext>T</mml:mtext>
<mml:mi>ln</mml:mi>
<mml:mo>,</mml:mo>
<mml:mi mathvariant="normal">&#x3b8;</mml:mi>
<mml:mo>&#x2061;</mml:mo>
<mml:mi>ln</mml:mi>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mtext>t</mml:mtext>
<mml:mo>&#x2212;</mml:mo>
<mml:msub>
<mml:mtext>t</mml:mtext>
<mml:mrow>
<mml:mtext>In</mml:mtext>
</mml:mrow>
</mml:msub>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
<mml:mo>,</mml:mo>
</mml:mrow>
</mml:math>
<label>(3)</label>
</disp-formula>where Hoce(Tose, &#x3b8;oce (t<sub>oce</sub>) represents a transformation of Earth&#x2019;s axis nutation cycles and cycle phase relations into a lunar forced sea surface spectrum Slst (Tlst, &#x3b8;lst (t-t<sub>lst</sub>)), where Tose &#x3d; 1 and t<sub>oce</sub> represents the phase lag in oceans. The transformed spectrum has cycle periods of Tlst &#x3d; Tose&#x2a;Tln &#x3d; Tln. The phase lag t<sub>lst</sub> &#x3d; t<sub>ln</sub> - t<sub>ose</sub> is period dependent and position dependent and must be estimated.</p>
</sec>
<sec id="s2-7">
<title>Solar-Lunar-Forced Temperature Oscillations on Earth</title>
<p>The effect of Jovian planets and lunar nodal cycles on the Earth&#x2019;s climate variation may be represented as a sum of solar lunar forced temperature variations by the simplified model:<disp-formula id="e4">
<mml:math id="m4">
<mml:mrow>
<mml:mtext>Sslt</mml:mtext>
<mml:mo>&#x3d;</mml:mo>
<mml:mtext>Stsi</mml:mtext>
<mml:mo>&#x2b;</mml:mo>
<mml:mtext>Ssst</mml:mtext>
<mml:mo>&#x2b;</mml:mo>
<mml:mtext>Slst</mml:mtext>
<mml:mo>&#x2b;</mml:mo>
<mml:mtext>Serr</mml:mtext>
<mml:mo>,</mml:mo>
</mml:mrow>
</mml:math>
<label>(4)</label>
</disp-formula>where Serr represents a spectrum from an unknown source. The direct solar-forced TSI spectrum, Stsi, the solar-forced sea surface temperature spectrum, Ssst, and the lunar-forced spectrum, Slst, have known cycle periods and cycle phase relations <xref ref-type="disp-formula" rid="e2">Eqs. 2</xref>, <xref ref-type="disp-formula" rid="e3">3</xref>. The total solar-lunar-forced amplitude variations, Aslt(t) &#x3d; Atsi(t) &#x2b; Asst(t) &#x2b; Alst(t) &#x2b; Aerr(t), are controlled by constructive and destructive interference between cycle periods and the cycle phase relations.</p>
</sec>
</sec>
<sec sec-type="materials" id="s3">
<title>Materials</title>
<p>This study uses the HadCRUT4 time series, which covers the interval from 1850 to 2020, as a representative proxy of Earth&#x2019;s global mean temperature. These time series are based on sea surface and land-air temperature estimates (<xref ref-type="bibr" rid="B27">Morice et al., 2012</xref>). The sea surface temperature time series (HadSST3) consists of anomalies on a 5&#xb0;-by-5&#xb0; global grid, while the land-air temperature time series (CRUTEM4) consists of anomalies on a 5&#xb0;-by-5&#xb0; grid and is supported by the Climatic Research Unit (<ext-link ext-link-type="uri" xlink:href="http://www.metoffice.gov.uk/hadobs/hadcrut4/">http://www.metoffice.gov.uk/hadobs/hadcrut4/</ext-link>). The Greenland temperatures are represented by the GISP2 time series covering the time periods from 1000 A.D. to 1993 A.D. and from 2000 B.C. to 1993 A.D.; these time series were estimated from nitrogen and argon isotope data extracted from air bubbles in Greenland ice cores at 72&#xb0;36&#x2019;N, 38&#xb0;30&#x2019;W, 3203&#xa0;m above sea level. These series are supported by the World Data Center for Paleoclimatology in Boulder, Colorado, United States, and the NOAA Paleoclimatology Program (<ext-link ext-link-type="uri" xlink:href="https://www.ncdc.noaa.gov/data-access/paleoclimatology-data">https://www.ncdc.noaa.gov/data-access/paleoclimatology-data</ext-link>) (<xref ref-type="bibr" rid="B17">Kobashi et al., 2011</xref>).</p>
</sec>
<sec sec-type="methods" id="s4">
<title>Methods</title>
<p>Cycle periods and cycle phase relations in Earth&#x2019;s temperature variation are identified in the wavelet spectra of Earth&#x2019;s temperature time series by the wavelet transform:<disp-formula id="e5">
<mml:math id="m5">
<mml:mrow>
<mml:msub>
<mml:mi>W</mml:mi>
<mml:mrow>
<mml:mi>a</mml:mi>
<mml:mo>,</mml:mo>
<mml:mi>b</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mi>t</mml:mi>
<mml:mo>)</mml:mo>
</mml:mrow>
<mml:mo>&#x3d;</mml:mo>
<mml:mfrac>
<mml:mn>1</mml:mn>
<mml:mrow>
<mml:mroot>
<mml:mi>a</mml:mi>
<mml:mo>&#xa0;</mml:mo>
</mml:mroot>
</mml:mrow>
</mml:mfrac>
<mml:mstyle displaystyle="true">
<mml:mrow>
<mml:munder>
<mml:mo>&#x222b;</mml:mo>
<mml:mi>R</mml:mi>
</mml:munder>
<mml:mrow>
<mml:mi>x</mml:mi>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mi>t</mml:mi>
<mml:mo>)</mml:mo>
</mml:mrow>
<mml:mtext>&#x3a8;</mml:mtext>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mfrac>
<mml:mrow>
<mml:mi>t</mml:mi>
<mml:mo>&#x2212;</mml:mo>
<mml:mi>b</mml:mi>
</mml:mrow>
<mml:mi>a</mml:mi>
</mml:mfrac>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
<mml:mi>d</mml:mi>
<mml:mi>t</mml:mi>
</mml:mrow>
</mml:mrow>
</mml:mstyle>
</mml:mrow>
</mml:math>
<label>(5)</label>
</disp-formula>where x(t) is the analyzed temperature time series after being transformed to a zero mean value and scaled by variance. &#x3a8;() is a coif3 wavelet impulse function. <inline-formula id="inf1">
<mml:math id="m6">
<mml:mrow>
<mml:msub>
<mml:mi>W</mml:mi>
<mml:mrow>
<mml:mi>a</mml:mi>
<mml:mo>,</mml:mo>
<mml:mi>b</mml:mi>
</mml:mrow>
</mml:msub>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mi>t</mml:mi>
<mml:mo>)</mml:mo>
</mml:mrow>
</mml:mrow>
</mml:math>
</inline-formula> is a set of wavelet cycles, b is the translation in time, and a is the time-scaling parameter in the wavelet transformation (<xref ref-type="bibr" rid="B7">Daubechies 1992</xref>; <xref ref-type="bibr" rid="B25">MATLAB, 2020</xref>). In this analysis, the time translation b &#x3d; 0, and the computed wavelet transformation, <inline-formula id="inf2">
<mml:math id="m7">
<mml:mrow>
<mml:msub>
<mml:mi>W</mml:mi>
<mml:mi>a</mml:mi>
</mml:msub>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mi>t</mml:mi>
<mml:mo>)</mml:mo>
</mml:mrow>
</mml:mrow>
</mml:math>
</inline-formula>, a moving correlation between x(t) and the impulse function &#x3a8;() over the entire time-series x(t). The moving correlated wavelets, s(t), are collected into a wavelet spectrum, W (s, t), for t &#x3d; (first &#x2026; last) (yr.) and s &#x3d; (1 &#x2026; (last-first)/2) (yr.). A wavelet power spectrum can be defined as:<disp-formula id="e6">
<mml:math id="m8">
<mml:mrow>
<mml:mi>W</mml:mi>
<mml:mi>P</mml:mi>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mi>s</mml:mi>
<mml:mo>,</mml:mo>
<mml:mo>&#xa0;</mml:mo>
<mml:mi>t</mml:mi>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
<mml:mo>&#x3d;</mml:mo>
<mml:msup>
<mml:mrow>
<mml:mrow>
<mml:mo>[</mml:mo>
<mml:mrow>
<mml:mi>W</mml:mi>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mi>s</mml:mi>
<mml:mo>,</mml:mo>
<mml:mi>t</mml:mi>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
</mml:mrow>
<mml:mo>]</mml:mo>
</mml:mrow>
</mml:mrow>
<mml:mn>2</mml:mn>
</mml:msup>
</mml:mrow>
</mml:math>
<label>(6)</label>
</disp-formula>
</p>
<p>In this study, the wavelet power spectrum (<xref ref-type="bibr" rid="B39">Torrence and Compo 1998</xref>) estimates the most dominant wavelet amplitude variations. Stationary cycles in the wavelet spectrum, W (s, t), coincide with stationary cycles, T, in the Earth&#x2019;s temperature spectrum Sest.</p>
<sec id="s4-1">
<title>Stationary Cycle Periods</title>
<p>Stationary cycles, T, in the Earth&#x2019;s temperature variability spectrum, Sest(t), are identified by computing the autocorrelation of the wavelet specter W (s, t), as follows:<disp-formula id="e7">
<mml:math id="m9">
<mml:mrow>
<mml:mtext>W</mml:mtext>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mtext>R</mml:mtext>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mtext>s</mml:mtext>
<mml:mo>)</mml:mo>
</mml:mrow>
<mml:mo>,</mml:mo>
<mml:mtext>m</mml:mtext>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
<mml:mo>&#x3d;</mml:mo>
<mml:mtext>E</mml:mtext>
<mml:mrow>
<mml:mo>[</mml:mo>
<mml:mrow>
<mml:mtext>W</mml:mtext>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mtext>s</mml:mtext>
<mml:mo>,</mml:mo>
<mml:mtext>t</mml:mtext>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
<mml:mtext>W</mml:mtext>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mtext>s</mml:mtext>
<mml:mo>,</mml:mo>
<mml:mtext>t</mml:mtext>
<mml:mo>&#x2b;</mml:mo>
<mml:mtext>m</mml:mtext>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
</mml:mrow>
<mml:mo>]</mml:mo>
</mml:mrow>
<mml:mo>,</mml:mo>
</mml:mrow>
</mml:math>
<label>(7)</label>
</disp-formula>where WR (R, T) represents a set of maximum correlations R &#x3d; (max 1 &#x2026; max n) to the stationary cycles T &#x3d; (T1 &#x2026; Tn) (yr.).</p>
</sec>
<sec id="s4-2">
<title>Source of Stationary Cycles</title>
<p>The effects of Jovian planets and lunar nodal cycles on the Earth&#x2019;s climate variability are identified by computing the coincidence differences between the estimated spectrum, (S (T, &#x3b8;(t<sub>0</sub>)), from Earth temperature data series and the deterministic solar-lunar forced spectra Stsi (Ttsi, &#x3b8;tsi (t<sub>0-tsi</sub>)), Ssst (Tsst, &#x3b8;sst (t<sub>0-sst</sub>)) and Slnt (lnt, &#x3b8;lnt (t<sub>0-lnt</sub>)).</p>
</sec>
</sec>
<sec sec-type="results" id="s5">
<title>Results</title>
<sec id="s5-1">
<title>Total Solar Irradiation Oscillations</title>
<p>The total solar irradiation spectrum, Stsi (Ttsi, (&#x3b8;tsi (t-t<sub>tsi</sub>))), may be computed as a linear spectrum transformation of the JSUN cycle periods into a TSI cycle spectrum <xref ref-type="disp-formula" rid="e1">Eq. 1</xref>. The transformed spectrum TSI spectrum has the computed amplitude variations:<disp-formula id="e8">
<mml:math id="m10">
<mml:mrow>
<mml:mtext>Atsi</mml:mtext>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mtext>jsun</mml:mtext>
<mml:mo>,</mml:mo>
<mml:mtext>t</mml:mtext>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
<mml:mo>&#x3d;</mml:mo>
<mml:msup>
<mml:mtext>Ktsi</mml:mtext>
<mml:mo>&#x2217;</mml:mo>
</mml:msup>
<mml:mi>cos</mml:mi>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mrow>
<mml:mrow>
<mml:mn>2</mml:mn>
<mml:mo>&#x3c0;</mml:mo>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mtext>t</mml:mtext>
<mml:mo>&#x2212;</mml:mo>
<mml:msub>
