Type II burst high time resolution and polarization characteristics at frequencies higher than 200 MHz

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4331

Full metadata record

DC Field	Value	Language
dc.contributor.author	Zlobec, P	-
dc.contributor.author	Thejappa, G	-
dc.date.accessioned	2009-02-04T16:31:37Z	-
dc.date.available	2009-02-04T16:31:37Z	-
dc.date.issued	1987	-
dc.identifier.citation	Hvar Observatory Bulletin, Vol. 11, No. 1, pp. 111 - 116	en
dc.identifier.issn	0351-2657	-
dc.identifier.uri	http://hdl.handle.net/2248/4331	-
dc.description.abstract	Some new results based on high time resolution and polarization studies of solar type II radio bursts are presented. It is found that the fine structures are present in some events whereas they are completely absent in few other cases. The fine structures generally appear at the beginning of an event. The polarization remains constant during the entire event.	en
dc.language.iso	en	en
dc.publisher	Hvar Observatory Bulletin	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1987HvaOB..11..111Z	en
dc.subject	Type II Burst	en
dc.subject	High Time Resolution	en
dc.subject	Polarization Characteristics	en
dc.subject	Solar Type II Radio Bursts	en
dc.title	Type II burst high time resolution and polarization characteristics at frequencies higher than 200 MHz	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

Files in This Item:

File	Description	Size	Format
Type II burst high time resolution and polarization		451.54 kB	Adobe PDF	View/Open

DSpace JSPUI