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http://hdl.handle.net/2248/943
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DC Field | Value | Language |
---|---|---|
dc.contributor.author | Joshi, M. N | - |
dc.contributor.author | Swarup, G | - |
dc.contributor.author | Bagri, D. S | - |
dc.contributor.author | Kher, R. K | - |
dc.date.accessioned | 2006-04-11T08:11:21Z | - |
dc.date.available | 2006-04-11T08:11:21Z | - |
dc.date.issued | 1988 | - |
dc.identifier.citation | BASI, Vol. 16, No. 2 & 3, pp. 111-121 | en |
dc.identifier.uri | http://hdl.handle.net/2248/943 | - |
dc.description.abstract | The electronically steerable 1056-element linear dipole array installed on the Ooty radio telescope in 1982 is described. The colinear dipole array consists of 22 subarrays of 48 dipole each and employs a low loss (about 0.6 dB) 4-bit PIN diode phase-shifter, after each dipole, for steering the telescope beam in declination. The phase-shifters are controlled by a computer and transistor drivers. The maximum VSWR at the input of any dipole is not above 2 over a scan range of + or - 40 deg, and the frequency range of + or - 6 MHz. | en |
dc.format.extent | 915631 bytes | - |
dc.format.mimetype | application/pdf | - |
dc.language.iso | en | en |
dc.publisher | Astronomical Society of Indian | en |
dc.subject | Radio telescope | en |
dc.subject | Phased array | en |
dc.title | A new electronically steerable 1056 dipole array at 327 MHz for the Ooty radio telescope | en |
dc.type | Article | en |
Appears in Collections: | BASI Publications |
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