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A substorm expansion model based on configuration instability of the near-Earth magnetotail: I. Configuration instability in the near-Earth magnetotail

MPS-Authors
http://pubman.mpdl.mpg.de/cone/persons/resource/persons104317

Zong,  Q.-G.
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;

http://pubman.mpdl.mpg.de/cone/persons/resource/persons104023

Korth,  A.
Department Planets and Comets, 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/persons103915

Friedel,  R. H. W.
MPI for Aeronomy, 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/persons104031

Kremser,  G.
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;

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Citation

Pu, Z. Y., Hong, M. H., Wang, X. M., Chen, Z. X., Fu, S. Y., Zong, Q.-G., et al. (1996). A substorm expansion model based on configuration instability of the near-Earth magnetotail: I. Configuration instability in the near-Earth magnetotail. Acta Geophysica Sinica, 39, 141.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0014-D666-E
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