Fast and slow responses of auroral indices to variations of the interplanetary magnetic field during a substorm

Details Fast and slow responses of auroral indices to variations of the interplanetary magnetic field during a substorm Fast and slow responses of auroral indices to variations of the interplanetary magnetic field during a substorm

Dec 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ge%26ae..23..979s&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 23, Nov.-Dec. 1983, p. 979-987. In Russian.

Computer Science

1

Auroral Electrojets, Geomagnetic Tail, Interplanetary Magnetic Fields, Magnetic Variations, Polar Substorms, Cross Correlation, Magnetic Disturbances, Time Lag

Scientific paper

A cross correlation of the AL, AU, and AE indices with the Bz component of the interplanetary magnetic field and the epsilon parameter is carried out on the basis of 4-min data individually for three substorm phases. The existence of fast and slow responses of auroral electrojets to IMF variations is observed. It is suggested that these responses correspond to different substorm components: with and without energy accumulation in the magnetotail.

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