著者 |
発表者 |
招待 講演 |
講演番号 |
ショートタイトル |
予稿集本文 |
MAEDA, Keisuke |
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S001-05 |
Continuous Human Resource Development Initiatives using Stratospheric Balloon Experiments. |
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MAEDA, Yuki |
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R005-P01 |
Non-thermal escape of hydrogen atmosphere on early Earth by a 3D multispecies MHD simulation |
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R009-P13 |
Comparison of Titan's atmospheric escape processes by Saturn and Solar winds |
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MAENO, Fukashi |
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R004-P07 |
Paleointensity and rock magnetic analyses of lavas on Nishinoshima, Ogasawara Islands |
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MAENO, Hideo |
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R005-P29 |
Horizontal structures and movements of sporadic E layers observed with ionosonde receiver networks |
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S002-P07 |
Ionospheric variations observed at Syowa Station, Antarctica during the May 2024 space weather event |
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MAEYAMA, Shinya |
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R008-04 |
Extension of gyrokinetic simulation for the dipole field configuration |
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MAHESWARAN, Veera Kumar |
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R005-P32 |
Statistical Analysis of the Local-time Dependence of the Coupling between MSTID and Es-layer |
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MANO, Kouhei |
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R009-P08 |
Photoelectron extent estimated from spacecraft potential at electric-field waveform distortion |
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MARC, Lessard |
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R006-P23 |
Over-darking of diffuse/pulsating aurora: LAMP sounding rocket observation |
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MARCQ, Emmanuel |
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R009-20 |
Distributions of SO2 and unidentified UV absorber retrieved using UV images taken by Akatsuki UVI |
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MARK, Sadgrove |
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R009-P12 |
Crystal Structure of NaCl on Europa's Surface Based on Plasma Irradiation Experiments |
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MARTIN, Connors |
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R006-13 |
Magnetospheric source of auroral emission at subauroral latitudes using Arase and ground imagers |
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R006-P27 |
Observation of auroral emission altitude during relativistic electron precipitation events |
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MARUBASHI, Katsuhide |
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R007-04 |
A New Scheme of GS Equation-Based Analysis for Expanding Interplanetary Flux Ropes |
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R010-P02 |
Multipoint spacecraft measurements of the ICME structure in October 2021 |
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MASAOKA, Kohei |
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R004-04 |
Archeointensity increase in Japan estimated from Middle and Late Yayoi potteries of 250 BCE to 50 CE |
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MASUDA, Ayune |
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R005-P05 |
Development of NLC Imager for observation in the high latitude region-The test observation in Kiruna |
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MASUDA, Satoshi |
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R010-11 |
Reproduction of electron density in the lower ionosphere during solar flares using PHITS code |
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R010-12 |
Solar Hydrogen Lyman line emissions from solar flares and their effects on the Earth's ionosphere |
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R010-P01 |
Hinode observation of long-term variation of magnetic fields in the Sun's polar regions |
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R010-P03 |
Solar Microwave Observations with the Yokosuka Radio Polarimeter (YoRP) |
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S002-P11 |
Evaluation of electron density variation using PHITS and GAIA models during solar flares in May 2024 |
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MASUI, Hirokazu |
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R010-P04 |
Current Status of the YOTSUBA-KULOVER Satellite for Precise Geomagnetic Observations |
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MASUNAGA, Kei |
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R009-08 |
Current status of LAPYUTA mission |
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R009-10 |
C{sup}+{/sup} 133.5 nm emission mechanisms on Mars revealed by MAVEN observations |
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R009-16 |
Influence of the solar wind on the hydrogen airglow in the Venusian upper atmosphere by Hisaki |
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R009-P04 |
Mass analysis of low-energy ions originating from the lunar surface and exosphere |
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MASUNO, Hayato |
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R006-P20 |
Investigation of the Plasma Environment Responsible for Spacecraft Surface Charging |
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R006-P21 |
Investigation of the relationship between satellite surface charging and chorus waves |
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MATSUDA, S. |
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S002-P05 |
EMIC waves during the May 2024 geomagnetic storm |
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MATSUDA, Shoya |
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R006-06 |
Origins of chorus waves in the inner magnetosphere |
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R006-07 |
Construction of empirical wave power model of chorus waves based on the Arase observation |
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R006-08 |
Analysis of space distribution and propagation properties of low frequency chorus observed by Arase |
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R006-09 |
Evaluation of a direction finding method using NWC transmitter signals observed by the Arase |
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R006-10 |
A statistical study on energy sources of mid-latitude lower hybrid waves observed by Arase |
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R006-20 |
Investigation of Omega Band Auroras: Ground and Magnetospheric Conjugate Observations |
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R006-P09 |
An Empirical Plasmapause Model using Arase/PWE Data and Machine Learning |
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R006-P21 |
Investigation of the relationship between satellite surface charging and chorus waves |
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R006-P24 |
Statistical analysis of pulsating auroras and high-latitude propagation of chorus waves |
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R006-P26 |
Statistical Survey of Dayside Energetic Electron Precipitation in the Inner Magnetosphere |
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R006-P28 |
Repetition period of REP and chorus observed during the conjunction event of ISS/CALET and Arase |
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R006-P29 |
Characteristics of MeV Electron Precipitation Spectra Observed by CALET/CHD |
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R006-P32 |
Noon-midnight difference in latitudinal occurrence of chorus waves observed by Arase |
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R006-P33 |
Chorus wave activity at marginal condition of electron temperature anisotropy instability |
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R006-P34 |
Frequency spectram of electrostatic waves driven by chorus waves observed by the Arase satellite |
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R006-P35 |
Study of propagation characteristics of EMIC wave using multipoint observation by Arase and Cluster |
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R006-P36 |
