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ARCSTONE: Calibration of Lunar Spectral Reflectance from SpaceDetecting and improving the scientific understanding of global trends in complex Earth systems, such as climate, increasingly depends on assimilating datasets from multiple instruments and platforms over decadal timescales. Calibration accuracy, stability, and inter-consistency among different instruments are key to developing reliable composite data records from sensors in low Earth and geostationary orbits, but achieving sufficiently low uncertainties for these performance metrics poses a significant challenge. Space-borne instruments commonly carry on-board references for calibration at various wavelengths, but these increase mass and mission complexity, and are subject to degradation in the space environment.

The Moon can be considered a natural solar diffuser which can be observed as a calibration target by most spaceborne Earth-observing instruments. Since the lunar surface reflectance is effectively time-invariant, establishing the Moon as a high-accuracy calibration reference enables broad inter-calibration opportunities even between temporally non-overlapping instruments and provides an exo-atmospheric absolute radiometric standard. The ARCSTONE mission goal is to establish the Moon as a reliable reference for high-accuracy on-orbit calibration in the visible and near-infrared spectral region. The ARCSTONE instrument is a compact spectrometer, which will be packaged on a CubeSat intended for low Earth orbit. It will measure the lunar spectral reflectance with accuracy < 0.5% (k=1), sufficient to establish an SI-traceable absolute lunar calibration standard when referenced to the spectral solar irradiance across the 350 to 2300 nm spectral range. This lunar reference will help to enable high-accuracy absolute calibration and inter-calibration of past, current, and future Earth-observing sensors, meteorological imagers, and long-term climate monitoring satellite systems. The ARCSTONE team will present the development status of a full-spectral-range (FSR) instrument, the intended approach to calibration and characterization, and the planned path toward mission implementation.
Document ID
20205007454
Acquisition Source
Langley Research Center
Document Type
Presentation
Authors
Cindy Young
(Langley Research Center Hampton, Virginia, United States)
C Lukashin
(Langley Research Center Hampton, Virginia, United States)
T Jackson
(Langley Research Center Hampton, Virginia, United States)
T Stone
(USGS, Flagstaff, AZ)
G Kopp
(Laboratory for Atmospheric and Space Physics Boulder, Colorado, United States)
R Swanson
(Resonon (United States) Bozeman, Montana, United States)
N Abraham
(Goddard Space Flight Center Greenbelt, Maryland, United States)
E Minda
(Quartus Engineering, San Diego, CA)
C Buleri
(Quartus Engineering, San Diego, CA)
J Carvo
(Blue Canyon Technologies (United States) Boulder, Colorado, United States)
M Cooney
(Langley Research Center Hampton, Virginia, United States)
H Courrier
(Resonon (United States) Bozeman, Montana, United States)
W Davis
(Langley Research Center Hampton, Virginia, United States)
A Halterman
(Quartus Engineering, San Diego, CA)
M Kehoe
(Resonon (United States) Bozeman, Montana, United States)
T Nguyen
(Langley Research Center Hampton, Virginia, United States)
N Ryan
(Langley Research Center Hampton, Virginia, United States)
P Smith
(Laboratory for Atmospheric and Space Physics Boulder, Colorado, United States)
M Stebbins
(Resonon (United States) Bozeman, Montana, United States)
Date Acquired
September 10, 2020
Subject Category
Geosciences (General)
Meeting Information
Meeting: CALCON 2020
Location: Virtual
Country: US
Start Date: September 21, 2020
End Date: September 24, 2020
Sponsors: National Institute of Standards and Technology
Funding Number(s)
WBS: 478643.02.01.53
Distribution Limits
Public
Copyright
Use by or on behalf of the US Gov. Permitted.
Technical Review
Professional Review
Keywords
Moon
Calibration
Reflectance
Spectral
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