Energy balance in cool quiescent prominences-Reference-Cited by-同舟云学术

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Energy balance in cool quiescent prominences

Published:1971-09 Issue:2 Volume:19 Page:401-413
ISSN:0038-0938
Container-title:Solar Physics
language:en
Short-container-title:Sol Phys

Author:

Poland A.,Anzer U.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1007/BF00146067.pdf

Reference14 articles.

1. Athay, R. G. and Thomas, R. N.: 1961, Physics of the Solar Chromosphere, Interscience Publishers, Inc., New York.

2. Giovanelli, R. G.: 1967, Australian J. Phys. 20, 81.

3. Hirayama, T.: 1964, Proc. Astron. Soc. Japan 16, 104.

4. Jefferies, J. T.: 1968, Spectral Line Formation, Blaisdell Publishing Co., Watham, Mass.

5. Jefferies, J. T. and Orrall, F. Q.: 1961, Astrophys. J. 134, 747.

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1. Plasma diagnostics and Alfvén wave heating of solar prominences by multiwavelength observations;Publications of the Astronomical Society of Japan;2023-07-27

2. Prominence oscillations;Living Reviews in Solar Physics;2018-04-23

3. Non-LTE modelling of prominence fine structures using hydrogen Lyman-line profiles;Astronomy & Astrophysics;2015-05

4. Energy Balance;Solar Prominences;2014-10-21

5. Non-linear force-free magnetic dip models of quiescent prominence fine structures;Astronomy & Astrophysics;2013-02-07

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