A quasi-optical transmission line (QOTL) has been developed as a low-loss transmission line for a spaceborne cloud-observing radar instrument that operates at a nominal frequency of 94 GHz. This QOTL could also readily be redesigned for use in terrestrial millimeter- wave radar systems and millimeter-wave imaging systems.

In the absence of this or another low-loss transmission line, it would be necessary to use a waveguide transmission line in the original radar application. Unfortunately, transmission losses increase and power-handling capacities of waveguides generally decrease with frequency, such that at 94 GHz, the limitation on transmitting power and the combined transmission and reception losses (> 5 dB) in a waveguide transmission line previously considered for the original application would be unacceptable.

The QOTL functions as a very-low-loss, three-port circulator. The QOTL includes a shaped input mirror that can be rotated to accept 94-GHz transmitter power from either of two high-power amplifiers. Inside the QOTL, the transmitter power takes the form of a linearly polarized beam radiated from a feed horn. This beam propagates through a system of mirrors, each of which refocuses the beam to minimize diffraction losses. A magnetically biased ferrite disc is placed at one of the foci to utilize the Faraday effect to rotate the polarization of the beam by 45°. The beam is then transmitted via an antenna system.

The radar return (scatter from clouds, and/or reflections from other objects) is collected by the same antenna and propagates through the Faraday rotator in the reverse of the direction of propagation of the transmitted beam. In the Faraday rotator, the polarization of the received signal is rotated a further 45°, so that upon emerging from the Faraday rotator, the received beam is polarized at 90° with respect to the transmitted beam. The transmitted and received signals are then separated by a wire-grid polarizer.

This work was done by Raul M. Perez and Watt Veruttipong of Caltech for NASA's Jet Propulsion Laboratory. For more information, contact This email address is being protected from spambots. You need JavaScript enabled to view it.. NPO-44236


NASA Tech Briefs Magazine

This article first appeared in the November, 2008 issue of NASA Tech Briefs Magazine.

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