Astronomy and Astrophysics – Astronomy
Scientific paper
Apr 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009stt..conf..191d&link_type=abstract
Proceedings of the 20th International Symposium on Space Terahertz Technology, held April 20-22, 2009, in Charlottesville, VA, U
Astronomy and Astrophysics
Astronomy
1
Scientific paper
We describe a simple orthomode transducer suitable for operation from centimeter to submillimeter wavelengths with appropriate scaling. It is fabricated as a split-block assembly with all waveguides in the same plane, and requires no septum or polarizing wires. The OMT operates over a 1.3:1 frequency band, narrower than a full waveguide band (typically 1.5:1). For a WR-10 version of the OMT, covering 78-102 GHz, the polarization isolation is > 37 dB and the return loss at the rectangular waveguide ports > 24 dB. The practical upper frequency for this design is probably limited by the precision of alignment that can be achieved between the block halves, which affects the polarization isolation.
Dunning Alexander
Kerr Anthony R.
Srikanth Sivasankaran
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