Prominences at centimetric and millimetric wavelengths-Reference-Cited by-同舟云学术

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Prominences at centimetric and millimetric wavelengths

Published:1980-06 Issue:2 Volume:66 Page:275-283
ISSN:0038-0938
Container-title:Solar Physics
language:en
Short-container-title:Sol Phys

Author:

Lantos P.,Raoult A.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1007/BF00150585.pdf

Reference27 articles.

1. Athay, R. G.: 1976, The Solar Chromosphere and Corona: Quiet Sun, D. Reidel Publ. Co., Dordrecht, Holland.

2. Beckman, J. E., Clark, C. D., and Ross, J.: 1973, Solar Phys. 31, 319.

3. Chambe, G.: 1978 Astron. Astrophys. 39, 000.

4. Chambe, G. and Lantos, P.: 1971, Solar Phys. 17, 97.

5. Chiuderi-Drago, F., Fürst, E., Hirth, W., and Lantos, P.: 1975, Astron. Astrophys. 39, 429.

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3. ALMA and the Sun;Astronomische Nachrichten;2002-08

4. A Study of Solar Prominences near lambda = 1 Millimeter;The Astrophysical Journal;1993-11

5. On the possible physical conditions which result in appearance of low brightness temperature microwave regions on the sun;Solar Physics;1993-03

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