Night-time F-region and daytime E-region ionospheric drifts measured at Udaipur during solar flares

Ionospheric drifts measured at a low latitude station, Udaipur (Geomag. Lat. 14.5° N), in the night-time F-region and daytime E-region during solar flares have been studied. The night-time observations, which correspond to the F-region drifts, were carried out on five different nights. The d...

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Main Authors: B. M. Vyas, R. Pandey
Format: Article
Language:English
Published: Copernicus Publications 2002-11-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/20/1837/2002/angeo-20-1837-2002.pdf
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spelling doaj-d535efad30914ca381ba8305a09881232020-11-24T21:30:50ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05762002-11-01201837184210.5194/angeo-20-1837-2002Night-time F-region and daytime E-region ionospheric drifts measured at Udaipur during solar flaresB. M. Vyas0B. M. Vyas1R. Pandey2Correspondence to: R. Pandey (pandey r@yahoo.com)Department of Physics, M. L. Sukhadia University, Udaipur 313 001, IndiaDepartment of Physics, M. L. Sukhadia University, Udaipur 313 001, IndiaIonospheric drifts measured at a low latitude station, Udaipur (Geomag. Lat. 14.5° N), in the night-time F-region and daytime E-region during solar flares have been studied. The night-time observations, which correspond to the F-region drifts, were carried out on five different nights. The daytime observation corresponding to the E-region drifts is only for one day. It is found that the apparent drift during the solar flare period is reduced considerably, in the daytime E-region as well as in the night-time F-region. The East-West and North-South components of the apparent drift speed are also similarly affected. For the daytime E-region drifts during a flare, increased ionization and subsequent reduction of reflection height is proposed to be the cause of reduced drift speeds. For the night-time F-region drifts, a reduced electric field at the F-region heights resulting from coupling of sunlit and dark hemispheres has been proposed to be the possible cause.<br><br><b>Key words. </b>Ionosphere (electric fields and currents; ionospheric disturbances)https://www.ann-geophys.net/20/1837/2002/angeo-20-1837-2002.pdf
collection DOAJ
language English
format Article
sources DOAJ
author B. M. Vyas
B. M. Vyas
R. Pandey
spellingShingle B. M. Vyas
B. M. Vyas
R. Pandey
Night-time F-region and daytime E-region ionospheric drifts measured at Udaipur during solar flares
Annales Geophysicae
author_facet B. M. Vyas
B. M. Vyas
R. Pandey
author_sort B. M. Vyas
title Night-time F-region and daytime E-region ionospheric drifts measured at Udaipur during solar flares
title_short Night-time F-region and daytime E-region ionospheric drifts measured at Udaipur during solar flares
title_full Night-time F-region and daytime E-region ionospheric drifts measured at Udaipur during solar flares
title_fullStr Night-time F-region and daytime E-region ionospheric drifts measured at Udaipur during solar flares
title_full_unstemmed Night-time F-region and daytime E-region ionospheric drifts measured at Udaipur during solar flares
title_sort night-time f-region and daytime e-region ionospheric drifts measured at udaipur during solar flares
publisher Copernicus Publications
series Annales Geophysicae
issn 0992-7689
1432-0576
publishDate 2002-11-01
description Ionospheric drifts measured at a low latitude station, Udaipur (Geomag. Lat. 14.5° N), in the night-time F-region and daytime E-region during solar flares have been studied. The night-time observations, which correspond to the F-region drifts, were carried out on five different nights. The daytime observation corresponding to the E-region drifts is only for one day. It is found that the apparent drift during the solar flare period is reduced considerably, in the daytime E-region as well as in the night-time F-region. The East-West and North-South components of the apparent drift speed are also similarly affected. For the daytime E-region drifts during a flare, increased ionization and subsequent reduction of reflection height is proposed to be the cause of reduced drift speeds. For the night-time F-region drifts, a reduced electric field at the F-region heights resulting from coupling of sunlit and dark hemispheres has been proposed to be the possible cause.<br><br><b>Key words. </b>Ionosphere (electric fields and currents; ionospheric disturbances)
url https://www.ann-geophys.net/20/1837/2002/angeo-20-1837-2002.pdf
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