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dc.contributor.authorMukherjee, G.K.
dc.contributor.authorCarlo, L.
dc.contributor.authorMahajan, S.H.
dc.date.accessioned2015-05-15T05:43:53Z
dc.date.accessioned2021-02-12T09:54:59Z-
dc.date.available2015-05-15T05:43:53Z
dc.date.available2021-02-12T09:54:59Z-
dc.date.issued2000
dc.identifier.citationEarth Planets Space, v.52, p.105-110, 2000.en_US
dc.identifier.urihttp://localhost:8080/xmlui/handle/123456789/80-
dc.description.abstractRegular measurements of [OI] 630 nm nightglow have been carried out at Kolhapur (16.8◦N, 74.2◦E, dip lat 10.6◦N) in India with the help of tilting filter photometers during clear moonless nights. Several characteristic nightglow data sets are presented in the report for geomagnetically quiet and disturbed nights. A comparison has been made between the simultaneous nightglow and the ionospheric parameters of virtual F-layer height and critical frequency of the F-layer at Ahmedabad (23.02◦N, 72.6◦E). In general, a good correlation (c.c. = 0.8 to 0.9) is found between the measured airglow emission and F-region peak electron densities during quiet periods but for intense magnetic disturbances the airglow fluctuations are mainly controlled by sharp changes in height variations of the h F layer. The period of airglow variation generally corresponds to periods of F-region height variation during magnetic disturbances. Using a long series of data between December 1989 and April 1996, the mean seasonal nocturnal variations of 630 nm emission have been compared during high and low solar activity periods.en_US
dc.language.isoenen_US
dc.subjectMagnetic disturbanceen_US
dc.subjectF-layeren_US
dc.subjectElectron densityen_US
dc.subjectSolar activityen_US
dc.title630 nm nightglow observations from 17 degree N latitudeen_US
dc.typeArticleen_US
dc.identifier.accession090571
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