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| Content Provider | IEEE Xplore Digital Library |
|---|---|
| Author | Bird, T.S. |
| Copyright Year | 1994 |
| Description | Author affiliation: Div. of Radiophys., CSIRO, Epping, NSW, Australia (Bird, T.S.) |
| Abstract | The Parkes radio-telescope is as busy as it ever was in its more than 30-year lifetime. To improve the telescope further, a multiple beam capability is being investigated. This would have considerable impact on a proposed detailed study of the southern sky in the frequency range 1.27 to 1.47 GHz. With the present, single, prime-focus feed, this would take about 10 years to complete, but by using multiple beams, each with two orthogonal linear polarizations, the survey time would be reduced to a more manageable observing period. A combination of reflector scan-gain loss, as the feeds are displaced from the focus, and the limited number of available correlator units, restricts a practical array to about nine elements which, nevertheless, gives a substantial order of magnitude reduction in observing time. We describe here a preliminary study of the Parkes antenna performance with a cluster of nine feed horns, where each horn in the cluster is responsible for two orthogonal linear polarizations within a beam.< |
| Starting Page | 966 |
| Ending Page | 969 |
| File Size | 220714 |
| Page Count | 4 |
| File Format | |
| ISBN | 0780320093 |
| DOI | 10.1109/APS.1994.407943 |
| Language | English |
| Publisher | Institute of Electrical and Electronics Engineers, Inc. (IEEE) |
| Publisher Date | 1994-06-20 |
| Access Restriction | Subscribed |
| Rights Holder | Institute of Electrical and Electronics Engineers, Inc. (IEEE) |
| Subject Keyword | Polarization Antenna feeds Transducers Sampling methods Dielectric losses Apertures Australia Telescopes Frequency Correlators |
| Content Type | Text |
| Resource Type | Article |
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