High Resolution Spectroscopy with Submillimeter-Wave

dc.contributor.author	Kumar, V
dc.contributor.author	Dave, H
dc.date.accessioned	2008-06-30T07:15:53Z
dc.date.available	2008-06-30T07:15:53Z
dc.date.issued	2003
dc.identifier.citation	BASI, Vol. 31, No. 3&4, pp. 475 - 477	en
dc.identifier.uri	http://hdl.handle.net/2248/2545
dc.description.abstract	In 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.extent	76702 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/2003BASI...31..475K	en
dc.subject	High-resolution spectroscopy	en
dc.subject	Heterodyne-receiver	en
dc.subject	Submillimeter region	en
dc.title	High Resolution Spectroscopy with Submillimeter-Wave	en
dc.type	Article	en