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CLARREO Pathfinder: Mission Status and Current StatusThe Climate Absolute Radiance and Refractivity Observatory (CLARREO) Pathfinder (CPF) mission consists of a high accuracy reflected solar spectrometer that will take measurements from the International Space Station for one year starting in 2023. CPF will demonstrate that its novel on-orbit absolute calibration approaches are capable of achieving 0.3% (1-sigma) radiometric uncertainty. Additionally, using its two-axis pointing gimbal which enables nearly-concurrent measurements matching look angles with other orbiting sensors, CPF will demonstrate a novel inter-calibration approach by inter-calibrating CERES and VIIRS. CPF is currently in its Final Design and Fabrication Stage and recently passed its Critical Design Review.
Document ID
20205004366
Acquisition Source
Langley Research Center
Document Type
Presentation
Authors
Yolanda Shea
(Langley Research Center Hampton, Virginia, United States)
Gary Fleming
(Langley Research Center Hampton, Virginia, United States)
Greg Kopp
(Laboratory for Atmospheric and Space Physics Boulder, Colorado, United States)
Constantine Lukashin
(Langley Research Center Hampton, Virginia, United States)
Peter Pilewskie
(Laboratory for Atmospheric and Space Physics Boulder, Colorado, United States)
Paul Smith
(Laboratory for Atmospheric and Space Physics Boulder, Colorado, United States)
Kurt Thome
(Goddard Space Flight Center Greenbelt, Maryland, United States)
Bruce Wielicki
(Langley Research Center Hampton, Virginia, United States)
Xu Liu
(Langley Research Center Hampton, Virginia, United States)
Wan Wu
(Science Systems and Applications (United States) Lanham, Maryland, United States)
Date Acquired
July 10, 2020
Subject Category
Meteorology And Climatology
Meeting Information
Meeting: 2020 IEEE International Geoscience and Remote Sensing Symposium
Location: Virtual
Country: US
Start Date: September 26, 2020
End Date: October 2, 2020
Sponsors: Institute of Electrical and Electronics Engineers
Funding Number(s)
WBS: 564940
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
Technical Review
NASA Peer Committee
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