The interplanetary shock wave of February 1, 1982 - Magnetic structure and power spectrum of the IMF

Details The interplanetary shock wave of February 1, 1982 - Magnetic structure and power spectrum of the IMF The interplanetary shock wave of February 1, 1982 - Magnetic structure and power spectrum of the IMF

Nov 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986kosis..24..917m&link_type=abstract

Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 24, Nov.-Dec. 1986, p. 917-925. In Russian.

Physics

Interplanetary Magnetic Fields, Shock Wave Propagation, Venera Satellites, Magnetohydrodynamics, Power Spectra, Propagation Velocity, Shock Fronts, Time Response

Scientific paper

Venera 13 and 14 magnetic-field data were used to study the magnetic structure of the flux beyond the interplanetary shock wave observed on February 1, 1982. The dynamics of MHD turbulence in the 0.0001-0.01 Hz frequency range beyond the shock front is analyzed. In addition, absolute values of the spectral power density of fluctuations of the interplanetary magnetic field are calculated for large-scale structure regions of the shock wave.

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