Polarization properties of reflector antennas used as radio telescopes

Author:

Ng T.,Landecker T. L.1,Cazzolato F.2,Routledge D.3,Gray A. D.1,Reid R. I.1,Veidt B. G.1

Affiliation:

1. Dominion Radio Astrophysical Observatory; Herzberg Institute of Astrophysics, Penticton, National Research Council; British Columbia; Canada

2. Département de Physique; Université Laval; Quebec, Quebec; Canada

3. Department of Electrical and Computer Engineering; University of Alberta; Edmonton, Alberta; Canada

Publisher

American Geophysical Union (AGU)

Subject

Electrical and Electronic Engineering,General Earth and Planetary Sciences,Condensed Matter Physics

Reference26 articles.

1. Comparison of three cross-polarization prediction methods for reflector antennas;Bach;IEE Proc. Part H Microwaves Opt. Antennas,1986

2. Linear polarization of the galactic background at frequencies between 408 and 1411 MHz: Reductions;Brouw;Astron. Astrophys. Suppl. Ser.,1976

3. Depolarization properties of offset reflector antennas;Chu;IEEE Trans. Antennas Propag.,1973

4. Cornwell , T. J. 2003 Full primary beam Stokes I, Q, U, V imaging EVLA Memo 62 Natl. Radio Astron. Obs. Charlottesville, Va

5. Parabolic-antenna design for microwaves;Cutler;Proc. IRE,1947

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