<mml:mtext>t</mml:mtext>
<mml:mrow>
<mml:mtext>tsi</mml:mtext>
</mml:mrow>
</mml:msub>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
</mml:mrow>
<mml:mo>/</mml:mo>
<mml:mrow>
<mml:mtext>Ttsi</mml:mtext>
</mml:mrow>
</mml:mrow>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
<mml:mo>,</mml:mo>
</mml:mrow>
</mml:math>
<label>(8)</label>
</disp-formula>where Atsi(jsun, t) &#x3d; (Atsi(ju, t), Atsi(sa, t), Atsi(ur, t), and Atsi(ne, t)) represent TSI amplitude variations from JSUN cycles and the transformed cycle periods Ttsi &#x3d; Tjsun. TSI cycles have minima when JSUN periods have perihelion phase coincidences for t<sub>tsi</sub> &#x3d; t<sub>per</sub> and Kjsun &#x3d; (Kju, Ksa, Kur, Kne) &#x3d; (&#x2212;1, &#x2212;1, &#x2212;1, &#x2212;1). Total amplitude variations are represented by the TSI index Atsi(t) &#x3d; (Atsi(ju, t) &#x2b; Atsi(sa, t) &#x2b; Atsi(ur, t) &#x2b; Atsi(ne, t)). Atsi(t) has a maximum in 512 B.C. and a minimum in 1712 A.D. The 4450-year TSI envelope period, Atsi-en(t), has phase shifts in the years: Atsi-en(t) &#x3d; ((&#x2212;0, &#x2212;1624.49), (max, &#x2212;512), (&#x2b;0, 600), (min, 1712), (&#x2212;0, 2825)).</p>
<p>The temporary Uranus and Neptune (UN) period coincidences in the envelope period cause temporary TSI minima and maxima. UN cycle periods have the following period coincidences: Tun-co &#x3d; [(2Tur, Tne), (4Tur, 2Tne), (6Tur, 3Tne), (12Tur, 6Tne), (23Tur, 12Tne), (29Tur, 15Tne), (51Tur, 26Tne), (53Tur, 27Tne)] (yr.), with mean period coincidences of Tun-mco &#x3d; [166.42, 332.83, 499.70, 998.49, 1954.97, 2454.22, 4284.78, 4451.20] (yr.). <xref ref-type="fig" rid="F1">Figure 1</xref> shows the computed <xref ref-type="disp-formula" rid="e8">Eq. 8</xref> amplitude variations, Atsi(un, t) &#x3d; Atsi(ur, t) &#x2b; Atsi(ne, t), for the years&#xa0;t &#x3d; (&#x2212;2000, &#x2026; 3000). From 1000 to 3000 A.D. TSI index values, Atsi(nu, t) &#x3c; &#x2212;1.90, have a minimum at Atsi(un, t) &#x3d; ((&#x2212;1.97, 1212), (&#x2212;1.98, 1379), (&#x2212;1.99, 1546), (&#x2212;2.00, 1713), (&#x2212;1.98, 1882), (&#x2212;1.95, 2049), (&#x2212;1.92, 2216)). &#x201c;The Little Ice Age&#x201d; covers five deep minima from 1379 to 2049 and an upcoming computed minimum in 2216.</p>
<fig id="F1" position="float">
<label>FIGURE 1</label>
<caption>
<p>Constructive and destructive interference between Uranus-Neptune forced TSI index values, Atsi(un, t) &#x3d; Atsi(ur, t) &#x2b; Atsi(ne, t), for the years&#xa0;t &#x3d; (&#x2212;2000 &#x2026; 3000). &#x201c;The Little Ice Age&#x201d; covers the six deepest Uranus-Neptune minima coincidences.</p>
</caption>
<graphic xlink:href="fspas-09-839794-g001.tif"/>
</fig>
<p>Saturn, Uranus, and Neptune (SUN) cycle periods (Tsa, Tur, Tun) have mean coincidences with the cycle periods: Tsun-mco &#x3d; (169.84, 499.70, 999.39, 1960.96, 2450.84, 4289.61 4449.63) (yr.). From 1000 to 3000 A.D., the TSI index, Atsi(t) &#x3d; (Atsi(sa, t) &#x2b; Atsi(ur, t) &#x2b; Atsi(ne, t)), experienced computed <xref ref-type="disp-formula" rid="e8">Eq. 8</xref> deep minima: (Atsi(t) &#x3c; &#x2212;2.8 for Atsi(t) &#x3d; ((&#x2212;2.90, 1210), (&#x2212;2.87, 1385), (&#x2212;2.92, 1710), (&#x2212;2.92, 1885), (&#x2212;2.79, 2211)).</p>
</sec>
<sec id="s5-2">
<title>Deep Solar Minima Coincidences</title>
<p>Real solar data from 1000 A.D. (<xref ref-type="bibr" rid="B40">Usoskin 2005</xref>) onward yield the following classified deep solar minima: (Oort (1010&#x2013;1070), Wolf (1270&#x2013;1340), Sp&#xf6;rer (1390&#x2013;1550), Maunder (1640&#x2013;1720), and Dalton (1790&#x2013;1820)). The ACRIM TSI time series from 1000 A.D. has estimated deep minima at Oort (1013&#x2013;1074), Wolf (1263&#x2013;1326), Sp&#xf6;rer (1510&#x2013;1571), Maunder (1636&#x2013;1706), Dalton (1773&#x2013;1833), and Next (2002&#x2013;2063) (<xref ref-type="bibr" rid="B41">Velasco et al., 2015</xref>). Solar variations are related to destructive and constructive interference between the SUN cycles.</p>
<p>Solar minima are correlated with a negative constructive interference when SUN cycles have amplitude minima <xref ref-type="disp-formula" rid="e8">Eq. 8</xref>. Oort (UN min, for t &#x3d; 1020&#x2013;1070), Wolf 1 (SUN min, for t &#x3d; 1197&#x2013;1294), Wolf 2 (SUN min, for t &#x3d; 1350&#x2013;1398), Sp&#xf6;rer (UN min, for t &#x3d; 1523&#x2013;1571), Maunder (SUN min, for t &#x3d; 1696&#x2013;1744), Dalton (SU min, for t &#x3d; 1791&#x2013;1804), Modern (SUN min, for t &#x3d; 1850&#x2013;1899), Next (UN min, for t &#x3d; 2024&#x2013;2072), Next deep (SUN min, for t &#x3d; 2197&#x2013;2245). Wolf, Sp&#xf6;rer and Maunder have the SUN cycle constructive negative interference, while Oort and Next have the UN cycle constructive negative interference. Dalton has SU cycle constructive negative interference. SUN cycles have positive constructive interference in the modern warm time period of 1981&#x2013;2024.</p>
</sec>
<sec id="s5-3">
<title>Solar Forced Sea Temperature Oscillations</title>
<p>The accumulation of heat in oceans transforms the solar forced spectrum Stsi <xref ref-type="disp-formula" rid="e1">Eq. 1</xref> into a solar-forced sea surface temperature (SST) spectrum Ssst <xref ref-type="disp-formula" rid="e2">Eq. 2</xref>. The solar-forced sea surface amplitude variations are computed using the following simplified sea surface temperature model:<disp-formula id="e9">
<mml:math id="m11">
<mml:mrow>
<mml:mtext>Asst</mml:mtext>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mtext>jsun</mml:mtext>
<mml:mo>,</mml:mo>
<mml:mtext>t</mml:mtext>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
<mml:mo>&#x3d;</mml:mo>
<mml:msup>
<mml:mtext>Ksst</mml:mtext>
<mml:mo>&#x2217;</mml:mo>
</mml:msup>
<mml:mi>cos</mml:mi>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mrow>
<mml:mrow>
<mml:mn>2</mml:mn>
<mml:mo>&#x3c0;</mml:mo>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mtext>t</mml:mtext>
<mml:mo>&#x2010;</mml:mo>
<mml:msub>
<mml:mtext>t</mml:mtext>
<mml:mrow>
<mml:mtext>sst</mml:mtext>
</mml:mrow>
</mml:msub>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
</mml:mrow>
<mml:mo>/</mml:mo>
<mml:mrow>
<mml:mtext>Tsst</mml:mtext>
</mml:mrow>
</mml:mrow>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
<mml:mo>,</mml:mo>
</mml:mrow>
</mml:math>
<label>(9)</label>
</disp-formula>where Asst (jsun, t) &#x3d; (Asst (ju, t), Asst (sa, t), Asst (ur, t), and Asst (ne, t)) represent solar-forced sea surface temperature amplitude variations. Ksst &#x3d; (Kju, Ksa, Kur, Kne) &#x3d; (&#x2212;1, &#x2212;1, &#x2212;1, &#x2212;1). The cycle periods Tsst &#x3d; Ttsi, where Ttsi &#x3d; Tjsun. The cycle phase reference t<sub>sst</sub> &#x3d; t<sub>tsi</sub> - Tjsun/4. The SST amplitude index Asst(t) &#x3d; (Asst (ju, t) &#x2b; Asst (sa, t) &#x2b; Asst (ur, t) &#x2b; Asst (ne, t)) covers an envelope period controlled by constructive and destructive interference between Tsst cycle periods.</p>
<p>The SST index, Asst(t), has a maximum in year 600 and a minimum in 2825 A.D. The new 4450-year SST envelope period has phase shifts in the years: Asst-en(t) &#x3d; ((min, &#x2212;1624.49), (-0, &#x2212;512), (max, 600), (&#x2212;0, 1712), (min, 2825)). From t &#x3d; 1000 &#x2026; 3000. the SST index <xref ref-type="disp-formula" rid="e9">Eq. 9</xref>, Asst(t) &#x3d; (Asst (sa, t) &#x2b; Asst (ur, t) &#x2b; Asst (ne, t), experienced sea temperature deep minima: (Asst(t) &#x3d; &#x3c; &#x2212;2.3, for Asst(t) &#x3d; ((&#x2212;2,48, 1069), (&#x2212;2.39, 1244), (&#x2212;2.73, 1375), (&#x2212;2.73, 1570), (&#x2212;2.70, 1745), (&#x2212;2.37, 1896), (&#x2212;2.88, 2070), (&#x2212;2.88, 2246)), and SST index maxima at (Asst(t) &#x3e; 2.4, for Asst(t) &#x3d; ((2.86, 1024), (2.76, 1379), (2.75, 1525), (2.47, 1850), (2.53, 2025)). From t &#x3d; 1850 &#x2026; 2100, the SST index <xref ref-type="disp-formula" rid="e9">Eq. 9</xref> experienced the following minima and maxima: Asst(t) &#x3d; ((1.35, 1875), (&#x2212;2.37, 1896), (&#x2212;2.19, 1921), (&#x2212;1.14, 1981), (2.53, 2025), (&#x2212;2.88, 2070)).</p>
<p>The modern SST index maximum Asst(t) &#x3d; (2.53, 2025) is a 500-year event after the maximum Asst(t) &#x3d; (2.75, 1525) and a 1000-year event from the SST index maximum Asst(t) &#x3d; (2.86, 1024). The SST index deep minimum at Asst(t) &#x3d; (-2.88, 2070) is the deepest SST index minimum since 1375 B.C. The amplitude shift from a 500-year Asst(t) maximum to a 3000-year Asst(t) minimum in only 45&#xa0;years is caused by SUN cycle period phase shifts from constructive positive interference to constructive negative interference.</p>
</sec>
</sec>
<sec id="s6">
<title>Lunar Forced Sea Temperature Oscillations</title>
<sec id="s6-1">
<title>Earth Nutation Oscillations</title>
<p>There is a chain of events from the Earth&#xb4;s axis nutation oscillations to lunar forced sea surface temperature (LST) oscillations. The Earth&#x2019;s axis nutation spectrum, Sln (Tln, &#x3b8;ln (t-t<sub>ln</sub>)), has a harmonic period spectrum Tln &#x3d; (1, 2, 3, 4, &#x2026; )18.61 (yr.). The dominant 18.61-year cycle reached a major standstill maximum at the year t<sub>ln</sub> &#x3d; 1932.3 and a minimum at the year t<sub>ln</sub> &#x3d; 1932.3 &#x2b; 18.61/2 &#x3d; 1941.6. A wavelet spectrum analysis of Earth&#xb4;s position in the y-direction identified the harmonic Earth nutation cycle period spectrum Tln &#x3d; (1/15, 1/3, 1, 4)18.61 &#x3d; (1.24, 6.31, 18.61, 74.42) (yr.) from 1845 to 2000 A.D. The unstable 1.24-year cycle is known as the Chandler cycle. The dominant cycles Tln &#x3d; (18.61, 74.44) (yr.) have estimated maxima in the years t<sub>ln</sub> &#x3d; (1943, 1979) and minima in the years (1933, 1942) (<xref ref-type="bibr" rid="B49">Yndestad 2004</xref>).</p>
</sec>
<sec id="s6-2">
<title>Lunar Nodal Tide Oscillations</title>
<p>The nutation spectrum, Sln (Tln, &#x3b8;ln (t-t<sub>ln</sub>)), introduces a global lunar nodal tide spectrum, Slnt (Tlnt, &#x3b8;lnt (t-t<sub>lnt</sub>)), as a standing wave between the pole and Equator. The vertical component follows the Earth nutation amplitude variations. The horizontal component influences the tidal current, which has maximum and minimum amplitudes at approximately 30&#xb0; from the equator. The horizontal tide current has a phase lag of approximately &#x3c0;/2 (rad). A wavelet spectrum analysis of the annual Aberdeen Sea level in North Atlantic water identified the lunar spectrum of Tlnt &#x3d; (1/2, 1, 4)18.61 &#x3d; (9.31, 18.61, 74.44) (yr.) in vertical amplitude variations. The estimated lunar nodal tide periods (18.61, 74.44) have minima in (1942, 1963) (<xref ref-type="bibr" rid="B49">Yndestad, 2006</xref>).</p>
