Analysis of two active prominences

Author:

Machado Marcos E.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference9 articles.

1. Gimse, O. and Hosinsky, G.: 1967, Solar Phys. 2, 192.

2. Hyder, C. L. and Lites, B. W.: 1970, Solar Phys. 14, 147.

3. Krat, V. A.: 1968, in Y. Öhman (ed.), ?Mass Motions in Solar Flares and Related Phenomena?, Nobel Symp. 9, 89.

4. Krat, V. A. and Krat, T. V.: 1971, Solar Phys. 17, 355.

5. Malville, J. M.: 1968, Solar Phys. 5, 236.

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1. Dynamics of solar coronal eruptions;Journal of Geophysical Research: Space Physics;2001-11-01

2. Structure and stability of prominences with helical structure;Solar Physics;1988-03

3. Reconnection driven by an erupting filament in the May 14, 1981 flare;Solar Physics;1987-09

4. A method of analysing the emission lines of solar prominences;Chinese Astronomy and Astrophysics;1983-12

5. Macroscopic motions in prominences;Solar Physics;1973-08

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