Summary
The Gauribidanur Radio Observatory is a radio telescope observatory located at Gauribidanur, near Bengaluru. It is operated jointly by Raman Research Institute and the Indian Institute of Astrophysics. The observatory has been in operation since 1976.
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| Organization | |
|---|---|
| Location | Gauribidanur, Karnataka, India |
| Coordinates | 13°36′N 77°26′E / 13.6°N 77.43°E |
| Established | 1976  |
| Website | www |
| Telescopes |
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  Location of Gauribidanur Radio Observatory | |
 Related media on Commons | |
Location edit
The Gauribidanur Observatory is located at Gauribidanur kolar district (Latitude:13.60° N; Longitude:77.44° E), 100 km north of Bengaluru.
Science and observation edit
The Observatory has been used for studying various aspects of the Sun, galaxies and pulsars.
A few observations with the array have been the first two-dimensional images of radio emission from slowly varying discrete sources in the outer solar corona, an all-sky survey of radio sources at 34.5 MHz in the declination range -30° S to 60° N, and a low frequency carbon recombination lines in astrophysical sources. Studies have also been done of gaseous remnants of exploding stars and the apparently vacant space between members of a cluster of galaxies. Currently, the studies are targeted at pulsars.
Facilities edit
The Gauribidanur Observatory has a 6-meter radio telescope, a radio heliograph, a high resolution radio spectrograph and a gravitational laboratory.
Gauribidanur Telescope edit
The Gauribidanur Telescope is a decameter wave radio telescope. It consists of 1000 dipoles arranged in a "T" configuration. It consists of 1.4 km East-West Arm and a 0.5 km South Arm.[1]
Gauribidanur Radio Heliograph edit
The Gauribidanur Radio Heliograph is a radioheliograph used to obtain two dimensional pictures of the outer solar corona at frequencies from 40-150 MHz. It has been operating since 1997. It consists of 192 log-periodic dipoles arranged in a "T" configuration.[2]
See also edit
References edit