</sec>
<sec id="s6-3">
<title>North Atlantic Water Oscillations</title>
<p>The stationary 18.61-year vertical and horizontal tide introduces a mix of warm surface sea temperatures with cold bottom temperatures; thus, heat is redistributed as a Tlnt &#x3d; 18.6-year sea surface temperature cycle throughout the large-scale oceanic thermohaline system. A wavelet spectrum time-series analysis of the North Atlantic water temperature anomaly on the Scottish side of the Faroe-Shetland Channel from 1900 to 2005 revealed dominant periods of approximately (9, 18, 27, 36, 55, 75) years and indicated a strong harmonic cycle of approximately 9 years. The temperature cycle periods coincide with the lunar forced sea temperature period spectrum Tlst &#x3d; (1/2, 2/2, 3/2, 4/2, 6/2, 8/2)18.61 years. The dominant periods (9, 18, 74) have maxima in (1940, 1942, 1943) (<xref ref-type="bibr" rid="B49">Yndestad, 2006</xref>).</p>
</sec>
<sec id="s6-4">
<title>Lunar Forced Sea Surface Amplitude Variations</title>
<p>Lunar forced sea surface temperature (LST) variations are represented as a transformation <xref ref-type="disp-formula" rid="e3">Eq. 3</xref> of the Earth&#x2019;s nodal spectrum, Tln, into a lunar forced sea surface temperature spectrum Slst (Alst(t), Tlst, Flst(t)). LST amplitude variations are computed using the following simplified sea surface temperature model:<disp-formula id="e10">
<mml:math id="m12">
<mml:mrow>
<mml:mtext>Alst</mml:mtext>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mtext>t</mml:mtext>
<mml:mo>)</mml:mo>
</mml:mrow>
<mml:mo>&#x3d;</mml:mo>
<mml:mi>cos</mml:mi>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mrow>
<mml:mrow>
<mml:mn>2</mml:mn>
<mml:mo>&#x3c0;</mml:mo>
<mml:mrow>
<mml:mo>(</mml:mo>
<mml:mrow>
<mml:mtext>t</mml:mtext>
<mml:mo>&#x2212;</mml:mo>
<mml:msub>
<mml:mtext>t</mml:mtext>
<mml:mrow>
<mml:mtext>lst</mml:mtext>
</mml:mrow>
</mml:msub>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
</mml:mrow>
<mml:mo>/</mml:mo>
<mml:mrow>
<mml:mtext>Tlst</mml:mtext>
</mml:mrow>
</mml:mrow>
</mml:mrow>
<mml:mo>)</mml:mo>
</mml:mrow>
<mml:mo>,</mml:mo>
</mml:mrow>
</mml:math>
<label>(10)</label>
</disp-formula>where the temperature variations are Alst(t) &#x3d; (Alst (1, t), Alst (2, t), Alst (3, t)...). The cycle periods represent a harmonic spectrum: Tlst &#x3d; (1/2, 2/2, 3/2, 4/2 &#x2026; )18.61 &#x3d; (9.31, 18.61, 27.92, 37.22, &#x2026; ) (yr.). The lunar forced sea surface temperature cycle periods Tlst &#x3d; (9.31, 18.61, 74.44) (yr.) has estimated maxima at the years t<sub>lst</sub> &#x3d; (1940, 1942, 1943) and minima in the years (1949, 1933, 1980). The 18.61-year cycle coincides with the Earth nutation in the y-direction, and the 74.44-year cycle period has a reversed-phase. (<xref ref-type="bibr" rid="B49">Yndestad, 2006</xref>).</p>
</sec>
<sec id="s6-5">
<title>Solar Lunar Cycle Coincidences</title>
<p>The solar-lunar-forced sea surface temperature spectrum, Sslt &#x3d; Ssst &#x2b; Slst, has amplitude variations, Aslt(t), controlled by cycle period coincidences and cycle phase coincidences. Sola forced cycle periods, Tsst, and lunar forced cycle period, Tln, have coincidences of ((Tsa, 3Tln/2), (Tur, 9Tln/2), (2Tsa, 6Tln/2), (Tne, 18Tln/2)) &#x3d; ((29.44, 27.92), (58.88, 55.83), (84.02, 83.76), (164.79, 167.52)) (yr.).</p>
<p>Solar forced sea temperature amplitude variations, Asst(t), <xref ref-type="disp-formula" rid="e9">Eq. 9</xref> has minima and maxima at Asst(t) &#x3d; ((min, 1890), (max, 2025), (min, 2070). Lunar forced amplitude variations, Alst(t), <xref ref-type="disp-formula" rid="e10">Eq. 10</xref> has minima and maxima at Alst(t) &#x3d; ((min, 1905), (max, 2017), (min, 2079), (min, 2054). The solar-lunar-forced temperature variations have a negative constructive interference from Asst(t) &#x3d; (min, 1890) to Alst(t) &#x3d; (min, 1905), constructive positive interference from Alst(t) &#x3d; (max, 2017) to Asst(t) &#x3d; (max, 2025), and negative constructive interference from Asst(t) &#x3d; (min, 2070) to Alst(t) &#x3d; (min, 2079).</p>
<p>The solar forced spectrum, Tsst, and the lunar forced spectrum have different properties. The solar forced spectrum, Tsst, is a coincidence spectrum of JSUN cycle periods. The lunar forced spectrum Tlst is a harmonic spectrum from the 18.61-year lunar cycle. The phase relation between solar forced cycle periods and lunar cycle periods is a time-variant process, which is never repeated. This means that global temperature variations, controlled by constructive and destructive interference between solar-forced and lunar-forced sea temperature variations, are time-variant coincidences, which are never repeated. Solar forced temperature variations and lunar forced temperature variations must therefore be estimated as single events. The single events may still be deterministic because JSUN cycles and lunar nodal cycles have deterministic cycle periods and phase relations.</p>
</sec>
</sec>
<sec id="s7">
<title>Earth Temperature Oscillations From 1850 A.D.</title>
<p>The Earth&#x2019;s global mean temperature increased by approximately 1.0&#xb0;C from 1850 to 2020. The temperature underwent a cold time period from 1850 to 1920, increased from 1920 to 1940, cooled from 1940 to 1978 and then increased again from 1978 to 2020 (<xref ref-type="fig" rid="F2">Figure 2</xref>). <xref ref-type="fig" rid="F2">Figure 2</xref> illustrates the close relation between the Earth&#x2019;s global mean temperature and the global sea surface temperature since 1850. The sea surface temperature exhibits a pattern similar to that of the global mean temperature. The global land surface temperature time series reveals a different trend, exhibiting a cycle with temperatures colder than the global temperature from 1850 to 1910 and a cycle with temperatures warmer than the global temperature from 1980 to 2015, indicating that heat accumulates in the sea. Wavelet analyses show correlations among global temperature, solar variation, lunar forcing, and a yet unidentified source. Thus, Earth&#x2019;s temperature variability spectrum may have a solar-forced temperature spectrum, a lunar-forced temperature spectrum or a spectrum from an unknown source Sert(t).</p>
<fig id="F2" position="float">
<label>FIGURE 2</label>
<caption>
<p>Earth&#x2019;s global mean temperature, (GMT), (HadCRUT4), global sea surface mean temperature, (GST), (HadSST3) and global land surface mean temperature, (GLT), (CRUTEM4) from 1850 to 2020 (Climate Research Unit).</p>
</caption>
<graphic xlink:href="fspas-09-839794-g002.tif"/>
</fig>
<sec id="s7-1">
<title>Global Sea Surface Temperature Oscillations</title>
<p>The global sea surface temperature (GST) (HadSST3) variability spectrum, Sgst (Tgst, &#x3b8;gst (t-t<sub>0</sub>))<bold>,</bold> is transformed <xref ref-type="disp-formula" rid="e5">Eq. 5</xref> into a wavelet spectrum Wgst (s, t). The wavelet spectrum, Wgst (s, t), is then computed for s &#x3d; (1 &#x2026; 85) and t &#x3d; (1850 &#x2026; 2020) (yr.), as shown in <xref ref-type="fig" rid="F3">Figure 3</xref>. The computed GST wavelet spectrum, Wgst (s, t), has minima and maxima Wgst (s &#x3d; min/max, t &#x3d; (t<sub>1</sub>,t<sub>0</sub>)) &#x3d; ((-2.2, 1860), (2.2, 1883), (-3.1, 1912), (3.0, 1943), (-3.9, 1977), (5.1, 2008)), at distances of (23, 29, 30, 34, 31) (yr.), and a mean cycle period of 58.8 years. The identified 58.8-year cycle in sea surface variability from 1850 coincides with the lunar forced cycles 3Tln &#x3d; 55.83&#xa0;years.</p>
<fig id="F3" position="float">
<label>FIGURE 3</label>
<caption>
<p>Global sea surface temperature (HadSST3) wavelet spectrum, Wgst (s, t), for s &#x3d; (1 &#x2026; 85) and t &#x3d; (1850 &#x2026; 2020) (yr.).</p>
</caption>
<graphic xlink:href="fspas-09-839794-g003.tif"/>
</fig>
<p>The stationary cycle periods in the wavelet spectrum Wgst (s, t) (<xref ref-type="fig" rid="F4">Figure 4</xref>) are estimated by computing wavelet autocorrelations <xref ref-type="disp-formula" rid="e7">Eq. 7</xref>. The computed autocorrelations, WRgst (Rgst(s), m), of the wavelet spectrum, Wgst (s, t), have maximum correlations, Rgst &#x3d; (0.20, 0.23, 0.20, 0.24, 0.30, 0.20, 0.12, 0.50, 0.23) with the stationary sea cycle surface periods Tgst &#x3d; (9, 18, 28, 29, 37, 48, 57, 64, 74) (yr.) (<xref ref-type="fig" rid="F5">Figure 5</xref>).</p>
<fig id="F4" position="float">
<label>FIGURE 4</label>
<caption>
<p>Global sea surface temperature wavelet autocorrelations: WRgst (Rgst(s), m) for s &#x3d; (1 &#x2026; 85) and m &#x3d; (0 &#x2026; 85) (yr.).</p>
</caption>
<graphic xlink:href="fspas-09-839794-g004.tif"/>
</fig>
<fig id="F5" position="float">
<label>FIGURE 5</label>
<caption>
<p>Global mean land temperature wavelet spectrum, Wglt (s, t), for s &#x3d; (1 &#x2026; 85) and t &#x3d; (1850 &#x2026; 2020) (yr.).</p>
</caption>
<graphic xlink:href="fspas-09-839794-g005.tif"/>
</fig>
</sec>
<sec id="s7-2">
<title>Solar Lunar Coincidences</title>
<p>The global sea surface temperature wavelet spectrum has a coincidence with the interference between deterministic solar forced cycle periods and lunar forced cycle periods. The estimated global sea surface temperature wavelet spectrum, Wgst (s, t), has coincidences with the deterministic lunar-forced sea surface spectrum, Slst, and the deterministic solar-forced sea surface temperature spectrum. Lunar-forced sea surface temperature spectrum Tlst &#x3d; (9.3, 18.6, 27.9, 37.2, 46.5, 55.8, 65.1, 74.4) (yr.) has a coincidence with the identified stationary sea surface temperature periods Tgst &#x3d; (9, 18, 28, 29, 37, 48, 57, 64, 74) (yr.), which confirms lunar-forced sea surface temperature variability. The identified 29-year cycle has a coincidence with the 29.44-year, Tsa, solar forced period.</p>
