<?xml version="1.0"?>
<feed xmlns="http://www.w3.org/2005/Atom" xml:lang="en">
	<id>https://lunarpedia.org/index.php?action=history&amp;feed=atom&amp;title=Solar_wind</id>
	<title>Solar wind - Revision history</title>
	<link rel="self" type="application/atom+xml" href="https://lunarpedia.org/index.php?action=history&amp;feed=atom&amp;title=Solar_wind"/>
	<link rel="alternate" type="text/html" href="https://lunarpedia.org/index.php?title=Solar_wind&amp;action=history"/>
	<updated>2026-04-30T16:23:08Z</updated>
	<subtitle>Revision history for this page on the wiki</subtitle>
	<generator>MediaWiki 1.34.2</generator>
	<entry>
		<id>https://lunarpedia.org/index.php?title=Solar_wind&amp;diff=12481&amp;oldid=prev</id>
		<title>Jarogers2001 at 17:44, 3 August 2008</title>
		<link rel="alternate" type="text/html" href="https://lunarpedia.org/index.php?title=Solar_wind&amp;diff=12481&amp;oldid=prev"/>
		<updated>2008-08-03T17:44:16Z</updated>

		<summary type="html">&lt;p&gt;&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;tr class=&quot;diff-title&quot; lang=&quot;en&quot;&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;Revision as of 17:44, 3 August 2008&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l1&quot; &gt;Line 1:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 1:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;The '''solar wind''' is a stream of charged particles emitted by the sun.  The solar wind is primarily protons ([[hydrogen]] ions), but also has some components of higher mass, including deuterium and [[helium]], as well as electrons. The solar wind has a density of a few particles per cubic centimeter, and moves at a speed of a bit over a million km/hr.  Both the density and the speed of the solar wind change with the activity of the sun.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;The '''solar wind''' is a stream of charged particles emitted by the sun.  The solar wind is primarily protons ([[hydrogen]] ions), but also has some components of higher mass, including deuterium and [[helium]], as well as electrons. The solar wind has a density of a few particles per cubic centimeter, and moves at a speed of a bit over a million km/hr.  Both the density and the speed of the solar wind change with the activity of the sun.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;The solar wind is deflected by magnetic fields, and hence does not directly impact the Earth's surface or atmosphere.  Lacking a magnetic field, the moon is directly exposed to the solar wind, and hence solar wind elements can be found implanted into [[Lunar regolith]].  Hydrogen implanted into the [[Lunar Soil]] might be a resource for lunar [[In Situ Resource Utilization]] (see [[&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;Volatile Scavenging&lt;/del&gt;]], and [[Helium 3]] from the solar wind has been proposed as possible fusion fuel.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;The solar wind is deflected by magnetic fields, and hence does not directly impact the Earth's surface or atmosphere.  Lacking a magnetic field, the moon is directly exposed to the solar wind, and hence solar wind elements can be found implanted into [[Lunar regolith]].  Hydrogen implanted into the [[Lunar Soil]] might be a resource for lunar [[In Situ Resource Utilization]] (see [[&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;Volatiles&lt;/ins&gt;]], and [[Helium 3]] from the solar wind has been proposed as possible fusion fuel.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;One proposed method of space propulsion is to ''sail'' on the solar wind using a &amp;quot;magnetic sail&amp;quot; (&amp;quot;Magsail&amp;quot;) or a &amp;quot;Mini-magnetosphere Plasma Propulsion&amp;quot; (&amp;quot;M2P2&amp;quot;) sail.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;One proposed method of space propulsion is to ''sail'' on the solar wind using a &amp;quot;magnetic sail&amp;quot; (&amp;quot;Magsail&amp;quot;) or a &amp;quot;Mini-magnetosphere Plasma Propulsion&amp;quot; (&amp;quot;M2P2&amp;quot;) sail.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;

&lt;!-- diff cache key lunarpedia_prod-mw_:diff::1.12:old-8664:rev-12481 --&gt;
&lt;/table&gt;</summary>
		<author><name>Jarogers2001</name></author>
		
