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    Specifying polarimetric tolerances of a high-resolution imaging multiple-species atmospheric profiler (HiMAP)

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    Author
    Richter, Juliana Mae
    Chipman, Russell
    Daugherty, Brian
    Diner, David J.
    Eldering, Annmarie
    Hyon, Jason J.
    Kupinski, Meredith
    Neu, Jessica L.
    Fu, Dejian
    Affiliation
    Univ Arizona, Opt Sci
    Issue Date
    2019-05-22
    Keywords
    polarization
    remote sensing
    spectroscopy
    tolerance analysis
    
    Metadata
    Show full item record
    Publisher
    SPIE-INT SOC OPTICAL ENGINEERING
    Citation
    Juliana Mae Richter, Russell Chipman, Brian Daugherty, David J. Diner, Annmarie Eldering, Jason J. Hyon, Meredith Kupinski, Jessica L. Neu, and Dejian Fu "Specifying polarimetric tolerances of a high-resolution imaging multiple-species atmospheric profiler (HiMAP)", Proc. SPIE 10925, Photonic Instrumentation Engineering VI, 109250F (22 May 2019); https://doi.org/10.1117/12.2510750
    Journal
    PHOTONIC INSTRUMENTATION ENGINEERING VI
    Rights
    Copyright © 2019 SPIE.
    Collection Information
    This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.
    Abstract
    The High-resolution Imaging Multiple-species Atmospheric Profiler (HiMAP) is an ultraviolet imaging spectro-polarimeter in development at the Jet Propulsion Laboratory for measuring O-3 and NO2 concentrations in the troposphere from an airborne platform or satellite. In this paper: (1) the HiMAP design is illustrated and modeled using 3D polarization ray tracing calculus, (2) the dependency between the condition number of the systems polarization measurement matrix and properties of individual optical components is used as a method for tolerancing, and (3) the polarimeter capabilities of manufacturable thin film designs of polarizing and non-polarizing beam splitters is explored using numerical methods. The condition number of an optical system is calculated from a polarization ray tracing (PRT) matrix model of the polarimeter. Deviations of the condition number are calculated for non-ideal polarization elements and coatings to understand component and alignment tolerances.
    ISSN
    0277-786X
    DOI
    10.1117/12.2510750
    Version
    Final published version
    Sponsors
    NASA ROSES-2013 Atmospheric Composition: Aura Science Team program [NNN13D455T]; Jet Propulsion Laboratory (JPL); JPL Strategic Initiatives R TD programs
    ae974a485f413a2113503eed53cd6c53
    10.1117/12.2510750
    Scopus Count
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    UA Faculty Publications

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