Comments concerning the origin of the Bz component of the interplanetary magnetic field and the geoefficiency index in Akasofu's model

Details Comments concerning the origin of the Bz component of the interplanetary magnetic field and the geoefficiency index in Akasofu's model Comments concerning the origin of the Bz component of the interplanetary magnetic field and the geoefficiency index in Akasofu's model

Feb 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ge%26ae..22..154p&link_type=abstract

Geomagnetizm i Aeronomiia, vol. 22, Jan.-Feb. 1982, p. 154, 155. In Russian.

Physics

Geophysics

Geophysics, Interplanetary Magnetic Fields, Solar Terrestrial Interactions, Solar Wind, Astronomical Models, Earth Magnetosphere, Poynting Theorem

Scientific paper

Calculations are presented supporting the hypothesis that singularities of the Bz component are localized along the magnetic flux tubes, this localization being due to the stretching of the solar magnetic field loops by the quasi-stationary solar wind. If this hypothesis is correct, Akasofu's (1979) hypothesis of the existence of a special slow epsilon-signal in the solar wind is unnecessary.

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