A 210-280 GHz SIS heterodyne receiver for the James Clerk Maxwell telescope. II - Calibration

Computer Science

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

2

Calibrating, Heterodyning, Noise Temperature, Radio Receivers, Sis (Superconductors), Volt-Ampere Characteristics, Broadband, Mixing Circuits, Radio Telescopes, Schottky Diodes, Very High Frequencies

Scientific paper

The comparison of a 240 GHz SIS heterodyne receiver with a Schottky diode receiver at the Maxwell telescope revealed difficulties with its calibration using continuum loads. The difficulties arise from the fact that the local oscillator power is not hugely greater than the total load power incident across the RF and IR band. This broadband power influences the receiver gain, principally by varying the slope of the I-V characteristic, and hence the output matching, as a result of the ac Josephson effect. Suppressing the Josephson effect with a magnetic field permits the standard calibration procedure, using hot/cold continuum loads, to be employed.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

A 210-280 GHz SIS heterodyne receiver for the James Clerk Maxwell telescope. II - Calibration 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 210-280 GHz SIS heterodyne receiver for the James Clerk Maxwell telescope. II - Calibration, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A 210-280 GHz SIS heterodyne receiver for the James Clerk Maxwell telescope. II - Calibration will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1517904

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.