EGU24-20477, updated on 11 Mar 2024
https://doi.org/10.5194/egusphere-egu24-20477
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

The non-axial dipolar magnetic field of Mercury

Zhaojin Rong
Zhaojin Rong
  • Institute of Geology and Geophysics,Chinese Academy of Sciences, Key Laboratory of Earth and Planetary Physics, Beijing, China (rongzhaojin@mail.iggcas.ac.cn)

Here,  we use a state-of-art method to diagnose the Mercury’s dipolar field which is assumed to originate from a magnetic dipole. This method can effectively separate and solve the dipole parameters, and gives the error of how much the dataset of sampled magnetic field deviated from the dipole field . By employing this method and the MESSENGER field data, the derived optimum dipole parameters demonstrated that the dipole center is at [x=5.0;y=-16.0;z=480.5]km, the dipole moment is about M=2.5*10^19 nA.m^2 (or 172 nT*RM^-3), the dipole tilt angle is 3.7 degree. Our yielded dipole moment is weaker than that estimated in previous studies. We compared and discussed with previous studies.

How to cite: Rong, Z.: The non-axial dipolar magnetic field of Mercury, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-20477, https://doi.org/10.5194/egusphere-egu24-20477, 2024.