Mesospheric temperature inversions over the Indian tropical region

To study the mesospheric temperature inversion, daily temperature profiles obtained from the Halogen Occultation Experiment (HALOE) aboard the Upper Atmospheric Research Satellite (UARS) during the period 1991-2001 over the Indian tropical region (0-30° N, 60-100° E) have been an...

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Main Authors: S. Fadnavis, G. Beig
Format: Article
Language:English
Published: Copernicus Publications 2004-11-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/22/3375/2004/angeo-22-3375-2004.pdf
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spelling doaj-a372ab9eff8d4f0d9fe62499693fa5f42020-11-24T20:55:22ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05762004-11-01223375338210.5194/angeo-22-3375-2004Mesospheric temperature inversions over the Indian tropical regionS. Fadnavis0G. Beig1Indian Institute of Tropical Meteorology, Dr. Homi Bhabha Road, 411008 Pashan Pune, IndiaIndian Institute of Tropical Meteorology, Dr. Homi Bhabha Road, 411008 Pashan Pune, IndiaTo study the mesospheric temperature inversion, daily temperature profiles obtained from the Halogen Occultation Experiment (HALOE) aboard the Upper Atmospheric Research Satellite (UARS) during the period 1991-2001 over the Indian tropical region (0-30° N, 60-100° E) have been analyzed for the altitude range 34-86km. The frequency of occurrence of inversion is found to be 67% over this period, which shows a strong semiannual cycle, with a maximum occurring one month after equinoxes (May and November). Amplitude of inversion is found to be as high as 40K. Variation of monthly mean peak and bottom heights along with amplitude of inversions also show the semiannual cycle. The inversion layer is detected most frequently in the altitude range of 70-85km, with peak height ranging from 80 to 83km and that of the bottom height from 72 to 74km. A comparison of frequency of temperature inversion with that obtained from Rayleigh lidar observations over Gadanki (13.5° N, 60-100° E) is found to be reasonable. The seasonal variation of amplitude and frequency of occurrence of temperature inversion indicates a good correlation with seasonal variation of average ozone concentration over the altitude range of the inversion layer.https://www.ann-geophys.net/22/3375/2004/angeo-22-3375-2004.pdf
collection DOAJ
language English
format Article
sources DOAJ
author S. Fadnavis
G. Beig
spellingShingle S. Fadnavis
G. Beig
Mesospheric temperature inversions over the Indian tropical region
Annales Geophysicae
author_facet S. Fadnavis
G. Beig
author_sort S. Fadnavis
title Mesospheric temperature inversions over the Indian tropical region
title_short Mesospheric temperature inversions over the Indian tropical region
title_full Mesospheric temperature inversions over the Indian tropical region
title_fullStr Mesospheric temperature inversions over the Indian tropical region
title_full_unstemmed Mesospheric temperature inversions over the Indian tropical region
title_sort mesospheric temperature inversions over the indian tropical region
publisher Copernicus Publications
series Annales Geophysicae
issn 0992-7689
1432-0576
publishDate 2004-11-01
description To study the mesospheric temperature inversion, daily temperature profiles obtained from the Halogen Occultation Experiment (HALOE) aboard the Upper Atmospheric Research Satellite (UARS) during the period 1991-2001 over the Indian tropical region (0-30° N, 60-100° E) have been analyzed for the altitude range 34-86km. The frequency of occurrence of inversion is found to be 67% over this period, which shows a strong semiannual cycle, with a maximum occurring one month after equinoxes (May and November). Amplitude of inversion is found to be as high as 40K. Variation of monthly mean peak and bottom heights along with amplitude of inversions also show the semiannual cycle. The inversion layer is detected most frequently in the altitude range of 70-85km, with peak height ranging from 80 to 83km and that of the bottom height from 72 to 74km. A comparison of frequency of temperature inversion with that obtained from Rayleigh lidar observations over Gadanki (13.5° N, 60-100° E) is found to be reasonable. The seasonal variation of amplitude and frequency of occurrence of temperature inversion indicates a good correlation with seasonal variation of average ozone concentration over the altitude range of the inversion layer.
url https://www.ann-geophys.net/22/3375/2004/angeo-22-3375-2004.pdf
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AT gbeig mesospherictemperatureinversionsovertheindiantropicalregion
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