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Please use this identifier to cite or link to this item: http://hdl.handle.net/2014/40833

Title: Ultra stable microwave radiometers for future sea surface salinity missions
Authors: Wilson, William J.
Tanner, Alan B.
Pellerano, Fernando A.
Horgan, Kevin A.
Keywords: sea surface salinity
Aquarius
radiometers
Earth Science System Pathfinder (ESSP)
Issue Date: Apr-2005
Publisher: Pasadena, CA : Jet Propulsion Laboratory, National Aeronautics and Space Administration, 2005.
Series/Report no.: JPL Report
D-31794
Abstract: The NASA Earth Science System Pathfinder (ESSP) mission Aquarius will measure global sea surface salinity with 100-km spatial resolution every 8 days with an average monthly salinity accuracy of 0.2 psu (parts per thousand). This requires an L-band low-noise radiometer with the long-term calibration stability of < 0.1 K over 8 days. This three-year research program on ultra stable radiometers has addressed the radiometer requirements and configuration necessary to achieve this objective for Aquarius and future ocean salinity missions. The system configuration and component performance have been evaluated with radiometer testbeds at both JPL and GSFC. The research has addressed several areas including component characterization as a function of temperature, a procedure for the measurement and correction for radiometer system non-linearity, noise diode calibration versus temperature, low noise amplifier performance over voltage, and temperature control requirements to achieve the required stability. A breadboard radiometer, utilizing microstrip-based technologies, has been built to demonstrate this long-term stability. This report also presents the results of the radiometer test program, a detailed radiometer noise model, and details of the operational switching sequence optimization that can be used to achieve the low noise and stability requirements. Many of the results of this research have been incorporated into the Aquarius radiometer design and will allow this instrument to achieve its goals.
URI: http://hdl.handle.net/2014/40833
Appears in Collections:JPL TRS 1992+

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