The Identification of Impact Craters from GRAIL-Acquired Gravity Data by U-Net Architecture
The identification of impact craters on the Moon and other planetary bodies is of great significance to studying and constraining the dynamical process and evolution of the Solar System. Traditionally, this has been performed through the visual examination of images. Due to the effect of overburden,...
Main Authors: | Zhaoxi Chen, Zidan Chen |
---|---|
Format: | Article |
Language: | English |
Published: |
MDPI AG
2022-06-01
|
Series: | Remote Sensing |
Subjects: | |
Online Access: | https://www.mdpi.com/2072-4292/14/12/2783 |
Similar Items
-
What Is a Polygonal Impact Crater? A Proposed Framework Toward Quantifying Crater Shapes
by: Stuart J. Robbins, et al.
Published: (2023-07-01) -
Automatic Mapping of Small Lunar Impact Craters Using LRO‐NAC Images
by: J. H. Fairweather, et al.
Published: (2022-07-01) -
Quantitative Analysis of the Sloping Terrain on Al-Biruni’s Floor and Implications for the Cratering Process
by: Feng Liu, et al.
Published: (2024-09-01) -
Study on the Degradation Pattern of Impact Crater Populations in Yutu-2′s Rovering Area
by: Xinyu Ma, et al.
Published: (2024-06-01) -
Crater Detection Dependence on Resolution, Incidence Angle, Emission Angle, and Phase Angle
by: Stuart J. Robbins, et al.
Published: (2025-02-01)