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Discussion and Debate
Discussion and Debate
Physical & Life Sciences
Micheal's solar model
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<blockquote data-quote="[serious]" data-source="post: 70487582" data-attributes="member: 160873"><p>I dont follow. walk me through it.</p><p></p><p>Let's start with there existing a temperature differential as you describe, with the core of the sun being cooler than the photosphere. the photosphere radiates heat, some of which escapes, some of which heats the core. How does the core get rid of that heat to prevent it from reaching thermal equalibrium with its surroundings? </p><p></p><p>For example, the mainstream understanding is that the corona is heated by magnetic forces from the core, as is the photosphere. because the photosphere is not as fully ionized, it is able to more effectively radiate that heat away to space. the corona is instead insulated in a way by the ionization and stays hot.</p></blockquote><p></p>
[QUOTE="[serious], post: 70487582, member: 160873"] I dont follow. walk me through it. Let's start with there existing a temperature differential as you describe, with the core of the sun being cooler than the photosphere. the photosphere radiates heat, some of which escapes, some of which heats the core. How does the core get rid of that heat to prevent it from reaching thermal equalibrium with its surroundings? For example, the mainstream understanding is that the corona is heated by magnetic forces from the core, as is the photosphere. because the photosphere is not as fully ionized, it is able to more effectively radiate that heat away to space. the corona is instead insulated in a way by the ionization and stays hot. [/QUOTE]
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