The buoyancy of magnetic clouds during solar flares and magnetospheric substorms

Details The buoyancy of magnetic clouds during solar flares and magnetospheric substorms The buoyancy of magnetic clouds during solar flares and magnetospheric substorms

Apr 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ge%26ae..24..177i&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 24, Mar.-Apr. 1984, p. 177-181. In Russian.

Physics

1

Interplanetary Medium, Magnetic Clouds, Magnetic Storms, Magnetospheric Instability, Plasma Clouds, Solar Flares, Solar Terrestrial Interactions, Electrohydrodynamics, Interplanetary Magnetic Fields, Nonuniform Magnetic Fields, Rotating Plasmas, Shock Waves, Solar Wind

Scientific paper

An expression is obtained for the buoyant force acting on ideally conducting ellipsoids of revolution in an inhomogeneous magnetic field. The application of this formula to the estimation of the buoyant forces that drive magnetic clouds into the interplanetary space during solar flares and magnetospheric substorms is discussed. The relationship between the buoyant force and the hydromagnetic shock (injection) is examined.

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