Temporal and spatial characteristics of Pc1 geomagnetic pulsations

Details Temporal and spatial characteristics of Pc1 geomagnetic pulsations Temporal and spatial characteristics of Pc1 geomagnetic pulsations

Jan 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006adspr..38.1572g&link_type=abstract

Advances in Space Research, Volume 38, Issue 8, p. 1572-1575.

Computer Science

Scientific paper

A long-term continuous series (1957 1992) of ground-based observations of ULF emissions in the frequency range of 0.2 5.0 Hz (Pc1) was investigated. To present information uniformly and facilitate comparative analysis, a so-called index N has been introduced, which describes Pc1 activity. Information on cyclic variation of Pc1 activity is given. Pc1 relation to the level of solar and geomagnetic activity, interplanetary magnetic field structure and solar wind parameters (such as the plasma density and bulk velocity, magnetic field strength and direction) in front of the magnetosphere is traced. Latitude dependence of Pc1 activity and its relation to the solar wind conditions are explored.

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