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http://hdl.handle.net/2289/2676
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DC Field | Value | Language |
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dc.contributor.author | Subrahmanya, C.R. | - |
dc.contributor.author | Ganesan, R. | - |
dc.contributor.author | Sarma, N.V.G. | - |
dc.contributor.author | Rangarajan, S. | - |
dc.contributor.author | Sukumar, S. | - |
dc.date.accessioned | 2007-06-11T06:47:20Z | - |
dc.date.available | 2007-06-11T06:47:20Z | - |
dc.date.issued | 2001 | - |
dc.identifier.citation | Proceedings ICTF, NPL, New Delhi, Feb 6-7, 2001, p133 | en |
dc.identifier.uri | http://hdl.handle.net/2289/2676 | - |
dc.description | Restricted Access. | en |
dc.description.abstract | This paper describes initial results from an on-going collaboration between Raman Research Institute and the Indian Space Research Organization on various aspects of astrometry of celestial radio sources and the geosynchronous satellite. As a first step, a prototype system has been developed for disseminating a high stability frequency reference from a pair of coherently generated tones broadcast through a geosynchronous satellite. This paper describes the system and presents some initial results related both to frequency dissemination and accurate measurements of range rate of INSAT 2A. | en |
dc.format.extent | 204681 bytes | - |
dc.format.mimetype | application/pdf | - |
dc.language.iso | en | en |
dc.publisher | NPL | en |
dc.rights | 2001 NPL | en |
dc.title | High stability frequency broadcast through INSAT | en |
dc.type | Article | en |
Appears in Collections: | Research Papers (A&A) |
Files in This Item:
File | Description | Size | Format | |
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2001. ICTF Proc. p133.pdf Restricted Access | Restricted Access | 199.88 kB | Adobe PDF | View/Open Request a copy |
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