Space and Planetary Sciences (P)
Session Sub-category Solar-Terrestrial Sciences, Space Electromagnetism & Space Environment(EM)
Session ID P-EM11
Title Frontiers in solar physics
Short Title Frontiers in solar physics
Main Convener Name Shin Toriumi
Affiliation Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency
Co-Convener 1 Name Alphonse Sterling
Affiliation NASA/MSFC
Co-Convener 2 Name Kyoko Watanabe
Affiliation National Defense Academy of Japan
Co-Convener 3 Name Shinsuke Imada
Affiliation Department of Earth and Planetary Science, Graduate School of Science, University of Tokyo
Session Language 
E
Scope 
As Solar Cycle 25 is reaching its maximum phase, we are witnessing a variety of activity phenomena, including large solar flares and powerful coronal mass ejections, some of which are potentially damaging to our terrestrial environment. While cutting-edge solar observations are now regularly obtained from ground-based observatories such as DKIST, a new space-borne solar observing network is also being established, including the Solar Orbiter and Parker Solar Probe explorers, as well as the recently launched CHASE, ASO-S, and Adytia-L1 missions. Moreover, exciting new space observatories, including MUSE and SOLAR-C, are only a few years away. Progress is also being made in state-of-the-art numerical modeling that is essential for disentangling complex observations and for gaining fresh insights into the highly dynamic nature of solar and solar-wind magnetism and fluid/particle motions. To share and discuss recent advancements in solar physics and related fields, we invite contributions from solar researchers, and also from researchers in heliospheric, planetary, and stellar physics, covering results from their latest observation, numerical modeling, and experimental investigations.
Presentation Format Oral and Poster presentation
Joint Session with AGU
Invited Authors Craig Edward DeForest (Polarimeter to UNify the Corona and Heliosphere mission)
Mah Asgari-Targhi (Harvard-Smithsonian Center for Astrophysics)
Yuanyong DENG dyy@nao.cas.cn (National Astronomical Observatories, Chinese Academy of Sciences)
Shota Chiba (Institute for Space-Earth Environmental Research, Nagoya University)
Time Presentation No Title Presenter
Oral Presentation May 26 AM1
9:01 - 9:23 PEM11-01 NASA's Polarimeter to Unify the Corona and Heliosphere (PUNCH) mission Craig Edward DeForest
9:23 - 9:45 PEM11-02 The heating of the Sun’s Outer Atmosphere: Insights from Modeling and Observations Mah Asgari-Targhi
9:45 - 10:00 PEM11-03 Measurements of electric fields using DKIST ANAN TETSU
10:00 - 10:15 PEM11-04 Wavelet 3D-Based Method for the Examination of Propagating Waves Inside a Quiescent Prominence Aneta Wisniewska
10:15 - 10:30 PEM11-05 Feasibility Study of the Radio and Plasma Wave Detector for the Korea-Led L4 Mission Yukinaga Miyashita
Oral Presentation May 26 AM2
10:46 - 11:08 PEM11-06 Introduction to the Solar Polar orbit Observatory Mission Yuanyong DENG dyy@nao.cas.cn
11:08 - 11:30 PEM11-07 Study of MHD modes population in the mid-corona comparing the radio sounding with MHD simulation and prospects for collaborating with other observations Shota Chiba
11:30 - 11:45 PEM11-08 Unveiling the Three-Dimensional Evolution of an Emerging Active Region with SUNRISE III/SCIP Yusuke Kawabata
11:45 - 12:00 PEM11-09 A Data-Constrained Magnetohydrodynamic Simulation of the X7.1 Solar Flare on 2024 October 1 Keitarou Matsumoto
12:00 - 12:15 PEM11-10 Rapid, short-duration prominence eruptions in M-dwarf: Insights from solar observations Yuto Kajikiya
Presentation No Title Presenter
Poster Presentation May 26 PM3
PEM11-P01 Accelerating Nonlinear Heat Conduction Simulations in High-Temperature Regions Using Deep Learning Koseki Yuma
PEM11-P02 Statistical Study of Appearance Timing of H-alpha Postflare Loops: Simple Scaling Law Based on Radiative Cooling Takato Otsu
PEM11-P03 Mass Contribution to Coronal Mass Ejections(CMEs) from Plasma Flow in Dimming Regions Yuto Hiraoka
PEM11-P04 Effects of Ionization Nonequilibrium on First Ionization Potential (FIP) Bias during Solar Flares Soto Komiyama
PEM11-P05 Testing a coronal heating model of the young Sun through Model-Observation Comparisons Bumpei Sakamoto
PEM11-P06 Statistical study about the characteristics of microflares observed with Nobeyama Radioheliograph (NoRH) Ayatoshi Taniguchi
PEM11-P07 The realistic radial evolution of decay instability of Alfvén waves considering temperature anisotropy in the solar wind Hayato Saguchi
PEM11-P08 How Small-scale Jet-like Solar Events from Miniature Flux Rope Eruptions Might Produce the Solar Wind Alphonse Sterling
PEM11-P09 Statistical study of solar flares by using multiple Time-of-Flight methods observed with Fermi Masaya Yakura
PEM11-P10 A robust MHD relaxation method for reconstructing the solar atmospheric magnetic field Takahiro Miyoshi
PEM11-P11 Comparison of multiple chromospheric lines for postflare loops accompanied by a flare Junya Natsume
PEM11-P12 Solar Flares on the Early Sun: Insights from TESS's Photometric Observations of a Young Sun-like Star, EK Dra. Daijiro Hitotsuyanagi
PEM11-P13 Magnetohydrostatic Three-dimensional Coronal Magnetic Field Extrapolation Based on MHD Relaxation Method Daiki Yamasaki
PEM11-P14 Prominence splitting and merging due to interchange instability in helical flux rope Takafumi Kaneko