Solar wing magnetic holes - Signatures of slow-mode type MHD solitons?

Details Solar wing magnetic holes - Signatures of slow-mode type MHD solitons? Solar wing magnetic holes - Signatures of slow-mode type MHD solitons?

Jan 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997adspr..20...69b&link_type=abstract

Advances in Space Research, vol. 20, p. 69

Physics

10

Solar Wind Velocity, Solar Magnetic Field, Magnetohydrodynamic Stability, Plasma Temperature, Magnetic Mirrors, Boundary Conditions, Magnetohydrodynamic Flow

Scientific paper

A mechanism for the generation of magnetic holes in the solar wind that is unrelated to the mirror mode instability is proposed. This invokes MHD solitons of mixed slow-mode/intermediate mode type, which propagate with small velocity at large angle to the magnetic field. From certain initial conditions in the solar wind plasma, such structures can evolve as a stable flow feature without the need for temperature anisotropy.

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