Spatial Distribution of Magnetosonic Waves Observed by the Arase Satellite |
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R009-06 |
HF of RPWI aboard JUICE: Lunar-Earth flyby in Aug 2024 and beyond |
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R009-P08 |
Photoelectron extent estimated from spacecraft potential at electric-field waveform distortion |
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R011-08 |
Development of BepiColombo/MMO data archive |
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S002-07 |
Arase satellite observations of the radiation belts for the May 2024 geospace storm |
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S002-10 |
Electron density variation in the plasmasphere and ionosphere during the May 2024 storm |
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S002-P04 |
Particle acceleration upon the SSC of May 2024 storm |
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MATSUI, Daichi |
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R010-08 |
Analysis of the surface charging events and their plasma environment of the Van Allen probes |
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MATSUI, Tatsuro |
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R009-23 |
Temporal Evolution of Mesoscale Structures seen in UV images of the Venusian Cloud Top |
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MATSUKIYO, Shuichi |
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R007-P01 |
Machine learning clustering of galactic cosmic ray trajectories in the heliosphere |
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R008-11 |
Study of nonstationary collisionless shock using high-power laser experiment |
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R008-P01 |
High-power laser experiment of collisionless shock generation using light gases |
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R008-P02 |
Study of Collective Thomson Scattering using 2D full Particle-in-cell Simulation |
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R008-P03 |
Electron acceleration efficiency by magnetic surfing at non-relativistic shocks |
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R008-P04 |
Relativistic Resonant and Wakefield Acceleration Driven by Large Amplitude Alfven Waves |
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R008-P05 |
Microstructure of magnetic island in collisionless reconnection |
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R008-P06 |
Reconstruction of MHD structures of magnetic reconnection using PINNs |
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R008-P08 |
Two-dimensional evolution of synchrotron maser instability in relativistic electron-ion plasmas |
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R008-P11 |
Numerical calculation of plasma-neutral fluid interactions using PINNs |
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MATSUMOTO, Haruhisa |
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S002-15 |
Status of JAXA Low Altitude Satellite and Radiation Environment in May 2024 Event |
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MATSUMOTO, Jin |
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R008-20 |
Implementation of a machine leaning model into the relativistic MHD simulation code |
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MATSUMOTO, Takuma |
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R010-P01 |
Hinode observation of long-term variation of magnetic fields in the Sun's polar regions |
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MATSUMOTO, Yosuke |
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R006-26 |
An Estimation of Magnetopause Reconnection Rate from Soft X-ray Imaging |
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R006-P45 |
Status of GEO-X mission |
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R008-12 |
Dependence of the electron SSA efficiency on shock speeds in non-relativistic high Mach shocks |
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R008-17 |
A preferential positron acceleration in relativistic magnetized electron-ion-positron shocks |
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R008-20 |
Implementation of a machine leaning model into the relativistic MHD simulation code |
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R009-09 |
Kelvin-Helmholtz instability at Mars: Properties of plasma boundaries with a large density gradient |
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MATSUNO, Tetsuo |
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R003-P03 |
Study of Tide-Induced Electromagnetic Field Response in the Kikai Caldera Sea Area |
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MATSUO, Takuma |
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S001-10 |
Preliminary results of LODEWAVE Phase II |
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MATSUOKA, A. |
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S002-P05 |
EMIC waves during the May 2024 geomagnetic storm |
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MATSUOKA, Ayako |
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R005-09 |
Examination of the method to derive the electric current in the sporadic E layer |
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R005-P34 |
Measurements of the neutral and ionized atmospheres around Es by a sounding rocket: RIDE campaign |
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R005-P38 |
Analog circuit chip dedicated to the Fundamental Mode Orthogonal Fluxgate Magnetometers |
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R006-03 |
Abrupt changes in Pc1 pulsations observed at the cusp: A event on 5 November 2023 |
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R006-04 |
Relationship Between Plasmapause Position and Solar Wind Electric Field Ey |
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R006-06 |
Origins of chorus waves in the inner magnetosphere |
表示 |
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R006-07 |
Construction of empirical wave power model of chorus waves based on the Arase observation |
表示 |
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R006-08 |
Analysis of space distribution and propagation properties of low frequency chorus observed by Arase |
表示 |
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R006-09 |
Evaluation of a direction finding method using NWC transmitter signals observed by the Arase |
表示 |
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R006-10 |
A statistical study on energy sources of mid-latitude lower hybrid waves observed by Arase |
表示 |
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R006-13 |
Magnetospheric source of auroral emission at subauroral latitudes using Arase and ground imagers |
表示 |
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R006-18 |
The source altitude distribution and heating property of electron conics |
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R006-20 |
Investigation of Omega Band Auroras: Ground and Magnetospheric Conjugate Observations |
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R006-24 |
Investigation and development of FPGA coding for digital-type fluxgate magnetometer |
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R006-29 |
Energy and pitch angle dispersed ion injections from the magnetotail during storms observed by Arase |
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R006-P12 |
Statistical survey of Ion 3D velocity distribution functions observed by the Arase satellite |
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R006-P14 |
Spatial distribution of low-energy (<1 keV) O+ plasma in the inner magnetosphere |
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R006-P16 |
Energy-spectral evolution of ring current ions of ionospheric origin during intense magnetic storms |
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R006-P17 |
Does isotropic proton precipitation correspond to isotropic distribution of magnetospheric protons? |
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R006-P21 |
Investigation of the relationship between satellite surface charging and chorus waves |
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R006-P26 |
Statistical Survey of Dayside Energetic Electron Precipitation in the Inner Magnetosphere |
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R006-P28 |
Repetition period of REP and chorus observed during the conjunction event of ISS/CALET and Arase |
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