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Proceedings Paper

A 2 THz Schottky solid-state heterodyne receiver for atmospheric studies
Author(s): Jeanne Treuttel; Erich Schlecht; Jose Siles; Choonsup Lee; Robert Lin; Bertrand Thomas; David Gonzalez-Olvero; Jeng-Hwa Yee; Dong Wu; Imran Mehdi
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Paper Abstract

Obtaining temperature, pressure, and composition profiles along with wind velocities in the Earth’s thermosphere/ionosphere system is a key NASA goal for understanding our planet. We report on the status of a technology development effort to build an all-solid-state heterodyne receiver at 2.06 THz that will allow the measurement of the 2.06 THz [OI] line for altitudes greater than 100 km. The receiver front end features low-parasitic Schottky diode mixer chips that are driven by a local oscillator (LO) source using Schottky diode based multipliers. The multiplier chain consists of a 38 GHz oscillator followed by a set of three cascaded triplers at 114 GHz, 343 GHz and 1.03 THz.

Paper Details

Date Published: 20 July 2016
PDF: 7 pages
Proc. SPIE 9914, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VIII, 99141O (20 July 2016); doi: 10.1117/12.2233744
Show Author Affiliations
Jeanne Treuttel, Jet Propulsion Lab. (United States)
Erich Schlecht, Jet Propulsion Lab. (United States)
Jose Siles, Jet Propulsion Lab. (United States)
Choonsup Lee, Jet Propulsion Lab. (United States)
Robert Lin, Jet Propulsion Lab. (United States)
Bertrand Thomas, Radiometer Physics GmbH (Germany)
David Gonzalez-Olvero, Jet Propulsion Lab. (United States)
Jeng-Hwa Yee, Johns Hopkins Univ. (United States)
Dong Wu, NASA Goddard Space Flight Ctr. (United States)
Imran Mehdi, Jet Propulsion Lab. (United States)


Published in SPIE Proceedings Vol. 9914:
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VIII
Wayne S. Holland; Jonas Zmuidzinas, Editor(s)

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