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	<id>https://www.myroms.org/wiki/index.php?action=history&amp;feed=atom&amp;title=Eigenproblem_Parameters</id>
	<title>Eigenproblem Parameters - Revision history</title>
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	<updated>2026-04-27T16:18:06Z</updated>
	<subtitle>Revision history for this page on the wiki</subtitle>
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	<entry>
		<id>https://www.myroms.org/wiki/index.php?title=Eigenproblem_Parameters&amp;diff=2950&amp;oldid=prev</id>
		<title>Robertson: New page: &lt;div class=&quot;title&quot;&gt;Eigenproblem Parameters&lt;/div&gt; {{#lst:Variables|NEV}}  {{#lst:Variables|NCV}}   &#039;&#039;&#039;Notice:&#039;&#039;&#039; At present, there is no a-priori analysis to guide the selection of &lt;span cl...</title>
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		<updated>2008-04-16T20:02:36Z</updated>

		<summary type="html">&lt;p&gt;New page: &amp;lt;div class=&amp;quot;title&amp;quot;&amp;gt;Eigenproblem Parameters&amp;lt;/div&amp;gt; {{#lst:Variables|NEV}}  {{#lst:Variables|NCV}}   &amp;#039;&amp;#039;&amp;#039;Notice:&amp;#039;&amp;#039;&amp;#039; At present, there is no a-priori analysis to guide the selection of &amp;lt;span cl...&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;&amp;lt;div class=&amp;quot;title&amp;quot;&amp;gt;Eigenproblem Parameters&amp;lt;/div&amp;gt;&lt;br /&gt;
{{#lst:Variables|NEV}}&lt;br /&gt;
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{{#lst:Variables|NCV}}&lt;br /&gt;
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&amp;#039;&amp;#039;&amp;#039;Notice:&amp;#039;&amp;#039;&amp;#039; At present, there is no a-priori analysis to guide the selection of &amp;lt;span class=&amp;quot;twilightBlue&amp;quot;&amp;gt;NCV&amp;lt;/span&amp;gt; relative to &amp;lt;span class=&amp;quot;twilightBlue&amp;quot;&amp;gt;NEV&amp;lt;/span&amp;gt;.  The only formal requirement is that &amp;lt;span class=&amp;quot;twilightBlue&amp;quot;&amp;gt;NCV &amp;gt; NEV&amp;lt;/span&amp;gt;. However in optimal perturbations, it is recommended to have &amp;lt;span class=&amp;quot;twilightBlue&amp;quot;&amp;gt;NCV &amp;amp;ge; 2*NEV&amp;lt;/span&amp;gt;. In Finite Time Eigenmodes (FTE) and Adjoint Finite Time Eigenmodes (AFTE) the requirement is to have &amp;lt;span class=&amp;quot;twilightBlue&amp;quot;&amp;gt;NCV &amp;amp;ge; 2*NEV+1&amp;lt;/span&amp;gt;. The efficiency of calculations depends critically on the combination of &amp;lt;span class=&amp;quot;twilightBlue&amp;quot;&amp;gt;NEV&amp;lt;/span&amp;gt; and &amp;lt;span class=&amp;quot;twilightBlue&amp;quot;&amp;gt;NCV&amp;lt;/span&amp;gt;.  If &amp;lt;span class=&amp;quot;twilightBlue&amp;quot;&amp;gt;NEV&amp;lt;/span&amp;gt; is large (greater than 10 say), you can use &amp;lt;span class=&amp;quot;twilightBlue&amp;quot;&amp;gt;NCV=2*NEV+1&amp;lt;/span&amp;gt; but for &amp;lt;span class=&amp;quot;twilightBlue&amp;quot;&amp;gt;NEV&amp;lt;/span&amp;gt; small (less than 6) it will be inefficient to use &amp;lt;span class=&amp;quot;twilightBlue&amp;quot;&amp;gt;NCV=2*NEV+1&amp;lt;/span&amp;gt;. In complicated applications, you can start with &amp;lt;span class=&amp;quot;twilightBlue&amp;quot;&amp;gt;NEV=2&amp;lt;/span&amp;gt; and &amp;lt;span class=&amp;quot;twilightBlue&amp;quot;&amp;gt;NCV=10&amp;lt;/span&amp;gt;. Otherwise, it will iterate for very long time.&lt;/div&gt;</summary>
		<author><name>Robertson</name></author>
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