Pulsed reconnection as a possible source of ipcl pulsations

Details Pulsed reconnection as a possible source of ipcl pulsations Pulsed reconnection as a possible source of ipcl pulsations

Oct 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ge%26ae..22..877b&link_type=abstract

Geomagnetizm i Aeronomiia, vol. 22, Sept.-Oct. 1982, p. 877-879. In Russian.

Computer Science

1

Geomagnetic Pulsations, Interplanetary Magnetic Fields, Magnetopause, Causes, Geomagnetism, Polar Caps, Solar Terrestrial Interactions, Solar Wind Velocity

Scientific paper

It is shown that several subclasses of ipcl pulsations of the geomagnetic field can be identified, each of which corresponds to a particular type of reconnection of the interplanetary and geomagnetic fields. It is noted that these pulsations, accompanying pulsed reconnection, possess the following specific features: maximum intensity in the polar-cusp region, where the reconnection process is localized; dependence of pulsation amplitude on solar wind velocity; determination of pulsation intensity by the Bz component of the IMF, which conditions the pulsed reconnection; and a characteristic regime in the form of individual intense bursts corresponding to pulsed reconnection.

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