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dc.contributor.authorRajaram, G.
dc.contributor.authorArun, T.
dc.contributor.authorDhar, Ajay
dc.date.accessioned2015-08-24T10:43:37Z
dc.date.accessioned2021-02-12T09:27:23Z-
dc.date.available2015-08-24T10:43:37Z
dc.date.available2021-02-12T09:27:23Z-
dc.date.issued2002
dc.identifier.citationAdv. Space Res., v.30/10, p. 2195-2201, 2002, doi: 10.1016/S0273-1177(02)80220-4en_US
dc.identifier.urihttp://localhost:8080/xmlui/handle/123456789/267-
dc.description.abstractA splendid display of “aurora australis” was observed over the Indian Antarctic station Maitri (geomag. lat. 62°.8 S, long. 52°.8 E; L = 4.8) on the night of 4–5 March 1999. The changes recorded by a fluxgate magnetometer, and a 30 MHz riometer operating at Maitri are interpreted in terms of currently - understood auroral physics. Interplanetary magnetic field and plasma parameters recorded by the WIND satellite indicate very high solar wind velocities (500–600 km/s), and prolonged southward Bz of average value (∼ 5 nT), during the auroral event. Ion density is however an average 3–4/cm3, and Ion pressure only 2–3 nano Pascals during the event.en_US
dc.language.isoenen_US
dc.subjectIndian Antarctic station Maitrien_US
dc.subjectMagnetosphereen_US
dc.subjectRiometer observationsen_US
dc.subjectMagnetosphere-ionosphere couplingen_US
dc.subjectAurora australisen_US
dc.titleDiagnostics of magnetosphere-ionosphere coupling over Indian Antarctic station Maitri, from magnetometer and riometer observations during the optical auroral event of 4–5 March 1999en_US
dc.typeArticleen_US
dc.identifier.accession090754
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