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dc.contributor.authorParihar, Navin
dc.contributor.authorMukherjee, G.K.
dc.date.accessioned2015-09-10T09:24:03Z
dc.date.accessioned2021-02-12T09:28:02Z-
dc.date.available2015-09-10T09:24:03Z
dc.date.available2021-02-12T09:28:02Z-
dc.date.issued2008
dc.identifier.citationAdvances in Space Research, v.41, p.660.-669, 2008, doi: 10.1016/j.asr.2007.05.002en_US
dc.identifier.urihttp://localhost:8080/xmlui/handle/123456789/375-
dc.description.abstractThe paper reports the nightglow observations of hydroxyl (8–3), (7–2) and (6–2) Meinel band carried out at a low latitude station Kolhapur (16.8°N, 74.2°E, dip latitude 10.6°N), India during November 2002 to May 2005 with the objective of investigating mesopause dynamics based on derived OH rotational temperature. Overall, 132 nights of quality data were collected using filter-tilting photometer and an all-sky scanning photometer. The mean mesopause temperature observed at Kolhapur is 195 ± 11, 196 ± 9 and 195 ± 7 K from OH (8–3), (7–2) and (6–2) band emissions, respectively, using transition probabilities given by Langhoff et al. [Langhoff, S.R., Werner, H.J., Rosmus, P. Theoretical transition probabilities for the OH Meinel system. Journal of Molecular Spectroscopy 118, 507–529, 1986]. Small wave-like variations (periodicities ∼ few hours) existing over long period variations in derived temperatures are also present. A steady decrease of emission intensities from evening to dawn hours has been observed in approximately 59% of nights. No significant change of nightly mean temperatures has been noted. Furthermore, about 62% of observed nightly mean temperatures lie within one error bar of MSISE-90 model predictions.en_US
dc.language.isoenen_US
dc.subjectMesopauseen_US
dc.subjectTemperaturesen_US
dc.subjectNightglowen_US
dc.subjectKolhapuren_US
dc.titleMeasurement of mesopause temperature from hydroxyl nightglow at Kolhapur (16.8°N, 74.2°E), Indiaen_US
dc.typeArticleen_US
dc.identifier.accession090868
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