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Titolo:
Effects of solar wind density on auroral electrojets
Autore:
Shue, JH; Kamide, Y;
Indirizzi:
Johns Hopkins Univ, Appl Phys Lab, Laurel, MD 20723 USA Johns Hopkins Univ Laurel MD USA 20723 ppl Phys Lab, Laurel, MD 20723 USA Nagoya Univ, Solar Terr Environm Lab, Aichi 4428507, Japan Nagoya Univ Aichi Japan 4428507 Terr Environm Lab, Aichi 4428507, Japan
Titolo Testata:
GEOPHYSICAL RESEARCH LETTERS
fascicolo: 11, volume: 28, anno: 2001,
pagine: 2181 - 2184
SICI:
0094-8276(20010601)28:11<2181:EOSWDO>2.0.ZU;2-P
Fonte:
ISI
Lingua:
ENG
Soggetto:
JANUARY 1997; CME EVENT;
Tipo documento:
Article
Natura:
Periodico
Settore Disciplinare:
Physical, Chemical & Earth Sciences
Citazioni:
16
Recensione:
Indirizzi per estratti:
Indirizzo: Shue, JH Johns Hopkins Univ, Appl Phys Lab, 11100 Johns Hopkins Rd, Laurel, MD 20723 USA Johns Hopkins Univ 11100 Johns Hopkins Rd Laurel MD USA 20723 USA
Citazione:
J.H. Shue e Y. Kamide, "Effects of solar wind density on auroral electrojets", GEOPHYS R L, 28(11), 2001, pp. 2181-2184

Abstract

During the magnetic cloud event of January 10-11, 1997, several density enhancements in the solar wind were observed while other solar wind parameters were relatively constant. By using this fortuitous opportunity, the effects of the solar wind density on the intensity of the auroral electrojets are examined. It is found that a positive relationship exists between the solar wind density and the intensity of the auroral electrojets. The relationship is found to be much weaker for northward interplanetary magnetic field (IMF) than for southward IMF. it is also shown that when the IMF is directed southward, the density effect is dominant in the westward electrojet, while it is most effective in the eastward electrojet when the IMF is directednorthward.

ASDD Area Sistemi Dipartimentali e Documentali, Università di Bologna, Catalogo delle riviste ed altri periodici
Documento generato il 26/09/20 alle ore 16:42:11