Zonal drifts of ionospheric irregularities at temperate latitude in the Indian region

The systematic time differences observed in the onset of postsunset VHF scintillations recorded simultaneously at Ujjain (Geogr. lat. 23.2<sup>°</sup>N, Geogr. long. 75.6<sup>°</sup>E) and Bhopal (Geogr. lat. 23.2<sup>°</sup>N, Geogr. long. 77.6<sup>°<...

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Main Authors: S. Kumar, A. K. Gwal, B. M. Pathan, D. R. K. Rao
Format: Article
Language:English
Published: Copernicus Publications 1995-07-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/13/724/1995/angeo-13-724-1995.pdf
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author S. Kumar
A. K. Gwal
B. M. Pathan
D. R. K. Rao
author_facet S. Kumar
A. K. Gwal
B. M. Pathan
D. R. K. Rao
author_sort S. Kumar
collection DOAJ
description The systematic time differences observed in the onset of postsunset VHF scintillations recorded simultaneously at Ujjain (Geogr. lat. 23.2<sup>°</sup>N, Geogr. long. 75.6<sup>°</sup>E) and Bhopal (Geogr. lat. 23.2<sup>°</sup>N, Geogr. long. 77.6<sup>°</sup>E), situated at the peak of the anomaly crest in the Indian region, have been analysed to determine the zonal drifts of scintillation-producing irregularities. The method is based on the assumption that the horizontal movement of irregularities does not change while crossing the F-region cross-over points of these stations. The calculated velocities of irregularities indicate an eastward drift decreasing from about 180 m s<sup>–1</sup> to 55 m s<sup>–1</sup> during the course of night. In the premidnight period, the drifts are reduced under the magnetically disturbed conditions. The average east-west extension of irregularites is found to be in the range of 200–500 km.
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spelling doaj.art-0404a96691e14a7c942c4aee755675642022-12-21T23:38:18ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05761995-07-011372472910.1007/s00585-995-0724-5Zonal drifts of ionospheric irregularities at temperate latitude in the Indian regionS. KumarA. K. GwalB. M. PathanD. R. K. RaoThe systematic time differences observed in the onset of postsunset VHF scintillations recorded simultaneously at Ujjain (Geogr. lat. 23.2<sup>°</sup>N, Geogr. long. 75.6<sup>°</sup>E) and Bhopal (Geogr. lat. 23.2<sup>°</sup>N, Geogr. long. 77.6<sup>°</sup>E), situated at the peak of the anomaly crest in the Indian region, have been analysed to determine the zonal drifts of scintillation-producing irregularities. The method is based on the assumption that the horizontal movement of irregularities does not change while crossing the F-region cross-over points of these stations. The calculated velocities of irregularities indicate an eastward drift decreasing from about 180 m s<sup>–1</sup> to 55 m s<sup>–1</sup> during the course of night. In the premidnight period, the drifts are reduced under the magnetically disturbed conditions. The average east-west extension of irregularites is found to be in the range of 200–500 km.https://www.ann-geophys.net/13/724/1995/angeo-13-724-1995.pdf
spellingShingle S. Kumar
A. K. Gwal
B. M. Pathan
D. R. K. Rao
Zonal drifts of ionospheric irregularities at temperate latitude in the Indian region
Annales Geophysicae
title Zonal drifts of ionospheric irregularities at temperate latitude in the Indian region
title_full Zonal drifts of ionospheric irregularities at temperate latitude in the Indian region
title_fullStr Zonal drifts of ionospheric irregularities at temperate latitude in the Indian region
title_full_unstemmed Zonal drifts of ionospheric irregularities at temperate latitude in the Indian region
title_short Zonal drifts of ionospheric irregularities at temperate latitude in the Indian region
title_sort zonal drifts of ionospheric irregularities at temperate latitude in the indian region
url https://www.ann-geophys.net/13/724/1995/angeo-13-724-1995.pdf
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