<?xml version="1.0"?>
<feed xmlns="http://www.w3.org/2005/Atom" xml:lang="en">
	<id>http://marspedia.org/index.php?action=history&amp;feed=atom&amp;title=Coronal_Mass_Ejections</id>
	<title>Coronal Mass Ejections - Revision history</title>
	<link rel="self" type="application/atom+xml" href="http://marspedia.org/index.php?action=history&amp;feed=atom&amp;title=Coronal_Mass_Ejections"/>
	<link rel="alternate" type="text/html" href="http://marspedia.org/index.php?title=Coronal_Mass_Ejections&amp;action=history"/>
	<updated>2026-05-05T22:32:16Z</updated>
	<subtitle>Revision history for this page on the wiki</subtitle>
	<generator>MediaWiki 1.34.2</generator>
	<entry>
		<id>http://marspedia.org/index.php?title=Coronal_Mass_Ejections&amp;diff=141665&amp;oldid=prev</id>
		<title>RichardWSmith: Gave common name in introduction.</title>
		<link rel="alternate" type="text/html" href="http://marspedia.org/index.php?title=Coronal_Mass_Ejections&amp;diff=141665&amp;oldid=prev"/>
		<updated>2024-09-20T17:12:28Z</updated>

		<summary type="html">&lt;p&gt;Gave common name in introduction.&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 17:12, 20 September 2024&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;[[Image:Cme.jpg|thumb|200px|right|A Solar and Heliospheric Observatory (LASCO) observation of a CME.]]  &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;[[Image:Cme.jpg|thumb|200px|right|A Solar and Heliospheric Observatory (LASCO) observation of a CME.]]  &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;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;'''Coronal Mass Ejections''' (CMEs) are a direct result of magnetic instabilities (i.e. [[solar flares]]) on the surface of the [[Sun]] erupting and expelling millions of tons of solar plasma into interplanetary space. CMEs are strongly influenced by the interplanetary magnetic field (IMF).  &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;'''Coronal Mass Ejections''' (CMEs&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;) (also known as &amp;quot;Solar Storms&amp;quot;&lt;/ins&gt;) are a direct result of magnetic instabilities (i.e. [[solar flares]]) on the surface of the [[Sun]] erupting and expelling millions of tons of solar plasma into interplanetary space. CMEs are strongly influenced by the interplanetary magnetic field (IMF).  &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;Note that most CME's are small and low energy.  However, rare powerful CME's create very dangerous solar storms which require far more shielding.  Space travellers and martian colonists should enter a [[Storm shelter]] for radiation protection.&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;Note that most CME's are small and low energy.  However, rare powerful CME's create very dangerous solar storms which require far more shielding.  Space travellers and martian colonists should enter a [[Storm shelter]] for radiation protection.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>RichardWSmith</name></author>
		
	</entry>
	<entry>
		<id>http://marspedia.org/index.php?title=Coronal_Mass_Ejections&amp;diff=141605&amp;oldid=prev</id>
		<title>RichardWSmith: /* A hazard to settlers? */ You need a storm shelter during a solar storm.</title>
		<link rel="alternate" type="text/html" href="http://marspedia.org/index.php?title=Coronal_Mass_Ejections&amp;diff=141605&amp;oldid=prev"/>
		<updated>2024-09-16T13:40:20Z</updated>

		<summary type="html">&lt;p&gt;&lt;span dir=&quot;auto&quot;&gt;&lt;span class=&quot;autocomment&quot;&gt;A hazard to settlers?: &lt;/span&gt; You need a storm shelter during a solar storm.&lt;/span&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 13:40, 16 September 2024&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-l14&quot; &gt;Line 14:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 14:&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;However, the assumption that we must have radiations level equal to or lower than the average level on Earth is very suspect.  The city of Ramsar in Iran has radiation levels 50 times higher than the typical value on Earth.  The people in this city exhibit no higher rates of cancer or disease than are typical for Earth.  (See [[Radiation]] for references.)  It is likely that people living on Mars will simply accept higher rates of radiation.&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;However, the assumption that we must have radiations level equal to or lower than the average level on Earth is very suspect.  The city of Ramsar in Iran has radiation levels 50 times higher than the typical value on Earth.  The people in this city exhibit no higher rates of cancer or disease than are typical for Earth.  (See [[Radiation]] for references.)  It is likely that people living on Mars will simply accept higher rates of radiation.&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 style=&quot;font-weight: bold; text-decoration: none;&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;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;That said, a powerful solar storm is dangerous, and if it happens during the day time, settlers will need to be in a storm shelter.&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;div&gt;==Detecting damaging CME ions==  &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;==Detecting damaging CME ions==  &lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;

