Electron–ion–neutral temperatures and their ratio comparisons over low latitude ionosphere

dc.contributor.authorBardhan, Ananna
dc.contributor.authorSharma, D.K.
dc.contributor.authorKhurana, M.S.
dc.contributor.authorAggarwal, Malini
dc.contributor.authorKumar, S.
dc.date.accessioned2017-10-26T06:37:58Z
dc.date.accessioned2021-02-12T09:56:02Z
dc.date.available2017-10-26T06:37:58Z
dc.date.available2021-02-12T09:56:02Z
dc.date.issued2015
dc.description.abstractAnnual variations in temperatures of plasma (electron–Te, ion–Ti) using SROSS-C2 satellite and neutral (Tn) using NRLMSIS-00 (neutral atmospheric model); have been investigated and their ratios have been compared over half solar cycle (year 1995–2000, F10.7 72–190). The region under consideration spans over 5–35 N geog. latitude and 65–95 E geog. longitude in the Indian sector, at an average altitude of 500 km. Te and Ti exhibit similar, while Tn show completely different diurnal features. During nighttime Te, Ti and Tn attain equilibrium with each other, but plasma cools faster than neutrals. Magnitude of Te and Ti reduces, while that of Tn increases with increasing solar activity. Ratio comparisons (Te/Tn, Ti/Tn and Te/Ti) show higher sensitivity of electrons compared to ions and neutrals. Te/Tn, Ti/Tn exhibits linear/direct relationship with solar flux, while Te/Ti doesn’t. The deviation of Te, Ti and Tn from equilibrium temperature decreases with increasing solar activity.en_US
dc.identifier.accession091538
dc.identifier.citationAdvances in Space Research, 56, p. 2117–2129, doi: 10.1016/j.asr.2015.08.031en_US
dc.identifier.urihttp://library.iigm.res.in:4000/handle/123456789/996
dc.language.isoenen_US
dc.subjectPlasma temperatures (Te and Ti)en_US
dc.subjectNeutral temperature (Tn)en_US
dc.subjectIonospheric temperature ratios (Te/Tn, Ti/Tn and Te/Ti)en_US
dc.subjectSROSS-C2 satelliteen_US
dc.subjectNeutral atmospheric model – NRLMSIS-00en_US
dc.subjectLow latitude F2 regionen_US
dc.titleElectron–ion–neutral temperatures and their ratio comparisons over low latitude ionosphereen_US
dc.typeArticleen_US

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