EGU26-3206, updated on 13 Mar 2026
https://doi.org/10.5194/egusphere-egu26-3206
EGU General Assembly 2026
© Author(s) 2026. This work is distributed under the Creative Commons Attribution 4.0 License.
Bimaterial Effect and Favorable Energy Ratio Enabled Supershear Rupture in the 2025 Mandalay Quake
1,2,3,4,7,- 1Department of Earth, Planetary and Space Sciences, University of California Los Angeles, Los Angeles, CA, USA (xuliuw1997@g.ucla.edu)
- 2Observatoire de la Cˆote d’Azur, Universit ́e Cˆote d’Azur, CNRS,IRD, G ́eoazur, Rue Albert Einstein, France.
- 3National Key Laboratory of Microwave Imaging, Aerospace Information Research Institute, Chinese Academy of Sciences, Beijing, China.
- 4School of Electronic, Electrical and Communication Engineering, University of Chinese Academy of Sciences, Beijing, China.
- 5National Engineering Research Center for Remote Sensing Satellite Applications, Aerospace Information Research Institute, Chinese Academy of Sciences, Beijing, China.
- 6School of Resources and Environment, University of Chinese Academy of Sciences, Beijing, China.
- 7State Key Laboratory for Mineral Deposits Research, School of Earth Sciences and Engineering, Nanjing University, Nanjing, China.
- 8School of Geoscience and Info-Physics, Central South University, Changsha, China
- 9Department of Earth Science, University of California, Santa Barbara, Santa Barbara, CA, USA.
How to cite: Xu, L., Meng, L., Yunjun, Z., Yang, Y., Wang, Y., Hu, C., Weng, H., Xu, W., Su, E., and Ji, C.: Bimaterial Effect and Favorable Energy Ratio Enabled Supershear Rupture in the 2025 Mandalay Quake, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3206, https://doi.org/10.5194/egusphere-egu26-3206, 2026.