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 |
YABUMOTO, Shoki |
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R006-22 |
Development of a small-size and wide-FOV electron analyzer for CubeSat to measure auroral electrons |
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YAGI, Yuto |
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R004-P02 |
Influence of Skin Effect on Mercury's Magnetic Field: A Dynamo Simulation Approach |
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YAGITANI, Satoshi |
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R008-07 |
Pitch angle diffusion coefficient of relativistic electrons using a matrix calculation in plasmas |
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R009-02 |
Whistler-driven electron precipitation by asymmetric loss cone in Mercury's miniature magnetosphere |
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R009-06 |
HF of RPWI aboard JUICE: Lunar-Earth flyby in Aug 2024 and beyond |
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YAMADA, Yuto |
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R009-02 |
Whistler-driven electron precipitation by asymmetric loss cone in Mercury's miniature magnetosphere |
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YAMAGATA, Mariko |
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R004-P13 |
Fundamental research on the magnetic properties of sediments from the Thu Bon River in Vietnam |
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YAMAGUCHI, Satoru |
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R003-P05 |
Analysis of Long-Period MT Data using LEMI recording equipment in the Kii Peninsula |
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YAMAKAWA, Tomotsugu |
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R006-05 |
Magnetic storms of a weakly magnetized planet based on global inner magnetospheric simulations |
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R006-P15 |
Variation of ring current ions during magnetic storms based on the GEMSIS M-I coupled model |
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YAMAMOTO, Atsushi |
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R005-P31 |
Observations of sporadic E using marine traffic radio waves |
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YAMAMOTO, K. |
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S002-P05 |
EMIC waves during the May 2024 geomagnetic storm |
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YAMAMOTO, Kazuaki |
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R010-03 |
Solar cycle and extreme space weather events in the Medieval Solar Activity Maximum |
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YAMAMOTO, Kazuhiro |
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R006-05 |
Magnetic storms of a weakly magnetized planet based on global inner magnetospheric simulations |
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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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R006-10 |
A statistical study on energy sources of mid-latitude lower hybrid waves observed by Arase |
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R006-13 |
Magnetospheric source of auroral emission at subauroral latitudes using Arase and ground imagers |
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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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R006-29 |
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-P15 |
Variation of ring current ions during magnetic storms based on the GEMSIS M-I coupled model |
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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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R006-P29 |
Characteristics of MeV Electron Precipitation Spectra Observed by CALET/CHD |
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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-P38 |
Accuracy evaluation of near-earth geomagnetic data measured by MGF on board the Arase Satellite |
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R011-08 |
Development of BepiColombo/MMO data archive |
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S002-06 |
Ring current development observed by the Arase satellite during the May 2024 super geomagnetic storm |
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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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YAMAMOTO, Kosuke |
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R006-P40 |
Development of the miniaturized and low-power plasma wave receiver for use on CubeSat |
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YAMAMOTO, Mamoru |
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R005-14 |
MAGE model analysis of electric field penetration with a strong substorm on October 24, 2003 |
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R005-15 |
North?south asymmetry during decay phase of midlatitude plasma bubbles during a storm in March 2013 |
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R005-P15 |
STARLINK satellites and upper atmospheric variations |
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R005-P22 |
Improvement of Tomography and the Launch of Near-Real-Time Services |
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R011-P08 |
Multimodal Fusion for Spatiotemporal Predictive Learning of Ionospheric Total Electron Content |
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S002-19 |
Impact of intense ionospheric disturbances in 2023-2024 on aeronautical GNSS applications |
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S002-P10 |
TEC Enhancement and Irregularities Over Japan During a Magnetic Storm on May 2024 |
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YAMAMOTO, Mare |
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R003-P06 |
AMT exploration of Zao Volcano, NE Japan |
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YAMAMOTO, Yojiro |
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R003-P03 |
Study of Tide-Induced Electromagnetic Field Response in the Kikai Caldera Sea Area |
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YAMAMOTO, Yuhji |
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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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R004-05 |
Rock magnetic properties of the lava samples from western Iceland |
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R004-P06 |
Rock magnetism of lava flows in eastern Iceland |
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R004-P07 |
Paleointensity and rock magnetic analyses of lavas on Nishinoshima, Ogasawara Islands |
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R004-P13 |
Fundamental research on the magnetic properties of sediments from the Thu Bon River in Vietnam |
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YAMASAKI, Noriko |
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S002-05 |
XRISM/Xtend observation of the intense space storm in 2024 May |
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YAMAYA, Yusuke |
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R003-04 |
MT explorations of the three-dimensional electrical resistivity structure under the Nikko-Ashio area |
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YAMAZAKI, Ashita |
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R009-P05 |
Optical Performance Evaluation of Hydrogen Imager onboard the Comet Interceptor Mission |
