dc.contributor.author |
Sastry, Ch. V |
|
dc.contributor.author |
Subramanian, K. R |
|
dc.date.accessioned |
2009-07-24T11:09:59Z |
|
dc.date.available |
2009-07-24T11:09:59Z |
|
dc.date.issued |
1974-09 |
|
dc.identifier.citation |
Indian Journal of Radio and Space Physics, Vol. 4, pp. 196 - 198 |
en |
dc.identifier.issn |
0367-8393 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/4674 |
|
dc.description.abstract |
Observations on the occultation of the radio source Tamas A (3C 144) during June 1971 at a wavelength of 12 m are presented. It is tentatively observed that there is no strong dependence between the amount of scattering
and solar activity. |
en |
dc.language.iso |
en |
en |
dc.publisher |
National Institute of Science Communication and Information Resources |
en |
dc.subject |
Radio Source Tauras |
en |
dc.subject |
Solar Corona |
en |
dc.subject |
Occultation |
en |
dc.title |
Observations on the occultation of the radio source Tauras A by the solar corona during June 1971 |
en |
dc.type |
Article |
en |