&lt;!-- diff cache key marspediaorg_www-mwmars_:diff::1.12:old-141601:rev-141605 --&gt;
&lt;/table&gt;</summary>
		<author><name>RichardWSmith</name></author>
		
	</entry>
	<entry>
		<id>http://marspedia.org/index.php?title=Coronal_Mass_Ejections&amp;diff=141601&amp;oldid=prev</id>
		<title>RichardWSmith: Added a paragraph that says Martians will likely accept higher radiation doses than what is found on Earth.</title>
		<link rel="alternate" type="text/html" href="http://marspedia.org/index.php?title=Coronal_Mass_Ejections&amp;diff=141601&amp;oldid=prev"/>
		<updated>2024-09-15T13:35:05Z</updated>

		<summary type="html">&lt;p&gt;Added a paragraph that says Martians will likely accept higher radiation doses than what is found on Earth.&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 13:35, 15 September 2024&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-l11&quot; &gt;Line 11:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 11:&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;In addition, the Earth's atmosphere is over 100 times thicker than Mars'. This greatly increases the insulation of the planet from solar energetic particles, magnifying the intensity of aurorae. The Earth's atmosphere has the protective thickness equivalent to 10.3 meters of water,&amp;lt;ref&amp;gt;See discussion section. &amp;lt;/ref&amp;gt; or approximately 3.4 meters of [[regolith]] (very important when considering [[hillside settlement|settlement design]]). The protective thickness of Mars' atmosphere is equal to only about a 27 cm thickness of water.  &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;In addition, the Earth's atmosphere is over 100 times thicker than Mars'. This greatly increases the insulation of the planet from solar energetic particles, magnifying the intensity of aurorae. The Earth's atmosphere has the protective thickness equivalent to 10.3 meters of water,&amp;lt;ref&amp;gt;See discussion section. &amp;lt;/ref&amp;gt; or approximately 3.4 meters of [[regolith]] (very important when considering [[hillside settlement|settlement design]]). The protective thickness of Mars' atmosphere is equal to only about a 27 cm thickness of water.  &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;[[Settlement]] designers must therefore assume that Mars' atmosphere will not protect settlers from high energy, ionizing particles emitted from the 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;[[Settlement]] designers must therefore assume that Mars' atmosphere will not protect settlers from high energy, ionizing particles emitted from the Sun&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;However, the assumption that we must have radiations level equal to or lower than the average level on Earth is very suspect.  The city of Ramsar in Iran has radiation levels 50 times higher than the typical value on Earth.  The people in this city exhibit no higher rates of cancer or disease than are typical for Earth.  (See [[Radiation]] for references.)  It is likely that people living on Mars will simply accept higher rates of radiation&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;div&gt;==Detecting damaging CME ions==  &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;==Detecting damaging CME ions==  &lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>RichardWSmith</name></author>
		
	</entry>
	<entry>
		<id>http://marspedia.org/index.php?title=Coronal_Mass_Ejections&amp;diff=141600&amp;oldid=prev</id>
		<title>RichardWSmith: Added two links, and mentioned powerful CME's are rare.</title>
		<link rel="alternate" type="text/html" href="http://marspedia.org/index.php?title=Coronal_Mass_Ejections&amp;diff=141600&amp;oldid=prev"/>
		<updated>2024-09-15T10:31:33Z</updated>

