Analysis of the connections between solar wind parameters and day-side geomagnetic pulsations based on data from the observatories Nagycenk (Hungary) and Uzur (U.S.S.R.)

Details Analysis of the connections between solar wind parameters and day-side geomagnetic pulsations based on data from the observatories Nagycenk (Hungary) and Uzur (U.S.S.R.) Analysis of the connections between solar wind parameters and day-side geomagnetic pulsations based on data from the observatories Nagycenk (Hungary) and Uzur (U.S.S.R.)

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985jatp...47..557v&link_type=abstract

Journal of Atmospheric and Terrestrial Physics (ISSN 0021-9169), vol. 47, June 1985, p. 557-565.

Physics

4

Geomagnetic Micropulsations, Magnetospheric Instability, Solar Terrestrial Interactions, Solar Wind, Statistical Correlation, Pulse Amplitude, Statistical Analysis, Wave Propagation

Scientific paper

A comparison is made of results obtained at two widely separated observatories, Nagycenk in Hungary and Uzur in Soviet Siberia (both at geomagnetic latitude 48 deg) and the connection is studied between pulsation parameters and parameters of the interplanetary medium. It is concluded that, in spite of differences in recording and processing, the results are similar and confirm earlier suppositions about these connections. Hypotheses about the location of the excitation clearly favor the pre-shock interplanetary medium with reflected protons counterstreaming to the solar wind. Propagation through the shock wave and the magnetopause, as well as infra-magnetospheric propagation, may later alter certain parameters of the pulsations.

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