Please use this identifier to cite or link to this item: https://dspace.iiti.ac.in/handle/123456789/10811
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dc.contributor.authorMangla, Sarvesh;Datta, Abhirup;en_US
dc.date.accessioned2022-11-03T19:41:21Z-
dc.date.available2022-11-03T19:41:21Z-
dc.date.issued2022-
dc.identifier.citationMangla, S., & Datta, A. (2022). Probing equatorial ionosphere using GMRT at sub-GHz frequencies. Paper presented at the 2022 3rd URSI Atlantic and Asia Pacific Radio Science Meeting, AT-AP-RASC 2022, doi:10.23919/AT-AP-RASC54737.2022.9814349 Retrieved from www.scopus.comen_US
dc.identifier.isbn978-9463968058-
dc.identifier.otherEID(2-s2.0-85134882438)-
dc.identifier.urihttps://doi.org/10.23919/AT-AP-RASC54737.2022.9814349-
dc.identifier.urihttps://dspace.iiti.ac.in/handle/123456789/10811-
dc.description.abstractRadio Interferometer is an array of elements that are simultaneously working together to measure spatial coherence function to provide images of astronomical sources with unmatched resolving power. The effect of the ionosphere limits our ability to explore the sky at sub-GHz frequencies by introducing an extra phase term, which is particularly hard to calibrate in the low signal-to-noise ratio (S/N) regime. Interferometers like Very Large Array (VLA), LOwFrequency ARray (LOFAR), Murchison Widefield Array (MWA), Giant Meterwave Radio Telescope (GMRT), and future instruments such as Square Kilometre Array (SKA) are all affected in the same way. © 2022 URSI.en_US
dc.language.isoenen_US
dc.publisherInstitute of Electrical and Electronics Engineers Inc.en_US
dc.source2022 3rd URSI Atlantic and Asia Pacific Radio Science Meeting, AT-AP-RASC 2022en_US
dc.subjectInterferometers; Ionospheric measurement; Radio astronomy; Radio telescopes; Signal to noise ratio; Astronomical sources; Coherence function; Equatorial ionosphere; GHz frequencies; Giant meterwave radio telescopes; Low signal-to-noise ratio; Radio interferometers; Spatial coherence; Sub-GHz; Very large arrays; Ionosphereen_US
dc.titleProbing equatorial ionosphere using GMRT at sub-GHz frequenciesen_US
dc.typeConference Paperen_US
Appears in Collections:Department of Astronomy, Astrophysics and Space Engineering

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