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Using Polarized PCRTM-Solar Model to Validate EMIT Surface Reflectance L2A Product Using the vector linearized discrete ordinate radiative transfer model (VLIDORT), a multiple-scattering multi-layer scattering code, coupled with a fast principal component (PC) radiative transfer model (PCRTM), we can simulate hyperspectral radiation fields from visible to shortwave infrared (VSWIR), i.e., 250 nm to 2500 nm. Since only limited accurate line-by-line calculation using VLIDORT is needed, this coupled PCRTM-VLIDORT approach is very efficient for simulating hyperspectral VSWIR spectra. These simulations incorporate accurately defined optical properties (gas absorptions, molecular and aerosol/cloud particle scattering) and detailed surface reflectance inputs. In this study we used the current L2A products of the Earth Surface Mineral Dust Source Investigation (EMIT) imaging spectrometer as the inputs to PCRTM-VLIDORT to simulate EMIT spectra. Comparing the simulated spectra with EMIT measurements provides an efficient method to validate the current EMIT product.
Document ID
20240014854
Acquisition Source
Langley Research Center
Document Type
Poster
Authors
Xiaozhen Xiong
(Langley Research Center Hampton, Virginia, United States)
Xu Liu
(Langley Research Center Hampton, Virginia, United States)
Ming Zhao
(Adnet Systems (United States) Bethesda, Maryland, United States)
Qiguang Yang
(Adnet Systems (United States) Bethesda, Maryland, United States)
Wan Wu
(Langley Research Center Hampton, VA, USA)
Liqiao Lei
(Adnet Systems (United States) Bethesda, Maryland, United States)
Robert Spurr
(RT Solutions, Inc Cambridge, MA)
Philip G Brodrick
(Jet Propulsion Laboratory La Cañada Flintridge, United States)
David R Thompson
(Jet Propulsion Laboratory La Cañada Flintridge, United States)
Robert O Green
(Jet Propulsion Laboratory La Cañada Flintridge, United States)
Date Acquired
November 20, 2024
Subject Category
Earth Resources and Remote Sensing
Meeting Information
Meeting: AGU Annual Meeting
Location: Washington DC
Country: US
Start Date: December 9, 2024
End Date: December 13, 2024
Sponsors: American Geophysical Union, National Aeronautics and Space Administration, Utah State University Space Dynamics Laboratory
Funding Number(s)
WBS: 437949.02.01.03.48
Distribution Limits
Public
Copyright
Use by or on behalf of the US Gov. Permitted.
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