Specifying polarimetric tolerances of a high-resolution imaging multiple-species atmospheric profiler (HiMAP)
Author
Richter, Juliana MaeChipman, Russell
Daugherty, Brian
Diner, David J.
Eldering, Annmarie
Hyon, Jason J.
Kupinski, Meredith
Neu, Jessica L.
Fu, Dejian
Affiliation
Univ Arizona, Opt SciIssue Date
2019-05-22
Metadata
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SPIE-INT SOC OPTICAL ENGINEERINGCitation
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/10.1117/12.2510750Rights
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
0277-786XVersion
Final published versionSponsors
NASA ROSES-2013 Atmospheric Composition: Aura Science Team program [NNN13D455T]; Jet Propulsion Laboratory (JPL); JPL Strategic Initiatives R TD programsae974a485f413a2113503eed53cd6c53
10.1117/12.2510750