Evidence of plasma resonance instability from observations of solar decimetric fine structures

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DC Field	Value	Language
dc.creator	Fernandes F.C.R.	-
dc.creator	Sawant H.S.	-
dc.creator	Cecatto J.R.	-
dc.creator	Krishan V.	-
dc.creator	Karlický M.	-
dc.creator	Rosa R.R.	-
dc.date	2003	-
dc.date.accessioned	2013-06-01T09:58:27Z	-
dc.date.available	2013-06-01T09:58:27Z	-
dc.date.issued	2013-06-01	-
dc.identifier	http://www.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332003000100009	-
dc.identifier	http://www.doaj.org/doaj?func=openurl&genre=article&issn=01039733&date=2003&volume=33&issue=1&spage=109	-
dc.identifier.uri	http://koha.mediu.edu.my:8181/jspui/handle/123456789/8009	-
dc.description	The solar radio emissions in the decimetric frequency range (above 1000 MHz) are very rich in temporal and/or spectral fine structures. The Brazilian Solar Spectroscope (BSS) at INPE started operating in 1998. Since then, various types of fine structures, in the frequency range of (1000-2500) MHz, with high time and frequency resolutions have been recorded. The observed bursts include dot-like emissions and chains of dots, lace bursts exhibiting intensity variations as a function of frequency and zebra pattern emissions. It is suggested that they can be generated by a plasma resonance instability mechanism. This model can explain many features of the observed fine structures.	-
dc.publisher	Sociedade Brasileira de Física	-
dc.source	Brazilian Journal of Physics	-
dc.title	Evidence of plasma resonance instability from observations of solar decimetric fine structures	-
Appears in Collections:	Physics and Astronomy

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