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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/8873
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dc.contributor.authorKathiravan, C-
dc.contributor.authorGireesh, G. V. S-
dc.contributor.authorBarve, Indrajit V-
dc.contributor.authorSayuf, Shaik-
dc.contributor.authorRamesh, R-
dc.date.accessioned2026-02-05T08:45:13Z-
dc.date.available2026-02-05T08:45:13Z-
dc.date.issued2025-12-
dc.identifier.citationJournal of Astrophysics and Astronomy, Vol. 46, No. 2, 63en_US
dc.identifier.issn0973-7758-
dc.identifier.urihttp://hdl.handle.net/2248/8873-
dc.descriptionRestricted Accessen_US
dc.descriptionThe original publication is available at springerlink.com-
dc.description.abstractWe 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.isoenen_US
dc.publisherSpringer Natureen_US
dc.relation.urihttps://doi.org/10.1007/s12036-025-10096-2-
dc.rights© Indian Academy of Sciences-
dc.subjectSunen_US
dc.subjectMagnetic fielden_US
dc.subjectRadio telescopesen_US
dc.subjectInterferometryen_US
dc.subjectPolarizationen_US
dc.titleA prototype radio interferometer system with commercial dish TV antennas for observations of the solar chromospheric magnetic fielden_US
dc.typeArticleen_US
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