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<blockquote data-quote="Rossim22" data-source="post: 11668762" data-attributes="member: 103156"><p>Ok, I understand the concept of kinetic temperature but it doesn't seem to apply where you're saying it does. The thermal readings show the entire corona spanning larger than the sun to be millions of degrees K. I comprehend our current model (obviously not as well or in-depth as you do) but it was created right as we were introduced to nuclear technology so our scientists needed a way of explaining how the sun was expelling so much energy and they ran with it. Here's an animation again showing how strong the influence of electrical currents and magnetic fields are in our own sun and the ejecting of material still remains unanswered. (Notice the energy)</p><p></p><p><img src="http://www-solar.mcs.st-and.ac.uk/~vasilis/nam2011/eruption_success_temp.gif" alt="" class="fr-fic fr-dii fr-draggable " style="" /></p></blockquote><p></p>
[QUOTE="Rossim22, post: 11668762, member: 103156"] Ok, I understand the concept of kinetic temperature but it doesn't seem to apply where you're saying it does. The thermal readings show the entire corona spanning larger than the sun to be millions of degrees K. I comprehend our current model (obviously not as well or in-depth as you do) but it was created right as we were introduced to nuclear technology so our scientists needed a way of explaining how the sun was expelling so much energy and they ran with it. Here's an animation again showing how strong the influence of electrical currents and magnetic fields are in our own sun and the ejecting of material still remains unanswered. (Notice the energy) [IMG]http://www-solar.mcs.st-and.ac.uk/~vasilis/nam2011/eruption_success_temp.gif[/IMG] [/QUOTE]
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