Paper
28 July 2014 A multi-pixel room-temperature local oscillator subsystem for array receivers at 1.9 THz
Jose V. Siles, Imran Mehdi, Choonsup Lee, Robert Lin, Jon Kawamura, Erich Schlecht, Peter Bruneau, Paul F. Goldsmith
Author Affiliations +
Abstract
We report on the first room-temperature modular multi-pixel Schottky diode-based, tunable, frequency-multiplied local oscillator sub-system at 1.9 THz. This source has been developed to enable efficient high-resolution mapping of the C+ line using suborbital platforms such as the SOFIA aircraft and balloons, as well as space instruments. This compact LO source features four multipliers (X3X2X3X3) to up-convert Ka-band power to 1.9 THz. Preliminary results at 300 K demonstrate more than 5 μW per pixel at 1.9 THz. The source is designed to provide a large output power dynamic range and can be expanded to larger array receivers.
© (2014) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Jose V. Siles, Imran Mehdi, Choonsup Lee, Robert Lin, Jon Kawamura, Erich Schlecht, Peter Bruneau, and Paul F. Goldsmith "A multi-pixel room-temperature local oscillator subsystem for array receivers at 1.9 THz", Proc. SPIE 9147, Ground-based and Airborne Instrumentation for Astronomy V, 914777 (28 July 2014); https://doi.org/10.1117/12.2055011
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Cited by 3 scholarly publications.
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KEYWORDS
Terahertz radiation

Oscillators

Receivers

Amplifiers

Ka band

Waveguides

Computer aided design

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