<p>The computed <xref ref-type="disp-formula" rid="e5">Eq. 5</xref> global sea temperature wavelet spectrum, Wgst (s, t), has maximum and minimum at Wgst (s &#x3d; max, min, t), &#x3d; ((3.0, 1943), (-3.9, 1977)). The deterministic 74.44-year lunar forced temperature period has computed <xref ref-type="disp-formula" rid="e10">Eq. 10</xref> maximum and minimum at Alst (74, t &#x3d; (t<sub>0</sub>, t<sub>1</sub>)) &#x3d; (1.0, 1942), (-1.0, 1979). The phase differences between the estimated sea surface temperature cycles and the deterministic lunar forced cycles are (1, 2) (yr.).</p>
<p>Lunar forced cycle periods Tlst &#x3d; (18.61, 74.44) have minima at the years&#xa0;t &#x3d; (1895, 1905, 1914) and a coincidence maximum at the year&#xa0;t &#x3d; 2016. The solar forced SUN cycles have a minimum and maximum at Asst (t &#x3d; (t<sub>1</sub>, t<sub>0</sub>)) &#x3d; ((-2.37, 1896), (2.52, 2025)). The solar-forced minimum in 1896 has a coincidence with the lunar-forced minimum in 1895. The solar-forced SUN cycle has a maximum in 2025. The computed phase difference is one year. The lunar forced temperature cycles Tlst &#x3d; (18.61, 74.44) have maxima in the time period 2007 to 2025 and coincidences with the solar forcing maximum in the year 2025.</p>
</sec>
<sec id="s7-3">
<title>Global Warming and Cooling</title>
<p>Global warming from 1895 to 2024 coincides with interference between solar-forced SST amplitude variations <xref ref-type="disp-formula" rid="e9">Eq. 9</xref>. The solar forced cycle SST index, Asst(t), has a minimum in 1895, the SST index, Asst(t), has a maximum in 2025, and coincides with sea temperature growth (<xref ref-type="fig" rid="F2">Figure 2</xref>) and the wavelet spectrum, Wgst (s, t), amplitude minima and maxima (<xref ref-type="fig" rid="F3">Figure 3</xref>). The solar forced cycles, Tsst, and lunar forced cycles, Tlst, show constructive negative interference in 1895 and positive constructive interference in 2025. The upcoming solar forcing SST index minimum is at Asst (t &#x3d; t<sub>1</sub>) &#x3d; (&#x2212;2.88, 2070), the deepest minimum since 1375 B.C., and has a destructive interference with the lunar forcing sea surface temperature at Alst (t &#x3d; t<sub>0</sub>) &#x3d; (1.00, 2072).</p>
</sec>
<sec id="s7-4">
<title>Global Mean Temperature Oscillations</title>
<p>The Earth&#x2019;s global mean temperature (GMT) time-series (HadCRUT4) variation is represented by the wavelet spectrum Wgmt (s, t). The wavelet spectrum, Wgmt (s, t), is computed for s &#x3d; (1 &#x2026; 85) and t &#x3d; (1850 &#x2026; 2020) (yr.). The computed wavelet spectrum, Wgmt (s, t), has the following minima and maxima: (Wgmt (s &#x3d; min, max, t &#x3d; (t<sub>1</sub>, t<sub>0</sub>)) &#x3d; ((-2.0, 1860), (1.62, 1882), (-2.0, 1910), (2.4, 1941), (-4.0, 1974), (5.8, 2008)). These coincide with the global sea surface temperature, GST, and wavelet spectrum Wgst (s, t).</p>
<p>The autocorrelation spectrum, WRgmt (Rgmt(s), m), obtained from the wavelet spectrum, Wgmt (s, t), has maxima correlations, Rgmt (max) &#x3d; (0.22, 0.23, 0.15, 0.27, 0.30, 0.20, 0.12, 0.38, 0.16), to the stationary global mean temperature cycle periods: Tgmt &#x3d; (9, 18, 28, 29, 37, 46, 57, 64, 74) (yr.). The identified global mean temperature cycle spectrum, Tgmt, coincides with the identified global sea temperature cycles, Tgst, revealing that the global mean temperature variation is greatly influenced by the sea surface temperature variation.</p>
</sec>
<sec id="s7-5">
<title>Global Land Surface Temperature Oscillations</title>
<p>The global land surface temperature (GLT) (CRUTEM4) (<xref ref-type="fig" rid="F2">Figure 2</xref>) variation is estimated from the wavelet spectrum Wglt (s, t). The wavelet spectrum, Wglt (s, t), is computed <xref ref-type="disp-formula" rid="e5">Eq. 5</xref> for s &#x3d; (1, &#x2026; 85) and t &#x3d; (1850, &#x2026; 2020) (yr.). The computed GLT wavelet spectrum, Wglt (s, t), (<xref ref-type="fig" rid="F5">Figure 5</xref>) has minima and maxima in (Wglt (s &#x3d; (max, min)), Fglt) &#x3d; ((&#x2212;4.0, 1884), (2.0, 1934), (&#x2212;4.5, 1972), (6.5, 2005)).</p>
<p>The computed autocorrelations <xref ref-type="disp-formula" rid="e7">Eq. 7</xref>, WRglt (Rglt(s), m), of the wavelet spectrum (<xref ref-type="fig" rid="F6">Figure 6</xref>), Wglt (s, t), have maximum correlations, Rglt &#x3d; (0.23, 0.18, 0.15, 0.20, 0.27, 0.13, 0.13, 0.23, 0.15, 0.28), to the identified stationary global land temperature cycle periods: Tglt &#x3d; (9, 19, 28, 29.37, 47, 57, 64, 74, 81) (yr.).</p>
<fig id="F6" position="float">
<label>FIGURE 6</label>
<caption>
<p>Autocorrelations of the global land temperature wavelet spectrum, WRglt (Rglt(s), m), for s &#x3d; (1 &#x2026; 85) and m &#x3d; (1 &#x2026; 85) (yr.).</p>
</caption>
<graphic xlink:href="fspas-09-839794-g006.tif"/>
</fig>
</sec>
<sec id="s7-6">
<title>Solar Lunar Coincidences</title>
<p>The identified stationary global land temperature spectrum, Tglt, coincides with the lunar forcing sea surface cycle periods, Tlst, and the solar forcing cycles (Tsa, Tur). Global land temperature variation and lunar-forced amplitude variations have reversed-phase coincidences. Lunar forced cycle periods have minima and maxima in the following years: Aglt (t &#x3d; (t<sub>0</sub>, t<sub>1</sub>)) &#x3d; ((&#x2212;4.0, 1884), (1.0, 1885.8), (2.0, 1934), (&#x2212;1.0, 1932.3)). Global land temperature cycles have minima and maxima in the following years: Alst (t &#x3d; (t<sub>1</sub>, t<sub>0</sub>)) &#x3d; ((&#x2212;4.5, 1972), (1.0, 1978.8)), ((6.5, 2005), (&#x2212;1.0, 2006.7)). The mean phase difference is only 2 years from 1884 to 2005.</p>
<p>After 1850, the TSI amplitude variation, Atsi(t), <xref ref-type="disp-formula" rid="e8">Eq. 8</xref> has minima and maxima in Atsi(t &#x3d; (t<sub>1</sub>, t<sub>0</sub>)) &#x3d; ((&#x2212;2.95, 1885), (2.36, 1930), (&#x2212;1.00, 1974), (1.21, 2017), (&#x2212;2.40, 2061)). The cycle-phase shift difference between global land temperature variations, Aglt(t), and the deterministic solar forcing amplitude variations, Atsi(t), <xref ref-type="disp-formula" rid="e5">Eq. 5</xref> are as follows: Aglt (t &#x3d; (t<sub>1</sub>, t<sub>0</sub>))&#x2014;Atsi(t &#x3d; (t<sub>1</sub>, t<sub>0</sub>)) &#x3d; (1, 4, 2, 12) (yr.),with a mean phase difference of 2.3&#xa0;years. The Saturn, Uranus (SU) cycles, (Tsa, Tur), show positive constructive interference in 2017 with a maximum of the GLT index, Aglt(t). Predictions of upcoming events show a deep minimum in 2061, when SUN forcing TSI cycles have negative constructive interference.</p>
</sec>
</sec>
<sec id="s8">
<title>Greenland&#xb4;S Temperature Oscillations From 2000 B.C.</title>
<p>The Greenland temperatures (GRT) are represented by the GISP2 time series (<xref ref-type="fig" rid="F7">Figure 7</xref>), which covers the time period from 2000 B.C. to 1993 A.D. The mean Greenland temperature decreased from 1100 to 1750 A.D. and then began to increase. The temperatures also exhibit large fluctuations that appear to be random. These fluctuation properties are studied by transforming the time series into a wavelet power spectrum.</p>
<fig id="F7" position="float">
<label>FIGURE 7</label>
<caption>
<p>Greenland temperature (GISP2) time series spanning t &#x3d; (&#x2212;2000 &#x2026; 1993) (yr.) and from t &#x3d; (1000 &#x2026; 1993) (yr.). &#x201c;The Little Ice Age&#x201d; is shown from approximately t &#x3d; (1200 &#x2026; 1850) (yr.).</p>
</caption>
<graphic xlink:href="fspas-09-839794-g007.tif"/>
</fig>
<p>
<xref ref-type="fig" rid="F8">Figure 8</xref> depicts the Greenland temperature (GISP2) autocorrelation spectrum <xref ref-type="disp-formula" rid="e7">Eq. 7</xref>, WRgrt (Rgrt(s), m), of the wavelet spectrum Wgrt (s, t) for s &#x3d; (1 &#x2026; 500) and m &#x3d; (1 &#x2026; 500). The autocorrelation spectrum, WRgrt (Rgrt(s), m), starting in 1000 A.D., has maxima correlations, Rgrt &#x3d; ((0.46, 0.43, 0.28, 0.21, 0.20, 0.26, 0.45), with stationary Greenland temperature cycle period: Tgrt &#x3d; (18, 76, 147, 296, 334, 375, 446) (yr.).</p>
<fig id="F8" position="float">
<label>FIGURE 8</label>
<caption>
<p>Greenland&#x2019;s temperature (GISP2) wavelet autocorrelation spectrum, WRgrt (Rgrt(s), m), for s &#x3d; (1 &#x2026; 500) and m &#x3d; (1...500) (yr.).</p>
</caption>
<graphic xlink:href="fspas-09-839794-g008.tif"/>
</fig>
<sec id="s8-1">
<title>Solar Lunar Coincidences</title>
<p>Lunar-forced cycle periods have a spectrum: Tlst &#x3d; (1, 4, 2&#x2a;4, 4&#x2a;4, 5&#x2a;4, 6&#x2a;4)Tln &#x3d; (18.6, 74.4, 148.9, 297.8, 372.2, 446) (yr.). The coincident difference Terr &#x3d; (Tgrt&#x2014;Tlst) &#x3d; (0, 1, 2, 3, 0) (yr.). The mean difference of one year confirms lunar-forced temperature variations have been occurring in Greenland for up to 446&#xa0;years, controlled by the lunar nodal cycle period 4Tln &#x3d; 74.44&#xa0;years. The identified 334-year Greenland temperature cycle period has a coincidence with the solar-forced interference cycle Tun-mco (2) &#x3d; 332.83&#xa0;years.</p>
<p>
<xref ref-type="fig" rid="F9">Figure 9</xref> shows the Greenland temperature (GISP2) wavelet power spectrum <xref ref-type="disp-formula" rid="e6">Eq. 6</xref> for s &#x3d; (1 &#x2026; 500) and t &#x3d; (1000 &#x2026; 1993) (yr.). The wavelet power spectrum reveals the most dominant cycle in the wavelet spectrum, starting from 1000 A.D. The identified wavelet power spectrum has computed maxima of WPgrt (s &#x3d; max, t &#x3d; t<sub>0</sub>) &#x3d; ((71, 1129), (71, 1290), (93, 1502), (285, 1750), (124, 1979)), where the years 1290 and 1750 represent maxima in cold climate periods. A mean cycle period of 440 years confirms a stationary 446-year lunar forcing cycle in Greenland temperature variation. The computed wavelet power maximum, WPgrt (s &#x3d; max, t &#x3d; t<sub>0</sub>) &#x3d; (285, 1750) (<xref ref-type="fig" rid="F9">Figure 9</xref>), reveals the deepest negative temperature event between 1000 and 2000 A.D. The 4450-year TSI envelope period, Atsi-en(t), has phase shifts in the years: Atsi-en(t) &#x3d; ((&#x2212;0, -1624.49), (max, &#x2212;512), (&#x2b;0, 600), (min, 1712), (&#x2212;0, 2825)). The phase lag from the deterministic TSI envelope minimum in 1712 to the estimated Greenland temperature minimum in 1750 is 38&#xa0;years.</p>
<fig id="F9" position="float">
<label>FIGURE 9</label>
<caption>
<p>Greenland&#x2019;s GISP2 temperature wavelet power spectrum, WPgrt (s, t), for s &#x3d; (1...500) and t &#x3d; (1000 &#x2026; 1993) (yr.). The wavelet power spectrum shows dominant warm cycles and cold cycles from 1000 A.D., and the &#x201c;The Little Ice Age&#x201d; from approximately t &#x3d; (1200 &#x2026; 1850) (yr.).</p>
