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DC Field | Value | Language |
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dc.contributor.author | Vivekanand, M. | - |
dc.contributor.author | Arora, R.S. | - |
dc.date.accessioned | 2006-01-04T11:15:08Z | - |
dc.date.available | 2006-01-04T11:15:08Z | - |
dc.date.issued | 1988-10-20 | - |
dc.identifier.citation | Current Science, 1988, Vol. 57, p1103 -1106. | en |
dc.identifier.issn | 0011-3891 | - |
dc.identifier.uri | http://hdl.handle.net/2289/1092 | - |
dc.description.abstract | In 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.extent | 246760 bytes | - |
dc.format.mimetype | application/pdf | - |
dc.language.iso | en | en |
dc.publisher | Indian Academy of Sciences, Bangalore, India. | en |
dc.rights | Indian Academy of Sciences, Bangalore, India. | en |
dc.title | Observations of atmospheric ozone above Bangalore ($13^{\circ}$ N latitude) at 110.836 GHz. | en |
dc.type | Article | en |
Appears in Collections: | Research Papers (A&A) |
Files in This Item:
File | Description | Size | Format | |
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1988 CS V57 p1103.pdf | 4p. | 240.98 kB | Adobe PDF | View/Open |
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