MHD turbulence behind the fronts of the quasi-perpendicular and quasi-parallel shock waves of Feb. 2 and 7, 1982

Details MHD turbulence behind the fronts of the quasi-perpendicular and quasi-parallel shock waves of Feb. 2 and 7, 1982 MHD turbulence behind the fronts of the quasi-perpendicular and quasi-parallel shock waves of Feb. 2 and 7, 1982

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989kosis..27..726m&link_type=abstract

Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 27, Sept.-Oct. 1989, p. 726-738. In Russian.

Physics

Interplanetary Medium, Magnetohydrodynamic Turbulence, Shock Waves, Interplanetary Magnetic Fields, Shock Layers, Space Plasmas, Venera Satellites

Scientific paper

Venera 13 and 14 data were used to study the dynamics of MHD magnetic-field fluctuations for frequencies less than 0.01 Hz in a region 0.5 AU behind the quasi-perpendicular and quasi-parallel interplanetary shock waves on Feb. 2 and 7, 1982, respectively. An analysis is made of the main types of fluctuations characteristic of large-scale plasma-flow structures in a shock layer and a flare ejection. The spectral power density of the fluctuations is evaluated.

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