		<summary type="html">&lt;p&gt;Added two links, and mentioned powerful CME&amp;#039;s are rare.&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 10:31, 15 September 2024&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;[[Image:Cme.jpg|thumb|200px|right|A Solar and Heliospheric Observatory (LASCO) observation of a CME.]]  &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;[[Image:Cme.jpg|thumb|200px|right|A Solar and Heliospheric Observatory (LASCO) observation of a CME.]]  &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;div&gt;'''Coronal Mass Ejections''' (CMEs) are a direct result of magnetic instabilities (i.e. [[solar flares]]) on the surface of the [[Sun]] erupting and expelling millions of tons of solar plasma into interplanetary space. CMEs are strongly influenced by the interplanetary magnetic field (IMF).  &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;'''Coronal Mass Ejections''' (CMEs) are a direct result of magnetic instabilities (i.e. [[solar flares]]) on the surface of the [[Sun]] erupting and expelling millions of tons of solar plasma into interplanetary space. CMEs are strongly influenced by the interplanetary magnetic field (IMF).  &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 style=&quot;font-weight: bold; text-decoration: none;&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;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;Note that most CME's are small and low energy.  However, rare powerful CME's create very dangerous solar storms which require far more shielding.  Space travellers and martian colonists should enter a [[Storm shelter]] for radiation protection.&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;ins style=&quot;font-weight: bold; text-decoration: none;&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;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;See also [[Solar Cosmic Rays]].&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;div&gt;==A hazard to settlers?==  &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;==A hazard to settlers?==  &lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;

&lt;!-- diff cache key marspediaorg_www-mwmars_:diff::1.12:old-141116:rev-141600 --&gt;
&lt;/table&gt;</summary>
		<author><name>RichardWSmith</name></author>
		
	</entry>
	<entry>
		<id>http://marspedia.org/index.php?title=Coronal_Mass_Ejections&amp;diff=141116&amp;oldid=prev</id>
		<title>RichardWSmith: Earth can warn Mars, except when in opposition.</title>
		<link rel="alternate" type="text/html" href="http://marspedia.org/index.php?title=Coronal_Mass_Ejections&amp;diff=141116&amp;oldid=prev"/>
		<updated>2024-07-02T08:30:16Z</updated>

		<summary type="html">&lt;p&gt;Earth can warn Mars, except when in opposition.&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 08:30, 2 July 2024&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-l14&quot; &gt;Line 14:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 14:&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;===A contingency for Mars===  &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;===A contingency for Mars===  &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;div&gt;Currently, Mars has no probe or observatory in the line of sight (LOS) of the Sun, leaving an unpatrolled expanse of interplanetary space for dangerous solar ions to pass unchecked. A possible solution (akin to the Earth's SoHO&amp;lt;ref&amp;gt;[http://sohowww.nascom.nasa.gov/ SoHO mission page.]&amp;lt;/ref&amp;gt; or ACE&amp;lt;ref&amp;gt;[http://www.swpc.noaa.gov/ace/ ACE mission page.]&amp;lt;/ref&amp;gt; observatories) could be to establish a simple and inexpensive solar observatory at the first Lagrangian Point&amp;lt;ref&amp;gt;[http://en.wikipedia.org/wiki/Lagrangian_point Lagrangian Point on Wikipedia.]&amp;lt;/ref&amp;gt; (L&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;) in the Mars-Sun system. This is a gravitationally stable point in direct LOS with the Sun where a probe can be inserted to orbit around the Sun at the same rate as Mars. This proposed system would provide some warning for Mars settlers of the propagation of solar ions toward the Red Planet. See also: [[Early warning system (solar radiation)|Early warning system]]. If no such sensors were positioned between the Sun and Mars, interplanetary spacecraft or Mars habitats might be designed to include a sensor that can detect the x-ray burst that preceeds a solar proton event.  However, this system would probably only provide a 20-minute advance warning.&amp;lt;ref&amp;gt;Rapp D. (2006). Radiation Effects and Shielding Requirements in Human Missions to the Moon and Mars. Mars 2:46-71. &amp;lt;nowiki&amp;gt;https://doi.org/10.1555/mars.2006.0004&amp;lt;/nowiki&amp;gt;&amp;lt;/ref&amp;gt;&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;Currently, Mars has no probe or observatory in the line of sight (LOS) of the Sun, leaving an unpatrolled expanse of interplanetary space for dangerous solar ions to pass unchecked. A possible solution (akin to the Earth's SoHO&amp;lt;ref&amp;gt;[http://sohowww.nascom.nasa.gov/ SoHO mission page.]&amp;lt;/ref&amp;gt; or ACE&amp;lt;ref&amp;gt;[http://www.swpc.noaa.gov/ace/ ACE mission page.]&amp;lt;/ref&amp;gt; observatories) could be to establish a simple and inexpensive solar observatory at the first Lagrangian Point&amp;lt;ref&amp;gt;[http://en.wikipedia.org/wiki/Lagrangian_point Lagrangian Point on Wikipedia.]&amp;lt;/ref&amp;gt; (L&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;) in the Mars-Sun system. This is a gravitationally stable point in direct LOS with the Sun where a probe can be inserted to orbit around the Sun at the same rate as Mars. This proposed system would provide some warning for Mars settlers of the propagation of solar ions toward the Red Planet. See also: [[Early warning system (solar radiation)|Early warning system]]. If no such sensors were positioned between the Sun and Mars, interplanetary spacecraft or Mars habitats might be designed to include a sensor that can detect the x-ray burst that preceeds a solar proton event.  However, this system would probably only provide a 20-minute advance warning.&amp;lt;ref&amp;gt;Rapp D. (2006). Radiation Effects and Shielding Requirements in Human Missions to the Moon and Mars. Mars 2:46-71. &amp;lt;nowiki&amp;gt;https://doi.org/10.1555/mars.2006.0004&amp;lt;/nowiki&amp;gt;&amp;lt;/ref&amp;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 style=&quot;font-weight: bold; text-decoration: none;&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;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;Unless the Earth and Mars have the Sun between them, warnings can be radioed from Earth as the warning times ranges from a couple hours to several hours.&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;div&gt;However, if the sun is active with flares that could create a CME pointing in the rough direction of Mars, the explorers there should be alert to the danger.  e.g. cancel long trips away from the habitat.&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;However, if the sun is active with flares that could create a CME pointing in the rough direction of Mars, the explorers there should be alert to the danger.  e.g. cancel long trips away from the habitat.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;

