A prototype radio interferometer system with commercial dish TV antennas for observations of the solar chromospheric magnetic field

dc.contributor.author	Kathiravan, C
dc.contributor.author	Gireesh, G. V. S
dc.contributor.author	Barve, Indrajit V
dc.contributor.author	Sayuf, Shaik
dc.contributor.author	Ramesh, R
dc.date.accessioned	2026-02-05T08:45:13Z
dc.date.available	2026-02-05T08:45:13Z
dc.date.issued	2025-12
dc.identifier.citation	Journal of Astrophysics and Astronomy, Vol. 46, No. 2, 63	en_US
dc.identifier.issn	0973-7758
dc.identifier.uri	http://hdl.handle.net/2248/8873
dc.description	Restricted Access	en_US
dc.description	The original publication is available at springerlink.com
dc.description.abstract	We are exploring the possibility of carrying out radio interferometric observations of the solar chromosphere at ≈ 11.2 GHz (λ=2.68 cm), in both total intensity (Stokes-I) and circularly polarized intensity (Stokes-V), using low-cost commercial dish TV antennas. Here, we present our initial results on the magnetic field strength (B) estimated using data obtained with a prototype set-up, and compare them with similar observations.	en_US
dc.language.iso	en	en_US
dc.publisher	Springer Nature	en_US
dc.relation.uri	https://doi.org/10.1007/s12036-025-10096-2
dc.rights	© Indian Academy of Sciences
dc.subject	Sun	en_US
dc.subject	Magnetic field	en_US
dc.subject	Radio telescopes	en_US
dc.subject	Interferometry	en_US
dc.subject	Polarization	en_US
dc.title	A prototype radio interferometer system with commercial dish TV antennas for observations of the solar chromospheric magnetic field	en_US
dc.type	Article	en_US