dc.contributor.author |
Ramesh, R |
|
dc.date.accessioned |
2012-02-17T11:07:03Z |
|
dc.date.available |
2012-02-17T11:07:03Z |
|
dc.date.issued |
2011 |
|
dc.identifier.citation |
ASI Conference Series, Vol. 2, pp. 55-61 |
en |
dc.identifier.isbn |
978-81-922926-0-1 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/5699 |
|
dc.description |
Open Access |
en |
dc.description.abstract |
IIA is presently involved in the expansion of its existing radioheliograph
operating in the frequency 120-40 MHz at the Gauribidanur radio
observatory located about 80 km north of Bangalore. Once completed, the
expanded array will have an angular resolution of ~1` at a typical frequency
of 100 MHz. This paper describes the development of solar radio
astronomy activities at IIA since 1952 when the first observations were carried
out. |
en |
dc.language.iso |
en |
en |
dc.publisher |
Astronomical Society of India |
en |
dc.rights |
© Astronomical Society of India |
en |
dc.subject |
Sun: corona |
en |
dc.subject |
Sun: radio radiation – telescopes |
en |
dc.title |
Low frequency solar radio astronomy at the Indian Institute of Astrophysics (IIA) |
en |
dc.type |
Article |
en |