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	<id>https://wiki.fusiongirl.app:443/index.php?action=history&amp;feed=atom&amp;title=Solar_Cycles</id>
	<title>Solar Cycles - Revision history</title>
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	<updated>2026-05-12T10:41:45Z</updated>
	<subtitle>Revision history for this page on the wiki</subtitle>
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	<entry>
		<id>https://wiki.fusiongirl.app:443/index.php?title=Solar_Cycles&amp;diff=7069&amp;oldid=prev</id>
		<title>JonoThora: Psionics expansion (01a + 01b): content authored / LaTeX-restored per local submodule; lint-clean.</title>
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		<updated>2026-05-11T20:54:03Z</updated>

		<summary type="html">&lt;p&gt;Psionics expansion (01a + 01b): content authored / LaTeX-restored per local submodule; lint-clean.&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;{{Audience_Sidebar&lt;br /&gt;
| difficulty   = Introductory&lt;br /&gt;
| reading_time = 5 minutes&lt;br /&gt;
| prerequisites = [[Psionics_Primer]]; basic astronomy.&lt;br /&gt;
| if_too_advanced_see = [[Space_Weather]]&lt;br /&gt;
| if_you_want_the_math_see = [[Space_Weather]]&lt;br /&gt;
}}&lt;br /&gt;
&lt;br /&gt;
== Summary ==&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;&amp;#039;Solar cycles&amp;#039;&amp;#039;&amp;#039; are the quasi-periodic variations in solar magnetic activity, most prominently the &amp;#039;&amp;#039;&amp;#039;~ 11-year sunspot cycle&amp;#039;&amp;#039;&amp;#039; first systematically recorded by Heinrich Schwabe in 1843. The cycle is now understood to be the half-period of the longer ~ 22-year &amp;#039;&amp;#039;&amp;#039;Hale magnetic-polarity cycle&amp;#039;&amp;#039;&amp;#039;. Cycles are numbered sequentially from the 1755 minimum (Cycle 1) through the current Cycle 25 (started December 2019).&lt;br /&gt;
&lt;br /&gt;
The cycle drives [[Space_Weather|space-weather]] activity, modulates [[Geomagnetic_Field|geomagnetic-field]] variability, and through these channels influences the Earth&amp;#039;s near-space EM environment.&lt;br /&gt;
&lt;br /&gt;
== Cycle Structure ==&lt;br /&gt;
&lt;br /&gt;
* &amp;#039;&amp;#039;&amp;#039;Minimum&amp;#039;&amp;#039;&amp;#039;: low sunspot count; few flares / CMEs; quiet magnetosphere.&lt;br /&gt;
* &amp;#039;&amp;#039;&amp;#039;Rising phase&amp;#039;&amp;#039;&amp;#039;: sunspot count increases; activity from low latitudes migrates equatorward over the cycle.&lt;br /&gt;
* &amp;#039;&amp;#039;&amp;#039;Maximum&amp;#039;&amp;#039;&amp;#039;: peak sunspot count (typically 100-300); maximum flare / CME activity; frequent geomagnetic storms.&lt;br /&gt;
* &amp;#039;&amp;#039;&amp;#039;Declining phase&amp;#039;&amp;#039;&amp;#039;: sunspot count falls; coronal-hole-driven recurring storms become dominant.&lt;br /&gt;
&lt;br /&gt;
The mean cycle length is 11 years but individual cycles range from ~ 9 to ~ 14 years. Cycle &amp;#039;&amp;#039;&amp;#039;amplitude&amp;#039;&amp;#039;&amp;#039; (peak sunspot count) varies substantially: the Maunder Minimum (1645-1715) had essentially no sunspots; the late 20th century cycles were among the strongest in instrumental history.&lt;br /&gt;
&lt;br /&gt;
== Hale Cycle ==&lt;br /&gt;
&lt;br /&gt;
The ~ 22-year Hale cycle reflects &amp;#039;&amp;#039;&amp;#039;magnetic-polarity reversal&amp;#039;&amp;#039;&amp;#039; between successive 11-year cycles: the magnetic polarity of leading sunspots in each hemisphere reverses between cycles. Two successive 11-year cycles thus complete one Hale cycle.&lt;br /&gt;
&lt;br /&gt;
== Effects on Earth ==&lt;br /&gt;
&lt;br /&gt;