&lt;!-- diff cache key marspediaorg_www-mwmars_:diff::1.12:old-141115:rev-141116 --&gt;
&lt;/table&gt;</summary>
		<author><name>RichardWSmith</name></author>
		
	</entry>
	<entry>
		<id>http://marspedia.org/index.php?title=Coronal_Mass_Ejections&amp;diff=141115&amp;oldid=prev</id>
		<title>RichardWSmith: Discussed a storm shelter for CME.</title>
		<link rel="alternate" type="text/html" href="http://marspedia.org/index.php?title=Coronal_Mass_Ejections&amp;diff=141115&amp;oldid=prev"/>
		<updated>2024-07-02T08:28:12Z</updated>

		<summary type="html">&lt;p&gt;Discussed a storm shelter for CME.&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 08:28, 2 July 2024&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-l16&quot; &gt;Line 16:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 16:&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;However, if the sun is active with flares that could create a CME pointing in the rough direction of Mars, the explorers there should be alert to the danger.  e.g. cancel long trips away from the habitat.&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;However, if the sun is active with flares that could create a CME pointing in the rough direction of Mars, the explorers there should be alert to the danger.  e.g. cancel long trips away from the habitat.&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 style=&quot;font-weight: bold; text-decoration: none;&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;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;If the base has a radiation storm shelter, the colonists should stay in this for the couple hour solar storm, if it happens during the day time.&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;div&gt;===References===  &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;===References===  &lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;

&lt;!-- diff cache key marspediaorg_www-mwmars_:diff::1.12:old-139015:rev-141115 --&gt;
&lt;/table&gt;</summary>
		<author><name>RichardWSmith</name></author>
		
	</entry>
	<entry>
		<id>http://marspedia.org/index.php?title=Coronal_Mass_Ejections&amp;diff=139015&amp;oldid=prev</id>
		<title>RichardWSmith: /* A contingency for Mars */ spelling</title>
		<link rel="alternate" type="text/html" href="http://marspedia.org/index.php?title=Coronal_Mass_Ejections&amp;diff=139015&amp;oldid=prev"/>
		<updated>2022-05-27T15:06:17Z</updated>

