The observation of a 'negative burst' with high spatial resolution

Details The observation of a 'negative burst' with high spatial resolution The observation of a 'negative burst' with high spatial resolution

Dec 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991soph..136..335m&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 136, Dec. 1991, p. 335-342.

Physics

6

H Alpha Line, Microwave Emission, Solar Activity, Solar Radio Bursts, Radio Telescopes, Spatial Resolution

Scientific paper

The case of a short-time 'disappearance' of the S-component source over the active region is described and its association with events in H-alpha is discussed. Under the assumption that in this case the radio source was observed to be covered by coronal mass ejection caused by filament eruption, estimates are made of the velocity of the ejection, its linear size, and of the optical thickness.

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