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Pixel-Based Model For High Latitude Dust DetectionDust has implications on the energy budget, ocean biodiversity, and economy at regional and global scales. Dust detection relies on spectral sensitivity at visible (RGB) and infrared wavelengths. Radiative properties of high latitude dust and the background surface albedo in these regions (>40°N, >40°S) complicate current dust detection methods. Leveraging supervised machine learning (ML) methods, we propose a new method accounting for regional differences of dust occurrence.
Document ID
20190030822
Acquisition Source
Marshall Space Flight Center
Document Type
Poster
Authors
Priftis, G.
(Alabama Univ. Huntsville, AL, United States)
Freitag, B.
(Alabama Univ. Huntsville, AL, United States)
Ramasubramanian, M.
(Alabama Univ. Huntsville, AL, United States)
Gurung, I.
(Alabama Univ. Huntsville, AL, United States)
Maskey, M.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Ramachandran, R.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Date Acquired
September 16, 2019
Publication Date
September 10, 2019
Subject Category
Earth Resources And Remote Sensing
Report/Patent Number
MSFC-E-DAA-TN72807
Meeting Information
Meeting: Wernher von Braun Memorial Symposium
Location: Huntsville, AL
Country: United States
Start Date: September 10, 2019
End Date: September 12, 2019
Sponsors: American Astronautical Society (AAS-HQ)
Funding Number(s)
CONTRACT_GRANT: NNM11AA01A
Distribution Limits
Public
Copyright
Public Use Permitted.
Technical Review
Single Expert
Keywords
High latitude dust
Deep learning
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