Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1349
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dc.contributor.authorAnanthasubramanian, P.G.-
dc.contributor.authorYamamoto, Satoshi-
dc.contributor.authorPrabhu, T.P.-
dc.date.accessioned2006-06-12T09:12:46Z-
dc.date.available2006-06-12T09:12:46Z-
dc.date.issued2001-09-
dc.identifier.citationBulletin of the Astronomical Society of India, 2001, Vol.29, p487-490en
dc.identifier.issn0304-9523-
dc.identifier.urihttp://hdl.handle.net/2289/1349-
dc.description.abstractIn this poster presentation, we describe the working principle, data acquisition method and data reduction scheme of a 220 GHz tipping radiometer. We also present the preliminary 220 GHz zenith optical depth results at Mt. Saraswati, Digpa Ratsa Ri, Hanle, Ladakh, India with some conclusions.en
dc.format.extent211040 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherThe Astronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/cgi-bin/bib_query?2001BASI...29..487Aen
dc.rights(2001) by the Astronomical Society of India. Scanned images provided by the NASA ADS Data System.en
dc.subjectOpacityen
dc.subjectPrecipitable Water Vapour (PWV)en
dc.title220 GHz tipping radiometer for monitoring atmospheric opacity at Hanleen
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

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