Astronomy and Astrophysics – Astronomy
Scientific paper
Nov 1976
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976itmtt..24..859g&link_type=abstract
IEEE Transactions on Microwave Theory and Techniques, vol. MTT-24, Nov. 1976, p. 859-861.
Astronomy and Astrophysics
Astronomy
4
Frequency Converters, Microwave Oscillators, Microwave Radiometers, Mixing Circuits, Harmonic Oscillators, Noise Temperature, Radio Astronomy, Schottky Diodes, Waveguides
Scientific paper
A radiometer system for use in the 1.3 mm region has been constructed and used for radio astronomical observations. A second-harmonic mixer employing a single Schottky diode downconverts the incident power to an IF frequency of about 1400 MHz. The measured double-sideband system noise temperature is 6000 K (noise figure = 13 dB) and the double-sideband mixer conversion loss is calculated to be 10 dB. The mixer is tunable over a range of at least 15 GHz.
Goldsmith Paul F.
Plambeck Richard L.
No associations
LandOfFree
A 230-GHz radiometer system employing a second-harmonic mixer 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 A 230-GHz radiometer system employing a second-harmonic mixer, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A 230-GHz radiometer system employing a second-harmonic mixer will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1726092