Post midnight spread-F occurrence over Waltair (17.7° N, 83.3° E) during low and ascending phases of solar activity

A study carried out on the occurrence of post midnight spread-F events at a low-latitude station, Waltair (17.7° N, 83.3° E), India revealed that its occurrence is maximum in the summer solstice months of the low solar activity period and decreases with an increase in the sunspot activity. T...

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Main Authors: K. Niranjan, P. S. Brahmanandam, P. Ramakrishna Rao, G. Uma, D. S. V. V. D. Prasad, P. V. S. Rama Rao
Format: Article
Language:English
Published: Copernicus Publications 2003-03-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/21/745/2003/angeo-21-745-2003.pdf
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spelling doaj-bb3f06d96b164515b6d79e72b323e13e2020-11-24T23:05:08ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05762003-03-012174575010.5194/angeo-21-745-2003Post midnight spread-F occurrence over Waltair (17.7° N, 83.3° E) during low and ascending phases of solar activityK. Niranjan0P. S. Brahmanandam1P. Ramakrishna Rao2G. Uma3D. S. V. V. D. Prasad4P. V. S. Rama Rao5Department of Physics, Andhra University, Visakhapatnam 530 003, IndiaDepartment of Physics, Andhra University, Visakhapatnam 530 003, IndiaDepartment of Physics, Andhra University, Visakhapatnam 530 003, IndiaDepartment of Physics, Andhra University, Visakhapatnam 530 003, IndiaDepartment of Physics, Andhra University, Visakhapatnam 530 003, IndiaDepartment of Physics, Andhra University, Visakhapatnam 530 003, IndiaA study carried out on the occurrence of post midnight spread-F events at a low-latitude station, Waltair (17.7° N, 83.3° E), India revealed that its occurrence is maximum in the summer solstice months of the low solar activity period and decreases with an increase in the sunspot activity. The F-region virtual height variations show that 80% of these spread-F cases are associated with an increase in the F-region altitude. It is suggested with the support of the night airglow 6300 A zenith intensity data obtained with co-located ground-based night airglow photometer and electron temperature data from the Indian SROSS C2 satellite that the seasonal variation of the occurrence and probable onset times of the post midnight spread-F depend on the characteristics of the highly variable semipermanent equatorial Midnight Temperature Maximum (MTM).<br><br><b>Key words. </b>Ionosphere (ionospheric irregularities; ionosphere atmosphere interactions) Atmospheric composition and structure (airglow and Aurora)https://www.ann-geophys.net/21/745/2003/angeo-21-745-2003.pdf
collection DOAJ
language English
format Article
sources DOAJ
author K. Niranjan
P. S. Brahmanandam
P. Ramakrishna Rao
G. Uma
D. S. V. V. D. Prasad
P. V. S. Rama Rao
spellingShingle K. Niranjan
P. S. Brahmanandam
P. Ramakrishna Rao
G. Uma
D. S. V. V. D. Prasad
P. V. S. Rama Rao
Post midnight spread-F occurrence over Waltair (17.7° N, 83.3° E) during low and ascending phases of solar activity
Annales Geophysicae
author_facet K. Niranjan
P. S. Brahmanandam
P. Ramakrishna Rao
G. Uma
D. S. V. V. D. Prasad
P. V. S. Rama Rao
author_sort K. Niranjan
title Post midnight spread-F occurrence over Waltair (17.7° N, 83.3° E) during low and ascending phases of solar activity
title_short Post midnight spread-F occurrence over Waltair (17.7° N, 83.3° E) during low and ascending phases of solar activity
title_full Post midnight spread-F occurrence over Waltair (17.7° N, 83.3° E) during low and ascending phases of solar activity
title_fullStr Post midnight spread-F occurrence over Waltair (17.7° N, 83.3° E) during low and ascending phases of solar activity
title_full_unstemmed Post midnight spread-F occurrence over Waltair (17.7° N, 83.3° E) during low and ascending phases of solar activity
title_sort post midnight spread-f occurrence over waltair (17.7° n, 83.3° e) during low and ascending phases of solar activity
publisher Copernicus Publications
series Annales Geophysicae
issn 0992-7689
1432-0576
publishDate 2003-03-01
description A study carried out on the occurrence of post midnight spread-F events at a low-latitude station, Waltair (17.7° N, 83.3° E), India revealed that its occurrence is maximum in the summer solstice months of the low solar activity period and decreases with an increase in the sunspot activity. The F-region virtual height variations show that 80% of these spread-F cases are associated with an increase in the F-region altitude. It is suggested with the support of the night airglow 6300 A zenith intensity data obtained with co-located ground-based night airglow photometer and electron temperature data from the Indian SROSS C2 satellite that the seasonal variation of the occurrence and probable onset times of the post midnight spread-F depend on the characteristics of the highly variable semipermanent equatorial Midnight Temperature Maximum (MTM).<br><br><b>Key words. </b>Ionosphere (ionospheric irregularities; ionosphere atmosphere interactions) Atmospheric composition and structure (airglow and Aurora)
url https://www.ann-geophys.net/21/745/2003/angeo-21-745-2003.pdf
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