TY - JOUR
T1 - A 650 GHz unilateral finline SIS mixer fed by a multiple flare-angle smooth-walled horn
AU - Tan, Boon Kok
AU - Yassin, Ghassan
AU - Grimes, Paul
AU - Leech, Jamie
AU - Jacobs, Karl
AU - Groppi, Christopher
N1 - Funding Information:
Manuscript received August 04, 2011; revised November 21, 2011; accepted November 21, 2011. Date of publication December 13, 2011; date of current version January 18, 2012. This work was supported in part by AMSTAR+ of RadioNet and an STFC follow-on-fund grant. The work of B.-K. Tan was supported in part by the Royal Family of Malaysia under the King’s Scholarship. B.-K. Tan, G. Yassin, and J. Leech are with the Department of Physics (Astrophysics), University of Oxford, OX1 3RH, Oxford, U.K. (e-mail: tanbk@astro.ox.ac.uk). P. Grimes is with the Harvard-Smithsonian Center For Astrophysics, Cambridge, MA 02138 USA. K. Jacobs is with KOSMA, I. Physikalisches Institut, University of Cologne, 50937 Cologne, Germany. C. Groppi is with ASU School of Earth and Space Exploration, Tempe, AZ 85287-1404 USA. Color versions of one or more of the figures in this paper are available online at http://ieeexplore.ieee.org. Digital Object Identifier 10.1109/TTHZ.2011.2177736
PY - 2012/1
Y1 - 2012/1
N2 - We report the design and successful operation of an superconductor- insulator-superconductor (SIS) mixer operating near the superconducting gap of niobium. A key feature of this design is the employment of a unilateral finline taper to transform the waveguide modes to microstrip signals. This transition is easy to design since it can be rigorously modeled, and also easy to fabricate being a single-layer structure. We will show that unilateral finline mixers have important advantages at THz frequencies since they exhibit wideband operation at both radio frequency (RF) and intermediate frequency (IF), allow elegant on-chip integration of the mixer circuits and result in an extremely simple mixer block that does not require a backshort or any mechanical tuners. The mixer we describe below is fed by a multiple flare-angle smooth-walled horn which exhibits beam pattern characteristic comparable to the conventional corrugated horn and yet is much easier to fabricate. In this paper, we shall present a brief discussion of the testing of the multiple flare-angle horn and detailed description of the design and testing of the mixer, covering ∼100 GHz bandwidth centered at 650 GHz. In particular, we will present full electromagnetic design description of the mixer chip including the superconducting effects, and the heterodyne properties of the mixer using quantum mixing theory. Mixer performance tests that we carried out from 595 to 702 GHz gave a best receiver noise temperature of 145 K at 600 GHz, corrected for a 75 μm beam splitter. Finally, we performed a thorough analysis of the mixer performance, comparing the experimental results with theoretical models. Our investigation demonstrated that unilateral finline mixers fed by a multiple flare-angle horn can yield performance comparable to conventional designs, hence are suitable for large format mixer array at THz frequencies.
AB - We report the design and successful operation of an superconductor- insulator-superconductor (SIS) mixer operating near the superconducting gap of niobium. A key feature of this design is the employment of a unilateral finline taper to transform the waveguide modes to microstrip signals. This transition is easy to design since it can be rigorously modeled, and also easy to fabricate being a single-layer structure. We will show that unilateral finline mixers have important advantages at THz frequencies since they exhibit wideband operation at both radio frequency (RF) and intermediate frequency (IF), allow elegant on-chip integration of the mixer circuits and result in an extremely simple mixer block that does not require a backshort or any mechanical tuners. The mixer we describe below is fed by a multiple flare-angle smooth-walled horn which exhibits beam pattern characteristic comparable to the conventional corrugated horn and yet is much easier to fabricate. In this paper, we shall present a brief discussion of the testing of the multiple flare-angle horn and detailed description of the design and testing of the mixer, covering ∼100 GHz bandwidth centered at 650 GHz. In particular, we will present full electromagnetic design description of the mixer chip including the superconducting effects, and the heterodyne properties of the mixer using quantum mixing theory. Mixer performance tests that we carried out from 595 to 702 GHz gave a best receiver noise temperature of 145 K at 600 GHz, corrected for a 75 μm beam splitter. Finally, we performed a thorough analysis of the mixer performance, comparing the experimental results with theoretical models. Our investigation demonstrated that unilateral finline mixers fed by a multiple flare-angle horn can yield performance comparable to conventional designs, hence are suitable for large format mixer array at THz frequencies.
KW - Horn antenna
KW - submillimeter receivers
KW - superconducting detectors
KW - superconductor-insulator-superconductor (SIS) mixers
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U2 - 10.1109/TTHZ.2011.2177736
DO - 10.1109/TTHZ.2011.2177736
M3 - Article
AN - SCOPUS:84856376805
SN - 2156-342X
VL - 2
SP - 40
EP - 49
JO - IEEE Transactions on Terahertz Science and Technology
JF - IEEE Transactions on Terahertz Science and Technology
IS - 1
M1 - 6104210
ER -