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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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 |
work_keys_str_mv |
AT bmvyas nighttimefregionanddaytimeeregionionosphericdriftsmeasuredatudaipurduringsolarflares AT bmvyas nighttimefregionanddaytimeeregionionosphericdriftsmeasuredatudaipurduringsolarflares AT rpandey nighttimefregionanddaytimeeregionionosphericdriftsmeasuredatudaipurduringsolarflares |
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