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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2545
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dc.contributor.authorKumar, V-
dc.contributor.authorDave, H-
dc.date.accessioned2008-06-30T07:15:53Z-
dc.date.available2008-06-30T07:15:53Z-
dc.date.issued2003-
dc.identifier.citationBASI, Vol. 31, No. 3&4, pp. 475 - 477en
dc.identifier.urihttp://hdl.handle.net/2248/2545-
dc.description.abstractIn order to explain the characteristic features of planetary atmosphere, detection and precise measurements of environmentally important gases such as CO, CIO, No becomes necessary. Since most of the polyatomic molecules have (ro-vibrational) transitions in submillimeter region 100 μ-1000μ), probing in this wavelength region is vital. The specific rotational and vibrational states are the result of interactions between different atoms in the molecule. Since each molecule has a unique arrangement of atoms, it has an exclusive submillimeter signature. We are developing a portable heterodyne receiver system at Physical Research Laboratory, Ahmedabad to perform high-resolution spectroscopy in this wavelength region.en
dc.format.extent76702 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2003BASI...31..475Ken
dc.subjectHigh-resolution spectroscopyen
dc.subjectHeterodyne-receiveren
dc.subjectSubmillimeter regionen
dc.titleHigh Resolution Spectroscopy with Submillimeter-Waveen
dc.typeArticleen
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