Fine structure in solar decametric radiation

dc.contributor.author	Thejappa, G
dc.contributor.author	Sastry, Ch. V
dc.contributor.author	Gopalswamy, N
dc.date.accessioned	2008-08-05T07:15:18Z
dc.date.available	2008-08-05T07:15:18Z
dc.date.issued	1984
dc.identifier.citation	Nonlinear and turbulent processes in physics; Proceedings of the Second International Workshop, Vol. 1, pp. 547 - 561.	en
dc.identifier.uri	http://hdl.handle.net/2248/3001
dc.description.abstract	Observations and interpretations of some of the fine structure in decametric solar radio emission -such as (1) the time structure of type III bursts, (2) absorption bursts, and (3) slowly drifting spikes -are presented. Physical parameters -such as the electron temperature, the characteristics of collisionless shocks, and the coronal magnetic field -are estimated.	en
dc.format.extent	453900 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Harwood Academic Publishers	en
dc.subject	Solar radio emission	en
dc.subject	Coronol magnetic field	en
dc.subject	Bursts	en
dc.title	Fine structure in solar decametric radiation	en
dc.type	Article	en