Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Shonan Institute of Technology
Nagoya University, Toyokawa, Japan
CSPAR, University of Alabama, Huntsville, AL 35899, USA
IGPP, University of California, Riverside, CA 92521
Nagoya Univ., Toyokawa, Japan
Shonan Institute of Technology, Tsujido, Fujisawa, Kanagawa 251
Institute of Geophysics and Planetary Physics, University of California, Riverside, CA 92521
Nagoya University, Japan
IGPP, University of California, University Ave., Riverside, CA 92521, USA Center for Space Plasma and Aeronomic Research The University of Alabama in Huntsville, Huntsville, AL, USA;
CSPAR, University of Alabama, Huntsville, AL, USA;
Institute of Geophysics and Planetary Physics, University of California Riverside, 900 University Ave., Riverside, CA 92521, USA University, Nagoya, Japan
Institute of Geophysics and Planetary Physics, University of California, Riverside, CA 92521, USA University of California, Riverside, 900 University Ave, Riverside, CA 92521, USA Institute of Technology, Fujisawa 251-8511, Japan
University of Alabama, CSPAR
Shonan Institute of Technology, 1-1-25, Nishi-kaigan, Tsujido, Fujisawa, 251-8511 Japan University of California at Riverside, 900 University Ave, Riverside, CA 92521, USA of Geophysics and Planetary Physics, UCR, Riverside, Riverside, CA 92521, USA Institute of Technology, Tsujido, Fujisawa 251, Japan
CSPAR / University of Alabama - Huntsville, Huntsville, AL, USA
University of Alabama, Huntsville, Huntsville, AL, USA
Shonan Institute of Technology, Tsujido, Fujisawa 251-8511, Japan.
The Institute of Geophysics and Planetary Physics at the University of California, Riverside, USA
CSPAR, University of Ala
3-D Magnetic Field and Current System in the Heliosphere
A dynamic and realistic heliospheric modelling using interplanetary scintillation and photospheric magnetic data
A Forecast of the Heliospheric Termination-Shock Position by Three-dimensional MHD Simulations
A Forecast of the Termination-Shock Position
A Global V-Shaped Channel Structure of the Termination Shock Due to a Magnetic Pressure Effect, and Its Physical Connection to Bipolar Flow Type Planetary Nebulae
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