dc.contributor.author |
Sastry, Ch. V |
|
dc.date.accessioned |
2009-03-25T10:48:01Z |
|
dc.date.available |
2009-03-25T10:48:01Z |
|
dc.date.issued |
1972-05 |
|
dc.identifier.citation |
Astrophysical Letters, Vol. 11, pp. 47 - 51 |
en |
dc.identifier.issn |
0888-6512 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/4415 |
|
dc.description.abstract |
The frequency drift and time splitting of solar radio bursts are observed
with a multi-channel radiometer and a polarimeter at frequencies around 25
MHz. It is found that a majority of noise storm bursts have drift rates
between + 1.0 and -1.0 MHz/sec. Two types of unusual bursts with frequency
drift are described. The two components of a double burst are found to be
polarized to the same degree and in the same sense. |
|
dc.language.iso |
en |
en |
dc.publisher |
Gordon and Breach, Science Publishers Ltd. |
en |
dc.relation.uri |
http://adsabs.harvard.edu/abs/1972ApL....11...47S |
en |
dc.subject |
Frequency Drift |
en |
dc.subject |
Time Splitting of Decameter |
en |
dc.subject |
Solar Radio Bursts |
en |
dc.title |
The frequency drift and time splitting of decameter solar radio bursts |
en |
dc.type |
Article |
en |