Magnetic field configurations which can produce prominences with inverse polarity-Reference-Cited by-同舟云学术

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Magnetic field configurations which can produce prominences with inverse polarity

Published:1990-12 Issue:1-2 Volume:130 Page:403-406
ISSN:0038-0938
Container-title:Solar Physics
language:en
Short-container-title:Sol Phys

Author:

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/BF00156803.pdf

Reference7 articles.

1. Anzer, U. and Priest, E.R.: 1985, Solar Phys., 95, 263

2. D�moulin, P. and Priest, E.R.: 1990, IAU Coll. N� 117 (V. Ru? djak and E. Tandberg-Hanssen, eds.), 269

3. Kuperus, M. and Raadu, M.: 1974, Astron. Astrophys., 31, 185

4. Leroy, J.L.: 1989 in Dynamics and Structure of Quiescent Solar Prominences, (E.R. Priest, ed), Kluwer

5. Leroy, J.L., Bommier, V. and Sahal-Br�chot, S.: 1984, Astron. Astrophys., 131, 33

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