	</entry>
	<entry>
		<id>https://lunarpedia.org/index.php?title=Solar_wind&amp;diff=8664&amp;oldid=prev</id>
		<title>Strangelv: sorted Space Stub</title>
		<link rel="alternate" type="text/html" href="https://lunarpedia.org/index.php?title=Solar_wind&amp;diff=8664&amp;oldid=prev"/>
		<updated>2007-04-19T20:37:43Z</updated>

		<summary type="html">&lt;p&gt;sorted Space Stub&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;tr class=&quot;diff-title&quot; lang=&quot;en&quot;&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;Revision as of 20:37, 19 April 2007&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l6&quot; &gt;Line 6:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 6:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;{{&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;stub&lt;/del&gt;}}&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;{{&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;Space Stub&lt;/ins&gt;}}&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;

&lt;!-- diff cache key lunarpedia_prod-mw_:diff::1.12:old-4257:rev-8664 --&gt;
&lt;/table&gt;</summary>
		<author><name>Strangelv</name></author>
		
	</entry>
	<entry>
		<id>https://lunarpedia.org/index.php?title=Solar_wind&amp;diff=4257&amp;oldid=prev</id>
		<title>Geoffrey.landis: corrected link</title>
		<link rel="alternate" type="text/html" href="https://lunarpedia.org/index.php?title=Solar_wind&amp;diff=4257&amp;oldid=prev"/>
		<updated>2007-02-06T22:45:10Z</updated>

		<summary type="html">&lt;p&gt;corrected link&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;tr class=&quot;diff-title&quot; lang=&quot;en&quot;&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;Revision as of 22:45, 6 February 2007&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l1&quot; &gt;Line 1:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 1:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;The '''solar wind''' is a stream of charged particles emitted by the sun.  The solar wind is primarily protons ([[hydrogen]] ions), but also has some components of higher mass, including deuterium and [[helium]], as well as electrons. The solar wind has a density of a few particles per cubic centimeter, and moves at a speed of a bit over a million km/hr.  Both the density and the speed of the solar wind change with the activity of the sun.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;The '''solar wind''' is a stream of charged particles emitted by the sun.  The solar wind is primarily protons ([[hydrogen]] ions), but also has some components of higher mass, including deuterium and [[helium]], as well as electrons. The solar wind has a density of a few particles per cubic centimeter, and moves at a speed of a bit over a million km/hr.  Both the density and the speed of the solar wind change with the activity of the sun.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;The solar wind is deflected by magnetic fields, and hence does not directly impact the Earth's surface or atmosphere.  Lacking a magnetic field, the moon is directly exposed to the solar wind, and hence solar wind elements can be found implanted into [[Lunar regolith]].  Hydrogen implanted into the [[Lunar &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;soil&lt;/del&gt;]] might be a resource for lunar [[In Situ Resource Utilization]] (see [[Volatile Scavenging]], and [[Helium 3]] from the solar wind has been proposed as possible fusion fuel.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;The solar wind is deflected by magnetic fields, and hence does not directly impact the Earth's surface or atmosphere.  Lacking a magnetic field, the moon is directly exposed to the solar wind, and hence solar wind elements can be found implanted into [[Lunar regolith]].  Hydrogen implanted into the [[Lunar &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;Soil&lt;/ins&gt;]] might be a resource for lunar [[In Situ Resource Utilization]] (see [[Volatile Scavenging]], and [[Helium 3]] from the solar wind has been proposed as possible fusion fuel.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;One proposed method of space propulsion is to ''sail'' on the solar wind using a &amp;quot;magnetic sail&amp;quot; (&amp;quot;Magsail&amp;quot;) or a &amp;quot;Mini-magnetosphere Plasma Propulsion&amp;quot; (&amp;quot;M2P2&amp;quot;) sail.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;One proposed method of space propulsion is to ''sail'' on the solar wind using a &amp;quot;magnetic sail&amp;quot; (&amp;quot;Magsail&amp;quot;) or a &amp;quot;Mini-magnetosphere Plasma Propulsion&amp;quot; (&amp;quot;M2P2&amp;quot;) sail.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;

