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| Content Provider | IEEE Xplore Digital Library |
|---|---|
| Author | Jamnejad, V. Rahmat-Samii, Y. |
| Copyright Year | 1991 |
| Description | Author affiliation: Jet Propulsion Lab., California Inst. of Technol., Pasadena, CA, USA (Jamnejad, V.) |
| Abstract | The Cassini mission requires that the reflector antenna be able to operate at four different frequencies. This means that in addition to the direct-fed S-band and Cassegrain-fed X-band operations, direct-fed Ku-band and Cassegrain-fed Ka-band operations are added on the Cassini antenna. A design scenario involving relatively simple and minor modifications to the existing Voyager dual-shaped symmetric antenna configuration is discussed. It is concluded that the subreflector displacement and the concomitant required surface reshaping, based on the phase-only geometrical-optics synthesis, is a good design alternative with an overall loss of less than 0.4 dB compared to that achievable with the original-shaped reflector, but still about 0.4 dB more than a nonshaped standard paraboloid/hyperboloid Cassegrain configuration, 5 dB more than a simple hyperboloid used with the shaped reflector, and several dB more than that achieved by simply moving the original shaped subreflector to a 1-in offset position.< |
| Starting Page | 670 |
| Ending Page | 673 |
| File Size | 153029 |
| Page Count | 4 |
| File Format | |
| ISBN | 0780301447 |
| DOI | 10.1109/APS.1991.174928 |
| Language | English |
| Publisher | Institute of Electrical and Electronics Engineers, Inc. (IEEE) |
| Publisher Date | 1991-06-24 |
| Publisher Place | Canada |
| Access Restriction | Subscribed |
| Rights Holder | Institute of Electrical and Electronics Engineers, Inc. (IEEE) |
| Subject Keyword | Diffraction Frequency selective surfaces Geometrical optics Feeds Lighting Space vehicles Apertures Propulsion Laboratories Space technology |
| Content Type | Text |
| Resource Type | Article |
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