Radio Interferometric Observations of the Sun Using Commercial Dish TV Antennas
arXiv:2109.07422 · doi:10.1007/s11207-021-01871-9
Abstract
The radio astronomy group in the Indian Institute of Astrophysics (IIA) has been carrying out routine observations of radio emission from the solar corona at low frequencies (40-440MHz) at the Gauribidanur observatory, about 100km north of Bangalore. Since IIA has been performing regular observations of the solar photosphere and chromosphere using different optical telescopes in its Kodaikanal Solar Observatory (KSO) also, the possibilities of obtaining two-dimensional radio images of the solar chromosphere using low-cost instrumentation to supplement the optical observations are being explored. As a part of the exercise, recently the group had developed prototype instrumentation for interferometric observations of radio emission from the solar chromosphere at high frequencies (11.2GHz) using two commercial dish TV antennas. The hardware set-up and initial observations are presented.
Published in Solar Physics, 11 pages, 6 figures
References in corpus (5)
- An estimate of the magnetic field strength associated with a solar coronal mass ejection from low frequency radio observations
- EOVSA Implementation of a Spectral Kurtosis Correlator for Transient Detection and Classification
- On the occurrence of type IV solar radio bursts in the solar cycle 24 and their association with coronal mass ejections
- The Brightness Temperature of the Quiet Solar Chromosphere at 2.6 mm
- Low frequency radio observations of the `quiet' corona during the descending phase of sunspot cycle 24