Paper Info
Title
SI-traceable top-of-the-atmosphere lunar irradiance: potential tie-points to the output of the ROLO model.
Abstract
The United States Geological Survey (USGS) has developed an empirical model, known as the Robotic Lunar Observatory (ROLO) Model, that predicts the reflectance of the Moon for any Sun-sensor-Moon configuration over the spectral range from 350 nm to 2500 nm. The lunar irradiance can be predicted from the modeled lunar reflectance using a spectrum of the incident solar irradiance. While extremely successful as a relative exo-atmospheric calibration target, the ROLO Model is not SI-traceable and has estimated uncertainties too large for the Moon to be used as an absolute celestial calibration target. In this work, two recent absolute, low uncertainty, SI-traceable top-of-the-atmosphere (TOA) lunar irradiances, measured over the spectral range from 380 nm to 1040 nm, at lunar phase angles of 6.6 degrees and 16.9 degrees, are used as tie-points to the output of the ROLO Model. Combined with empirically derived phase and libration corrections to the output of the ROLO Model and uncertainty estimates in those corrections, the measurements enable development of a corrected TOA lunar irradiance model and its uncertainty budget for phase angles between +/- 80 degrees and libration angles from 7 degrees to 51 degrees. The uncertainties in the empirically corrected output from the ROLO model are approximately 1 % from 440 nm to 865 nm and increase to almost 3 % at 412 nm. The dominant components in the uncertainty budget are the uncertainty in the absolute TOA lunar irradiance and the uncertainty in the fit to the phase correction from the output of the ROLO model.
Year
DOI
Venue
2017
10.1117/12.2274064
Proceedings of SPIE
Keywords
DocType
Volume
calibration,lunar model,moon
Conference
10402
ISSN
Citations 
PageRank 
0277-786X
0
0.34
References 
Authors
0
3
Name
Order
Citations
PageRank
Brown, S.W.127542.65
robert e eplee222.73
Xiaoxiong Xiong3427123.62