Phase observations of geomagnetic pulsations

Details Phase observations of geomagnetic pulsations Phase observations of geomagnetic pulsations

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ge%26ae..22..267g&link_type=abstract

Geomagnetizm i Aeronomiia, vol. 22, Mar.-Apr. 1982, p. 267-271. In Russian.

Mathematics

1

Earth Magnetosphere, Geomagnetic Pulsations, Magnetohydrodynamic Waves, Earth Surface, Geomagnetic Latitude, Mathematical Models, Periodic Variations, Pulse Duration, Solar Wind, Time Dependence

Scientific paper

It is shown that azimuth wavenumbers of MHD waves measured near the equatorial plane of the magnetosphere and numbers measured for corresponding waves of geomagnetic pulsations on the earth's surface should differ. The difference is due to the azimuth dependence of the time of propagation of an MHD disturbance from the equatorial plane to the earth's surface.

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