* &amp;#039;&amp;#039;&amp;#039;Atmospheric heating&amp;#039;&amp;#039;&amp;#039; (small): increased solar UV / EUV at maximum heats the upper atmosphere, slightly inflating the thermosphere.&lt;br /&gt;
* &amp;#039;&amp;#039;&amp;#039;Cosmic-ray modulation&amp;#039;&amp;#039;&amp;#039; (anti-correlated with cycle): strong solar wind during high-activity periods deflects galactic cosmic rays; ground-level cosmic-ray flux is highest at solar minimum.&lt;br /&gt;
* &amp;#039;&amp;#039;&amp;#039;Climate effects&amp;#039;&amp;#039;&amp;#039;: contested. Total solar irradiance varies by only ~ 0.1% across the cycle, producing climate effects of similar order. Cosmic-ray modulation effects on cloud cover (Svensmark hypothesis) are debated.&lt;br /&gt;
* &amp;#039;&amp;#039;&amp;#039;Space-weather frequency&amp;#039;&amp;#039;&amp;#039;: dramatically higher during cycle maximum.&lt;br /&gt;
* &amp;#039;&amp;#039;&amp;#039;Ozone-layer variability&amp;#039;&amp;#039;&amp;#039;: solar UV modulation drives small (~ 1-3%) ozone variation tracking the cycle.&lt;br /&gt;
&lt;br /&gt;
== Long-Term Variability ==&lt;br /&gt;
&lt;br /&gt;
Beyond the 11/22-year cycles, longer-term modulations include:&lt;br /&gt;
&lt;br /&gt;
* &amp;#039;&amp;#039;&amp;#039;Gleissberg cycle&amp;#039;&amp;#039;&amp;#039; (~ 87 years): amplitude modulation of successive 11-year cycles.&lt;br /&gt;
* &amp;#039;&amp;#039;&amp;#039;Suess / de Vries cycle&amp;#039;&amp;#039;&amp;#039; (~ 208 years).&lt;br /&gt;
* &amp;#039;&amp;#039;&amp;#039;Hallstatt cycle&amp;#039;&amp;#039;&amp;#039; (~ 2400 years).&lt;br /&gt;
* &amp;#039;&amp;#039;&amp;#039;Grand minima&amp;#039;&amp;#039;&amp;#039; (Maunder 1645-1715, Spörer ~ 1450-1550, Wolf ~ 1280-1350, Oort ~ 1010-1050): periods of suppressed activity lasting decades.&lt;br /&gt;
&lt;br /&gt;
These long-term variations are derived from cosmogenic-isotope (¹⁴C, ¹⁰Be) records in tree rings and ice cores.&lt;br /&gt;
&lt;br /&gt;
== Current Cycle Status ==&lt;br /&gt;
&lt;br /&gt;
Cycle 25 (started December 2019) has been more active than predicted; peak now expected late 2024 - mid 2025. Cycle 24 (2008-2019) was the weakest cycle since Cycle 14 (early 20th century).&lt;br /&gt;
&lt;br /&gt;
== Psionic Relevance ==&lt;br /&gt;
&lt;br /&gt;
In the [[Psionics|psionic framework]], the solar cycle is the dominant &amp;#039;&amp;#039;&amp;#039;long-timescale modulator&amp;#039;&amp;#039;&amp;#039; of the Earth&amp;#039;s near-space EM environment. Predicted ψ-field-mediated environmental-coupling effects should show solar-cycle modulation, providing one of the framework&amp;#039;s longer-timescale empirical-test windows.&lt;br /&gt;
&lt;br /&gt;
== See Also ==&lt;br /&gt;
&lt;br /&gt;
* [[Space_Weather]]&lt;br /&gt;
* [[Geomagnetic_Field]]&lt;br /&gt;
* [[Geomagnetic_Indices_Kp_Dst]]&lt;br /&gt;
* [[Solar_Cycle_24]]&lt;br /&gt;
* [[Solar_Cycle_25]]&lt;br /&gt;
&lt;br /&gt;
== External Links ==&lt;br /&gt;
&lt;br /&gt;
* Wikipedia: Solar cycle&lt;br /&gt;
* SILSO (Sunspot Index and Long-term Solar Observations).&lt;br /&gt;
* NOAA Solar Cycle Progression.&lt;br /&gt;
&lt;br /&gt;
== References ==&lt;br /&gt;
&lt;br /&gt;
* Hathaway, D. H. (2015). &amp;quot;The solar cycle.&amp;quot; &amp;#039;&amp;#039;Living Reviews in Solar Physics&amp;#039;&amp;#039; 12: 4.&lt;br /&gt;
* Usoskin, I. G. (2017). &amp;quot;A history of solar activity over millennia.&amp;quot; &amp;#039;&amp;#039;Living Reviews in Solar Physics&amp;#039;&amp;#039; 14: 3.&lt;br /&gt;
&lt;br /&gt;
[[Category:Psionics]]&lt;br /&gt;
[[Category:Environmental EM]]&lt;br /&gt;
[[Category:Solar Physics]]&lt;/div&gt;</summary>
		<author><name>JonoThora</name></author>
	</entry>
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