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

Citation
D. Maia et al., Radio signatures of a fast coronal mass ejection development on November 6, 1997, J GEO R-S P, 104(A6), 1999, pp. 12507-12513
Citations number
18
Categorie Soggetti
Space Sciences
Journal title
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
ISSN journal
21699380 → ACNP
Volume
104
Issue
A6
Year of publication
1999
Pages
12507 - 12513
Database
ISI
SICI code
0148-0227(19990601)104:A6<12507:RSOAFC>2.0.ZU;2-G
Abstract
The Oporto radiospectrograph and the Nancay radioheliograph recorded a radi o event on November 6, 1997, closely related in time with a flare on Nation al Oceanic and Atmospheric Administration (NOAA) active region 8100. At the beginning: of the event the radio sources are located on a rather small vo lume in the vicinity of the flare site. In a timescale df only a few minute s the radio emission sites spread over a large volume in the corona, coveri ng a range of 100 degrees in heliolatitude. During the period of the radio event the Large Angle and Spectrometric Coronagraph (LASCO) on board the So lar 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 re miniscent 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 ra dio sources recorded by the radio instruments.