&lt;!-- diff cache key lunarpedia_prod-mw_:diff::1.12:old-4256:rev-4257 --&gt;
&lt;/table&gt;</summary>
		<author><name>Geoffrey.landis</name></author>
		
	</entry>
	<entry>
		<id>https://lunarpedia.org/index.php?title=Solar_wind&amp;diff=4256&amp;oldid=prev</id>
		<title>Geoffrey.landis: updated links</title>
		<link rel="alternate" type="text/html" href="https://lunarpedia.org/index.php?title=Solar_wind&amp;diff=4256&amp;oldid=prev"/>
		<updated>2007-02-06T22:44:18Z</updated>

		<summary type="html">&lt;p&gt;updated links&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;tr class=&quot;diff-title&quot; lang=&quot;en&quot;&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;Revision as of 22:44, 6 February 2007&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l1&quot; &gt;Line 1:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 1:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;The '''solar wind''' is a stream of charged particles emitted by the sun.  The solar wind is primarily protons ([[hydrogen]] ions), but also has some components of higher mass, including deuterium and [[helium]], as well as electrons. The solar wind has a density of a few particles per cubic centimeter, and moves at a speed of a bit over a million km/hr.  Both the density and the speed of the solar wind change with the activity of the sun.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;The '''solar wind''' is a stream of charged particles emitted by the sun.  The solar wind is primarily protons ([[hydrogen]] ions), but also has some components of higher mass, including deuterium and [[helium]], as well as electrons. The solar wind has a density of a few particles per cubic centimeter, and moves at a speed of a bit over a million km/hr.  Both the density and the speed of the solar wind change with the activity of the sun.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;The solar wind is deflected by magnetic fields, and hence does not directly impact the Earth's surface or atmosphere.  Lacking a magnetic field, the moon is directly exposed to the solar wind, and hence solar wind elements can be found implanted into &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;lunar &lt;/del&gt;[[regolith]].  Hydrogen implanted into the soil might be a resource for lunar [[In Situ Resource Utilization]] (see [[Volatile Scavenging]], and [[Helium 3]] from the solar wind has been proposed as possible fusion fuel.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;The solar wind is deflected by magnetic fields, and hence does not directly impact the Earth's surface or atmosphere.  Lacking a magnetic field, the moon is directly exposed to the solar wind, and hence solar wind elements can be found implanted into [[&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;Lunar &lt;/ins&gt;regolith]].  Hydrogen implanted into the &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;[[Lunar &lt;/ins&gt;soil&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;]] &lt;/ins&gt;might be a resource for lunar [[In Situ Resource Utilization]] (see [[Volatile Scavenging]], and [[Helium 3]] from the solar wind has been proposed as possible fusion fuel.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;One proposed method of space propulsion is to ''sail'' on the solar wind using a &amp;quot;magnetic sail&amp;quot; (&amp;quot;Magsail&amp;quot;) or a &amp;quot;Mini-magnetosphere Plasma Propulsion&amp;quot; (&amp;quot;M2P2&amp;quot;) sail.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;One proposed method of space propulsion is to ''sail'' on the solar wind using a &amp;quot;magnetic sail&amp;quot; (&amp;quot;Magsail&amp;quot;) or a &amp;quot;Mini-magnetosphere Plasma Propulsion&amp;quot; (&amp;quot;M2P2&amp;quot;) sail.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;

&lt;!-- diff cache key lunarpedia_prod-mw_:diff::1.12:old-4255:rev-4256 --&gt;
&lt;/table&gt;</summary>
		<author><name>Geoffrey.landis</name></author>
		
	</entry>
	<entry>
		<id>https://lunarpedia.org/index.php?title=Solar_wind&amp;diff=4255&amp;oldid=prev</id>
		<title>Geoffrey.landis: added links, and references to sailing</title>
		<link rel="alternate" type="text/html" href="https://lunarpedia.org/index.php?title=Solar_wind&amp;diff=4255&amp;oldid=prev"/>
		<updated>2007-02-06T22:40:30Z</updated>

