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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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 |
work_keys_str_mv |
AT kniranjan postmidnightspreadfoccurrenceoverwaltair177n833eduringlowandascendingphasesofsolaractivity AT psbrahmanandam postmidnightspreadfoccurrenceoverwaltair177n833eduringlowandascendingphasesofsolaractivity AT pramakrishnarao postmidnightspreadfoccurrenceoverwaltair177n833eduringlowandascendingphasesofsolaractivity AT guma postmidnightspreadfoccurrenceoverwaltair177n833eduringlowandascendingphasesofsolaractivity AT dsvvdprasad postmidnightspreadfoccurrenceoverwaltair177n833eduringlowandascendingphasesofsolaractivity AT pvsramarao postmidnightspreadfoccurrenceoverwaltair177n833eduringlowandascendingphasesofsolaractivity |
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