Eclipse Observations of Compact Sources in the Outer Solar Corona

dc.contributor.author	Ramesh, R
dc.contributor.author	Subramanian, K. R
dc.contributor.author	Sastry, Ch. V
dc.date.accessioned	2008-08-14T09:46:05Z
dc.date.available	2008-08-14T09:46:05Z
dc.date.issued	1999-03
dc.identifier.citation	Solar Physics, Vol. 185, No. 1, pp. 77 - 85	en
dc.identifier.uri	http://hdl.handle.net/2248/3132
dc.description.abstract	We report here on high angular resolution observations of solar noise storm sources at a frequency of 75MHz. The data for the study were obtained at the Gauribidanur Radio Observatory (long.: 77 deg26'12''E, lat.: 13 deg36'12''N) about 100km north of Bangalore, India, during the solar eclipse of 24October 1995. Our main conclusion is that there are structures of angular size <=2.5arcmin in the outer solar corona.	en
dc.format.extent	128908 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Kluwer Academic Publishers	en
dc.relation.uri	http://www.springerlink.com/content/k76784k767q13967/	en
dc.subject	Eclipse Observations	en
dc.subject	Outer Solar Corona	en
dc.title	Eclipse Observations of Compact Sources in the Outer Solar Corona	en
dc.type	Article	en