Unusual spatial-temporal dynamics of geomagnetic disturbances during the main phase of the extremely strong magnetic storm of November 7-8, 2004

Details Unusual spatial-temporal dynamics of geomagnetic disturbances during the main phase of the extremely strong magnetic storm of November 7-8, 2004 Unusual spatial-temporal dynamics of geomagnetic disturbances during the main phase of the extremely strong magnetic storm of November 7-8, 2004

Oct 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ge%26ae..46..580k&link_type=abstract

Geomagnetism and Aeronomy, Volume 46, Issue 5, pp.580-592

Computer Science

1

Magnetic Storms, Substorms, Magnetic Pulsations

Scientific paper

The spatial dynamics of geomagnetic variations and pulsations, auroras, and riometer absorption during the development of the main phase of the extremely strong magnetic storm of November 7-8, 2004, has been studied. It has been indicated that intense disturbances were observed in the early morning sector of auroral latitudes rather than in the nighttime sector, as usually takes place during magnetic storms. The unusual spatial dynamics was revealed at the beginning of the storm main phase. A rapid poleward expansion of disturbances from geomagnetic latitudes of 65°-66° to 74°-75° and the development of the so-called polar cap substorm with a negative bay amplitude of up to 2500 nT, accompanied by precipitation of energetic electrons (riometer absorption) and generation of Pi2-Pi3 pulsations, were observed when IMF B z was about -45 nT. The geomagnetic activity maximum subsequently sharply shifted equatorward to 60°-61°. The spatial dynamics of the westward electrojet, Pi2-Pi3 geomagnetic pulsations, and riometer absorption was similar, which can indicate that the source of these phenomena is common.

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