		<summary type="html">&lt;p&gt;&lt;span dir=&quot;auto&quot;&gt;&lt;span class=&quot;autocomment&quot;&gt;A contingency for Mars: &lt;/span&gt; spelling&lt;/span&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 15:06, 27 May 2022&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-l14&quot; &gt;Line 14:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 14:&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;===A contingency for Mars===  &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;===A contingency for Mars===  &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;div&gt;Currently, Mars has no probe or observatory in the line of sight (LOS) of the Sun, leaving an unpatrolled expanse of interplanetary space for dangerous solar ions to pass unchecked. A possible solution (akin to the Earth's SoHO&amp;lt;ref&amp;gt;[http://sohowww.nascom.nasa.gov/ SoHO mission page.]&amp;lt;/ref&amp;gt; or ACE&amp;lt;ref&amp;gt;[http://www.swpc.noaa.gov/ace/ ACE mission page.]&amp;lt;/ref&amp;gt; observatories) could be to establish a simple and inexpensive solar observatory at the first Lagrangian Point&amp;lt;ref&amp;gt;[http://en.wikipedia.org/wiki/Lagrangian_point Lagrangian Point on Wikipedia.]&amp;lt;/ref&amp;gt; (L&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;) in the Mars-Sun system. This is a gravitationally stable point in direct LOS with the Sun where a probe can be inserted to orbit around the Sun at the same rate as Mars. This proposed system would provide some warning for Mars settlers of the propagation of solar ions toward the Red Planet. See also: [[Early warning system (solar radiation)|Early warning system]]. If no such sensors were positioned between the Sun and Mars, interplanetary spacecraft or Mars habitats might be designed to include a sensor that can detect the x-ray burst that preceeds a solar proton event.  However, this system would probably only provide a 20-minute advance warning.&amp;lt;ref&amp;gt;Rapp D. (2006). Radiation Effects and Shielding Requirements in Human Missions to the Moon and Mars. Mars 2:46-71. &amp;lt;nowiki&amp;gt;https://doi.org/10.1555/mars.2006.0004&amp;lt;/nowiki&amp;gt;&amp;lt;/ref&amp;gt;&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;Currently, Mars has no probe or observatory in the line of sight (LOS) of the Sun, leaving an unpatrolled expanse of interplanetary space for dangerous solar ions to pass unchecked. A possible solution (akin to the Earth's SoHO&amp;lt;ref&amp;gt;[http://sohowww.nascom.nasa.gov/ SoHO mission page.]&amp;lt;/ref&amp;gt; or ACE&amp;lt;ref&amp;gt;[http://www.swpc.noaa.gov/ace/ ACE mission page.]&amp;lt;/ref&amp;gt; observatories) could be to establish a simple and inexpensive solar observatory at the first Lagrangian Point&amp;lt;ref&amp;gt;[http://en.wikipedia.org/wiki/Lagrangian_point Lagrangian Point on Wikipedia.]&amp;lt;/ref&amp;gt; (L&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;) in the Mars-Sun system. This is a gravitationally stable point in direct LOS with the Sun where a probe can be inserted to orbit around the Sun at the same rate as Mars. This proposed system would provide some warning for Mars settlers of the propagation of solar ions toward the Red Planet. See also: [[Early warning system (solar radiation)|Early warning system]]. If no such sensors were positioned between the Sun and Mars, interplanetary spacecraft or Mars habitats might be designed to include a sensor that can detect the x-ray burst that preceeds a solar proton event.  However, this system would probably only provide a 20-minute advance warning.&amp;lt;ref&amp;gt;Rapp D. (2006). Radiation Effects and Shielding Requirements in Human Missions to the Moon and Mars. Mars 2:46-71. &amp;lt;nowiki&amp;gt;https://doi.org/10.1555/mars.2006.0004&amp;lt;/nowiki&amp;gt;&amp;lt;/ref&amp;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;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;However, if the sun is active with flares that could &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;created &lt;/del&gt;a CME pointing in the rough direction of Mars, the explorers there should be alert to the danger.  e.g. cancel long trips away from the habitat.&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;/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;However, if the sun is active with flares that could &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;create &lt;/ins&gt;a CME pointing in the rough direction of Mars, the explorers there should be alert to the danger.  e.g. cancel long trips away from the habitat.&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;===References===  &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;===References===  &lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>RichardWSmith</name></author>
		
