Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1092
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dc.contributor.authorVivekanand, M.-
dc.contributor.authorArora, R.S.-
dc.date.accessioned2006-01-04T11:15:08Z-
dc.date.available2006-01-04T11:15:08Z-
dc.date.issued1988-10-20-
dc.identifier.citationCurrent Science, 1988, Vol. 57, p1103 -1106.en
dc.identifier.issn0011-3891-
dc.identifier.urihttp://hdl.handle.net/2289/1092-
dc.description.abstractIn the course of radio astronomical observations at Bangalore (13° N latitude). of emission spectra in the mm-wave region of the electromagnetic spectrum. the strong emission line at 110.836 GHz from atmospheric ozone was observed. The present paper shows how using this essentially simple ground-based technique, and a radioative transfer model. Continuous cost-effective measurements of the height-distribution of ozone can be made.en
dc.format.extent246760 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherIndian Academy of Sciences, Bangalore, India.en
dc.rightsIndian Academy of Sciences, Bangalore, India.en
dc.titleObservations of atmospheric ozone above Bangalore ($13^{\circ}$ N latitude) at 110.836 GHz.en
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

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