Physics
Scientific paper
Aug 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ge%26ae..31..135p&link_type=abstract
Geomagn. Aeron., Vol. 31, No. 1, p. 135 - 136
Physics
1
Solar Wind: Hydrodynamics, Solar Wind: Interplanetary Plasma
Scientific paper
Long-period (T ⪆ 300 seconds) geomagnetic field pulsations in the Earth's magnetosphere are modeled on the basis of a forced oscillation representation. The oscillation generator is considered to be a large-scale eddy formed during the flow of the solar wind around the magnetosphere. With this model representation the characteristic pulsation periods as a function of the solar wind parameters and criteria characterizing the quasi-turbulent flow regime can be found. To visualize the flow around the magnetosphere, use is made of the data on comets, for which rotations and oscillations of the tail relative to the Sun-Earth line are frequently observed. A joint analysis is made of specific events - the sudden rotation of the tail of the Bradfield comet and pulsations at the Earth, 6 February 1980.
Kereselidze Z. A.
Ptitsyna N. G.
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