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Factors related to the origin of a gradual coronal mass ejection associated with an eruptive prominence on 1998 June 21-22

MPS-Authors
http://pubman.mpdl.mpg.de/cone/persons/resource/persons104222

Srivastava,  N.
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;

http://pubman.mpdl.mpg.de/cone/persons/resource/persons104200

Schwenn,  R.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;

http://pubman.mpdl.mpg.de/cone/persons/resource/persons103978

Inhester,  B.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;

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Srivastava, N., Schwenn, R., Inhester, B., Martin, S. F., & Hanaoka, Y. (2000). Factors related to the origin of a gradual coronal mass ejection associated with an eruptive prominence on 1998 June 21-22. Astrophysical Journal, 534, 468-481.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0014-E15A-C
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