Mapping of the simultaneous movement of the equatorial ionization anomaly (EIA) and ionospheric plasma bubbles through all-sky imaging of OI630nm emission

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dc.contributor.author Mukherjee, G.K.
dc.date.accessioned 2015-06-10T11:08:25Z
dc.date.accessioned 2021-02-12T09:59:39Z
dc.date.available 2015-06-10T11:08:25Z
dc.date.available 2021-02-12T09:59:39Z
dc.date.issued 2002
dc.identifier.citation Terrestrial, Atmospheric and Oceanic Sciences, v.13/1, p.53-64, 2002. en_US
dc.identifier.uri http://localhost:8080/xmlui/handle/123456789/160
dc.description.abstract An all-sky imager with 180° field of view has been operating at Kolhapur (16.8°N, 74.2°E; dip lat 10.6°N) in India to study the ionosphere-thermosphere dynamics through the imaging of OI 630.0 nm oxygen emission line. It is observed that large number of events are characterized by the development of strong Equatorial Ionization Anomaly (EIA). Two examples of equatorward movement of the Appleton Anomaly crests (reverse ionization anomaly) with speed of 36-40 m/s on the night of January 26, 1998 and January 18, 1999 during the observation of ionospheric bubbles have been reported showing the observed correlation between EIA and bubbles. Our results agree well with fountain from Indian low latitude region. Generally, the background emission rates were low when no bubbles were observed. en_US
dc.language.iso en en_US
dc.subject Appleton anomaly en_US
dc.subject Ionospheric plasma bubbles en_US
dc.subject OI630 nm emission en_US
dc.subject Equatorial ionization anomaly en_US
dc.title Mapping of the simultaneous movement of the equatorial ionization anomaly (EIA) and ionospheric plasma bubbles through all-sky imaging of OI630nm emission en_US
dc.type Article en_US
dc.identifier.accession 090678


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