RADIO BURSTS OF VERY SHORT DURATION: FINE STRUCTURE OF SOLAR FLARE EMISSIONS

dc.contributor.author	Méndez Berhondo A.L.
dc.contributor.author	Rodríguez Toboada R.E.
dc.date.accessioned	2024-12-02T06:55:59Z
dc.date.available	2024-12-02T06:55:59Z
dc.date.issued	2006
dc.identifier	https://www.elibrary.ru/item.asp?id=14529925
dc.identifier.citation	Geofisica International, 2006, 45, 4, 271-276
dc.identifier.issn	0016-7169
dc.identifier.uri	https://repository.geologyscience.ru/handle/123456789/46779
dc.description.abstract	The fine time structure of sub-second radio events of solar flare emissions is described on the multichannel polarimeter of Station Basovizza at 237, 327, and 408 MHz frequencies. We selected the February 8 and July 9, 1982 solar radio bursts, both associated to gamma flares. We considered only events with more than 100 solar flux units. The relationship between the intensity of the impulsive radio events and the background radio emission is discussed.
dc.subject	POLARIZATION DIAGRAM
dc.subject	SOLAR RADIO EMISSION
dc.subject	SPIKES
dc.title	RADIO BURSTS OF VERY SHORT DURATION: FINE STRUCTURE OF SOLAR FLARE EMISSIONS
dc.type	Статья

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