Daytime Pi1C pulsations in the polar cap when the Bz component of the IMF is much greater than 0

Details Daytime Pi1C pulsations in the polar cap when the Bz component of the IMF is much greater than 0 Daytime Pi1C pulsations in the polar cap when the Bz component of the IMF is much greater than 0

Jun 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ge%26ae..28..514b&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 28, May-June 1988, p. 514-516. In Russian.

Computer Science

Geomagnetic Micropulsations, Interplanetary Magnetic Fields, Polar Caps, Current Distribution, Daytime, Earth Magnetosphere, Field Aligned Currents

Scientific paper

Pi1C pulsations were detected in the daytime southern polar cap when the Bz component was much greater than 0. Their appearance is shown to be due to a specific combination of the azimuthal and radial components of the IMF, where By is less than 0 and Bx is greater than 0. The daytime Pi1C pulsations in the daytime polar cap are shown to be closely correlated with the NBZ system of field-aligned currents, which makes it possible to use observations of such pulsations when Bz is much greater than 0 for the diagnostics of field-aligned currents in the polar cap.

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