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Ultrasharp Images Of A Sunspot
SigurRosFan
post Oct 6 2005, 08:15 AM
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New optics produce ultrasharp images of sunspot

News article: http://spaceflightnow.com/news/n0510/05sunspots/

More images: http://www.nso.edu/press/DALSA/

NOAA 0805:


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SigurRosFan
post Oct 7 2005, 07:02 AM
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Abyss! Abyss! biggrin.gif


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chris
post Oct 7 2005, 09:31 AM
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QUOTE (SigurRosFan @ Oct 7 2005, 07:02 AM)
Abyss! Abyss! biggrin.gif
*


laugh.gif

We won't have to worry about power either...
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ljk4-1
post Feb 7 2006, 07:03 PM
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Astrophysics, abstract
astro-ph/0602129

From: Juan Manuel Borrero [view email]

Date: Mon, 6 Feb 2006 17:20:10 GMT (28kb)

The uncombed penumbra

Authors: J.M. Borrero, M. Rempel, S.K. Solanki

Comments: 6 pages, 2 figures. to appear in the proceedings of the Solar Polarization Workshop IV

The uncombed penumbral model explains the structure of the sunspot penumbra in terms of thick magnetic fibrils embedded in a magnetic surrounding atmosphere. This model has been successfully applied to explain the polarization signals emerging from the sunspot penumbra. Thick penumbral fibrils face some physical problems, however. In this contribution we will offer possible solutions to these shortcomings.

http://arxiv.org/abs/astro-ph/0602129


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"After having some business dealings with men, I am occasionally chagrined,
and feel as if I had done some wrong, and it is hard to forget the ugly circumstance.
I see that such intercourse long continued would make one thoroughly prosaic, hard,
and coarse. But the longest intercourse with Nature, though in her rudest moods, does
not thus harden and make coarse. A hard, sensible man whom we liken to a rock is
indeed much harder than a rock. From hard, coarse, insensible men with whom I have
no sympathy, I go to commune with the rocks, whose hearts are comparatively soft."

- Henry David Thoreau, November 15, 1853

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ljk4-1
post Feb 9 2006, 03:33 PM
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Astrophysics, abstract
astro-ph/0602176

From: Huw Morgan [view email]

Date: Wed, 8 Feb 2006 01:26:00 GMT (54kb)

The Impact of Sunspots on the Interpretation of Coronal Observations of the O VI Doublet

Authors: H. Morgan, Shadia Rifai Habbal

Comments: 4 pages, 3 figures

Journal-ref: ApJ Letters, 630, 2005, L189

Due to their high intensity of emission in the O VI 1031.9 and 1037.6A lines, even small sunspots on the solar disk can strongly influence the intensity of the radiative scattering component of O VI lines in the corona. Observations of O VI disk spectra show a 1032/1038 line intensity ratio of >2.6 in a sunspot compared to quiet disk values of 2. The enhancement of the 1032 line in comparison to the 1038 is likely due to interaction between molecular hydrogen emission from the sunspot and the chromospheric O5+. Modeling shows that a contribution from sunspots increases the coronal O VI 1032/1038 intensity ratio to values considerably higher than those achieved with a quiet disk or coronal hole spectrum. Therefore a re-examination of flow velocities derived from UVCS/SOHO streamer observations must be made. This modeling demonstrates that the inclusion of sunspots, when present, may lead to non-zero outflow velocities at lower heights in streamer cores in contrast to some existing model results.

http://arxiv.org/abs/astro-ph/0602176


--------------------
"After having some business dealings with men, I am occasionally chagrined,
and feel as if I had done some wrong, and it is hard to forget the ugly circumstance.
I see that such intercourse long continued would make one thoroughly prosaic, hard,
and coarse. But the longest intercourse with Nature, though in her rudest moods, does
not thus harden and make coarse. A hard, sensible man whom we liken to a rock is
indeed much harder than a rock. From hard, coarse, insensible men with whom I have
no sympathy, I go to commune with the rocks, whose hearts are comparatively soft."

- Henry David Thoreau, November 15, 1853

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