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• W58751646 abstract "Various mechanisms which could cause heating of the electrons of the solar wind in a collisionless shock wave are examined. The results of measurements of the properties of the plasma and the fields at the front of the quasiperpendicular supercritical shock wave near the earth during one crossing of this wave by the Prognoz-10-Interkosmos satellite are discussed (this study was part of the joint Soviet--Czechoslovak program INTERSHOK). Most of the electron heating occurs in the immediate vicinity (within a few seconds) of the discontinuity in the magnetic field (the ramp). Estimates indicate that such processes as the adiabatic expansion of the plasma at the front and the interaction of electrons with large-amplitude electromagnetic waves contribute substantially to this heating." @default.
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• W58751646 date "1988-11-01" @default.
• W58751646 modified "2023-09-24" @default.
• W58751646 title "Electron heating in a supercritical shock wave" @default.
• W58751646 hasPublicationYear "1988" @default.
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