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YAMAZAKI, Atsushi |
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R006-P45 |
Status of GEO-X mission |
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R009-08 |
Current status of LAPYUTA mission |
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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-P09 |
Plasma parameters at Europa's orbit estimated from the Hisaki observation |
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R009-P19 |
Test observations of natural lights by the mid-IR heterodyne spectrometer with the fiber coupler |
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R009-P21 |
LAPYUTA mission: instrument overview and technical developments |
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YAMAZAKI, Kenichi |
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R003-02 |
Continuous EM Field monitoring to Detect Changes in Subsurface Resistivity Structure |
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YAMAZAKI, Ryo |
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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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YAMAZAKI, Takashi |
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R006-P36 |
Spatial Distribution of Magnetosonic Waves Observed by the Arase Satellite |
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YAMAZAKI, Tomoya |
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R003-02 |
Continuous EM Field monitoring to Detect Changes in Subsurface Resistivity Structure |
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YAMAZAKI, Toshitsugu |
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R004-P03 |
Long-term geodynamo cycle revealed from relationship between reversal frequency and dipole strength |
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R004-P04 |
Miocene relative paleointensity of deep-sea sediments at IODP Site U1490 |
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YANAGISAWA, Kyutaro |
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R006-P27 |
Observation of auroral emission altitude during relativistic electron precipitation events |
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YANG, Jingxuan |
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R006-P33 |
Chorus wave activity at marginal condition of electron temperature anisotropy instability |
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YASHIMA, Kazuki |
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R006-15 |
2D distribution of the low-energy electron precipitation from auroral images and its characteristics |
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YASHIRO, Hisashi |
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R009-19 |
Non-hydrostatic global simulations of the Venus atmosphere: effects of vertical convection |
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YASHIRO, Seiji |
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S002-P01 |
Interaction among multiple CMEs to result in May 2024 Superstorm |
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YASUDA, Rikuto |
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R009-06 |
HF of RPWI aboard JUICE: Lunar-Earth flyby in Aug 2024 and beyond |
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YIN, Zhenxing |
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R008-P07 |
Parametric dependence of nonlinear wave growth of whistler-mode hiss emissions |
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YOKOTA, Kumiko |
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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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YOKOTA, Shoichiro |
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R005-P37 |
Development of a Neutral Mass Spectrometer NMS for RIDE Rocket Campaign |
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R006-06 |
Origins of chorus waves in the inner magnetosphere |
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R006-13 |
Magnetospheric source of auroral emission at subauroral latitudes using Arase and ground imagers |
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R006-20 |
Investigation of Omega Band Auroras: Ground and Magnetospheric Conjugate Observations |
表示 |
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R006-29 |
Energy and pitch angle dispersed ion injections from the magnetotail during storms observed by Arase |
表示 |
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R006-P12 |
Statistical survey of Ion 3D velocity distribution functions observed by the Arase satellite |
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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-P26 |
Statistical Survey of Dayside Energetic Electron Precipitation in the Inner Magnetosphere |
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R006-P33 |
Chorus wave activity at marginal condition of electron temperature anisotropy instability |
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R006-P41 |
Geometry design of orbit deflection mechanisms for field-of-view sweeping in space plasma analyzers. |
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R006-P42 |
Development of a Multifunctional ASIC for Plasma Particle Detectors on board Satellites |
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R009-03 |
Analysis of the lunar surface potential distribution based on a model and Kaguya observations |
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R009-04 |
Solar wind interaction with multiple lunar magnetic anomalies: Kaguya low-altitude observations |
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R009-P02 |
Performance of the Engineering Model of TRITON for LUPEX |
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R009-P03 |
A search for magnetic reconnection signatures on lunar crustal magnetic fields |
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R009-P04 |
Mass analysis of low-energy ions originating from the lunar surface and exosphere |
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R009-P06 |
Engineering model of the ion mass spectrometer for the Comet Interceptor mission |
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R009-P22 |
Calibration test of an ion energy mass spectrum analyzer onboard the MMX spacecraft |
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S002-06 |
Ring current development observed by the Arase satellite during the May 2024 super geomagnetic storm |
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S002-07 |
Arase satellite observations of the radiation belts for the May 2024 geospace storm |
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S002-P04 |
Particle acceleration upon the SSC of May 2024 storm |
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YOKOYAMA, Tatsuhiro |
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R005-P33 |
prediction of sporadic E layer by machine learning |
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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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R011-P08 |
Multimodal Fusion for Spatiotemporal Predictive Learning of Ionospheric Total Electron Content |
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S002-P10 |
TEC Enhancement and Irregularities Over Japan During a Magnetic Storm on May 2024 |
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YOKOYAMA, Yoshihiro |
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R005-20 |
A short period Pc3 pulsation possibly caused by a Lamb wave and plasmaspheric cavity resonance |
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