	</entry>
	<entry>
		<id>http://marspedia.org/index.php?title=Coronal_Mass_Ejections&amp;diff=139014&amp;oldid=prev</id>
		<title>RichardWSmith: /* A contingency for Mars */  If explorers are alert they should avoid making distant trips during flares.</title>
		<link rel="alternate" type="text/html" href="http://marspedia.org/index.php?title=Coronal_Mass_Ejections&amp;diff=139014&amp;oldid=prev"/>
		<updated>2022-05-27T15:05:36Z</updated>

		<summary type="html">&lt;p&gt;&lt;span dir=&quot;auto&quot;&gt;&lt;span class=&quot;autocomment&quot;&gt;A contingency for Mars: &lt;/span&gt;  If explorers are alert they should avoid making distant trips during flares.&lt;/span&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 15:05, 27 May 2022&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-l14&quot; &gt;Line 14:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 14:&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;===A contingency for Mars===  &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;===A contingency for Mars===  &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;div&gt;Currently, Mars has no probe or observatory in the line of sight (LOS) of the Sun, leaving an unpatrolled expanse of interplanetary space for dangerous solar ions to pass unchecked. A possible solution (akin to the Earth's SoHO&amp;lt;ref&amp;gt;[http://sohowww.nascom.nasa.gov/ SoHO mission page.]&amp;lt;/ref&amp;gt; or ACE&amp;lt;ref&amp;gt;[http://www.swpc.noaa.gov/ace/ ACE mission page.]&amp;lt;/ref&amp;gt; observatories) could be to establish a simple and inexpensive solar observatory at the first Lagrangian Point&amp;lt;ref&amp;gt;[http://en.wikipedia.org/wiki/Lagrangian_point Lagrangian Point on Wikipedia.]&amp;lt;/ref&amp;gt; (L&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;) in the Mars-Sun system. This is a gravitationally stable point in direct LOS with the Sun where a probe can be inserted to orbit around the Sun at the same rate as Mars. This proposed system would provide some warning for Mars settlers of the propagation of solar ions toward the Red Planet. See also: [[Early warning system (solar radiation)|Early warning system]]. If no such sensors were positioned between the Sun and Mars, interplanetary spacecraft or Mars habitats might be designed to include a sensor that can detect the x-ray burst that preceeds a solar proton event.  However, this system would probably only provide a 20-minute advance warning.&amp;lt;ref&amp;gt;Rapp D. (2006). Radiation Effects and Shielding Requirements in Human Missions to the Moon and Mars. Mars 2:46-71. &amp;lt;nowiki&amp;gt;https://doi.org/10.1555/mars.2006.0004&amp;lt;/nowiki&amp;gt;&amp;lt;/ref&amp;gt;&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;Currently, Mars has no probe or observatory in the line of sight (LOS) of the Sun, leaving an unpatrolled expanse of interplanetary space for dangerous solar ions to pass unchecked. A possible solution (akin to the Earth's SoHO&amp;lt;ref&amp;gt;[http://sohowww.nascom.nasa.gov/ SoHO mission page.]&amp;lt;/ref&amp;gt; or ACE&amp;lt;ref&amp;gt;[http://www.swpc.noaa.gov/ace/ ACE mission page.]&amp;lt;/ref&amp;gt; observatories) could be to establish a simple and inexpensive solar observatory at the first Lagrangian Point&amp;lt;ref&amp;gt;[http://en.wikipedia.org/wiki/Lagrangian_point Lagrangian Point on Wikipedia.]&amp;lt;/ref&amp;gt; (L&amp;lt;sub&amp;gt;1&amp;lt;/sub&amp;gt;) in the Mars-Sun system. This is a gravitationally stable point in direct LOS with the Sun where a probe can be inserted to orbit around the Sun at the same rate as Mars. This proposed system would provide some warning for Mars settlers of the propagation of solar ions toward the Red Planet. See also: [[Early warning system (solar radiation)|Early warning system]]. If no such sensors were positioned between the Sun and Mars, interplanetary spacecraft or Mars habitats might be designed to include a sensor that can detect the x-ray burst that preceeds a solar proton event.  However, this system would probably only provide a 20-minute advance warning.&amp;lt;ref&amp;gt;Rapp D. (2006). Radiation Effects and Shielding Requirements in Human Missions to the Moon and Mars. Mars 2:46-71. &amp;lt;nowiki&amp;gt;https://doi.org/10.1555/mars.2006.0004&amp;lt;/nowiki&amp;gt;&amp;lt;/ref&amp;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 style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;However, if the sun is active with flares that could created a CME pointing in the rough direction of Mars, the explorers there should be alert to the danger.  e.g. cancel long trips away from the habitat.&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;div&gt;===References===  &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;===References===  &lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;

