Aaaaand I have some time to answer. *finally*.
Better late than never.
Meh. Don't have the time nor interest for it.
That's a pity IMO. Solar physics is a fascinating subject IMO, and the leaps in technology over the past five years are staggering in terms of their implication on solar theory.
Honestly I don't see any of your publications supporting what you've been claiming, you'd need something extremely explicit.
The published papers have nothing to do with SDO images. The published papers describe a "rigid" set of subsurface features, illuminated by 171A and 195A light that is emitted from flux ropes as observed by TRACE and SOHO.
The thing is that I want to see them explaining it before I make up my mind whether your claim is credible or not.
In terms of your timing, "waiting" worked out in your favor. I think we've now firmly established that the single image in question did *not* show what I assumed it showed. It also pretty much blows out the whole concept of a "transitional region" as well. The transition from bright horizon to opaque dark region along the limb is nothing more than a transition point in the dusty chromosphere, where the chromosphere turns from transparent to opaque in these specific wavelengths along the limb. Such limb images however tell us *little or nothing* about the actual "origin" of flux ropes, particularly in face on images of the sun.
In such instance, we need to look at the math (Kosovichev and the sunspot models) and see how well they jive with the SDO images. In this case the mathematical models predicting strong subsurface EM fields are supported by the SDO images that show 171A light descending into the penumbral filaments *as predicted* in the models.
In terms of mass flow differences however, there are some very unique "predictions" related to a cathode solar model, which I've addressed in those flare images. The SDO images show that electrical discharges can not only occur *above* the surface of the photosphere, but they can occur below that surface as well. Some flares blow hot material up and through that layer, whereas some events blow material down *into* that surface.
In a Birkeland model, the 'reconnection' of current in the circuits can occur anywhere in the solar atmosphere, both above and below the surface of the double layer called a "photosphere" by the mainstream.
Unfortunately for the mainstream, the SDO images and data sets haven't been kind. There's no real "transition region" to be observed in SDO images. Even along the limb, we aren't observing anything other than an opaque horizon. It's no the 'origin' of flux ropes we observe along the limb, just the point they become "visible" above the 'dust" in the atmosphere along the 100+ kilometers of chromospheric plasma along the limb.
Unless this comes from something peer-reviewed that's kind of unverifiable to me.
That recent paper on "slow" convection was "peer reviewed". Care to comment?
Were we discussing the pictures or the models?
Both at various times.
I don't see how you can discern the different colors they've used, the best thing would be an explicit statement similar to "here we use this and this".
I'd guess that I still selected the wavelengths and the various colors correctly, even if I was incorrect about the size of the inside disk that was "subtracted" from the 304A image. The colors and wavelengths really relate to the image, and the temperature ranges they mentioned. The 304A wavelength specifically relates to 50,000 degree plasma. The iron lines I mentioned (171A, 195A, 211A) all related to "lower' temperature iron ionization states, vs. the 94A, 131, and higher energy wavelengths.
Either way, it's pretty much a moot point now.
And not we're back to post
#101. Not once do they mention iron lines. So how am I, as a layman, to "see" darkening at those?
I would assume that a "layman" probably wouldn't know that there is a link between iron and say 171A, or 195A, nor a link between HeII and 304A. These are things you'd have to know from reading some of the technical specs on satellite images.
I think this may have been covered in the time I've been absent, but I still thought I should reply.
Well, thanks for thinking of me.
Now that you're caught up from 3 weeks or so ago, you might be interested in some of the more recent data we've discussed, like this SDO image of a flare in 1700A.
http://www.thesurfaceofthesun.com/sdo/2012_04_16_16_30_07_2012_04_16_19_29_19_AIA_1700-hq.mp4