Japan Geoscience Union Meeting 2014

Presentation information

International Session (Oral)

Symbol S (Solid Earth Sciences) » S-IT Science of the Earth's Interior & Techtonophysics

[S-IT03_29PM2] Structure and dynamics of Earth and Planetary deep interiors

Tue. Apr 29, 2014 4:15 PM - 6:00 PM 418 (4F)

Convener:*Satoru Tanaka(Institute for Research on Earth Evolution Japan Agency for Marine-Earth Science and Technology), Takashi Yoshino(Institute for Study of the Earth's Interior, Okayama University), Masanori Kameyama(Geodynamics Research Center, Ehime University), Dapeng Zhao(Department of Geophysics, Tohoku University), John Hernlund(ELSI, Tokyo TECH), Chair:John Hernlund(Earth-Life Science Institute, Tokyo Institute of Technology), Kenji Ohta(Department of Earth and Planetary Sciences, Tokyo Institute of Technology)

4:15 PM - 4:30 PM

[SIT03-22] A generating process of the geomagnetic drifting field

*Takesi YUKUTAKE1, Hisayoshi SHIMIZU2 (1.None, 2.Earthquake Research Institute, University of Tokyo)

Keywords:geomagnetic secular variation, westward drift, drifting field, core surface flow

The geomagnetic field is comprised of drifting and standing field. The drifting field is the field that drifts westwards nearly steadily over the past several hundred years and the standing field is that stays at the same place. The drifting field has two major characteristic features. When the field is expressed in a spherical harmonic series, the drifting field mainly consists of sectorial harmonics. Secondly the rate of drift is uniform irrespective of the harmonics. This means the drift velocity is non-dispersive. We here propose a model of the generating process of the drifting field. Because of the non-dispersive nature of the drift velocity, we assume the westward drift is a phenomenon closely tied with material flow rather than a magnetohydrodynamic wave. Furthermore we take it a phenomenon near the surface of the core where the dipole field is dominant. If the mantle is approximated by an electrical insulator, the electric current in the core normal to the core-mantle boundary must be zero. This provides a strong constraint on the liquid flow near the surface. If we assume infinite conductivity of the core for simplicity, only the sectorial flow is allowed for the toroidal flow, and the meridional flow for the poloidal flow. The sectorial toroidal flow, interacting with the dipole field, induces sectorial poloidal field, whereas the meridional poloidal flow produces the meridional poloidal field. The surface layer, which is rotating westwards as a whole, carries these fields westwards together. Since the rotation of the meridional field is unrecognizable, only the sectorial field is observed as the drifting field. We present a simplified model that describes the above process.