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Pixel Based Model for High Latitude Dust DetectionHigh Latitude Dust (HLD, ≥ 50°𝑁 𝑎𝑛𝑑 ≥ 40°𝑆 ) load has implications on the energy budget, ocean biodiversity and economy on a regional and global scale. Current methods of dust detection rely on spectral sensitivity at visible (RGB) and infrared wavelengths. The characteristics of HLD vary according to the sediments and sedimentary processes operating on the land surface that are the source of the dust particles. Leveraging machine learning (ML) methods, we propose a new detection method based on convolutional neural network (CNN) using true color images.
Document ID
20190033967
Acquisition Source
Marshall Space Flight Center
Document Type
Poster
Authors
Priftis, Georgios
(Alabama Univ. Huntsville, AL, United States)
Freitag, Brian
(Alabama Univ. Huntsville, AL, United States)
Ramasubramanian, Muthukumaran
(Alabama Univ. Huntsville, AL, United States)
Gurung, Iksha
(Alabama Univ. Huntsville, AL, United States)
Gasso, Santiago
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Maskey, Manil
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Ramachandran, Rahul
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Date Acquired
December 16, 2019
Publication Date
December 9, 2019
Subject Category
Geosciences (General)
Report/Patent Number
MSFC-E-DAA-TN76101
Report Number: MSFC-E-DAA-TN76101
Meeting Information
Meeting: AGU 2019 Fall Meeting
Location: San Francisco, CA
Country: United States
Start Date: December 9, 2019
End Date: December 13, 2019
Sponsors: American Geophysical Union (AGU)
Funding Number(s)
CONTRACT_GRANT: NNM11AA01A
Distribution Limits
Public
Copyright
Public Use Permitted.
Technical Review
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