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A solid-state frequency source for radio astronomy in the 100 to 1000 GHz range |
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| Authors: | H. Rothermel T. G. Phillips Jocelyn Keene |
| Affiliation: | (1) George W. Downs Laboratory of Physics, California Institute of Technology, 91125 Pasadena, CA;(2) Present address: Max-Planck-Institut f. Physik und Astrophysik, Institut für extraterrestrische Physik, 8046 Garching, FRG |
| Abstract: | A compact Gunn oscillator-multiplier combination can provide the for SIS receivers necessary LO power up to 1000 GHz. Frequency multiplication factors of 2 to 8 are accomplished in a single step using a Schottky mixer diode in the varistor mode. |
| Keywords: | Radio Astronomy Receiver Submillimeter Techniques Local Oscillator Gunn Oscillator Frequency Multiplier Schottky Diode |
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