Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/943
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dc.contributor.authorJoshi, M. N-
dc.contributor.authorSwarup, G-
dc.contributor.authorBagri, D. S-
dc.contributor.authorKher, R. K-
dc.date.accessioned2006-04-11T08:11:21Z-
dc.date.available2006-04-11T08:11:21Z-
dc.date.issued1988-
dc.identifier.citationBASI, Vol. 16, No. 2 & 3, pp. 111-121en
dc.identifier.urihttp://hdl.handle.net/2248/943-
dc.description.abstractThe 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.extent915631 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indianen
dc.subjectRadio telescopeen
dc.subjectPhased arrayen
dc.titleA new electronically steerable 1056 dipole array at 327 MHz for the Ooty radio telescopeen
dc.typeArticleen
Appears in Collections:BASI Publications

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