Improvements on a cryogenically cooled mixer for 80-120 GHz

Details Improvements on a cryogenically cooled mixer for 80-120 GHz Improvements on a cryogenically cooled mixer for 80-120 GHz

Feb 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979ell....15..115h&link_type=abstract

Electronics Letters, vol. 15, Feb. 15, 1979, p. 115, 116.

Astronomy and Astrophysics

Astronomy

Cryogenic Equipment, Microwave Equipment, Mixing Circuits, Radio Astronomy, Liquid Cooling, Noise Temperature, Radio Telescopes, Tuning

Scientific paper

A previously developed low-noise mixer for radio astronomy has been significantly improved, resulting in greater bandwidth and higher reliability. After modification a single-sideband conversion loss and mixer temperature of 6.1 dB and 635 K, respectively, have been achieved for a local-oscillator frequency of 111.4 GHz and 5.3 dB and 525 K, respectively, for a frequency of 84 GHz.

Affiliated with

Also associated with

No associations

Rating

Improvements on a cryogenically cooled mixer for 80-120 GHz does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Improvements on a cryogenically cooled mixer for 80-120 GHz, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Improvements on a cryogenically cooled mixer for 80-120 GHz will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-829568