Because that is physically impossible to the best of my knowledge. The primary wavelengths that actually penetrate the photosphere are the iron ion wavelengths and those wavelengths are absorbed by our atmosphere. Only SOHO and STEREO satellite images can actually see under the photosphere IMO.
I am talking about SOHO, STEREO and TRACE satellite images.
They have telescopes (many telescopes even on Earth are CCD detectors) and the appropriate filters.
But I am glad that you know that this is only your humble opinion.
It is a pity that the actual physics says that you are incorrect, e.g the
optical depth of the photosphere means that you can only see a few hundred kilometers into it (this varies with wavelength).
I asked this in another thread but it is now appropriate here:
First asked 22 July 2009
Michael Mozina:
Your assertion is that images taken in the the 171A pass band of the TRACE instrument can see 4800 kilometers into the Sun down to your hypothetical, thermodynamically impossible iron surface/crust.
Images taken in the the visible light pass band of the TRACE instrument will show only the photosphere.
The physics tells us that this is wrong since the optical depth of the photosphere is too low to allow this (around 500 kilometers from memory).
An effect of your assertion would be that if images are taken of the same event at the same time in the 171A pass band and in visible light then the surface seen in the images will move by 4800 kilometers.
For an image of the entire Sun, the diameter will change by about 0.7%. The TRACE instrument uses a 1024 by 1024 CCD detector. Thus the 2 images will differ by about 7 pixels, i.e. the Sun will shrink by ~3 pixels on all sides between a visible light image and a 171A pass band image.
The effect will be larger for events on the limb of the Sun.
These effects would be quite easy to see so there are two questions here:
- Can you give some examples of images showing this effect?
- Why have no astronomers noticed this?
To start you off: Have a look at these
171A pass band and white light pass band images.
Quote:
This solar X-class flare was observed by TRACE at 16:43UT on 22 November 1998, in the 171Å passband (characteristic of 1-million degree gas; in gold, on the left), 1600Å UV passband (characteristic of thousands to hundred thousand degrees; in red on the right), and in the white-light passband (mostly visible light; in pale yellow in the right).
The 171A pass band image does not have a clear "surface" crossing the lower edge but it does have one crossing the left edge.
To my eye the 171 A pass band image "surface" is about the same (or even a few pixels above)the white band pass band image "surface" on the left hand side. I would have expected it to be tens of pixels blow the white light pass band image according to your assertion.
There is an unclear crossing of the 171A "surface" at the bottom and it does appear below the white light surface (photosphere). But that still means that your iron surface pokes up onto the photosphere at least one point.