Michael Mozina
Banned
- Joined
- Feb 10, 2009
- Messages
- 9,361
Yep, I made this point and MM ignored it. And as a general rule there are more bound-bound absorption lines accessible in hotter plasmas. In the neighborhood of 171A there are lines from Mg III, Mg IV, Ne VIII, O VIII, Fe VII, Fe X. Keep turning up the temperature and you'll keep adding more.
Ya, except I believe that all the iron lines and metals all relate to the coronal loops, not necessarily the material in the photosphere, and elements embedded in the neon are likely to also be highly ionized.
I'm also amused that, after five+ (?) years of doing his "iron sun" image analysis, MM learned from this thread that the photosphere isn't transparent.
I simply had no idea you actually thought sunspots were "opaque". Frankly I never thought that was part of your beliefs.
And within about 24 hours of learning this, he suddenly "realized", and is quite confident,that there's no such thing as continuum photoionizationthat his model's entire photosphere is obviously super-ultra-hyper-ionized. That's some premature confidence, to say the least.
Er, you have that completely backwards. I never worried about the photoionization issue because I have *ALWAYS* known that the neon that is present is in a very high energy state and that's why you underestimated it in the first place. I knew that from day one from the SERTS data, along with the fact that the silicon layer is also highly ionized. In any electric sun theory, the high ionization of the lower atmosphere is a given. It's only because you "made" the photoionization aspect a "big deal" that we got sidetracked IMO. It was worth it however to learn about one way to "test" both theories in Ne+3/Ne+4 images. That's useful information.
Enjoy the rest of your weekend. I'll be back.....
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