dc.contributor.author |
Ramesh, R |
|
dc.contributor.author |
Subramanian, K. R |
|
dc.contributor.author |
Sastry, Ch. V |
|
dc.date.accessioned |
2008-08-18T06:52:15Z |
|
dc.date.available |
2008-08-18T06:52:15Z |
|
dc.date.issued |
2000 |
|
dc.identifier.citation |
Advances in Space Research, Vol. 25, No. 9, pp. 1847 - 1850 |
en |
dc.identifier.issn |
0273-1177 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/3157 |
|
dc.description |
Restricted Access |
en |
dc.description.abstract |
We report high angular resolution observations of the outer solar corona carried out at 75 MHz from the Gauribidanur Radio Observatory (Long: 77°26'12" E, Lat: 13°36'12" N) about 100 km north of Bangalore, India, during the solar eclipse of October 24, 1995. Our main conclusion is that there are structures of angular size <= 2.5' in the outer solar corona at a height of <<< 0.4 R⊚ above the photosphere |
en |
dc.format.extent |
320635 bytes |
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dc.format.mimetype |
application/pdf |
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dc.language.iso |
en |
en |
dc.publisher |
Elsevier |
en |
dc.relation.uri |
http://dx.doi.org/doi:10.1016/S0273-1177(99)00596-7 |
en |
dc.subject |
High angular resolution |
en |
dc.subject |
Outer solar corona |
en |
dc.title |
High Angular Resolution Radio Observations of the Outer Solar Corona |
en |
dc.type |
Article |
en |