</caption>
<graphic xlink:href="fspas-09-839794-g009.tif"/>
</fig>
</sec>
<sec id="s8-2">
<title>Solar Lunar-Forced Interference From 1000 A.D.</title>
<p>The identified lunar-forced 446-year Greenland temperature cycle and the solar-forced SST cycle <xref ref-type="disp-formula" rid="e9">Eq. 9</xref>, Tun-mco (2) &#x3d; 332.83, has a (3, 4) cycle coincidence interference in a total cycle of 1320 years. The 333-year solar-forced sea surface temperature cycle <xref ref-type="disp-formula" rid="e9">Eq. 9</xref> and the 446-year lunar-forced sea surface temperature cycle experience computed positive constructive interference in (590&#x2013;500) B.C., destructive interference in (1000&#x2013;1160), negative constructive interference in (1330&#x2013;1420) and (1660&#x2013;1825), positive constructive interference in (1864&#x2013;1995) and negative constructive interference in (2085&#x2013;2160). The solar-forced sea temperature index, Asst(t), <xref ref-type="disp-formula" rid="e9">Eq. 9</xref> has a minimum at Asst (t &#x3d; t<sub>1</sub>) &#x3d; (&#x2212;2.70, 1745), which coincides with the Greenland temperature minimum in 1750 (<xref ref-type="fig" rid="F9">Figure 9</xref>) (<xref ref-type="fig" rid="F11">Figure 11</xref>). The positive constructive interference time period 1864&#x2013;1995 is known as a &#x201c;modern warm time period&#x201d;. The negative constructive interference occurring from (2085&#x2013;2160) represents a computed upcoming cold time period.</p>
</sec>
<sec id="s8-3">
<title>Solar Lunar-Forced Interference From 2000 B.C.</title>
<p>From 2000 B.C., Greenland&#x2019;s temperature wavelet power spectrum <xref ref-type="disp-formula" rid="e6">Eq. 6</xref>, WPgrt (s, t), for t &#x3d; (-2000 &#x2026; 1993) (yr.) and s &#x3d; (1...2000) has maxima of WPgrt (s &#x3d; max, t &#x3d; t<sub>0</sub>) &#x3d; ((200, &#x2212;1300), (120, &#x2212;513), (147, 585), (392, 1620)), where the years 513 B.C. and 1620 A.D. represent maxima in cold climate periods. (<xref ref-type="fig" rid="F10">Figure 10</xref>). The time period spanning from 513 B.C. to 1620 A.D. covers a total time period of 2133 years. The stationary temperature cycle, Tgrt (7), has computed phase shifts in the years: Agrt(t &#x3d; (t<sub>1</sub>, t<sub>0</sub>)) &#x3d; ((min, &#x2212;513), (max, 554), (&#x2b;0, 1086), (min, 1620), (&#x2212;0, 2153), (max, 2686)).</p>
<fig id="F10" position="float">
<label>FIGURE 10</label>
<caption>
<p>Greenland&#x2019;s GISP2 temperature wavelet power spectrum, WPgrt (s, t), for t &#x3d; (&#x2212;2000 &#x2026; 1993) (yr.) and s &#x3d; (1...2000). The wavelet power spectrum shows dominant warm time periods and cold time periods from 2000 B.C.</p>
</caption>
<graphic xlink:href="fspas-09-839794-g010.tif"/>
</fig>
<p>The identified stationary 2133-year Greenland temperature cycle period from 2000 B.C. has a (2, 1) interference with the solar-forced envelope period Tun-mco (7) &#x3d; 4285&#xa0;years. The 2133-year Greenland temperature cycle and the 4285-year solar-forced cycle, Tun-mco (7), show destructive interference in 512 B.C. and negative constructive interference in 1620 A.D.</p>
</sec>
<sec id="s8-4">
<title>Solar Lunar-Forced Coincidences to &#x201c;the Little Ice Age&#x201d;</title>
<p>The Greenland temperature variation from 1000 A.D. (<xref ref-type="fig" rid="F7">Figures7</xref>, <xref ref-type="fig" rid="F9">9</xref>) is controlled by the solar-forced UN sea surface temperature periods, (Tsst-mco (8), Tsst-mco (7)/2, Tsst-mco (2) &#x3d; (4450, 2142, 333) (yr.), and the lunar forced sea temperature period, Tlst () &#x3d; 446&#xa0;years (<xref ref-type="fig" rid="F11">Figure 11</xref>). The 332-year solar forced cycle and the 446-year lunar forced cycle have positive constructive interference in the years 165&#x2013;320, destructive interference in 600&#x2013;1160, and negative constructive interference in 1330&#x2013;1420 and 1660&#x2013;1825. The solar-lunar cycle periods have a computed upcoming negative constructive interference from 2085 to 2150 A.D. (<xref ref-type="fig" rid="F11">Figure 11</xref>). Temporary negative constructive interference between the identified solar-lunar cycles indicates that &#x201c;The Little Ice Age&#x201d; covers a total time period of 820&#xa0;years from 1330 to 2150 A.D.</p>
<fig id="F11" position="float">
<label>FIGURE 11</label>
<caption>
<p>Stationary solar forced sea temperature cycler [Tsst (mco, 8], Tsst-mco (7)/2, Tsst-mco (2) &#x3d; (4450, 2142, 333) (yr.) and lunar forced temperature period, Tlst, of 446&#xa0;years in the time period t &#x3d; (0 &#x2026; 2500).</p>
</caption>
<graphic xlink:href="fspas-09-839794-g011.tif"/>
</fig>
</sec>
</sec>
<sec sec-type="discussion" id="s9">
<title>Discussion</title>
<sec id="s9-1">
<title>Solar Forced Oscillations</title>
<p>The origin of total solar irradiation variation is not well understood. <xref ref-type="bibr" rid="B28">M&#xf6;rth and Schlamminger (1979)</xref> investigated the relation between planetary motion, sunspots and climate and assumed that the transmission of gravitational torque in the solar system causes changes in the solar photosphere. This study of solar irradiation variation is based on a deterministic JSUN cycle spectrum model. The study reveals that TSI oscillation may be computed by the simple linear spectrum transform from JSUN cycle period oscillations to TSI cycle period oscillations. The TSI amplitude variations have minima when the JSUN cycles have perihelion coincidences and maxima when the JSUN cycles have aphelion coincidences. The total envelope time period covers a cycle period of 4450&#xa0;years.</p>
<p>The computed TSI index <xref ref-type="disp-formula" rid="e8">Eq. 8</xref> has minima coincidences to known deep solar minima from 1000 A.D. (<xref ref-type="bibr" rid="B40">Usoskin 2005</xref>), (<xref ref-type="bibr" rid="B41">Velasco et al., 2015</xref>). The new information from this study is deep solar minima coincidences with negative constructive interference between SUN cycles. Wolf, Sp&#xf6;rer and Maunder have SUN cycle constructive interference, Oort has UN cycle constructive interference, and Dalton has SU cycle constructive interference. SUN cycles have negative constructive interference in the cold time period 1850&#x2013;1899 and positive constructive interference in the modern warm time period 1981&#x2013;2025. Solar deep minima amplitude variations are controlled by SUN perihelion coincidences in distances of Tsun-mco years. The Maunder minimum is a one-time event in the SUN envelope time period of 4450&#xa0;years. The TSI envelope time period has a JSUN cycle minimum in 1712 A.D. coincident with the &#x201c;Deep Freeze&#x201d; year in 1709, when the winter temperature in Europe dropped to &#x2212;15&#xb0;C. (<xref ref-type="bibr" rid="B32">S&#xe1;nchez Arreseigor, 2019</xref>).</p>
<p>Computed TSI variations coincide with solar activity (<xref ref-type="bibr" rid="B19">Kremliovsky 1994</xref>), (<xref ref-type="bibr" rid="B2">Bhowmik and Nandy 2018</xref>), (<xref ref-type="bibr" rid="B43">Velasco et al., 2021</xref>). <xref ref-type="bibr" rid="B5">Courtillot et al. (2021)</xref> identified Jovian cycles in solar activity and estimated an upcoming Solar Cycle 25 maximum in 2026. In upcoming events, SUN cycles have positive constructive interference in 1980&#x2013;2000, and SU cycles have positive constructive interference in 2007&#x2013;2025. The upcoming computed <xref ref-type="disp-formula" rid="e8">Eq. 8</xref>, the next solar minima have UN-type negative constructive interference from 2025 to 2072 and SUN-type negative constructive interference from 2197 to 2245. Stationary cycles in the ACRIM TSI time series from 1700 reveal a computed Next Dalton-type TSI minimum in 2035&#x2013;2065 and a deep solar minimum in 2049 A.D. (<xref ref-type="bibr" rid="B48">Yndestad and Solheim 2017</xref>). <xref ref-type="bibr" rid="B51">Zharkova (2020)</xref> estimated an upcoming Maunder-type solar minimum time period from 2020 to 2053 A.D. (<xref ref-type="bibr" rid="B42">Velasco et al., 2022</xref>).</p>
</sec>
<sec id="s9-2">
<title>Solar-Forced Accumulation of Heat in Oceans</title>
<p>The study reveals a direct relation between the computed solar-forced sea temperature spectrum and the estimated global sea surface spectrum (<xref ref-type="table" rid="T1">Table 1</xref> and <xref ref-type="table" rid="T2">Table 2</xref>). The direct relation confirms the linear spectrum transform <xref ref-type="disp-formula" rid="e2">Eq. 2</xref>, where the solar forced cycle periods coincide with the TSI cycles and Jovian planet cycles. A &#x3c0;/2 (rad) phase lag in the accumulation of heat from solar-forced TSI cycles introduces a new constructive and destructive interference between solar-forced sea surface temperature cycles.</p>
<table-wrap id="T1" position="float">
<label>TABLE 1</label>
<caption>
<p>Cycle- and phase-coincidences between Jovian planet oscillations (JSUN), total solar irradiation oscillations (TSI) and lunar nodal forced sea temperature oscillations (LST).</p>
</caption>
<table>
<tbody valign="top">
<tr>
<td align="left"/>
<td align="center">
<bold>Jovian planets oscillations</bold>
</td>
</tr>
<tr>
<td align="left">Tjsun</td>
<td align="center">(11.862, 29.447, 84.02, 164.79) (yr.)</td>
</tr>
<tr>
<td align="left">t &#x3d; t<sub>per</sub>
</td>
<td align="center">(1714.69, 1709.00, 1714.32, 1711.88) (yr.).</td>
</tr>
<tr>
<td align="left">t &#x3d; t<sub>ape</sub>)</td>
<td align="center">(&#x2212;509.43, &#x2212;514.25, -512.21, &#x2212;512.79) (yr.).</td>
</tr>
<tr>
<td align="left">t &#x3d; t<sub>aph</sub>
</td>
<td align="center">(&#x2212;509.43, &#x2212;514.25, -512.21, -512.79) (yr.)</td>
</tr>
<tr>
<td align="left">Ajsun-ecp(t)</td>
<td align="center">((-0, 1624.49), (aph, -512.17), (&#x2b;0, 600.15), (per, 1712.47), (&#x2212;0, 2824.79)).</td>
</tr>
<tr>
<td align="left"/>
<td align="center">
<bold>Total Solar irradiation oscillations</bold>
</td>
</tr>
<tr>
<td align="left">Ttsi</td>
<td align="center">(11.862, 29.447, 84.02, 164.79) (yr.)</td>
</tr>
<tr>
<td align="left">Tun-mco</td>
<td align="center">(166.42, 332.83, 499.70, 998.49, 1954.97, 2454.22, 4284.78, 4451.20) (yr.).</td>
</tr>
<tr>
<td align="left">Tsun-mco</td>
