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Snow and Water Imaging Spectrometer (SWIS): First alignment and characterization results

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dc.contributor.author Bender, Holly A.
dc.contributor.author Mouroulis, Pantazis
dc.contributor.author Haag, Justin
dc.contributor.author Smith, Christopher D.
dc.contributor.author Van Gorp, Byron E.
dc.date.accessioned 2020-03-23T19:15:19Z
dc.date.available 2020-03-23T19:15:19Z
dc.date.issued 2017-08-06
dc.identifier.citation 2017 SPIE Optics and Photonics, San Diego, California, August 6-10, 2017 en_US
dc.identifier.clearanceno CL#17-4228
dc.identifier.uri http://hdl.handle.net/2014/47752
dc.description.abstract The Snow and Water Imaging Spectrometer (SWIS) is a fast, high-uniformity, low-polarization sensitivity imaging spectrometer and telescope system designed for integration on a 6U CubeSat platform. Operating in the 350-1700 nm spectral region with 5.7 nm sampling, SWIS is capable of simultaneously addressing the demanding needs of coastal ocean science and snow and ice monitoring. New key technologies that facilitate the development of this instrument include a linear variable anti-reflection (LVAR) detector coating for stray light management, and a single drive on-board calibration mechanism utilizing a transmissive diffuser for solar calibration. We provide an overview of the SWIS instrument design and potential science applications and describe the instrument assembly and alignment, supported by laboratory measurements. en_US
dc.description.sponsorship NASA/JPL en_US
dc.language.iso en_US en_US
dc.publisher Pasadena, CA: Jet Propulsion Laboratory, National Aeronautics and Space Administration, 2017 en_US
dc.title Snow and Water Imaging Spectrometer (SWIS): First alignment and characterization results en_US
dc.type Preprint en_US


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