&lt;!-- diff cache key marspediaorg_www-mwmars_:diff::1.12:old-139013:rev-139014 --&gt;
&lt;/table&gt;</summary>
		<author><name>RichardWSmith</name></author>
		
	</entry>
	<entry>
		<id>http://marspedia.org/index.php?title=Coronal_Mass_Ejections&amp;diff=139013&amp;oldid=prev</id>
		<title>RichardWSmith: /* Detecting damaging CME ions */</title>
		<link rel="alternate" type="text/html" href="http://marspedia.org/index.php?title=Coronal_Mass_Ejections&amp;diff=139013&amp;oldid=prev"/>
		<updated>2022-05-27T15:02:07Z</updated>

		<summary type="html">&lt;p&gt;&lt;span dir=&quot;auto&quot;&gt;&lt;span class=&quot;autocomment&quot;&gt;Detecting damaging CME ions&lt;/span&gt;&lt;/span&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 15:02, 27 May 2022&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-l10&quot; &gt;Line 10:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 10:&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;==Detecting damaging CME ions==  &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;==Detecting damaging CME ions==  &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;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;Warning Mars settlers about the onset of damaging ions is therefore a high priority. Even on Earth, predicting CMEs and dangerous ions is very important as a massive current of global scale is applied during solar storms. This effect can [[static electricity|damage delicate satellite circuits]], thermally expand the upper atmosphere (thickening the atmosphere in low Earth orbit, [[Aerobreaking|slowing down satellites and decreasing their orbital altitudes]]) and even cause damage to power grids on the ground ([[aurora|auroral electrojets]] can have the effect of overloading country-wide electricity grids).&amp;lt;ref&amp;gt;[http://www.agu.org/sci_soc/eiskappenman.html ''Geomagnetic Storms Can Threaten Electric Power Grid'' - American Geophysical Union article.]&amp;lt;/ref&amp;gt; Methods of predicting and detecting Coronal Mass Ejections are constantly being developed, including &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;sun &lt;/del&gt;observatories, but the most effective way of detecting the onset of an Earth-bound CME is to have a probe between the Earth and Sun.&amp;lt;ref&amp;gt;[http://science.nasa.gov/headlines/y2007/25may_costep.htm The Solar and Heliospheric Observatory (SoHO) acting as an early warning device.]&amp;lt;/ref&amp;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;Warning Mars settlers about the onset of damaging ions is therefore a high priority. Even on Earth, predicting CMEs and dangerous ions is very important as a massive current of global scale is applied during solar storms. This effect can [[static electricity|damage delicate satellite circuits]], thermally expand the upper atmosphere (thickening the atmosphere in low Earth orbit, [[Aerobreaking|slowing down satellites and decreasing their orbital altitudes]]) and even cause damage to power grids on the ground ([[aurora|auroral electrojets]] can have the effect of overloading country-wide electricity grids).&amp;lt;ref&amp;gt;[http://www.agu.org/sci_soc/eiskappenman.html ''Geomagnetic Storms Can Threaten Electric Power Grid'' - American Geophysical Union article.]&amp;lt;/ref&amp;gt; Methods of predicting and detecting Coronal Mass Ejections are constantly being developed, including &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;solar &lt;/ins&gt;observatories, but the most effective way of detecting the onset of an Earth-bound CME is to have a probe between the Earth and Sun.&amp;lt;ref&amp;gt;[http://science.nasa.gov/headlines/y2007/25may_costep.htm The Solar and Heliospheric Observatory (SoHO) acting as an early warning device.]&amp;lt;/ref&amp;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;div&gt;===A contingency for Mars===  &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;===A contingency for Mars===  &lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;

