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http://hdl.handle.net/2248/3070
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DC Field | Value | Language |
---|---|---|
dc.contributor.author | Ramesh, R | - |
dc.date.accessioned | 2008-08-12T08:55:01Z | - |
dc.date.available | 2008-08-12T08:55:01Z | - |
dc.date.issued | 2000-12 | - |
dc.identifier.citation | Journal of Astrophysics and Astronomy, Vol. 21, No. 3 – 4, pp. 237 - 240 | en |
dc.identifier.issn | 0250-6335 | - |
dc.identifier.uri | http://hdl.handle.net/2248/3070 | - |
dc.description.abstract | We present observations of the 'quiet' Sun close to the recent solar minimum (Cycle 22), with the Gauribidanur radioheliograph. Our main conclusion is that coronal streamers also influence the observed radio brightness temperature. | en |
dc.format.extent | 333230 bytes | - |
dc.format.mimetype | application/pdf | - |
dc.language.iso | en | en |
dc.publisher | Indian Academy of Sciences | en |
dc.relation.uri | http://adsabs.harvard.edu/abs/2000JApA...21..237R | en |
dc.subject | Sun | en |
dc.subject | Corona | en |
dc.subject | Radio Observations | en |
dc.subject | Streamers | en |
dc.subject | Scattering | en |
dc.title | Low Frequency Radio Emission from the 'Quiet Sun' | en |
dc.type | Article | en |
Appears in Collections: | IIAP Publications |
Files in This Item:
File | Description | Size | Format | |
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Ramesh R.pdf | 325.42 kB | Adobe PDF | ![]() View/Open |
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