On the form of the flow in the magnetosheath

Details On the form of the flow in the magnetosheath On the form of the flow in the magnetosheath

Mar 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992jgr....97.2873s&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 97, no. A3, March 1, 1992, p. 2873-2879.

Physics

50

Bow Waves, Gas Dynamics, Magnetohydrodynamic Flow, Magnetopause, Magnetosheath, Solar Wind, Boundary Conditions, Planetary Boundary Layer, Polarization (Waves), Solar Terrestrial Interactions, Space Plasmas

Scientific paper

This paper describes the reason for the formation of an upstream compressional front standing near magnetopause, describes its form and geometry, and explains the likely relationship between the compression region and a depletion layer. The model accounts for the variation of density and magnetic field strength with radial distance from the magnetopause and makes predictions regarding the orientation and geometry of the front.

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