Quantum multitone simulations of saturation in SIS mixers
P SOC PHOTO-OPT INS 5498 (2004) 158-167
Abstract:
The Quantum Theory of Mixing developed by Tucker provides a solid framework for understanding the behaviour of SIS mixers, and subsequent developments allow the simulation of complete mixer circuits. These methods operate, however, under the assumption of small signal levels, and so neglect the non-linear behaviour of the signal path. The non-linearity of the mixer's response to applied signals is of vital importance to the calibration of SIS receiver systems. We have previously reported(1) a procedure for calculating the full quantum behaviour of tunnel junction circuits under multiple high-level signals, allowing the accurate prediction of the saturation characteristics of SIS mixers. In this paper, we apply our procedure to both an idealized SIS mixer and one of our previously tested 700 GHz finline mixers. We find that the small signal behaviour predicted by our procedure agrees well with other simulation methods, and that the saturation properties of both of these mixers differ from that predicted by previous estimates of saturation behaviour.High precision (1 part in 104) reflectivity measurement for the study of reflective materials used in solar collectors
Solar Energy Materials and Solar Cells Elsevier 80:3 (2003) 305-314
Multitone quantum simulations of saturating tunnel junction mixers
Journal of Applied Physics 93:12 (2003) 9812-9822
Abstract:
A theoretical technique was developed for simulating the quantum-mechanical multitone behavior of superconducting tunnel junction circuits. The procedure was based on a full quantum-mechanical description of photon-assisted tunneling. It was expected to be used to model saturation in submillimeter-wave SIS mixers. SIS mixers were used extensively in submillimeter-wave astronomy.Beam-combining superconducting detector for submillimetre-wave astronomical interferometry
Electronics Letters 39:7 (2003) 605-606
Abstract:
The feasibility of making single-chip, superconducting detectors for submillimetre-wave astronomical inteferometry is demonstrated. An experimental device based on back-to-back corrugated horns, and back-to-back finline transitions, was fabricated. The detector was illuminated at 350 GHz, using a coherent laboratory source, and 0.6° fringes were measured.A full-height waveguide to thin-film microstrip transition with exceptional RF bandwidth and coupling efficiency
International Journal of Infrared and Millimeter Waves 24:3 (2003) 261-284