The effect of geomagnetic field structure and plasma density distribution on Pc1 pulsation propagation in the magnetosphere

Details The effect of geomagnetic field structure and plasma density distribution on Pc1 pulsation propagation in the magnetosphere The effect of geomagnetic field structure and plasma density distribution on Pc1 pulsation propagation in the magnetosphere

Jun 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981ge%26ae..21..511a&link_type=abstract

Geomagnetizm i Aeronomiia, vol. 21, May-June 1981, p. 511-516. In Russian.

Physics

Geomagnetic Micropulsations, Geomagnetism, Magnetospheric Electron Density, Plasma Density, Solar Wind, Density Distribution, Field Theory (Physics), Plasma-Electromagnetic Interaction

Scientific paper

A numerical analysis has been made of the effect of plasma and geomagnetic field parameters on Pc1 pulsation propagation in the magnetosphere. On the basis of a two-dipole model of the magnetosphere, the interaction between the field and solar wind flux was investigated. The results are compared to calculations made for a dipole model of the field.

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