Bulletin of the American Physical Society
2024 Annual Meeting of the APS Four Corners Section
Friday–Saturday, October 11–12, 2024; Northern Arizona University, Flagstaff, Arizona
Session E06: Atmospheric Physics/Geophysics
10:30 AM–12:04 PM,
Friday, October 11, 2024
Northern Arizona University
Room: Pinyon
Chair: Richard Sonnenfeld, Langmuir Lab at New Mexico Tech
Abstract: E06.00006 : Enhancing Atmospheric Gravity Wave Studies through Advanced Cloud Classification and Segmentation in Satellite Infrared Imagery: A Contribution to the AWE Mission*
11:50 AM–12:04 PM
Presenter:
Anh Phan
(Utah State University)
Authors:
Anh Phan
(Utah State University)
Dallin Tucker
(Utah State University)
P.-Dominique Pautet
(Utah State University)
Yucheng Zhao
(Utah State University Center for Space and Atmospheric Sciences)
Ludger Scherliess
(Utah State University)
The work presented here supports the AWE mission by addressing the task of sorting AMTM images into two categories: 'Cloud' and 'No-cloud'. Accurately determining whether clouds are present in the image data is essential for ensuring the AWE temperature measurements are reliable. The AMTM’s four cameras measure specific emission lines to derive the OH (3,1) band rotational temperature, an excellent proxy for the mesospheric temperature. Clouds and background emissions can interfere with these measurements, making it important to identify and correct for cloud presence. To enhance this classification process, we have developed a machine learning model using transfer learning, achieving over 80% accuracy in categorizing satellite images into 'cloud' and 'clear'.
Building on this success, we are now advancing to image segmentation. This involves dividing each image into 45 small rectangles and identifying which rectangles contain clouds. This refined approach will significantly improve the precision of cloud detection, allowing for more accurate corrections of temperature measurements.
*The material is based upon work supported by the National Aeronautics and Space Administration under Contract Number 80GSFC18C0007. Any opinions, findings, and conclusions or recommendations expressed in this material are those of the author(s) and do not necessarily reflect the views of NASA.
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