[E] Poster
P (Space and Planetary Sciences ) » P-EM Solar-Terrestrial Sciences, Space Electromagnetism & Space Environment
convener:Shinsuke Imada(Institute for Space-Earth Environmental Research, Nagoya University), Alphonse Sterling(NASA/MSFC), Takaaki Yokoyama(School of Science, University of Tokyo), Toshifumi Shimizu(Institute of Space and Astronautical Science, JAXA)
Over recent decades, Sun-observing satellite missions have told us much about the dynamic solar atmosphere. These satellites can observe magnetic activity in the solar corona at wavelengths inaccessible from ground-based telescopes, such as X-rays and EUV. Additionally, the seeing-free conditions of space allow for consistent, high-spatial resolution at visible wavelengths; e.g. the HInode satellite can observe solar surface magnetic field elements down to ~0.2 arcsec. From observations such as these, we have identified three important points regarding what is required form future space-based solar missions to solve fundamental solar problems, such as how the corona is heated and what drives solar eruptions: (1) seamless observation over all temperature regimes of the solar atmosphere, from the chromosphere to the corona, at the same time; (2) high spatial and temporal resolution to resolve elemental structures of the solar atmosphere, and to track their evolution; and (3) plasma diagnostic capability to quantify the dynamics of elementary process taking place in the solar atmosphere. To meet these requirements, recently the solar physics community in Japan proposed the Solar-C_EUVST mission, which will be launched in the mid-2020s. Furthermore, additional top-rate solar observatories, such as the Parker Solar Probe (PSP), Solar Orbiter, and the Daniel K. Inouye Solar Telescope (DKIST), will be operating in the years leading up to Solar-C_EUVST. In this session we will discuss what solar physics observational and numerical-simulation studies are required prior to the mid-2020s, to prepare most efficiently for the new observational era. We welcome contributions dealing with remote-sensing space-based observations (e.g. from Hinode and SDO), in-situ observations from near- and deep-space (e.g., PSP, Pioneer), ground-based observations, and numerical studies.
*Kento Michiwaki1, Shinsuke Imada1, Yoshizumi Miyoshi1 (1.Institute for Space-Earth Environmental Research, Nagoya University)
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*SHOMA UNEME1, Shinsuke Imada1, Hisashi hayakawa2, Lee Harim3, Moon Yongjae3, Park Eunsu3, Yoshizumi Miyoshi1 (1.nagoya university institutive for Space Earth for enviornmental research, 2.Osaka University School of Letters , 3.School of Space Research, Kyung Hee University)
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*Kengo Matoba1, Shinsuke Imada1 (1.Institute for Space-Earth Environmental Research, Nagoya University)
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*Haruhisa Iijima1, Hideyuki Hotta2, Shinsuke Imada1 (1.Institute for Space-Earth Environmental Research, Nagoya University, 2.Faculty of Science, Chiba University)
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*Shinsuke Imada1 (1.Institute for Space-Earth Environmental Research, Nagoya University)
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*Kyohei Murakami1, Shinsuke Imada1, Haruhisa Iijima1, Yoshizumi Miyoshi1 (1.Nagoya University Institute for Space-Earth Environmental)
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*Kyoko Watanabe1, Kosuke Tsuruda1, Satoshi Masuda2, Sam Krucker2,3,4 (1.National Defense Academy of Japan, 2.Institute for Space-Earth Environmental Research, Nagoya University, 3.University of Applied Sciences Northwestern Switzerland, 4.UC Berkeley)
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*Shohei Nishimoto1, Kyoko Watanabe1, Shinsuke Imada2, Toshiki Kawai2, Tomoko Kawate3, Hidekatsu Jin5, Kyoung-Sun Lee4 (1.National Defense Academy, 2.Institune for Space-Earth Environmental Research, Nagoya University, 3.Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 4.Center for Space Plasma and Aeronomic Research, University of Alabama in Huntsville, 5.National Institute of Information and Communications Technology)
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*Alphonse Sterling1, Ronald Moore2,1, Navdeep Panesar3,4 (1.NASA/MSFC, 2.U of Alabama Huntsville, 3.LMSAL, 4.Baeri)
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Cancelled
*Hirohisa Hara1, Nozomi Ono2,1, Nobuyuki Nakamura3, Naoki Numadate3, Izumi Murakami4 (1.National Astronomical Obserbvatory of Japan, 2.The University of Tokyo , 3.The University of Electro-Communications, 4.National Institute for Fusion Science)
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*Takaaki Yokoyama1, Shinsuke Imada2, Haruhisa Iijima2, Shin Toriumi3 (1.School of Science, The University of Tokyo, 2.Institute for Space-Earth Environmental Research, Nagoya University, 3.Institute of Space and Aeronautical Science, JAXA)
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