Faint H? emission in the solar corona: Morphological, situational and hydromagnetic analysis

Author:

Dermendjiev V. N.,Duchlev P.,Mouradian Z.,Leroy J. -L.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference14 articles.

1. Allen, C. W.: 1973,Astrophysical Quantities, Athlone Press, London.

2. An, C. H., Suess, S. T., Tandberg-Hanssen, E., and Steinolfson, R. S.: 1985,Solar Phys. 102, 165.

3. Engvold, O.: 1976,Solar Phys. 49, 283.

4. Friden, B.: 1980,Computers in the Optical Research, Topics in Applied Physics, Vol. 44, Springer-Verlag, Berlin (in Russian translation, 1983).

5. Georgiev, T. B.: 1987, in S. Marx (ed.),Proceedings of the IAU Workshop ?Astrophotography?, Springer-Verlag, Berlin, p. 162.

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1. A statistical analysis of faint H alpha coronal emission associated with prominences;Solar Physics;2001

2. Observations of Filament Structure and Dynamics;International Astronomical Union Colloquium;1998

3. Faint “Chromospheric” Emission in the Solar Corona: Observational and Theoretical Problems;Theoretical and Observational Problems Related to Solar Eclipses;1997

4. Filament Channels in the Corona;Theoretical and Observational Problems Related to Solar Eclipses;1997

5. On the two classes of filament-prominence disappearance and their relation to coronal mass ejections;Solar Physics;1995-05

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