<td align="center">(169.84, 499.70, 999.39, 1960.96, 2450.84, 4289.61 4449.63) (yr.)</td>
</tr>
<tr>
<td align="left">Atsi(un, t &#x3d;(t<sub>0</sub>, t<sub>1</sub>))</td>
<td align="center">((2.00, &#x2212;512), (&#x2b;0, 433), (&#x2212;2.00, 1546), (&#x2212;0, 2658))</td>
</tr>
<tr>
<td align="left">Atsi(sun, t&#x3d;(t<sub>0</sub>, t<sub>1</sub>))</td>
<td align="center">((2.99, &#x2212;514), (&#x2b;0, 598), (&#x2212;2.92, 1710), (&#x2212;0, 2820)).</td>
</tr>
<tr>
<td align="left">TSI min</td>
<td align="center">Oort (1020&#x2013;1070), Wolf 1 (1197&#x2013;1294), Wolf 2 (1350&#x2013;1398), Sp&#xf6;rer (1523&#x2013;1571), Maunder (1696&#x2013;1744), Dalton (1791&#x2013;1804), Modern (1850&#x2013;1899), Next (2024&#x2013;2072), Next deep (2197&#x2013;2245).</td>
</tr>
<tr>
<td align="left"/>
<td align="center">
<bold>Lunar Nodal oscillations</bold>
</td>
</tr>
<tr>
<td align="left">Tln</td>
<td align="center">(1, 2, 3, 4, 6&#x2026;.24)&#x2a;18,61 (yr.)</td>
</tr>
<tr>
<td align="left">Aln(t &#x3d; t<sub>0</sub>)</td>
<td align="center">(&#x2026;,1941.6&#x2013;18.6, 1941.6, 1941.6 &#x2b; 18.6, &#x2026; ) (yr.).</td>
</tr>
</tbody>
</table>
</table-wrap>
<table-wrap id="T2" position="float">
<label>TABLE 2</label>
<caption>
<p>Cycle- and phase-coincidences between stationary solar-forced sea temperature cycles (GST), global sea surface temperature cycles (GST), global mean temperature cycles (GMT), global land temperature cycles (GLT) and Greenland temperature cycles (GRT).</p>
</caption>
<table>
<tbody>
<tr>
<td align="left"/>
<td align="center">
<bold>Solar-Forced sea temperature cycles</bold>
</td>
</tr>
<tr>
<td align="left">Tsst (sun)</td>
<td align="center">(11.862, 29.447, 84.02, 164.79) (yr.)</td>
</tr>
<tr>
<td align="left">Tsst-mco</td>
<td align="center">(169.84, 499.70, 999.39, 1960.96, 2450.84, 4289.61 4449.63) (yr.)</td>
</tr>
<tr>
<td align="left">Asst-mco, t &#x3d; (t<sub>0</sub>, t<sub>1</sub>)</td>
<td align="center">((&#x2212;0.00, -514), (3.0, 598), (&#x2b;0.00, 1710), (&#x2212;3.0, 2820)).</td>
</tr>
<tr>
<td align="left">Asst(t) &#x3d; min, t &#x3d; t<sub>1</sub>
</td>
<td align="center">((&#x2212;2,48, 1069), (&#x2212;2.39, 1244), (&#x2212;2.73, 1375), (&#x2212;2.73, 1570), (&#x2212;2.70, 1745), (&#x2212;2.37, 1896), (&#x2212;2.88, 2070), (&#x2212;2.88, 2246))</td>
</tr>
<tr>
<td align="left">Asst(t) &#x3d; max, t &#x3d; t<sub>0</sub>
</td>
<td align="center">((2.86, 1024), (2.76, 1379), (2.75, 1525), (2.47, 1850), (2.53, 2025)).</td>
</tr>
<tr>
<td align="left"/>
<td align="center">
<bold>Global Sea surface temperature variability (GST)</bold>
</td>
</tr>
<tr>
<td align="left">Tgst</td>
<td align="center">(9, 18, 28, 29, 37, 46, 57, 64, 74, 85) (yr.)</td>
</tr>
<tr>
<td align="left">Tlst/2</td>
<td align="center">(9.3, 18.6, 27.9, 37.2, 46.5, 55.8, 65.1, 74.4) (yr.)</td>
</tr>
<tr>
<td align="left">Tst</td>
<td align="center">(29.44, 84.02) (yr.)</td>
</tr>
<tr>
<td align="left">Wgst (s &#x3d; min, max, t&#x3d;(t<sub>1</sub>, t<sub>0</sub>)</td>
<td align="center">((&#x2212;2.2, 1860), (2.2, 1883), (&#x2212;3.1, 1912), (3.0, 1943), (&#x2212;3.9, 1977), (5.1, 2008))</td>
</tr>
<tr>
<td align="left">Alst(t) &#x3d; min, max, t&#x3d;(t<sub>1</sub>, t<sub>0</sub>)</td>
<td align="center">((&#x2212;1.0, 1857.8), (1.0, 1885.8), (&#x2212;1.0, 1913.8), (1.0, 1941.6), (100, 1978.8), (&#x2212;1.0, 2006.7))</td>
</tr>
<tr>
<td align="left">Asst(t) &#x3d; min, max, t&#x3d;(t<sub>1</sub>, t<sub>0</sub>)</td>
<td align="center">((&#x2212;2.37, 1896), (1.13, 1939), (2.52, 2025), (&#x2212;2.88, 2070))</td>
</tr>
<tr>
<td align="left"/>
<td align="center">
<bold>Global Mean temperature variability (GMT)</bold>
</td>
</tr>
<tr>
<td align="left">Tgmt</td>
<td align="center">(9, 18, 28, 29, 37, 46, 57, 64, 74) (yr.)</td>
</tr>
<tr>
<td align="left">Tln/2</td>
<td align="center">(9.3, 18.6, 27.9, 37.2, 46.5, 55.8, 65.1, 74.4) (yr.)</td>
</tr>
<tr>
<td align="left">Tsst</td>
<td align="center">(29) (yr.)</td>
</tr>
<tr>
<td align="left">Wgmt (s &#x3d; min, max, t &#x3d;(t<sub>1</sub>, t<sub>0</sub>)</td>
<td align="center">((&#x2212;2.0, 1860), (1.62, 1882), (&#x2212;2.0, 1910), (2.4, 1941), (&#x2212;4.0, 1974), (5.8, 2008))</td>
</tr>
<tr>
<td align="left">Alst(t) &#x3d; min, max, t &#x3d;(t<sub>1</sub>, t<sub>0</sub>)</td>
<td align="center">((&#x2212;1.0, 1857.8), (1.0, 1885.8), (&#x2212;1.0, 1913.8), (1.0, 1941.6), (1.0, 1978.8), (&#x2212;1.0, 2006.7))</td>
</tr>
<tr>
<td align="left">Asst(t) &#x3d; min, max, t &#x3d;(t<sub>1</sub>, t<sub>0</sub>)</td>
<td align="center">((&#x2212;2.36, 1895), (1.13, 1939), (2.23, 2026), (&#x2212;2.88, 2070)).</td>
</tr>
<tr>
<td align="left"/>
<td align="center">
<bold>Global Land surface temperature variability (GLT)</bold>
</td>
</tr>
<tr>
<td align="left">Tglt</td>
<td align="center">(9, 19, 28, 29, 37, 47, 57, 64, 74, 81) (yr.)</td>
</tr>
<tr>
<td align="left">Tlst/2</td>
<td align="center">(9.3, 18.6, 27.9, 37.2, 46.5, 55.8, 65.1, 74.4) (yr.)</td>
</tr>
<tr>
<td align="left">Tsst</td>
<td align="center">(29.45, 84.02) (yr.)</td>
</tr>
<tr>
<td align="left">Wglt (s &#x3d; min, max, t &#x3d;(t<sub>1</sub>, t<sub>0</sub>)</td>
<td align="center">((&#x2212;4.0, 1884), (2.0, 1934), (&#x2212;4.5, 1972), (6.5, 2005))</td>
</tr>
<tr>
<td align="left">Alst (s &#x3d; min, max, t &#x3d;(t<sub>1</sub>, t<sub>0</sub>)</td>
<td align="center">((&#x2212;1.0, 1857.8), (1.0, 1885.8), (&#x2212;1.0, 1913.8), (1.0, 1941.6), (1.0, 1978.8), (&#x2212;1.0, 2006.7))</td>
</tr>
<tr>
<td align="left">Atsi(s &#x3d; min, max), t &#x3d;(t<sub>1</sub>, t<sub>0</sub>)</td>
<td align="center">((&#x2212;2.95 1885), (2.36, 1930), (&#x2212;1.00, 1974), (1.21, 2017), (&#x2212;2.40, 2061)).</td>
</tr>
<tr>
<td align="left"/>
<td align="center">
<bold>Greenland temperature variability (GRT) from 2000B.C. and 1000 A.D.</bold>
</td>
</tr>
<tr>
<td align="left">Tgrt</td>
<td align="center">(18, 76, 147, 296, 334, 375, 446) (yr.)</td>
</tr>
<tr>
<td align="left">Tlst</td>
<td align="center">(18.6, 74.4, 148.9, 297.8, 372.2, 446) (yr.).</td>
</tr>
<tr>
<td align="left">Tsst (un)</td>
<td align="center">(332.8, 2142, 4450) (yr.)</td>
</tr>
<tr>
<td align="left">WPgrt1k (s &#x3d; max, t &#x3d; ,t<sub>0</sub>
</td>
<td align="center">((71, 1129), (71, 1290), (93, 1502), (124, 1750), (124, 1979)) (yr.)</td>
</tr>
<tr>
<td align="left">WPgrt4k (s &#x3d; max, t &#x3d; ,t<sub>0</sub>
</td>
<td align="center">((200, -1300), (120, &#x2212;513), (147, 585), (392, 1620))</td>
</tr>
<tr>
<td align="left">Atsi(t) &#x3d; max, t &#x3d;(t<sub>0</sub>,t<sub>1</sub>)</td>
<td align="center">((max, &#x2212;522), (&#x2b;0, 559), (min, 1630), (&#x2212;0, 2691))</td>
</tr>
</tbody>
</table>
</table-wrap>
<p>New phase relations between Jovian planet cycles have unexpected influences on climate variations. The modern warm cycle in 1920&#x2013;2050 coincides with positive UN cycles <xref ref-type="disp-formula" rid="e9">Eq. 9</xref>. SUN cycles have positive constructive interference in 2025. The computed SST index (2.53, 2025) has the highest sea surface temperature index in 500&#xa0;years, which reveals that the modern warm time period is a rare event controlled by the solar forced accumulation of heat in oceans. The 45-year SST index shift, from a 500-year maximum in 2025 to a 3000-year index minimum in 2070, is caused by a rare phase shift relation between the SUN cycles. The computed solar-forced deep minimum in 2070 indicates an upcoming deep cold climate period.</p>
<p>A wavelet spectrum analysis of the Arctic ice edge position from 1579 to 2020 revealed a computed upcoming maximum ice extent in 2073 (<xref ref-type="bibr" rid="B47">Yndestad 2021</xref>). A.D. Yu et al. (2011) published a study of variations in Earth temperatures over the past 2485&#xa0;years. The study was based on a power spectrum analysis of temperature variations based on tree rings and predicted that temperatures will decrease in the future until 2068 A.D. and then increase again.</p>
</sec>
<sec id="s9-3">
<title>Lunar Forced Oscillations</title>
<p>The lunar-forced temperature variability is explained by a lunar-forced tidal vertical mixing process in oceans and interference between lunar-forced temperature cycles in the thermohaline circulation flow. <xref ref-type="bibr" rid="B22">Maksimov and Smirnov (1967)</xref> estimated a global standing 19-year tide in the Atlantic Ocean. The identified standing lunar node tide had a maximum amplitude at the Arctic pole, a 50% maximum amplitude at the equator and a zero-amplitude node at 35 degrees latitude. This study has revealed cycle period- and cycle phase coincidences between the Earth axis nutation spectrum in the y-direction, the lunar nodal tide, North Atlantic water temperature variations, Earth&#x2019;s global temperature variations from 1850 and Greenland temperature variations from 2000 B.C. This close relation confirms the simplified lunar forced sea surface spectrum model. Greenland temperature variation reveals lunar-forced temperature cycles of up to 446&#xa0;years and controlled subharmonic periods from the 74.44-year lunar cycle. The 74.44-year cycle is confirmed in the NAO index and Arctic data series (<xref ref-type="bibr" rid="B49">Yndestad 2006</xref>).</p>
</sec>
<sec id="s9-4">
<title>Global Temperature Oscillations</title>
<p>Global sea surface variability is controlled by the interreference between the solar-forced spectrum and the lunar-forced spectrum. The wavelet spectrum analysis of global temperature variations from 1850 confirms the hypothesis from <xref ref-type="disp-formula" rid="e4">Eq. 4</xref> (<xref ref-type="table" rid="T2">Table 2</xref>). The global temperature variations from 1850 to 2020 have coincides with constructive and destructive interference between solar forced cycle periods and lunar forced cycle periods. Solar lunar forced coincidence to Greenland temperature variations from 2000 B.C. indicate that global sea surface temperature is period- and phase-locked to the 4450-year solar forced envelope period. The implication of interference is temporary warm and cold climate periods. The solar-forced sea temperature index computes a 500-year modern temperature maximum in 2025 and an upcoming 3000-year deep minimum temperature in 2070. The implication of this deep minimum is unclear.</p>
</sec>
<sec id="s9-5">
<title>Global Mean Temperature Variability</title>
