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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Bibliographic Details
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
Description
Summary: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)
ISSN:0992-7689
1432-0576