EGU24-4978, updated on 08 Mar 2024
https://doi.org/10.5194/egusphere-egu24-4978
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

Three-dimensional MHD simulation of lunar induced magnetic field generated by lunar metallic core

Siqi Yi1, Xiaojun Xu1, Lianghai Xie2, Xing Wang1, Qi Xu2, Zilu Zhou1, Hengyan Man1, Lei Luo1, Peishan He1, and Pu Yang1
Siqi Yi et al.
  • 1Macau University of Science and Technology, State Key Laboratory of Lunar and Planetary Sciences, Macau, China (962399411@qq.com)
  • 2Center for Space Science and Applied Research, Chinese Academy of Sciences, Beijing 100190, China

Comprehending the internal structure of the Moon is crucial for uncovering its formation and evolution. The existence of the lunar core can be proved by several pieces of evidence, including electromagnetic sounding analyses, mass and moment of inertia analyses, and seismic analyses. However, the precise size and composition of the lunar core are still unknown. In this study, the induced magnetic field generated by the lunar metallic core is illustrated through a three-dimensional MHD simulation. Several cases have been discussed in which the lunar core are set with different electrical conductivities and thicknesses. Compared to the hybrid model, our MHD model can calculate more accurate results with a more refined grid. Our simulation can capture the variations of parameters (plasma densities, temperature, and flow speed) in original and final conditions, while the hybrid model cannot.

How to cite: Yi, S., Xu, X., Xie, L., Wang, X., Xu, Q., Zhou, Z., Man, H., Luo, L., He, P., and Yang, P.: Three-dimensional MHD simulation of lunar induced magnetic field generated by lunar metallic core, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-4978, https://doi.org/10.5194/egusphere-egu24-4978, 2024.