<p>Global mean temperature variation coincides with the global sea temperature variation spectrum, revealing a major influence from the latter. Solar-lunar-forced interference in the oceans explains the origin of Earth&#x2019;s climate variation, with multidecadal cycles as a major cause of the global temperature variations that occurred from 1850 to 2020. The global sea surface temperature has approximately the same variation in the Northern and Southern Hemispheres. This confirms lunar forced cycles as a global standing wave and a coherent source of heat distribution in the oceans and solar forced TSI cycles as a coherent source of accumulated heat in the oceans (<xref ref-type="table" rid="T2">Table 2</xref>). Solar-forced temperature cycles and lunar-forced temperature cycles have different properties in the global temperature grid. Coherent solar forced cycles accumulate, while lunar forced cycles have phase variations in the global grid. This difference explains why lunar forced cycles have correlation R-values of 0.2&#x2013;0.5 to the global temperature time series.</p>
<p>In this study, global sea surface temperature has an estimated amplitude maximum in 1941. <xref ref-type="bibr" rid="B18">Kravstov et al. (2018)</xref> suggested that the North Atlantic Ocean is the major center of the Global Multidecadal Oscillation. The Atlantic Multidecadal Oscillation index has a maximum in 1942. The North Atlantic Water (NAW) inflows to the Norwegian Sea and has a maximum in 1943 (<xref ref-type="bibr" rid="B50">Yndestad et al., 2008</xref>).</p>
</sec>
<sec id="s9-6">
<title>Global Land Temperature Variability</title>
<p>The identified global land surface temperature spectrum has a TSI forced spectrum and a lunar forced spectrum. A direct relation to the TSI spectrum explains why the global land surface temperature time series reveals a different trend, exhibiting a time period with temperatures colder than the global temperature from 1850 to 1910 and a warmer period from 2000 to 2020 (<xref ref-type="fig" rid="F2">Figure 2</xref>). The lunar-forced spectrum in the global land surface spectrum may be explained by the wind-driven heat from global sea surface temperature variation. The lunar-forced land surface temperature variations and lunar force sea surface temperature variations have reversed-phase relations. A possible explanation is a &#x3c0;/2 (rad) phase lag from sea surface temperature to air temperature and a new &#x3c0;/2 (rad) phase lag in the integration of heat into land surface temperature.</p>
</sec>
<sec id="s9-7">
<title>Greenland Temperature Oscillations</title>
<p>Greenland&#x2019;s temperature variation is controlled by the NAW temperature and the North Atlantic Oscillation (NAO) (<xref ref-type="bibr" rid="B44">Vinther 2006</xref>; <xref ref-type="bibr" rid="B45">Vinther et al., 2003</xref>, <xref ref-type="bibr" rid="B46">2010</xref>). The NAO winter index variation has a lunar-forced cycle spectrum that coincides with the North Atlantic Water inflows to the Norwegian Sea, the Barents Sea and the Arctic Sea ice extent (<xref ref-type="bibr" rid="B49">Yndestad 2006</xref>). These close relations among the global temperature variation, North Atlantic water temperature and Greenland temperature confirm the close relation between Greenland&#x2019;s temperature variation and the global sea surface temperature variation.</p>
<p>Greenland temperature variation coincides with solar- and lunar-forced sea temperature variability. Lunar forced temperature periods are subharmonic periods from the 74.44-year lunar period up to 446 years. Long cycle periods in Greenland temperature variations (<xref ref-type="fig" rid="F9">Figure 9</xref>, <xref ref-type="fig" rid="F10">Figure 10</xref>) have cycle periods and cycle phase coincidences to solar-forced sea surface periods of 333, 2142 and 4450 years (<xref ref-type="fig" rid="F11">Figure 11</xref>). Negative constructive interference between the solar-lunar-forced sea temperature period explains temporary cold and warm climate periods from 1330 to 2150 A.D. (<xref ref-type="fig" rid="F11">Figure 11</xref>). The next upcoming cold period has negative constructive interference from 2085 to 2150 A.D. Longer cycle periods continue the computed solar forced minimum in 2072. A wavelet spectrum analysis of Arctic ice extent from 1579 confirms a 223-year lunar forced cycle and a computed upcoming maximum ice extent in 2073 A.D. (<xref ref-type="bibr" rid="B47">Yndestad 2021</xref>).</p>
<p>
<xref ref-type="bibr" rid="B21">Ljungqvist (2010)</xref> reconstructed temperature variability in the Northern Hemisphere (30&#x2013;90&#xb0;N) based on 30 proxy records during the last two millennia and identified a warm time period in the years 1&#x2013;300, a cold time period 300&#x2013;800, a warm time period 800&#x2013;1300 and a cold time period in the years 1300&#x2013;1900. The Briksdal glacier in the western part of Norway began to grow in 500 B.C. and reached its maximum extent in 1755 A.D. (<xref ref-type="bibr" rid="B3">Burki et al., 2009</xref>). The Greenland temperature power spectrum has a deep minimum in 1750 A.D. (<xref ref-type="fig" rid="F9">Figure 9</xref>).</p>
</sec>
</sec>
<sec sec-type="conclusions" id="s10">
<title>Conclusions</title>
<p>This study suggests that Earth&#x2019;s global temperature variabilities starting in 1850 and Greenland temperature variabilities starting in 2000 B.C. have solar-lunar-forced stationary temperature cycles up to 4450&#xa0;years. The primary causes of the identified multidecadal temperature variation is the stationary orbital cycles from the Jovian planets (Jupiter, Saturn, Uranus, Neptune) and the 18.6-year lunar nodal cycle from the Earth&#x2019;s axis nutation.</p>
<sec id="s10-1">
<title>Solar Lunar Spectrum Transformations</title>
<p>The chain of events from Jovian planet oscillations and the Earth&#x2019;s axis nutation oscillations may be represented as linear spectrum transformations of cycle periods and cycle period phase relations. The Jovian planet oscillation spectrum may be transformed into a solar irradiation spectrum and a solar forced sea surface temperature spectrum. The Earth&#x2019;s nutation oscillation spectrum may be transformed into a lunar forced sea surface temperature spectrum.</p>
</sec>
<sec id="s10-2">
<title>Solar Lunar Cycle Interference</title>
<p>This study has revealed the importance of cycle period phase relations in climate variations. TSI amplitude variations coincide with constructive and destructive interference between Jovian planet cycles in an envelope period of 4450&#xa0;years. The TSI envelope period has a minimum when JSUN periods have perihelion coincidences and a maximum when JSUN periods have aphelion coincidences. The accumulation of solar-forced heat in oceans introduces a &#x3c0;/2 (rad) phase lag in solar-forced sea temperature cycles and a new envelope cycle of solar-forced minima and maxima temperatures. Temperature variations from 2000 B.C. coincide with constructive and destructive interference between solar-forced and lunar-forced temperature variations. Solar lunar-forced global temperature cycles have time-variant phase relations and time-variant interference. The time-variant climate variations are never repeated. Climate variation may still be deterministic because the Jovian planet cycles and the Earth nutation cycles have approximately deterministic period and phase relations.</p>
</sec>
<sec id="s10-3">
<title>Sola Lunar-Forced Global Earth Temperature Variations Since 1850</title>
<p>Global temperature variations from 1850 to 2020 (Climate Research Unit) coincide with interference between solar lunar forced cycles. The global sea surface temperature (HadSST3) variability spectrum coincides with interference between solar-forced and lunar-forced sea temperature variations. The sea temperature variations from 1890 to 2020 coincide with a solar forced sea temperature minimum in 1896 and a solar forced sea temperature maximum in 2025. In terms of upcoming events, computations suggest the sea surface temperature will have a deep minimum in 2070.</p>
<p>Sea surface temperature and global mean temperature (HadCRUTE4) have cycle period coincidences and cycle phase coincidences. The spectrum coincidence confirms that sea surface temperature has a major influence on global temperature variations. Global land temperature (CRUTEM4) variation coincides with interference between solar forced irradiation cycles and lunar forced temperature cycles. The solar forced irradiation spectrum has a direct influence on Earth&#x2019;s global land surface temperature variations. The lunar forced temperature variations are explained by wind-driven heat from sea surface temperature variations.</p>
</sec>
<sec id="s10-4">
<title>Solar Lunar Forced Temperature Variations in Greenland From 2000 B.C.</title>
<p>Greenland&#x2019;s temperature (GISP2) variations and North Atlantic temperature variations are closely related to global sea surface temperature variations. The variation in Greenland&#x2019;s temperature, beginning in 2000 B.C., reflects solar-lunar-forced interference cycles up to 4450&#xa0;years. The Greenland temperature variation has lunar forced cycle periods up to 446&#xa0;years, solar forced sea temperature cycles of 333 and 2142&#xa0;years and a 4450-year TSI envelope cycle. The 4450-year envelope cycle has a minimum in 1745 when the identified Greenland temperature variation is at a minimum. Negative constructive interference between the identified solar-lunar cycles indicates that &#x201c;The Little Ice Age&#x201d; covers temporary cold periods from 1330 to 2150 A.D. The next upcoming negative constructive interference period covers the computed time period from 2070 to 2150.</p>
</sec>
</sec>
</body>
<back>
<sec id="s12">
<title>Data Availability Statement</title>
<p>Publicly available datasets were analyzed in this study. This data can be found here: and; Climatic Research Unit (<ext-link ext-link-type="uri" xlink:href="http://www.metoffice.gov.uk/hadobs/hadcrut4/">http://www.metoffice.gov.uk/hadobs/hadcrut4/</ext-link>). Paleoclimatology Program (<ext-link ext-link-type="uri" xlink:href="https://www.ncdc.noaa.gov/data-access/paleoclimatology-data">https://www.ncdc.noaa.gov/data-access/paleoclimatology-data</ext-link>) (<xref ref-type="bibr" rid="B17">Kobashi et al. 2011</xref>).</p>
