Magnetic field evolution during prominence eruptions and two-ribbon flares-Reference-Cited by-同舟云学术

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Magnetic field evolution during prominence eruptions and two-ribbon flares

Published:1990-04 Issue:2 Volume:126 Page:319-350
ISSN:0038-0938
Container-title:Solar Physics
language:en
Short-container-title:Sol Phys

Author:

Priest E. R.,Forbes T. G.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1007/BF00153054.pdf

Reference26 articles.

1. Amari, T. and Aly, J. J.: 1989, Astron. Astrophys. 208, 261.

2. Anzer, U.: 1989, in E. R. Priest (ed.), Dynamics and Structure of Quiescent Solar Prominences, Kluwer Academic Publishers, Dordrecht, The Netherlands, Ch. 6.

3. Biskamp, D. and Welter, H.: 1989, Solar Phys. 120, 49.

4. Browning, P. K. and Priest, E. R.: 1986, Solar Phys. 106, 335.

5. Demoulin, P. K. and Priest, E. R.: 1988, Astron. Astrophys. 206, 336.

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