Highly ionized atoms: what do they teach us about the solar atmosphere?-Reference-Cited by-同舟云学术

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Highly ionized atoms: what do they teach us about the solar atmosphere?

Published:1993-01-01 Issue: Volume:T47 Page:128-132
ISSN:0031-8949
Container-title:Physica Scripta
language:
Short-container-title:Phys. Scr.

Author:

Feldman Uri

Publisher

IOP Publishing

Subject

Condensed Matter Physics,Mathematical Physics,Atomic and Molecular Physics, and Optics

Link

http://stacks.iop.org/1402-4896/1993/i=T47/a=020/pdf

Reference31 articles.

1. On the unresolved fine structures of the solar atmosphere in the 30,000-200,000 K temperature region

2. On the unresolved fine structures of the solar atmosphere. II - The temperature region 200,000 - 500,000 K

3. Solar abundances from X-ray flare observations

4. Solar-stellar outer atmospheres and energetic particles, and galactic cosmic rays

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1. Challenges;Astrophysics and Space Science Library;2024

2. Spectroscopic diagnostics in the VUV for solar and stellar plasmas;The Astronomy and Astrophysics Review;1994-03

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