Session Details
[P-EM14]Frontiers in solar physics
Wed. May 24, 2023 10:45 AM - 12:15 PM JST
Wed. May 24, 2023 1:45 AM - 3:15 AM UTC
Wed. May 24, 2023 1:45 AM - 3:15 AM UTC
Online Poster Zoom Room (2) Online Poster
convener:Shin Toriumi(Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency), Takaaki Yokoyama(School of Science, Kyoto University), Shinsuke Imada(Department of Earth and Planetary Science, Graduate School of Science, University of Tokyo), Alphonse Sterling(NASA/MSFC)
On-site poster schedule(2023/5/23 17:15-18:45)
This session is for discussion of recent advancement in solar physics and related fields including heliospheric, planetary, and stellar physics. As Solar Cycle 25 progresses on pace to surpass the previous cycle, we have already witnessed numerous massive flares and CMEs. With the addition of new missions such as Parker Solar Probe, Solar Orbiter, CHASE, and ASO-S, the fleet of solar-observing spacecraft continues to watch the Sun to solve its mysteries. In Japan, the SOLAR-C mission completed its mission definition review in the summer of 2022 and is moving into the next phase, anticipating joint observations with NASA's upcoming MUSE mission. We invite contributions not only by solar researchers but also from all related disciplines (including helio, plasma, astrophysics, etc.), covering observations, numerical modeling, and experiments.
[PEM14-P01]One-dimentional MHD simulation on the prominence formation considering the shock and the Alfven wave turbulence heating
*Takero Yoshihisa1, Takaaki Yokoyama1, Takafumi Kanko2 (1.Kyoto University, 2.LMSAL, HAO/NCAR)
[PEM14-P02]Quantitative study of pitch angle distribution through microwave fast propagation in a solar flare observed with Nobeyama Radioheliograph
*Keitaro Matsumoto1, Satoshi Masuda1, Kazumasa Iwai1, Takafumi Kaneko2, Takashi Minoshima3 (1.Institute for Space-Earth Environmental Research, Nagoya University, 2.LMSAL, HAO/NCAR, 3.Center for Mathematical Science and Advanced Technology, Japan Agency for Marine-Earth Science and Technology)
[PEM14-P03]Multiwavelength Sun-as-a-star Analysis of an M8.7 Flare on 2022 Oct. 2 with H-alpha and EUV Using SMART/SDDI and SDO/EVE
*Takato Otsu1,2, Ayumi Asai2 (1.Department of Astronomy, Kyoto University, 2.Astronomical Observatory, Kyoto University)
[PEM14-P04]Differential Emission Measure (DEM) Analysis of Small-scale Eruptions in AR 12860
*Cheng-Ying Chiang1, Ya-Hui Yang1 (1.Department of Space Science and Engineering, National Central University, Taiwan)
[PEM14-P05]Inconspicuous Solar Polar Coronal X-ray Jets as the Source of Conspicuous Hinode/EUV Imaging Spectrometer (EIS) Doppler Outflows
*Alphonse Sterling1, Conrad Schwanitz2,3, Louise K Harra2,3, Nour E Raouafi4, Navdeep K Panesar5,6, Ronald L Moore7,1 (1.NASA/MSFC, Huntsville, AL, 35812, USA, 2.Institute for Particle Physics and Astrophysics, ETH, 8092 Zurich, Switzerland, 3.Physikalisch Meteorologisches Observatorium Davos, World Radiation Center, 7260 Davos, Switzerland, 4.The John Hopkins University Applied Physics Laboratory, Laurel, MD 20723, USA, 5. Bay Area Environmental Research Institute, NASA Research Park, Moffett Field, CA 94035, USA, 6.Lockheed Martin Solar and Astrophysics Laboratory, 3251 Hanover Street, Building 252, Palo Alto, CA 94304, USA, 7.Center for Space Plasma and Aeronomic Research, University of Alabama in Huntsville, Huntsville, AL 35805, USA)
[PEM14-P06]Solar p-mode as an additional energy source for coronal heating
*Hidetaka Kuniyoshi1, Richard Morton2, Takaaki Yokoyama3 (1.The University of Tokyo, 2.Northumbria University, 3.Kyoto University)
[PEM14-P07]Comprehensive simulation of solar wind formation from the solar interior
*Haruhisa Iijima1, Takuma Matsumoto1,2, Hideyuki Hotta3, Shinsuke Imada4 (1.Nagoya University, 2.National Astronomical Observatory of Japan, 3.Chiba University, 4.The University of Tokyo)
[PEM14-P08]Study on the time evolution of the electron acceleration site in a solar flare by using Time-of-Flight analysis method
*Masaya Yakura1, Satoshi Masuda1 (1.Nagoya University)
[PEM14-P09]Verification of the inversion method for electric field and velocity on the photosphere
*Masahiro Nobata1, Takafumi Kaneko2,3, Kanya Kusano1 (1.Institute for Space-Earth Environmental Research, Nagoya University, 2.Lockheed Martin Solar and Astrophysics Laboratory, 3.High Altitude Observatory/National Center for Atmospheric Research)
[PEM14-P10]Investigating differences of magnetic fields in Solar active regions that produce eruptive and confined flares
*Ichiro Goto1, Kanya Kusano1, KD Leka1,2 (1.Institute for Space-Earth Environmental Research Higashiyama Campus, Nagoya University, 2.NorthWest Research Associates)