"Recent progress in heliospheric physics by direct measurements of unexplored space plasmas"
- February 25 (Mon.) - 28 (Thu), 2019
- Nagoya University, Furo-cho, Chikusa-ku, Nagoya, Japan
Research Institute Building II, 3F-Hall (F3-3 in campus map)
The International ISEE symposium "Recent progress in heliospheric physics by direct measurements of unexplored space plasmas" will be held from 25-28 Feb. 2019 at Nagoya University, Japan. The purpose of the symposium is to bring heliospheric physicists together for discussions about new developments of heliospheric physics driven by recent and forthcoming spacecraft missions. The symposium covers broad topics related to the recent progress and future outline in heliospheric physics with invited and contributed talks. The 2018 ISEE prize winner will also give a plenary talk at the symposium.
- Gary Zank - University of Alabama in Huntsville
- Physics of the Interaction of the Solar Wind with the Very Local Interstellar Medium
- Ming Zhang - Florida Institute of Technology
- Heliospheric influence on the anisotropy of cosmic rays
- Marco Velli - University of California, Los Angeles (UCLA)
- Understanding Coronal Heating and Solar Wind Acceleration: Parker Solar Probe
- Daniel Verscharen - University College London
- Studying large-scale and small-scale solar-wind turbulence with Solar Orbiter: particles and fields
- John Richardson - Massachusetts Institute of Technology
- Recent Observations from the Voyager Spacecraft
- Zhongwei Yang - Chinese Academy of Science
- Analysis of energy spectra observed by New Horizons: PIC simulation results versus observations in the environment of Pluto
- Mahboubeh Asgari-Targhi - Harvard-Smithsonian Center for Astrophysics
- Modeling and observations of density fluctuations in the solar wind
- Mitsuo Oka - UC Berkeley
- Electron Acceleration at Earth's Bow Shock: MMS Observation
- Justyna M. Sokol - Space Research Centre, Polish Academy of Sciences
- From IBEX to IMAP: imaging the distant heliosphere by energetic neutral atoms and interstellar neutral gas
- Makoto Sasaki - Kyushu University
- On the spatial profile of turbulence in magnetically confined plasmas
- Munehito Shoda - University of Tokyo
- Three-dimensional, self-consistent MHD simulation of the solar wind acceleration
- Daikou Shiota - National Institute of Information and Communications Technology
- Three-dimensional MHD modeling of solar corona and inner heliosphere for space weather forecast
- Ken Tsubouchi - University of Electro-Communications
- Properties of pickup ion density variations in the outer heliosheath as a probe for the heliopause fluctuation
- Hirohisa Hara - National Astronomical Observatory of Japan
- Plasma Dynamics in the Solar Corona Revealed by Emission Line Spectroscopy
- Kazuoki Munakata* - Shinshu University
- Long-term variation of cosmic ray intensity observed with Nagoya muon detector
- Haruichi Washimi - Kyushu University
- An MHD analysis of time-varying outer heliospheric structure using OMNI solar-wind daily data
- Takeru Suzuki - University of Tokyo
- Stellar winds and coronae from solar-type stars with different metallicities
- Nobumitsu Yokoi- University of Tokyo
- Multiple-scale analysis of turbulent transport in strongly compressible magnetohydrodynamic plasmas
- Tomo-Hiko Watanabe - Nagoya University
- Generation of Alfvenic turbulence and implication to auroral particle acceleration
- Kanya Kusano - Nagoya University, ISEE
- Toward the physics-based prediction of solar flares and coronal mass ejections
Yasuhiro Nariyuki (Toyama University), Shuichi Matsukiyo (Kyushu University), Chihiro Kato, Kazuoki Munakata (Shinshu University),
Yutaka Matsubara, Munetoshi Tokumaru (ISEE, Nagoya University)
Sponsored by Institute for Space-Earth Environmental Research (ISEE), Nogaoya University
, cosponsored by Society of Geomagnetism, Earth, Planetary and Space Sciences (SGEPSS)
Partly supported by a grant from Society for Promotion of Space Science
- Poster Size: h 180cm by w 90cm, enabling to put a poster with a A0 size (h118.9cm X w84.1cm).
- The ISEE Award ceremony will be held during the conference period; on February 27 afternoon at the ES hall of the ES building 1st floor (C2-4 in the campus map).
- Memorial Lecture by Professer Hisao Takahashi, INPE, Brazil
Title: "Our Concern for Space Weather: Equatorial Ionospheric Plasma Bubbles"
16:00 - 17:30
- The conference dinner will start on February 27 6:00 PM at the Restaurant "Hananoki" (D1-4 in the campus map).
All participants are invited to this dinner. The fee is 4000 yen.
- Locations of venue, restaurant, ES hall
- Campus map including information of restaurants and cafes
- Area Guid map around the campus
- The meeting for result presentations of collaborative research on the heliosphere and cosmic rays will be held on February 28 AM, simultaneously with the poster seesion. All presentations of this meeting will be given in Japanese.
- Wifi connection: The eduroam service is available throughout the campus. For those who have no eduroam account, we can provide a guest account to connect the wifi service "nuwnet" of Nagoya University.
- Metro station: Nagoya Daigaku station of Meijo Line
- Airport: Chubu Cnetair International Airport, Nagoya
- Access to Nagoya University (Higashiyama campus)
- Higashiyama campus map