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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/776
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dc.contributor.authorGeorge, K-
dc.contributor.authorChandrasekhar, T-
dc.date.accessioned2006-03-14T11:00:27Z-
dc.date.available2006-03-14T11:00:27Z-
dc.date.issued2005-06-
dc.identifier.citationBASI, Vol. 33, No. 2, pp. 233-236en
dc.identifier.urihttp://hdl.handle.net/2248/776-
dc.description.abstractWe report on the detection at Mt.Abu of H+ 3 molecular ion emissions in the near infrared spectra of the northern auroral zone of Jupiter. These H+3 transitions are of rotational-vibrational origin and are due to the dynamics of Jovian auroral ionosphere located mainly at high Jovian latitudes, which confirms their magnetospheric origin. The main overtone transition at 2.093 m and several other transitions including that of H2 have been detected. Details are presenteden
dc.format.extent129572 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectJovian Auroraeen
dc.subjectInfrared spectroscopyen
dc.subjectK banden
dc.titleInfrared spectroscopy of Jovian auroraeen
dc.typeArticleen
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