Distinctive features of Pi1B geomagnetic pulsations

Details Distinctive features of Pi1B geomagnetic pulsations Distinctive features of Pi1B geomagnetic pulsations

Feb 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ge%26ae..27..160s&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 27, Jan.-Feb. 1987, p. 160-162. In Russian.

Physics

Geomagnetic Pulsations, Midlatitude Atmosphere, Polar Regions, Signal Analysis, Ground Stations, Magnetometers

Scientific paper

Based on experimental data, Pi1B pulsations are divided into two types. Type Pi1B-rPi2 has a period of about 1-7 sec, is regional, and has an intensity peak that is observed at the same moment at all stations from low to high latitudes. Type Pi1B-rPip has a period of about 7-24 sec, is local, is observed only in the electrojet region, and has an intensity peak that travels poleward following the electrojet.

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