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Deep Earth Physics

  • KANESHIMA Satoshi, Professor
  • TAKAHASHI Futoshi, Associate Professor
Research subjects of our group focus on understanding the structure and dynamics of the deep interior of the Earth, planets and moons based on seismology and electromagnetism. In particular, the center of the Earth called the core is our final frontier, which we cannot see directly. We study the core using observations of the seismic wave and numerical simulations of the magnetic field generation processes (geodynamo). We also study planets and moons such as Mercury, Mars, our Moon, Jovian and Saturnian moons. Investigation of the current internal structure of the bodies helps us understand their evolution histories and clarify their origin.

1. Seismology

We analyze seismic waves passing through the Earth in order to explore the structure and dynamics of Earth's deep interior. Issues investigated in this laboratory include:

  1. Seismic waves that are multiply reflected at the core-mantle boundary and stratification of the outermost part of the Earth's outer core
  2. Seismic wave speed models of the bottom of the outer core and their implications on the inner growth
  3. Seismic scattering at kilometer-scale heterogeneity in the mid-lower mantle and its implication on the fate of basaltic oceanic crust and vigor of mantle convection
  4. Fine structure of seismic discontinuity at the bottom of the Earth's upper mantle and its implication on the phase transitions of mantle minerals
  5. Mechanism of deep earthquakes and the fate of subducted slabs

2. Earth and planetary dynamos

A result of numerical dynamo simulation.

While it is well-known that the Earth has its own magnetic field, which is approximated by a bar magnetic centered in the Earth, it is not well-known why the Earth has the magnetic field. The origin of the geomagnetic field is a process of electromagnetic induction called “dynamo”. The Earth's dynamo works in the outer core, which mostly consists of liquid iron. Flows of such highly electrically conducting material can generate and maintain the magnetic field for billions of years. Since dynamo action is a highly non-linear problem, we cannot solve the equations analytically. Instead, we perform numerical modeling using high-performance computing (HPC).

Magnetic field of other planets and moons are also our interest. Dynamos of the Moon and Mars are now extinct, but operated in the past. Remanence of the past dynamos are recorded in the crust. Thus, we could extract information about the evolution history by analyzing the crustal magnetic field observed by orbiting satellites. One of the currently most interesting subjects is the Mercury's magnetic field, which is maintained by dynamo in Mercury's core. In 2017, Mercury's orbiter BepiColombo, with which magnetometers are equipped, will be launched. We study how the Mercury's magnetic field is at present, and is maintained based on observation and numerical modeling.