Please use this identifier to cite or link to this item: https://dspace.iiti.ac.in/handle/123456789/3727
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dc.contributor.authorChakraborty, Sumanjiten_US
dc.contributor.authorDatta, Abhirupen_US
dc.contributor.authorAyyagari, Deepthien_US
dc.date.accessioned2022-03-17T01:00:00Z-
dc.date.accessioned2022-03-17T15:30:02Z-
dc.date.available2022-03-17T01:00:00Z-
dc.date.available2022-03-17T15:30:02Z-
dc.date.issued2020-
dc.identifier.citationChakraborty, S., Datta, A., Ray, S., Ayyagari, D., & Paul, A. (2020). Comparative studies of ionospheric models with GNSS and NavIC over the indian longitudinal sector during geomagnetic activities. Advances in Space Research, 66(4), 895-910. doi:10.1016/j.asr.2020.04.047en_US
dc.identifier.issn0273-1177-
dc.identifier.otherEID(2-s2.0-85085071390)-
dc.identifier.urihttps://doi.org/10.1016/j.asr.2020.04.047-
dc.identifier.urihttps://dspace.iiti.ac.in/handle/123456789/3727-
dc.description.abstractThis paper presents the storm time comparative analysis of the performances of latest versions of global ionospheric models: International Reference Ionosphere (IRI) 2016, NeQuick 2 (NeQ) and the IRI extended to Plasmasphere (IRI-P) 2017 with respect to Navigation with Indian Constellation (NavIC) and Global Navigation Satellite System (GNSS) derived ionospheric Total Electron Content (TEC). The analysis is carried out under varying geomagnetic storm conditions during September 2017-November 2018, falling in the declining phase of solar cycle 24. TEC data from Indore, located near the northern crest of the Equatorial Ionization Anomaly (EIA) along with data obtained from the International GNSS Service (IGS) stations at Lucknow, located beyond the anomaly crest; Hyderabad, located between anomaly crest and magnetic equator and Bangalore, located near the magnetic equator have been analysed. The models generally overestimated during the storm periods with the exception of IRI-P, which matched (with an offset of about 3–5 TECU) with the enhancement observed on September 7, 2017 (during the strong storm of September 2017), from stations around the anomaly crest. No significant match was observed by the other two models. This match of IRI-P is attributed to the plasmaspheric contribution as well as the capability of assimilating measured TEC values into this model. In the present study, to the best of our knowledge, first comparisons of the empirical model derived TEC with NavIC and GNSS measurements from an anomaly crest location, combined with the IGS observations from the magnetic equator to locations beyond the anomaly crest, are conducted during geomagnetically disturbed conditions. Since NavIC satellites are at higher altitudes (~ 36000 km), the inclusion of NavIC data to the existing model could give better ionospheric predictions over the Indian subcontinent. © 2020 COSPARen_US
dc.language.isoenen_US
dc.publisherElsevier Ltden_US
dc.sourceAdvances in Space Researchen_US
dc.subjectGeomagnetismen_US
dc.subjectIonosphereen_US
dc.subjectMagnetosphereen_US
dc.subjectSolar energyen_US
dc.subjectStormsen_US
dc.subjectComparative analysisen_US
dc.subjectComparative studiesen_US
dc.subjectEquatorial ionization anomalies (EIA)en_US
dc.subjectGeomagnetic activitiesen_US
dc.subjectGlobal Navigation Satellite Systemsen_US
dc.subjectIndian subcontinentsen_US
dc.subjectInternational reference ionospheresen_US
dc.subjectIonospheric total electron contenten_US
dc.subjectGlobal positioning systemen_US
dc.titleComparative studies of ionospheric models with GNSS and NavIC over the Indian longitudinal sector during geomagnetic activitiesen_US
dc.typeJournal Articleen_US
dc.rights.licenseAll Open Access, Green-
Appears in Collections:Department of Astronomy, Astrophysics and Space Engineering

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