Wide If 230-GHz Superconductor-Insulator-Superconductor Mixer

A 230 GHz Superconductor-Insulator-Superconductor (SIS) mixer is designed focusing on a good performance in the IF frequency range of 4–16 GHz over the RF band from 211 to 275 GHz. A transition from a full-height waveguide to a probe is designed using HFSS. The mixer chips containing SIS junctions are designed and optimized to have low total capacitance of circuits to ensure wide IF bandwidth. The chip fabrication was done in Academia Sinica Institute of Astronomy and Astrophysics (ASIAA), where the masks were conducted by TSMC. A lab test was conducted on a superconducting mixer with a cryogenic dewar. The gap voltage in the I-V curve of the mixer is approximately 8 mV, and there is a clear nonlinearity around a current of 110 μA, which matches well with the simulation. The receiver noise temperature is approximately 60 K including optical losses and the noise from the RF input.

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Publication Details

Published
2024-10-16
DOI
https://doi.org/10.1109/ictc62082.2024.10827305
Primary Topic
Physics of Superconductivity and Magnetism
Type
article
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article

Wide If 230-GHz Superconductor-Insulator-Superconductor Mixer

Naechul Shin, Ming-Jye Wang, Jung‐Won Lee
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Physics of Superconductivity and Magnetism
article

Wide If 230-GHz Superconductor-Insulator-Superconductor Mixer

Naechul Shin, Ming-Jye Wang, Jung‐Won Lee
article en

Abstract

A 230 GHz Superconductor-Insulator-Superconductor (SIS) mixer is designed focusing on a good performance in the IF frequency range of 4–16 GHz over the RF band from 211 to 275 GHz. A transition from a full-height waveguide to a probe is designed using HFSS. The mixer chips containing SIS junctions are designed and optimized to have low total capacitance of circuits to ensure wide IF bandwidth. The chip fabrication was done in Academia Sinica Institute of Astronomy and Astrophysics (ASIAA), where the masks were conducted by TSMC. A lab test was conducted on a superconducting mixer with a cryogenic dewar. The gap voltage in the I-V curve of the mixer is approximately 8 mV, and there is a clear nonlinearity around a current of 110 μA, which matches well with the simulation. The receiver noise temperature is approximately 60 K including optical losses and the noise from the RF input.

Institute of Astronomy and Astrophysics, Academia Sinica (TW), Electronics and Telecommunications Research Institute (KR), Korea Astronomy and Space Science Institute (KR)
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Openalex Percentile: Top 84%
Physics of Superconductivity and Magnetism
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