A 100-GHz-band heterodyne sis receiver for the trao telescope-Reference-Cited by-同舟云学术

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A 100-GHz-band heterodyne sis receiver for the trao telescope

Published:1996-01 Issue:1 Volume:17 Page:105-119
ISSN:0195-9271
Container-title:International Journal of Infrared and Millimeter Waves
language:en
Short-container-title:Int J Infrared Milli Waves

Author:

Han Seog-Tae,Lee Chang-Hoon,Kim Hyo-Ryoung,Park Dong-Chul

Publisher

Springer Science and Business Media LLC

Subject

Electrical and Electronic Engineering,Condensed Matter Physics,Instrumentation,Radiation

Link

http://link.springer.com/content/pdf/10.1007/BF02088186.pdf

Reference12 articles.

1. S. H. Pan and A. R. Kerr, “An 85–116 GHz SIS Receiver Using Inductively Shunted Edge Junctions,”IEEE Trans. Microwave Theory Tech., vol. MTT-37, No. 3, pp. 580–590, Mar. 1989.

2. C. E. Honigh and G. De Lange, “Performance of a Two Junction Array SIS-Mixer Operating Around 345 GHz,”IEEE Trans. Microwave Theory Tech., vol. 1, No. 4, pp. 616–623, Apr. 1993.

3. H. Ogawa and A. Mizuno, “A 110 GHz SIS Receiver for Radio Astronomy,”International Journal of Infrared and Millimeter Waves, vol. 11, No. 6, pp. 717–726, 1990.

4. C. K. Walker, J. W. Kooi and M. Chant, “A Low-Noise 492 GHz SIS Waveguide Receiver,”International Journal of Infrared and Millimeter Waves, vol. 13, No. 6, pp. 785–798, 1990.

5. T. S. Chu, “An Imaging Beam Waveguide Feed,”IEEE Trans. Antennas Propagat., vol. AP-31, pp. 614–619, July 1983.

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