&lt;!-- diff cache key marspediaorg_www-mwmars_:diff::1.12:old-139012:rev-139013 --&gt;
&lt;/table&gt;</summary>
		<author><name>RichardWSmith</name></author>
		
	</entry>
	<entry>
		<id>http://marspedia.org/index.php?title=Coronal_Mass_Ejections&amp;diff=139012&amp;oldid=prev</id>
		<title>RichardWSmith: /* Detecting damaging CME ions */  Pointed out, that solar observatories watch for CME.</title>
		<link rel="alternate" type="text/html" href="http://marspedia.org/index.php?title=Coronal_Mass_Ejections&amp;diff=139012&amp;oldid=prev"/>
		<updated>2022-05-27T15:01:23Z</updated>

		<summary type="html">&lt;p&gt;&lt;span dir=&quot;auto&quot;&gt;&lt;span class=&quot;autocomment&quot;&gt;Detecting damaging CME ions: &lt;/span&gt;  Pointed out, that solar observatories watch for CME.&lt;/span&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 15:01, 27 May 2022&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-l10&quot; &gt;Line 10:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 10:&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;==Detecting damaging CME ions==  &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;==Detecting damaging CME ions==  &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;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;Warning Mars settlers about the onset of damaging ions is therefore a high priority. Even on Earth, predicting CMEs and dangerous ions is very important as a massive current of global scale is applied during solar storms. This effect can [[static electricity|damage delicate satellite circuits]], thermally expand the upper atmosphere (thickening the atmosphere in low Earth orbit, [[Aerobreaking|slowing down satellites and decreasing their orbital altitudes]]) and even cause damage to power grids on the ground ([[aurora|auroral electrojets]] can have the effect of overloading country-wide electricity grids).&amp;lt;ref&amp;gt;[http://www.agu.org/sci_soc/eiskappenman.html ''Geomagnetic Storms Can Threaten Electric Power Grid'' - American Geophysical Union article.]&amp;lt;/ref&amp;gt; Methods of predicting and detecting Coronal Mass Ejections are constantly being developed, but the most effective way of detecting the onset of an Earth-bound CME is to have a probe between the Earth and Sun.&amp;lt;ref&amp;gt;[http://science.nasa.gov/headlines/y2007/25may_costep.htm The Solar and Heliospheric Observatory (SoHO) acting as an early warning device.]&amp;lt;/ref&amp;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;Warning Mars settlers about the onset of damaging ions is therefore a high priority. Even on Earth, predicting CMEs and dangerous ions is very important as a massive current of global scale is applied during solar storms. This effect can [[static electricity|damage delicate satellite circuits]], thermally expand the upper atmosphere (thickening the atmosphere in low Earth orbit, [[Aerobreaking|slowing down satellites and decreasing their orbital altitudes]]) and even cause damage to power grids on the ground ([[aurora|auroral electrojets]] can have the effect of overloading country-wide electricity grids).&amp;lt;ref&amp;gt;[http://www.agu.org/sci_soc/eiskappenman.html ''Geomagnetic Storms Can Threaten Electric Power Grid'' - American Geophysical Union article.]&amp;lt;/ref&amp;gt; Methods of predicting and detecting Coronal Mass Ejections are constantly being developed&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;, including sun observatories&lt;/ins&gt;, but the most effective way of detecting the onset of an Earth-bound CME is to have a probe between the Earth and Sun.&amp;lt;ref&amp;gt;[http://science.nasa.gov/headlines/y2007/25may_costep.htm The Solar and Heliospheric Observatory (SoHO) acting as an early warning device.]&amp;lt;/ref&amp;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;div&gt;===A contingency for Mars===  &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;===A contingency for Mars===  &lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;

&lt;!-- diff cache key marspediaorg_www-mwmars_:diff::1.12:old-127177:rev-139012 --&gt;
&lt;/table&gt;</summary>
		<author><name>RichardWSmith</name></author>
		
	</entry>
</feed>