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Plenary session: Waves and turbulence
Tuesday, 3 September 2019
10:20 - 13:00
Ito Hall
Chair: Takashi Sakurai, National Astronomical Observatory of Japan
10:20 - 10:50 Constraining coronal heating with multiwavelength measurements.
10:50 - 11:20 Waves and turbulence in the solar wind.
11:20 - 11:50 Laboratory experiments on plasma waves relevant to solar and space plasmas.
11:50 - 12:20 Parker Solar Probe: First results after three solar encounters and outlook.
12:20 - 12:40 First results from the FIELDS instrument suite on Parker Solar Probe.
12:40 - 13:00 Three-dimensional simulation of the fast solar wind driven by compressible magnetohydrodynamic turbulence.
- Constraining coronal heating with multiwavelength measurements
- Lindsay Glesener, University of Minnesota, United States
- Säm Krucker, FHNW, Switzerland
- Shin-nosuke Ishikawa, Nagoya University, Japan
- Waves and turbulence in the solar wind
- Dipankar Banerjee, Indian Institute of Astrophysics, India
- Laboratory Experiments on Plasma Waves Relevant to Solar and Space Plasmas
- Walter Gekelman, University of California, Los Angeles, United States
- Parker Solar Probe: First Results After Three Solar Encounters and Outlook
- Nour E. Raouafi, Johns Hopkins University Applied Physics Laboratory, Laurel, Maryland, United States
- Stuart D. Bale, Space Sciences Laboratory, University of California, Berkeley, CA, United States
- Justin C. Kasper, Climate and Space Sciences and Engineering, University of Michigan Ann Arbor, United States
- Russel A. Howard, Space Science Division, U.S. Naval Research Laboratory, Washington, DC, United States
- David J. McComas, Department of Astrophysical Sciences, Princeton University, Princeton, NJ, United States
- Marco Velli, EPSS, University of California, Los Angeles, CA, United States
- Arik Posner, SMD/Heliophysics Division, NASA Headquarters, Washington, DC, United States
- Adam Szabo, NASA Goddard Space Flight Center, Greenbelt, MD, United States
- First results from the FIELDS instrument suite on Parker Solar Probe
- Stuart Bale, University of California, Berkeley, United States
- Three-dimensional simulation of the fast solar wind driven by compressible magnetohydrodynamic turbulence
- Munehito Shoda, National Astronomical Observatory of Japan, Japan
- Takeru Suzuki, The University of Tokyo, Japan
- Mahboubeh Asgari-Targhi, Harvard-Smithsonian Center for Astrophysics, United States
- Takaaki Yokoyama, The University of Tokyo, Japan