The Halo CME Event Of 23 October 1997 – Low-Frequency Radio Observations Of The Pre-Event Corona.

Autor: Ramesh, R.
Zdroj: Solar Physics; Sep2000, Vol. 196 Issue 1, p213-220, 8p
Abstrakt: We report low-frequency observations of an enhancement in the solar corona prior to the halo coronal mass ejection of 23 October 1997, with the Gauribidanur radioheliograph. The Sun was ‘quiet’ and no radio bursts were observed either prior to or in the aftermath of the event. The radio method would be useful in studying the pre-event structures associated with the eruptive solar activity, particularly from the ground. [ABSTRACT FROM AUTHOR]
Databáze: Complementary Index
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