|
Detailed Reference Information |
Maia, D., Vourlidas, A., Pick, M., Howard, R., Schwenn, R. and Magalhães, A. (1999). Radio signatures of a fast coronal mass ejection development on November 6, 1997. Journal of Geophysical Research 104: doi: 10.1029/1999JA900033. issn: 0148-0227. |
|
The Oporto radiospectrograph and the Nan¿ay 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 of only a few minutes the radio emission sites spread over a large volume in the corona, covering a range of 100¿ 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. ¿ 1999 American Geophysical Union |
|
|
|
BACKGROUND DATA FILES |
|
|
Abstract |
|
|
|
|
|
Keywords
Solar Physics, Astrophysics, and Astronomy, Solar Physics, Astrophysics, and Astronomy, Coronal mass ejections, Solar Physics, Astrophysics, and Astronomy, Flares, Solar Physics, Astrophysics, and Astronomy, Radio emissions, Space Plasma Physics, Nonlinear phenomena |
|
Publisher
American Geophysical Union 2000 Florida Avenue N.W. Washington, D.C. 20009-1277 USA 1-202-462-6900 1-202-328-0566 service@agu.org |
|
|
|