		<summary type="html">&lt;p&gt;added links, and references to sailing&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;tr class=&quot;diff-title&quot; lang=&quot;en&quot;&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;Revision as of 22:40, 6 February 2007&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l1&quot; &gt;Line 1:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 1:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;The '''solar wind''' is a stream of charged particles emitted by the sun.  The solar wind is primarily protons ([[hydrogen]] ions), but also has some components of higher mass, including deuterium and helium, as well as electrons. The solar wind has a density of a few particles per cubic centimeter, and moves at a speed of a bit over a million km/hr.  Both the density and the speed of the solar wind change with the activity of the &lt;del class=&quot;diffchange diffchange-inline&quot;&gt; &lt;/del&gt;sun.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;The '''solar wind''' is a stream of charged particles emitted by the sun.  The solar wind is primarily protons ([[hydrogen]] ions), but also has some components of higher mass, including deuterium and &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;[[&lt;/ins&gt;helium&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;]]&lt;/ins&gt;, as well as electrons. The solar wind has a density of a few particles per cubic centimeter, and moves at a speed of a bit over a million km/hr.  Both the density and the speed of the solar wind change with the activity of the sun.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;The solar wind is deflected by magnetic fields, and hence does not directly impact the Earth's surface or atmosphere.  Lacking a magnetic field, the moon is directly exposed to the solar wind, and hence solar wind elements can be found implanted into lunar &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;soil&lt;/del&gt;.  Hydrogen implanted into the soil might be a resource for lunar [[In Situ Resource Utilization]] (see [[Volatile Scavenging]], and [[Helium 3]] from the solar wind has been proposed as possible fusion fuel.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;The solar wind is deflected by magnetic fields, and hence does not directly impact the Earth's surface or atmosphere.  Lacking a magnetic field, the moon is directly exposed to the solar wind, and hence solar wind elements can be found implanted into lunar &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;[[regolith]]&lt;/ins&gt;.  Hydrogen implanted into the soil might be a resource for lunar [[In Situ Resource Utilization]] (see [[Volatile Scavenging]], and [[Helium 3]] from the solar wind has been proposed as possible fusion fuel&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;.&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt; &lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt; &lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt; &lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;One proposed method of space propulsion is to ''sail'' on the solar wind using a &amp;quot;magnetic sail&amp;quot; (&amp;quot;Magsail&amp;quot;) or a &amp;quot;Mini-magnetosphere Plasma Propulsion&amp;quot; (&amp;quot;M2P2&amp;quot;) sail&lt;/ins&gt;.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;{{stub}}&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;{{stub}}&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;

&lt;!-- diff cache key lunarpedia_prod-mw_:diff::1.12:old-4197:rev-4255 --&gt;
&lt;/table&gt;</summary>
		<author><name>Geoffrey.landis</name></author>
		
	</entry>
	<entry>
		<id>https://lunarpedia.org/index.php?title=Solar_wind&amp;diff=4197&amp;oldid=prev</id>
		<title>Geoffrey.landis: stub</title>
		<link rel="alternate" type="text/html" href="https://lunarpedia.org/index.php?title=Solar_wind&amp;diff=4197&amp;oldid=prev"/>
		<updated>2007-02-06T21:42:13Z</updated>

		<summary type="html">&lt;p&gt;stub&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;The '''solar wind''' is a stream of charged particles emitted by the sun.  The solar wind is primarily protons ([[hydrogen]] ions), but also has some components of higher mass, including deuterium and helium, as well as electrons. The solar wind has a density of a few particles per cubic centimeter, and moves at a speed of a bit over a million km/hr.  Both the density and the speed of the solar wind change with the activity of the  sun.&lt;br /&gt;
&lt;br /&gt;
The solar wind is deflected by magnetic fields, and hence does not directly impact the Earth's surface or atmosphere.  Lacking a magnetic field, the moon is directly exposed to the solar wind, and hence solar wind elements can be found implanted into lunar soil.  Hydrogen implanted into the soil might be a resource for lunar [[In Situ Resource Utilization]] (see [[Volatile Scavenging]], and [[Helium 3]] from the solar wind has been proposed as possible fusion fuel.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{{stub}}&lt;/div&gt;</summary>
		<author><name>Geoffrey.landis</name></author>
		
	</entry>
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