On Physical condition in the early Heliosphere

Takeru SUZUKI

Presentation information

International Session (Oral)

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

[P-EM07] Space Weather, Space Climate, and VarSITI

Mon. May 25, 2015 2:15 PM - 4:00 PM 302 (3F)

Convener:*Ryuho Kataoka(National Institute of Polar Research), Yusuke Ebihara(Research Institute for Sustainable Humanosphere, Kyoto University), Yoshizumi Miyoshi(Solar-Terrestrial Environement Laboratory, Nagoya University), Toshifumi Shimizu(Institute of Space and Astronautical Science, JAXA), Ayumi Asai(Unit for Synergetic Studies of Space, Kyoto University), Hidekatsu Jin(National Institude of Information and Communications Technology), Tatsuhiko Sato(Japan Atomic Energy Agency), Kanya Kusano(Solar-Terrestrial Environment Laboratory, Nagoya University), Hiroko Miyahara(College of Art and Design, Musashino Art University), Takuji Nakamura(National Institute of Polar Research), Kazuo Shiokawa(Solar-Terrestrial Environment Laboratory, Nagoya University), Kiminori Itoh(Graduate School of Engineering, Yokohama National University), Chair:Ryuho Kataoka(National Institute of Polar Research)

2:15 PM - 2:30 PM

[PEM07-19] On Physical condition in the early Heliosphere

*Takeru SUZUKI¹ (1.School of Science, Nagoya University)

Keywords:Solar Wind, Protoplanetary Disk, Magnetohydrodynamics, wave, turbulence

In this talk, I would like to discuss the evolution of physical properties in the heliosphere at early epochs. After briefly reviewing the evolution of the protoplanetary disk with particularly focus on the role of turbulence-driven disk wind, I introduce the evolution of the solar wind. We also discuss effects of variation of the physical condition in the heliosphere on the formation and evolution of solar-system planets.