Japan Geoscience Union Meeting 2015

Presentation information

International Session (Poster)

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

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

Tue. May 26, 2015 6:15 PM - 7:30 PM Convention Hall (2F)

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)

6:15 PM - 7:30 PM

[PEM07-P10] Reception of real-time solar wind data from DSCOVR and its application

*Shinichi WATARI1, Yuki KUBO1, Mamoru ISHII1 (1.National Institute of Information and Communications Technology)

Keywords:solar wind, space weather, L1, ACE, DSCOVR

DSCOVR (Deep Space Climate Observatory) was successfully launched on February 11, 2015 (UT) from Cape Canaveral, USA. DSCOVR is a successor of NASA scientific mission, ACE (Advanced Composition Explorer) and the first operational mission for space weather. It takes approximately 110 days for DSCOVR to reach the Lagrangian point (L1). DSCOVR provides one-second and one-minute data of three components of magnetic field and three-second and one-minute data of three components of velocity, temperature, and density in near real-time. We will present overview of DSCOVR data and their application, such as identification of regime of solar wind.