Normal distribution of flare colours and its interpretation-Reference-Cited by-同舟云学术

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Normal distribution of flare colours and its interpretation

Published:1985 Issue:1 Volume:116 Page:189-195
ISSN:0004-640X
Container-title:Astrophysics and Space Science
language:en
Short-container-title:Astrophys Space Sci

Author:

Grandpierre Attila,Melikian Norik D.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1007/BF00649284.pdf

Reference23 articles.

1. Ambartsumian, V.A.: 1954,Soobsch. Byur. Obs. 13 (in Russian).

2. Ambartsumian, V.A.: 1971,Astrofizika 7, 557 (in Russian).

3. Cram, L.E. and Woods, D.T.: 1982,Astrophys. J. 257, 269.

4. Gershberg, R.E.: 1964,Izv. Krimsk. Astrofiz. Obs. 32, 133 (in Russian).

5. Gershberg, R.E.: 1974,Izv. Krimsk. Astrofiz. Obs. 51, 117 (in Russian).

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 Inadequacies of the Magnetic Flare Theories and the Resolution of these Problems with the Convective Flare Theory;International Astronomical Union Colloquium;1989

2. Flares: Magnetic or Convective Origin?;Activity in Cool Star Envelopes;1988

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