Please use this identifier to cite or link to this item: https://dspace.iiti.ac.in/handle/123456789/16712
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dc.contributor.authorBrawar, Bhuvneshen_US
dc.contributor.authorDatta, Abhirupen_US
dc.contributor.authorMangla, Sarveshen_US
dc.date.accessioned2025-09-04T12:47:43Z-
dc.date.available2025-09-04T12:47:43Z-
dc.date.issued2025-
dc.identifier.citationBrawar, B., Datta, A., & Mangla, S. (2025). Imaging ionosphere’s wave like structure using interferometry data. Advances in Space Research. https://doi.org/10.1016/j.asr.2025.07.059en_US
dc.identifier.isbn0080283969-
dc.identifier.isbn0080304273-
dc.identifier.isbn0080271618-
dc.identifier.isbn0080304222-
dc.identifier.isbn0080283802-
dc.identifier.isbn0080304281-
dc.identifier.isbn0080304311-
dc.identifier.isbn0080304443-
dc.identifier.issn1879-1948-
dc.identifier.issn0273-1177-
dc.identifier.otherEID(2-s2.0-105012730982)-
dc.identifier.urihttps://dx.doi.org/10.1016/j.asr.2025.07.059-
dc.identifier.urihttps://dspace.iiti.ac.in:8080/jspui/handle/123456789/16712-
dc.description.abstractThe ionosphere is an ionised region in the Earth's upper atmosphere, which significantly impacts radio signal propagation by refracting and reflecting them. As a result, ionospheric disturbances can degrade the performance of navigation, communication, and space-based systems. Understanding the dynamics and processes of the ionosphere is essential, leading to significant advancements in instrumentation and analytical techniques. This study presents an ionospheric imaging technique using interferometric data. Radio interferometers, such as the Giant Meter-wave Radio Telescope (GMRT), are highly sensitive to phase fluctuations, enabling the detection of total electron content (TEC) variations with a precision of 10-3TECu and TEC gradients with an accuracy of approximately 7×10-4TECukm-1. We introduce an antenna-based approach for constructing phase screens using measured TEC gradients for each interferometric baseline by employing a surface reconstruction algorithm. To incorporate the necessary integral constant as a boundary condition, we utilized output from the International Reference Ionosphere (IRI-2016) model. The generalized least squares method was applied to ensure an optimal reconstruction of the ionospheric phase screen, enhancing the accuracy of ionospheric imaging. © 2025 Elsevier B.V., All rights reserved.en_US
dc.language.isoenen_US
dc.publisherElsevier Ltden_US
dc.sourceAdvances in Space Researchen_US
dc.subjectGmrten_US
dc.subjectIrien_US
dc.subjectTecen_US
dc.subjectAntennasen_US
dc.subjectInterferometersen_US
dc.subjectInterferometryen_US
dc.subjectIonosphereen_US
dc.subjectIonospheric Electromagnetic Wave Propagationen_US
dc.subjectIonospheric Measurementen_US
dc.subjectNavigationen_US
dc.subjectRadio Astronomyen_US
dc.subjectRadio Transmissionen_US
dc.subjectRadio Wavesen_US
dc.subjectSurface Reconstructionen_US
dc.subjectGiant Meter-wave Radio Telescopeen_US
dc.subjectInterferometry Dataen_US
dc.subjectIonospheric Disturbanceen_US
dc.subjectIonospheric Imagingen_US
dc.subjectIrien_US
dc.subjectMeter Wave Radio Telescopesen_US
dc.subjectPerformanceen_US
dc.subjectPhase Screenen_US
dc.subjectRadio Signal Propagationen_US
dc.subjectTotal Electron Contenten_US
dc.subjectLeast Squares Approximationsen_US
dc.titleImaging ionosphere's wave like structure using interferometry dataen_US
dc.typeJournal Articleen_US
Appears in Collections:Department of Astronomy, Astrophysics and Space Engineering

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