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Wind direction azimuthal signature in the stokes emission vector from the ocean surface at microwave frequencies

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dc.contributor.authorCamps. A. J., author
dc.contributor.authorReising, S. C., author
dc.contributor.authorJohn Wiley & Sons, Inc., publisher
dc.date.accessioned2007-01-03T08:10:57Z
dc.date.available2007-01-03T08:10:57Z
dc.date.issued2001
dc.description.abstractAn ocean polarimetric emission model is presented. It is found that skewness and upwind/cross-wind rms slopes are responsible for the first and second azimuthal harmonic, respectively. Atmospheric effects contribute significantly at low wind speeds, and at horizontal polarization at certain observation angles. Simulation results compare favorably with reported JPL-WINDRAD measurements.
dc.format.mediumborn digital
dc.format.mediumarticles
dc.identifier.bibliographicCitationCamps, A. J. and S. C. Reising, Wind Direction Azimuthal Signature in the Stokes Emission Vector from the Ocean Surface at Microwave Frequencies, Microwave and Optical Technology Letters 29, no. 6 (June 20, 2001): 426-431.
dc.identifier.urihttp://hdl.handle.net/10217/68073
dc.languageEnglish
dc.language.isoeng
dc.publisherColorado State University. Libraries
dc.relation.ispartofFaculty Publications
dc.rights©2001 John Wiley & Sons, Inc.
dc.rightsCopyright and other restrictions may apply. User is responsible for compliance with all applicable laws. For information about copyright law, please see https://libguides.colostate.edu/copyright.
dc.titleWind direction azimuthal signature in the stokes emission vector from the ocean surface at microwave frequencies
dc.typeText

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