On the spatial and temporal characteristics and formation mechanisms of soft X-ray emission in the solar corona-Reference-Cited by-同舟云学术

On the spatial and temporal characteristics and formation mechanisms of soft X-ray emission in the solar corona

Published:2007-06 Issue:6 Volume:33 Page:396-410
ISSN:1063-7737
Container-title:Astronomy Letters
language:en
Short-container-title:Astron. Lett.

Author:

Urnov A. M.,Shestov S. V.,Bogachev S. A.,Goryaev F. F.,Zhitnik I. A.,Kuzin S. V.

Publisher

Pleiades Publishing Ltd

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1134/S1063773707060059.pdf

Reference28 articles.

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3. M. J. Aschwanden, Physics of the Solar Corona (Springer, PRAXIS, 2006).

4. S. A. Bogachev, B. V. Somov, and S. Masuda, Pis’ma Astron. Zh. 24, 631 (1998) [Astron. Lett. 24, 543 (1998)].

5. U. Feldman and K. J. H. Phillips, Astron. Astrophys. 304, 563 (1995).

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