Radio signatures of a fast coronal mass ejection development on November 6, 1997

被引:77
作者
Maia, D
Vourlidas, A
Pick, M
Howard, R
Schwenn, R
Magalhaes, A
机构
[1] Observ Paris, DASOP, Sect Meudon, CNRS,UMR 8645, F-92195 Meudon, France
[2] USN, Res Lab, Washington, DC 20375 USA
[3] Observ Astron Monte Virgem, Oporto, Portugal
[4] Max Planck Inst Aeron, D-37189 Katlenburg Lindau, Germany
[5] George Mason Univ, Inst Computat Sci & Informat, Fairfax, VA 22030 USA
[6] Univ Lisbon, Fac Ciencias, Lisbon, Portugal
关键词
D O I
10.1029/1999JA900033
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Oporto radiospectrograph and the Nancay radioheliograph recorded a radio event on November 6, 1997, closely related in time with a flare on National Oceanic and Atmospheric Administration (NOAA) active region 8100. At the beginning: of the event the radio sources are located on a rather small volume in the vicinity of the flare site. In a timescale df only a few minutes the radio emission sites spread over a large volume in the corona, covering a range of 100 degrees in heliolatitude. During the period of the radio event the Large Angle and Spectrometric Coronagraph (LASCO) on board the Solar and Heliospheric Observatory (SOHO) observed an extremely fast coronal mass ejection (CME), with a velocity around 2000 km s(-1) This CME presents the particularity of having a fast lateral expansion, giving it a shape reminiscent of a "coat hanger." There is a very good association between the latitudinal extent and time development of the CME seen by LASCO and the radio sources recorded by the radio instruments.
引用
收藏
页码:12507 / 12513
页数:7
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