Infrared spectroscopy of Jovian aurorae

dc.contributor.author	George, K
dc.contributor.author	Chandrasekhar, T
dc.date.accessioned	2006-03-14T11:00:27Z
dc.date.available	2006-03-14T11:00:27Z
dc.date.issued	2005-06
dc.identifier.citation	BASI, Vol. 33, No. 2, pp. 233-236	en
dc.identifier.uri	http://hdl.handle.net/2248/776
dc.description.abstract	We 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 presented	en
dc.format.extent	129572 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.subject	Jovian Aurorae	en
dc.subject	Infrared spectroscopy	en
dc.subject	K band	en
dc.title	Infrared spectroscopy of Jovian aurorae	en
dc.type	Article	en