On the classic heat conduction in the chromosphere-corona transition region of the solar atmosphere-Reference-Cited by-同舟云学术

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On the classic heat conduction in the chromosphere-corona transition region of the solar atmosphere

Published:2010-12 Issue:6 Volume:65 Page:527-530
ISSN:0027-1349
Container-title:Moscow University Physics Bulletin
language:en
Short-container-title:Moscow Univ. Phys.

Author:

Ptitsyna O. V.,Somov B. V.

Publisher

Allerton Press

Subject

General Physics and Astronomy

Link

http://link.springer.com/content/pdf/10.3103/S0027134910060184.pdf

Reference12 articles.

1. P. A. Bespalov and O. N. Savina, Pis’ma Astron. Zh. 34, 378 (2008) [Astron. Lett. 34, 344 (2008)].

2. P. A. Bespalov and O. N. Savina, Pis’ma Astron. Zh. 35, 382 (2009) [Astron. Lett. 35, 343 (2009)].

3. O. P. Shmeleva and S. I. Syrovatskii, Solar Phys. 33, 341 (1973).

4. D. P. Cox and W. H. Tucker, Astrophys. J. 157, 1157 (1969).

5. W. Kalkofen, P. Ulmschneider, and E. H. Avrett, Astrophys. J. 521, 141 (1999).

Cited by 2 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. On the Problem of Heat Transport in the Solar Atmosphere;The Sun: New Challenges;2012

2. On the stability of the solar chromosphere-corona transition region;Moscow University Physics Bulletin;2011-10

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