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dc.contributor.authorThiemann, H.
dc.contributor.authorSojka, J.J.
dc.contributor.authorEccles, J.J.
dc.contributor.authorRao, P.B.
dc.contributor.authorRao, P.V.S. Rama
dc.contributor.authorSridharan, R.
dc.contributor.authorLakhina, G.S.
dc.date.accessioned2015-08-24T07:01:50Z
dc.date.accessioned2021-02-12T09:27:28Z-
dc.date.available2015-08-24T07:01:50Z
dc.date.available2021-02-12T09:27:28Z-
dc.date.issued2001
dc.identifier.citationAdvances in Space Research, v.27/6-7, p.1065-1069, 2001, doi: 10.1016/S0273-1177(01)00139-9en_US
dc.identifier.urihttp://localhost:8080/xmlui/handle/123456789/260-
dc.description.abstractTwo spread-F flights were performed under equinox conditions in April and September 1998 from the Indian low-latitude station SHAR. Both flights detected plasma bubbles confined to a narrow longitudinal extent. Plasma parameters are measured under two different conditions in the post-sunset ionosphere; when the F-layer is moving upward (19:21 IST launch) and when the F-layer is stationary (20:41 IST launch). Low altitude bubbles during upwelling of the F-region in the prereversal current enhancement phase are characterized by turbulent, non Maxwellian regions. Transitional scale waves with k=−3.6 are observed in the bubbles. This flight also detects strong sharp E-layers during downleg and an intermediate layer at 170km. Nighttime bubbles during almost stationary F-layer conditions show turbulent, Maxwellian features with moderate cooling compared to the undisturbed environment. Transitional scale waves in the bubble region show a spectral index k=−3.1. The spectral power is reduced by around 20dB compared to the sunset flight.en_US
dc.language.isoenen_US
dc.subjectPlasma bubblesen_US
dc.subjectF-regionen_US
dc.subjectF-layeren_US
dc.subjectPost sunseten_US
dc.subjectEquatorial F-regionen_US
dc.titleIndo-German low-latitude project deos: plasma bubbles in the post sunset and nighttime sectoren_US
dc.typeArticleen_US
dc.identifier.accession090747
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