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TEMPEST-D Radiometer: Instrument Description and Prelaunch Calibration.

Authors :
Padmanabhan, Sharmila
Gaier, Todd C.
Tanner, Alan B.
Brown, Shannon T.
Lim, Boon H.
Reising, Steven C.
Stachnik, Robert
Bendig, Rudi
Cofield, Richard
Source :
IEEE Transactions on Geoscience & Remote Sensing. Dec2021, Vol. 59 Issue 12, p10213-10226. 14p.
Publication Year :
2021

Abstract

The Temporal Experiment for Storms and Tropical Systems Technology Demonstration (TEMPEST-D) instrument is a five-frequency millimeter-wave radiometer operating from 87 to 181 GHz. The cross-track scanning radiometer has been operating on a 6U CubeSat in low Earth orbit since September 5, 2018. The direct-detection architecture of the radiometer reduces its mass and power consumption by eliminating the need for a local oscillator and mixer, also reducing system complexity. The instrument includes a scanning reflector and ambient calibration target. The reflector rotates continuously to scan the antenna beams in the cross-track direction, first across the blackbody calibration target, then toward the Earth over the full range of incidence angles, and finally to cosmic microwave background radiation at 2.73 K. This enables precision end-to-end calibration of the millimeter-wave receivers during every 2-s scan period. The TEMPEST-D millimeter-wave radiometers are based on 35-nm indium phosphide (InP) high-electron-mobility transistor (HEMT) low-noise amplifiers. This article describes the instrument and its characterization prior to launch. [ABSTRACT FROM AUTHOR]

Details

Language :
English
ISSN :
01962892
Volume :
59
Issue :
12
Database :
Academic Search Index
Journal :
IEEE Transactions on Geoscience & Remote Sensing
Publication Type :
Academic Journal
Accession number :
153854122
Full Text :
https://doi.org/10.1109/TGRS.2020.3041455