</sec>
<sec id="s13">
<title>Author Contributions</title>
<p>The author confirms being the sole contributor of this work and has approved it for publication.</p>
</sec>
<sec sec-type="COI-statement" id="s14">
<title>Conflict of Interest</title>
<p>The authors declare that the research was conducted in the absence of any commercial or financial relationships that could be construed as a potential conflict of interest.</p>
</sec>
<sec sec-type="disclaimer" id="s15">
<title>Publisher&#x2019;s Note</title>
<p>All claims expressed in this article are solely those of the authors and do not necessarily represent those of their affiliated organizations, or those of the publisher, the editors and the reviewers. Any product that may be evaluated in this article, or claim that may be made by its manufacturer, is not guaranteed or endorsed by the publisher.</p>
</sec>
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</ref-list>
<sec id="s11">
<title>Nomenclature</title>
<def-list>
<def-item>
<term id="G1-fspas.2022.839794">
<bold>JSUN</bold>
</term>
<def>
<p>jupiter, Saturn, Uranus, Neptune</p>
</def>
</def-item>
<def-item>
<term id="G2-fspas.2022.839794">
<bold>SUN</bold>
</term>
<def>
<p>saturn, Uranus, Neptune</p>
</def>
</def-item>
<def-item>
<term id="G3-fspas.2022.839794">
<bold>UN</bold>
</term>
<def>
<p>uranus, Neptune</p>
</def>
</def-item>
<def-item>
<term id="G4-fspas.2022.839794">
<bold>SU</bold>
</term>
<def>
<p>saturn, Uranus</p>
</def>
</def-item>
<def-item>
<term id="G5-fspas.2022.839794">
<bold>SPO</bold>
</term>
<def>
<p>solar position oscillations</p>
</def>
</def-item>
<def-item>
<term id="G6-fspas.2022.839794">
<bold>TSI</bold>
</term>
<def>
<p>total solar irradiation</p>
</def>
</def-item>
<def-item>
<term id="G7-fspas.2022.839794">
<bold>SST</bold>
</term>
<def>
<p>solar forced sea temperature</p>
</def>
</def-item>
<def-item>
<term id="G8-fspas.2022.839794">
<bold>LST</bold>
</term>
<def>
<p>lunar forced sea surface temperature</p>
</def>
</def-item>
<def-item>
<term id="G9-fspas.2022.839794">
<bold>NAO</bold>
</term>
<def>
<p>north Atlantic Oscillation</p>
</def>
</def-item>
<def-item>
<term id="G10-fspas.2022.839794">
<bold>Cycle is a series of events that lead back to the starting point</bold>
</term>
<def>
<p>y(t) &#x3d; y(t &#x2b; T)</p>
</def>
</def-item>
<def-item>
<term id="G11-fspas.2022.839794">
<bold>Cycle period is the time taken to complete one cycle of an oscillation</bold>
</term>
<def>
<p>T &#x3d; [t<sub>0</sub> &#x2026; t<sub>n</sub>]</p>
</def>
</def-item>
<def-item>
<term id="G12-fspas.2022.839794">
<bold>Oscillation</bold>
</term>
<def>
<p>is a periodic variation for y(t) &#x3d; y(t &#x2b; kT) for k &#x3d; 0, 1, 2, 3,&#x2026;</p>
</def>
</def-item>
<def-item>
<term id="G13-fspas.2022.839794">
<bold>Frequency is the number of occurrences of a repeating event per unit time</bold>
</term>
<def>
<p>f &#x3d; 1/T</p>
</def>
</def-item>
<def-item>
<term id="G14-fspas.2022.839794">
<bold>Angular frequency is the rate of change of angular displacement, &#x3b8; (theta), or the rate of the change of the argument of the sine function or a cosine function</bold>
</term>
<def>
<p>y(t) &#x3d; cos(&#x3b8;(t)) &#x3d; cos(&#x3c9;t) &#x3d; cos(2&#x3c0;ft) &#x3d; cos(2&#x3c0;t/T)</p>
</def>
</def-item>
<def-item>
<term id="G15-fspas.2022.839794">
<bold>Cycle phase reference is the time when the cycle period has a maximum</bold>
</term>
<def>
<p>y(t) &#x3d; cos(&#x3b8;(t)-&#x3b8;(t<sub>0</sub>) &#x3d; cos(&#x3c9;t-&#x3c9;t<sub>0</sub>) &#x3d; cos(2&#x3c0;ft-2&#x3c0;ft<sub>0</sub>) &#x3d; cos(2&#x3c0;t/T-2&#x3c0;t<sub>0</sub>/T) &#x3d; cos(2&#x3c0;(t-t<sub>0</sub>)/T)</p>
</def>
</def-item>
<def-item>
<term id="G16-fspas.2022.839794">
<bold>Cycle maximum and minimum reference</bold>
</term>
<def>
<p>y(t &#x3d; (t<sub>0</sub>, t<sub>1</sub>))</p>
</def>
</def-item>
<def-item>
<term id="G17-fspas.2022.839794">
<bold>Cycle phase shifts</bold>
</term>
<def>
<p>y(t) &#x3d; (max, &#x2b;0, min, -0), for t &#x3d; (t<sub>0</sub>, t<sub>0</sub>&#x2b;T/4, t<sub>0</sub>&#x2b;T/2, t<sub>0</sub>&#x2b;3T/4)</p>
</def>
</def-item>
<def-item>
<term id="G18-fspas.2022.839794">
<bold>Interference</bold>
</term>
<def>
<p>two cycle periods [T<sub>1</sub>, T<sub>2</sub>] have constructive interference, y<sub>1</sub>(t)&#x2b;y<sub>2</sub>(t) &#x3d; max, when the cycle periods have phase coincidences &#x3b8;<sub>1</sub>(t<sub>0</sub>) &#x3d; &#x3b8;<sub>2</sub>(t<sub>0</sub>
<underline>)</underline> and destructive interference, y<sub>1</sub>(t)&#x2b;y<sub>2</sub>(t) &#x3d; 0, when the periods have reversed-phase coincidences &#x3b8;<sub>1</sub>(t<sub>0</sub>) &#x3d;-&#x3b8;<sub>2</sub>(t<sub>0</sub>)</p>
</def>
</def-item>
<def-item>
<term id="G19-fspas.2022.839794">
<bold>Cycle envelope period, of two cycle periods [T<sub>1</sub>, T<sub>2</sub>], is a smooth curve outlining its extremes</bold>
</term>
<def>
<p>y(t) &#x3d; y<sub>1</sub>(t)&#x2b;y<sub>2</sub>(t)</p>
</def>
</def-item>
<def-item>
<term id="G20-fspas.2022.839794">
<bold>Spectrum</bold>
</term>
<def>
<p>is a classification on a scale between two extreme points</p>
</def>
</def-item>
<def-item>
<term id="G21-fspas.2022.839794">
<bold>Cycle spectrum</bold>
</term>
<def>
<p>S(T, (&#x3b8;(t-t<sub>0</sub>)), where T &#x3d; (T<sub>1</sub> &#x2026; T<sub>n</sub>), and &#x3b8;(t-t<sub>0</sub>) &#x3d; (&#x3b8;(t-t<sub>0</sub>)<sub>1</sub> &#x2026; &#x3b8;(t-t<sub>0</sub>)<sub>n</sub>)</p>
</def>
</def-item>
<def-item>
<term id="G22-fspas.2022.839794">
<bold>Cycle period k in a spectrum</bold>
</term>
<def>
<p>T(k) &#x3d; (T<sub>1</sub> &#x2026; T<sub>k</sub> &#x2026; T<sub>n</sub>)</p>
</def>
</def-item>
<def-item>
<term id="G23-fspas.2022.839794">
<bold>Harmonic cycle spectrum</bold>
</term>
<def>
<p>T<sub>har</sub> &#x3d; (T, 2T, 3&#xa0;T &#x2026; )</p>
</def>
</def-item>
<def-item>
<term id="G24-fspas.2022.839794">
<bold>Cycle coincidence spectrum</bold>
</term>
<def>
<p>T<sub>co</sub> &#x3d; (A&#x2217;T<sub>1</sub> &#x3d; B&#x2217;T<sub>2</sub> &#x3d; C&#x2217;T<sub>1</sub>)</p>
</def>
</def-item>
<def-item>
<term id="G25-fspas.2022.839794">
<bold>Sjsun(Tjsun, &#x3b8;jsub(t-t<sub>0</sub>))</bold>
</term>
<def>
<p>jovian planets (Jupiter, Saturn, Uranus, Neptune) cycle spectrum</p>
</def>
</def-item>
<def-item>
<term id="G28-fspas.2022.839794">
<bold>Ssst(Tsst, &#x3b8;sst(t-t<sub>0</sub>))</bold>
</term>
<def>
<p>solar forced Sea surface (SST) cycle spectrum</p>
</def>
</def-item>
<def-item>
<term id="G29-fspas.2022.839794">
<bold>Sln(Tln, &#x3b8;ln(t-t<sub>0</sub>))</bold>
</term>
<def>
<p>lunar Nodal (LN) cycle spectrum</p>
</def>
</def-item>
<def-item>
<term id="G30-fspas.2022.839794">
<bold>Slst(Tlst, &#x3b8;lst(t-t<sub>0</sub>))</bold>
</term>
<def>
<p>lunar forced Sea surface (LST) cycle spectrum</p>
</def>
</def-item>
<def-item>
<term id="G31-fspas.2022.839794">
<bold>Sglt(Tglt, &#x3b8;glt(t-t<sub>0</sub>))</bold>
</term>
<def>
<p>global Land surface temperature (GLT) cycle spectrum</p>
</def>
</def-item>
<def-item>
<term id="G32-fspas.2022.839794">
<bold>Sgst(Tgst, &#x3b8;gst(t-t<sub>0</sub>))</bold>
</term>
<def>
<p>global Sea surface temperature (GST) cycle spectrum</p>
</def>
</def-item>
<def-item>
<term id="G33-fspas.2022.839794">
<bold>Sgmt(Tgmt, &#x3b8;gmt(t-t<sub>0</sub>))</bold>
</term>
<def>
<p>global Mean Temperature (GMT) cycle spectrum</p>
</def>
</def-item>
<def-item>
<term id="G34-fspas.2022.839794">
<bold>Sgrt(Tgrt, &#x3b8;grt(t-t<sub>0</sub>))</bold>
</term>
<def>
<p>Greenland Temperature (GRT) cycle spectrum</p>
</def>
</def-item>
<def-item>
<term id="G35-fspas.2022.839794">
<bold>Serr(Terr, &#x3b8;err(t-t<sub>0</sub>))</bold>
</term>
<def>
<p>temperature cycle spectrum from an unknown source</p>
</def>
</def-item>
<def-item>
<term id="G36-fspas.2022.839794">
<bold>Spectrum transfer function</bold>
</term>
<def>
<p>H(T<sub>h</sub>, &#x3b8;<sub>h</sub>(t<sub>h</sub>)) &#x3d; H(T<sub>2</sub>/T<sub>1</sub>, &#x3b8;<sub>h</sub>(t<sub>h</sub>))&#x3d; &#x3b8;<sub>1</sub>(t<sub>1</sub>)-&#x3b8;<sub>2</sub>(t<sub>2</sub>))</p>
</def>
</def-item>
<def-item>
<term id="G37-fspas.2022.839794">
<bold>Spectrum transformation</bold>
</term>
<def>
<p>S<sub>2</sub>(T<sub>2</sub>, &#x3d; T<sub>h</sub>&#x2217;T<sub>1</sub>, &#x3b8;<sub>2</sub>(t<sub>1</sub>-t<sub>h</sub>)) &#x3d; H(T<sub>h</sub>, &#x3b8;<sub>1</sub>(t<sub>h</sub>))S<sub>1</sub>(T<sub>1</sub>, &#x3b8;<sub>1</sub>(t<sub>1</sub>
<underline>)</underline>)</p>
</def>
</def-item>
<def-item>
<term id="G38-fspas.2022.839794">
<bold>Hsun(Tsun, &#x3b8;sun(t<sub>sun</sub>))</bold>
</term>
<def>
<p>linear transform of JSUN cycles to TSI cycles</p>
</def>
</def-item>
<def-item>
<term id="G40-fspas.2022.839794">
<bold>Hoce(Toce, &#x3b8;oce(t<sub>oce</sub>))</bold>
</term>
<def>
<p>linear transform of Earth nutation cycles to LSR cycles</p>
</def>
</def-item>
<def-item>
<term id="G41-fspas.2022.839794">
<bold>Wglt(s, t))</bold>
</term>
<def>
<p>global land surface temperature wavelet spectrum</p>
</def>
</def-item>
<def-item>
<term id="G42-fspas.2022.839794">
<bold>Wgst(s, t))</bold>
</term>
<def>
<p>global sea surface temperature wavelet spectrum</p>
</def>
</def-item>
<def-item>
<term id="G43-fspas.2022.839794">
<bold>Wgms(s, t))</bold>
</term>
<def>
<p>global mean surface temperature wavelet spectrum</p>
</def>
</def-item>
<def-item>
<term id="G44-fspas.2022.839794">
<bold>Wgrt(s, t))</bold>
</term>
<def>
<p>greenland temperature wavelet spectrum</p>
</def>
</def-item>
<def-item>
<term id="G45-fspas.2022.839794">
<bold>WPgrt(s, t))</bold>
</term>
<def>
<p>greenland temperature wavelet power spectrum</p>
</def>
</def-item>
<def-item>
<term id="G46-fspas.2022.839794">
<bold>WAglt(R, m))</bold>
</term>
<def>
<p>global land surface temperature wavelet autocorrelation spectrum</p>
</def>
</def-item>
<def-item>
<term id="G47-fspas.2022.839794">
<bold>WAgst(R, m))</bold>
</term>
<def>
<p>global sea surface temperature wavelet autocorrelation spectrum</p>
</def>
</def-item>
<def-item>
<term id="G48-fspas.2022.839794">
<bold>WAgms(R, m))</bold>
</term>
<def>
<p>global mean surface temperature wavelet autocorrelation spectrum</p>
</def>
</def-item>
<def-item>
<term id="G49-fspas.2022.839794">
<bold>WAgrt(R, m))</bold>
</term>
<def>
<p>greenland temperature wavelet autocorrelation spectrum</p>
</def>
</def-item>
</def-list>
</sec>
</back>
</article>