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

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

Sep 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000soph..196..213r&link_type=abstract

Solar Physics, v. 196, Issue 1, p. 213-220 (2000).

Physics

4

Scientific paper

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.

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