Michael Mozina said:
Sure.
http://aia.lmsal.com/public/firstlight/20100418_000108/
http://aia.lmsal.com/public/firstlig...0108/f4500.gif
http://aia.lmsal.com/public/firstlig...0108/f1700.gif
http://aia.lmsal.com/public/firstlig...0108/f1600.gif
If you layer the two images as Zig suggested yesterday, you'll notice that the 1700A image produces a much smaller disk. The 1600A produces a *THIRD* sized disk that fits between the 4500A and 1700A. That's consistent with a plasma separated (non opaque) photosphere, but I don't know how to explain that with the SSM.
Yup, I measure just under 28000km difference in diameter between the 1700A and 4500A images. But that's assuming the images are scaled properly to match each other, which I doubt. Features near the limb don't line up between the 4500 and 1700 images, they move outward by the same amount as the scale difference between the images.
I also see differences between the images with the same filter but at different times. Did the sun's diameter change a couple percent in a few days?
Some time ago now - many pages I expect - Tim Thompson wrote an excellent post on PR images and science images (actually data).
A bit later MM posted his hilarious "empirical" 6-step method for proving there is a solid iron surface below the chromosphere (or some such) using RD images (and I posted one or two comments on just how hopeless this is, in terms of the MM's declared objective).
Yet we still see MM using non-science images!
What makes this all so astonishingly ironic is MM's bald, bold, unambiguous declarations concerning the role of maths in observations and empirical science in general (you haven't forgotten have you dear reader?)
To take just one, tiny, example:
To determine where any feature that you unambiguously and objectively identify in the data (image) from the output datastream from one waveband channel of one AIA telescope is - in relation to a disk of radius r, centered at location (x, y) on the sky, at a distance d from the SDO - involves an enormous amount of work, and a great deal of math (much of it far, far more advanced than any MM has himself used, in any post here in JREF, to date).
To determine the spatial relationship between two such features - one from channel A on telescope A, the other from channel B on telescope B - is doubly challenging.
Now the people who designed, built, calibrated, and operate SDO and the AIA put a huge amount of effort into addressing these questions (and many more besides of course), and have published a great deal of material on their solutions, and from this material you can at least begin to develop a plan to make estimates of the relative separation of a pair of features, one in a channel A/telescope dataset, the other in a channel B/telescope B dataset.
If you want to produce a robust estimate, one that is independently verifiable (where one 'line' is in relation to another 'line', say), you will have to do a lot of detailed, quantitative work. Curiously (or not), MM has declared that all such work is invalid, and that he can overthrow standard solar models merely by visual inspection of PR images.
What sorts of things might you have to address, to make robust estimates of the projected separation of two features in separate AIA datasets, two 'lines' say?
Here are some:
* geometric distortion (crudely, the image of a perfectly rectangular grid will not be perfectly rectangular; how to map one to the other?)
* SDO's distance from the Sun
* image scale (crudely, how many arcsecs does one pixel correspond to?)
* unambiguous, quantitative, objective definition of the location of a feature (think of how you'd go about defining the position of a crater on the Moon, say, from an image taken through your backyard telescope)
* registration (crudely, what is the difference between the centres of two images, and how much is one rotated with respect to the other?)
On top of that, to be of any use scientifically, you need to make robust estimates of your uncertainties, and explain - objectively, in a manner that is independently verifiable - how you accounted for the known uncertainties (if you aren't familiar with 'uncertainty', think 'error') ... etc.
Who wants to bet that MM hadn't even thought of most of this (before he read it, assuming he does), and is essentially clueless wrt actually *doing* any of the above?