dc.contributor.author |
Mukherjee, G.K. |
|
dc.contributor.author |
Carlo, L. |
|
dc.contributor.author |
Mahajan, S.H. |
|
dc.date.accessioned |
2015-05-15T05:43:53Z |
|
dc.date.accessioned |
2021-02-12T09:54:59Z |
|
dc.date.available |
2015-05-15T05:43:53Z |
|
dc.date.available |
2021-02-12T09:54:59Z |
|
dc.date.issued |
2000 |
|
dc.identifier.citation |
Earth Planets Space, v.52, p.105-110, 2000. |
en_US |
dc.identifier.uri |
http://localhost:8080/xmlui/handle/123456789/80 |
|
dc.description.abstract |
Regular 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.iso |
en |
en_US |
dc.subject |
Magnetic disturbance |
en_US |
dc.subject |
F-layer |
en_US |
dc.subject |
Electron density |
en_US |
dc.subject |
Solar activity |
en_US |
dc.title |
630 nm nightglow observations from 17 degree N latitude |
en_US |
dc.type |
Article |
en_US |
dc.identifier.accession |
090571 |
|