The low-frequency radio spectrum of the continuum emission from the undisturbed Sun
| dc.contributor.author | Subramanian, K.R. | |
| dc.contributor.author | Sastry, Ch.V. | |
| dc.date.accessioned | 2006-01-06T05:53:06Z | |
| dc.date.available | 2006-01-06T05:53:06Z | |
| dc.date.issued | 1988 | |
| dc.description.abstract | The low-frequency radio spectrum of the continuum emission from the undisturbed sun is determined for 24 days during the period May-September 1985. It is found that the spectral index varied from + 1.6 to + 3.6 during this period. It is suggested that the large positive spectral indices are due to the existence of temperature gradients in the outer corona. | en |
| dc.format.extent | 484957 bytes | |
| dc.format.mimetype | application/pdf | |
| dc.identifier.citation | Journal of Astrophysics and Astronomy, 1988, Vol. 9, p 225-229. | en |
| dc.identifier.issn | 0250-6335 | |
| dc.identifier.uri | http://hdl.handle.net/2289/1110 | |
| dc.language.iso | en | en |
| dc.publisher | Indian Academy of Sciences, Bangalore, India. | en |
| dc.rights | Indian Academy of Sciences, Bangalore, India. | en |
| dc.subject | Sun | en |
| dc.subject | Low-frequency radio observation | en |
| dc.subject | Sun, Corona | en |
| dc.title | The low-frequency radio spectrum of the continuum emission from the undisturbed Sun | en |
| dc.type | Article | en |