dc.contributor.author |
Ramesh, R |
|
dc.contributor.author |
Kathiravan, C |
|
dc.contributor.author |
Sastry, Ch. V |
|
dc.date.accessioned |
2010-03-08T14:23:20Z |
|
dc.date.available |
2010-03-08T14:23:20Z |
|
dc.date.issued |
2010-03 |
|
dc.identifier.citation |
The Astrophysical Journal, Vol. 711, No. 2, pp. 1029 – 1032 |
en |
dc.identifier.issn |
0004-637X |
|
dc.identifier.uri |
http://hdl.handle.net/2248/5057 |
|
dc.description |
Open Access |
en |
dc.description.abstract |
The observations of circularly polarized thermal radio emission from solar coronal streamers at two low frequencies, viz., 77 and 109 MHz, are used to estimate the magnetic field strength (B) at their corresponding radial distances r≈ 1.7 and 1.5 solar radii given by the electron density model of Newkirk. The estimated values of B at the above two distances are ≈5 ± 1 G and 6 ± 2 G, respectively. |
en |
dc.language.iso |
en |
en |
dc.publisher |
Institute of Physics |
en |
dc.relation.uri |
http://www.iop.org/EJ/abstract/0004-637X/711/2/1029 |
en |
dc.rights |
© Institute of Physics |
en |
dc.subject |
Sun: Activity |
en |
dc.subject |
Sun: Corona |
en |
dc.subject |
Sun: Magnetic Topology |
en |
dc.subject |
Sun: Radio Radiation |
en |
dc.title |
Estimation of magnetic field in the solar coronal streamers through low frequency radio observations |
en |
dc.type |
Article |
en |