<html><head></head><body style="word-wrap: break-word; -webkit-nbsp-mode: space; -webkit-line-break: after-white-space; ">Stephen Anderson did a very thorough analysis of how Coulomb collisions affect the model.<div><br></div><div><a href="http://adsabs.harvard.edu/abs/1994ApJ...437..860A">http://adsabs.harvard.edu/abs/1994ApJ...437..860A</a></div><div><br></div><div>dana</div><div><br><div><div>
<div><span class="Apple-style-span" style="font-size: 12px; "><div>-----------------------------------------------------------</div><div>Dana Longcope | Dept. of Physics</div><div> Professor | Montana State University</div><div> (406) 994-7851 | Bozeman, MT 59717</div><div> <a href="mailto:dana@solar.physics.montana.edu">dana@solar.physics.montana.edu</a></div><div><br></div></span></div><br class="Apple-interchange-newline">
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<br><div><div>On Jul 31, 2012, at 9:20 AM, Petrus Martens wrote:</div><br class="Apple-interchange-newline"><blockquote type="cite"><div><br><blockquote type="cite"> Do you mean velocity filtration, where the corona is simply particles from the<br></blockquote>tail of the chromospheric distribution function? That theory has been largely discredited.<br><br>That's news to me. Do you have a reference?<br><br>Piet<br><br><br><br><span><martens.vcf></span>_______________________________________________<br>Loops mailing list<br><a href="mailto:Loops@solar.physics.montana.edu">Loops@solar.physics.montana.edu</a><br>https://mithra.physics.montana.edu/mailman/listinfo/loops<br></div></blockquote></div><br></div></div></body></html>