Space and Planetary Sciences (P) | ||
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Session Sub-category | Solar-Terrestrial Sciences, Space Electromagnetism & Space Environment(EM) | |
Session ID | P-EM16 | |
Title | Heliosphere and Interplanetary Space | |
Short Title | Heliosphere | |
Main Convener | Name | Kazumasa Iwai |
Affiliation | Institute for Space–Earth Environmental Research (ISEE), Nagoya University | |
Co-Convener 1 | Name | Yasuhiro Nariyuki |
Affiliation | Faculty of Education, University of Toyama | |
Co-Convener 2 | Name | Masaki N Nishino |
Affiliation | Japan Aerospace Exploration Agency, Institute of Space and Astronautical Science | |
Co-Convener 3 | Name | Ken Tsubouchi |
Affiliation | University of Electro-Communications | |
Session Language |
J |
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Scope |
This session aims to share new findings on the heliosphere and interplanetary space. Presentations of the recent studies from any approaches (integrated observation/theoretical modeling/massive numerical simulation/development of instrumentation) are welcomed. The topic of this session contains a wide range of phenomena and regions: solar corona/solar flares/CMEs/solar wind/high-energy particles, and their impact on the terrestrial/planetary/lunar environment, solar activity, global structure of the heliosphere, cosmic rays, and outer heliosphere. Related fundamental physics problems such as shocks/waves/turbulence/particle transport and acceleration are also included in the main target. |
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Presentation Format | Oral and Poster presentation |
Time | Presentation No | Title | Presenter |
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Oral Presentation May 28 PM2 | |||
15:30 - 15:45 | PEM16-01 | Evaluation of CME observation performance of next generation solar wind observation system using model simulation | Kazumasa Iwai |
15:45 - 16:00 | PEM16-02 | Validation of initial Parameter dependence of CME Propagation and its Time of Arrival at Earth in SUSANOO-CME | Hirofumi Isogai |
16:00 - 16:15 | PEM16-03 | MHD waves and a CME in the solar corona observed by using radio occultation technique with Akatsuki spacecraft | Shota Chiba |
16:15 - 16:30 | PEM16-04 | Sustained Gamma-Ray Emission: Case study of an X-class flare occurred on 7 March 2012 | Satoshi Masuda |
16:30 - 16:45 | PEM16-05 | Conceptual research for a cosmic-ray muon observation in the Arctic region | Masayoshi Kozai |
16:45 - 17:00 | PEM16-06 | Dependence of plasma properties on the pickup ion density in the heliosheath | Ken Tsubouchi |
Oral Presentation May 29 AM1 | |||
09:00 - 09:15 | PEM16-07 | Relationship between slow solar wind and plasma-upflow obtained from interplanetary scintillation observation, Hinode/EIS observation and PFSS model | Keita Morishima |
09:15 - 09:30 | PEM16-08 | BepiColombo and STELEO observations and numerical modelling of solar energetic particle events in March 2022. | Takashi Minoshima |
09:30 - 09:45 | PEM16-09 | Development of the calibration method for the radiation instruments onboard Mercury explorer BepiColombo and its application to the inner heliosphere exploration | Gaku Kinoshita |
09:45 - 10:00 | PEM16-10 | Analysis and generalization of a two-modes model for solar wind magnetohydrodynamic turbulence | Yasuhiro Nariyuki |
Presentation No | Title | Presenter |
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Poster Presentation May 29 PM3 | ||
PEM16-P01 | Development of the phased array antenna system for next generation solar wind observation system:design of sub-array | Yusuke Kagao |
PEM16-P02 | Development of the analog signal combination system for next-generation solar wind observation system | Haruto Watanabe |
PEM16-P03 | Development of a digital multi-beamformer for a next-generation solar wind observation system | Takehara Daichi |
PEM16-P04 | Development of a wideband feed system for the solar and planetary radio telescope in Tohoku University | Yozi Kuwayama |
PEM16-P05 | Characteristics of spectral fine structures of metric type II radio bursts | Hiroaki Misawa |
PEM16-P06 | Motion of the source region of the type-II solar radio burst derived from the spectra in MF-HF frequency range | Naoto Kinno |
PEM16-P07 | Interplanetary Scintillation Observations of Solar Wind During Solar Cycles 24 and 25: Challenges for Enhanced Reconstruction | Ken'ichi Fujiki |
PEM16-P08 | Linear analysis of the parametric decay instability in the expanding solar corona considering temperature anisotropy | Hayato Saguchi |
PEM16-P09 | Bifurcation of Magnetic Field Topology using Polynomial Reconstructed MMS data | Bhola Raj Panta |