<?xml version="1.0" encoding='utf-8'?>
<!DOCTYPE wml PUBLIC "-//WAPFORUM//DTD WML 1.1//EN" "http://www.wapforum.org/DTD/wml_1.1.xml">
<wml>
<card id="card1" title="Solar flare - Page 15 - Wikipedia">
<p>
<a accesskey="1" href="page.php?w=solar_flare&amp;p=14">1.Previous</a><br />
<a accesskey="3" href="page.php?w=solar_flare&amp;p=16">3.Next</a>
</p>
<p>and is commonly known as the <a href="page.php?w=Erich_Rieger">''Rieger period''</a>. The period's <a href="page.php?w=resonance">resonance</a> <a href="page.php?w=harmonics">harmonics</a> also have been reported from most data types in the <a href="page.php?w=heliosphere">heliosphere</a>.</p>

<p>The <a href="page.php?w=frequency_distribution">frequency distribution</a>s of various flare phenomena can be characterized by <a href="page.php?w=power-law_distribution">power-law distribution</a>s. For example, the peak fluxes of radio, extreme ultraviolet,</p><p>
<a accesskey="1" href="page.php?w=solar_flare&amp;p=14">1.Previous</a><br />
<a accesskey="3" href="page.php?w=solar_flare&amp;p=16">3.Next</a>
</p>

<do type="prev" label="Search">
        <go href="search.wml"/>
</do>

</card>
</wml>
