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Abstract Form

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Solar wind control of the substorm westward electrojet

I.V. Despirak 1 , A.G. Yahnin 1 , A.A. Lubchich 1 , A.B. Pashin 1 and A.L. Kotikov 2

1. Polar Geophysical Institute, Apatity, Russia
2. Institute of Physics, University of St-Petersburg, St-Petersburg, Russia

During the expansion phase of a substorm the westward electrojet expands poleward following the auroral expansion. Sometimes the electrojet propagates from the auroral zone up to very high latitudes (CGLat >75-80). These substorms are called "high-latitudinal" substorms. Sergeev et al (1979) and Dmitrieva and Sergeev (1984) showed that such "high-latitudinal" substorms occur under high-speed solar wind, and the latitude of the electrojet propagation is higher when the solar wind velocity is larger. It was shown that "high-latitudinal" substorms occur more frequently during the solar cycle
Address:
Polar Geophysical Institute RAS
184209 Apatity Murmansk region
Akademgorodok 26a
Russia 		Program committee:
Dr. I.V. Mingalev (Chairman, PGI, Apatity)
Dr. A.A. Lubchich (V.C., PGI, Apatity)
Dr. B.V. Kozelov (PGI, Apatity)
Dr. A.G. Demekhov (IAP RAS/PGI, Nizhny Novgorod/Apatity)
Dr. I.I. Alexeev (SINP MSU, Moscow)
Dr. V.V. Kalegaev (SINP MSU, Moscow)
Dr. M.V. Klimenko (West Department of IZMIRAN RAS, Kaliningrad)
Dr. V.V. Mishin (ISTP SB RAS, Irkutsk)
Dr. A.A. Petrukovich (SRI, Moscow)
Dr. V.A. Pilipenko (IPE RAS, Moscow)
Dr. V.S. Semenov (St Petersburg State University, Saint-Petersburg)
Dr. V.A. Sergeev (St Petersburg State University, Saint-Petersburg)
Dr. E.V. Rozanov (Davos World Radiation Centre, Davos, Switzerland) 		Organizing committee:
Dr. Andrey Demekhov (Chairman)
Dr. Andris Lubchich
Dr. Irina Despirak
Dr. Boris Gvozdevsky
Dr. Konstantin Orlov
Tatyana Popova
Pavel Setsko