Japan Geoscience Union Meeting 2021

Presentation information

[E] Poster

P (Space and Planetary Sciences ) » P-EM Solar-Terrestrial Sciences, Space Electromagnetism & Space Environment

[P-EM09] Dynamics of Magnetosphere and Ionosphere

Sun. Jun 6, 2021 5:15 PM - 6:30 PM Ch.05

convener:Akiko Fujimoto(Kyushu Institute of Technology), Mitsunori Ozaki(Faculty of Electrical and Computer Engineering, Institute of Science and Engineering, Kanazawa University), Yuka Sato(Nippon Institute of Technology), Aoi Nakamizo(Applied Electromagnetic Research Institute, National Institute of Information and Communications Technology)

5:15 PM - 6:30 PM

[PEM09-P05] Development of a new M-I coupling algorithm in global MHD magnetosphere simulation: Alfvénic-Coupling

*Aoi Nakamizo1, Akimasa Yoshikawa2, Hiroyuki Nakata3, Keiichiro Fukazawa4, Takashi Tanaka2 (1.Applied Electromagnetic Research Institute, National Institute of Information and Communications Technology, 2.Faculty of Science, Kyushu University, 3.Faculty of Engineering, Chiba University, 4.Academic Center for Computing and Media Studies, Kyoto University)

Keywords:M-I Coupling, Global Magnetosphere Simulation, Alfven Mode, Algorithm

Presently, most global MHD magnetosphere models equip ionospheric solvers at their inner boundaries and then simulate the magnetospheric and ionosphere (M-I) processes. Here the ionospheric solver is the so-called 'thin shell model' which solves the Ohm’s law under the thin shell approximated ionosphere with FACs in the polar region and the height-integrated ionospheric conductivity. With this solver, the global MHD models solve the inner boundary condition of electromagnetic field in the following manner. (1) The FAC distribution obtained from the rotation of the magnetic field at the inner boundary (usually placed at the altitude of 2–3 Re) is mapped to the ionospheric altitude. (2) The mapped FAC is inputted to the solvers equipped at the ionospheric altitude, then the ionospheric potential is calculated. (3) The potential is mapped back to the inner boundary and the bulk velocity is updated there.
On the other hand, Yoshikawa et al. [2010] proposed a new M-I coupling algorithm which guarantees the continuities of physical quantities between the magnetosphere and ionosphere and therefore the momentum and energy conservations by considering the incident and reflection process of shear Alfvén waves. We call the new algorithm ‘Alfvénic-coupling.’ We discuss in detail the characteristics of the traditional algorithm and the concept of Alfvénic-coupling algorithm. We report on the progress of the implementation of Alfvénic-coupling in a global MHD code and will show the preliminary results.

Reference
Yoshikawa, A., H. Nakata, A. Nakamizo, T. Uozumi, M. Itonaga, S. Fujita, K. Yumoto, and T. Tanaka, Alfvenic-coupling algorithm for global and dynamical magnetosphere-ionosphere coupled system, J. Geophys. Res., 115, A04211, 2010, dot:10.1029/2009JA014924.