Published December 8, 2006
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Millimeter-wave array receivers for remote sensing
Chicago
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Abstract
Recent developments in millimeter-wave receiver have enabled new remote sensing capabilities. MMIC circuits operating at frequencies as high as 200 GHz have enabled low-cost mass producible integrated receivers suitable for array applications. We will describe several ground-based demonstrations of this technology including development of integrated spectral line receivers for atmospheric remote sensing, a synthetic thinned aperture radiometer for atmospheric sounding and imaging and polarimetric array radiometers for astrophysics applications.
Additional Information
© 2006 Society of Photo-Optical Instrumentation Engineers (SPIE). This work has been supported by in part by NASA ESTO IIP funds. Additional funding was provided by NASA Astrophysics RTOP, Exploration Systems Directorate technology program and the National Science Foundation through a Small Grants For Extraordinary Research grant. Funding for the 40 GHz polarimetric receivers has been provided by JPL Research and Technology Funds. The authors would like to thank George Komar, Amy Walton. Jonathan Hartley, Janice Buckner, Nigel Sharp, Thomas Cwik, Jason Hyon and Thomas Prince for their continued support and encouragement. Portions of this work were carried out the Jet Propulsion Laboratory a division of the California Institute of Technology under a contract with the National Aeronautics and Space Administration.Attached Files
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Additional details
- Eprint ID
- 99653
- Resolver ID
- CaltechAUTHORS:20191104-125020941
- NASA/JPL/Caltech
- NSF
- JPL Research and Technology Development Fund
- Created
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2019-11-04Created from EPrint's datestamp field
- Updated
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2021-11-16Created from EPrint's last_modified field
- Series Name
- Proceedings of SPIE
- Series Volume or Issue Number
- 6410