The ARASE (ERG) magnetic field investigation
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DOI[10.1186/s40623-018-0800-1]to the data of the same series
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- Material Type
- 記事
- Author/Editor
- Ayako MatsuokaMariko TeramotoReiko Nomura
- Publication, Distribution, etc.
- Publication Date
- 2018-03-14
- Publication Date (W3CDTF)
- 2018-03-14
- Periodical title
- EPS : Earth, Planets and Space
- No. or year of volume/issue
- 70(43)
- Volume
- 70(43)
- ISSN (Periodical Title)
- 1880-5981
- ISSN-L (Periodical Title)
- 1343-8832
- Text Language Code
- eng
- DOI
- 10.1186/s40623-018-0800-1
- Persistent ID (NDL)
- info:ndljp/pid/11067500
- Collection
- Collection (Materials For Handicapped People:1)
- Collection (particular)
- 国立国会図書館デジタルコレクション > 電子書籍・電子雑誌 > その他
- Acquisition Basis
- オンライン資料収集制度
- Date Accepted (W3CDTF)
- 2018-04-12T16:47:48+09:00
- Date Captured (W3CDTF)
- 2018-04-12
- Format (IMT)
- application/pdf
- Access Restrictions
- 国立国会図書館内限定公開
- Service for the Digitized Contents Transmission Service
- 図書館・個人送信対象外
- Availability of remote photoduplication service
- 可
- Periodical Title (URI)
- Periodical Title (Persistent ID (NDL))
- info:ndljp/pid/11067456
- Data Provider (Database)
- 国立国会図書館 : 国立国会図書館デジタルコレクション
- Summary, etc.
- The fluxgate magnetometer for the Arase (ERG) spacecraft mission was built to investigate particle acceleration processes in the inner magnetosphere. Precise measurements of the field intensity and direction are essential in studying the motion of particles, the properties of waves interacting with the particles, and magnetic field variations induced by electric currents. By observing temporal field variations, we will more deeply understand magnetohydrodynamic and electromagnetic ion-cyclotron waves in the ultra-low-frequency range, which can cause production and loss of relativistic electrons and ring-current particles. The hardware and software designs of the Magnetic Field Experiment (MGF) were optimized to meet the requirements for studying these phenomena. The MGF makes measurements at a sampling rate of 256 vectors/s, and the data are averaged onboard to fit the telemetry budget. The magnetometer switches the dynamic range between ± 8000 and ± 60, 000 nT, depending on the local magnetic field intensity. The experiment is calibrated by preflight tests and through analysis of in-orbit data. MGF data are edited into files with a common data file format, archived on a data server, and made available to the science community. Magnetic field observation by the MGF will significantly improve our knowledge of the growth and decay of radiation belts and ring currents, as well as the dynamics of geospace storms.
- DOI
- 10.1186/s40623-018-0800-1
- Access Restrictions
- インターネット公開
- Rights (production)
- © The Author(s) 2018. This article is distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution, and reproduction in any medium, provided you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made.
- Related Material
- The ARASE (ERG) magnetic field investigation
- Related Material (URI)
- Is Referenced By
- The Plasma Wave Experiment (PWE) on board the Arase (ERG) satelliteMagnetic Search Coil (MSC) of Plasma Wave Experiment (PWE) aboard the Arase (ERG) satelliteDirect Comparison Between Magnetospheric Plasma Waves and Polar Mesosphere Winter Echoes in Both HemispheresPenetration of MeV electrons into the mesosphere accompanying pulsating auroraeMulti‐Event Analysis of Plasma and Field Variations in Source of Stable Auroral Red (SAR) Arcs in Inner Magnetosphere During Non‐Storm‐Time SubstormsField‐Aligned Low‐Energy O<sup>+</sup> Flux Enhancements in the Inner Magnetosphere Observed by AraseArase Observation of Simultaneous Electron Scatterings by Upper‐Band and Lower‐Band Chorus EmissionsMultipoint Measurement of Fine‐Structured EMIC Waves by Arase, Van Allen Probe A, and Ground StationsSignatures of auroral potential structure extending through the near-equatorial inner magnetosphereDeep Learning Model Size Performance Evaluation for Lightning Whistler Detection on Arase Satellite DatasetHigh frequency analyzer (HFA) of plasma wave experiment (PWE) onboard the Arase spacecraft, EarthMeridional Distribution of Middle‐Energy Protons and Pressure‐Driven Currents in the Nightside Inner Magnetosphere: Arase ObservationsActive auroral arc powered by accelerated electrons from very high altitudesDiscovery of proton hill in the phase space during interactions between ions and electromagnetic ion cyclotron wavesRelationship between the locations of the midlatitude trough and plasmapause using GNSS-TEC and Arase satellite observation dataFlux Enhancements of Field‐Aligned Low‐Energy O<sup>+</sup> Ion (FALEO) in the Inner Magnetosphere: A Possible Source of Warm Plasma Cloak and Oxygen TorusThe Mars system revealed by the Martian Moons eXploration missionData processing in Software-type Wave–Particle Interaction Analyzer onboard the Arase satelliteSpatial Extent of Quasiperiodic Emissions Simultaneously Observed by Arase and Van Allen Probes on 29 November 2018Magnetic Field and Energetic Particle Flux Oscillations and High‐Frequency Waves Deep in the Inner Magnetosphere During Substorm Dipolarization: ERG ObservationsA Statistical Study of the Solar Wind Dependence of Multi‐Harmonic Toroidal ULF Waves Observed by the Arase SatelliteGeneration of equatorial plasma bubble after the 2022 Tonga volcanic eruptionDetection of ultrafast electron energization by whistler-mode chorus waves in the magnetosphere of EarthOnboard software of Plasma Wave Experiment aboard Arase: instrument management and signal processing of Waveform Capture/Onboard Frequency AnalyzerPlasma Waves Causing Relativistic Electron Precipitation Events at International Space Station: Lessons From Conjunction Observations With Arase SatellitePlasma and field observations in the magnetospheric source region of a stable auroral red (SAR) arc by the Arase satellite on March 28, 2017Study of an Equatorward Detachment of Auroral Arc From the Oval Using Ground‐Space Observations and the BATS‐R‐US–CIMI ModelOff‐Equatorial Pi2 Pulsations Inside and Outside the Plasmapause Observed by the Arase SatelliteImpulsively Excited Nightside Ultralow Frequency Waves Simultaneously Observed on and off the Magnetic EquatorDrift‐Bounce Resonance Between Pc5 Pulsations and Ions at Multiple Energies in the Nightside Magnetosphere: Arase and MMS ObservationsInstantaneous Frequency Analysis on Nonlinear EMIC Emissions: Arase ObservationInvestigation of Small‐Scale Electron Density Irregularities Observed by the Arase and Van Allen Probes Satellites Inside and Outside the PlasmasphereRocket Observation of Sub‐Relativistic Electrons in the Quiet Dayside Auroral IonosphereThe Characteristics of EMIC Waves in the Magnetosphere Based on the Van Allen Probes and Arase ObservationsInter‐Calibrated Measurements of Intense Whistlers by Arase and Van Allen ProbesSimultaneous Observations of EMIC‐Induced Drifting Electron Holes (EDEHs) in the Earth's Radiation Belt by the Arase Satellite, Van Allen Probes, and THEMISRole of Ducting in Relativistic Electron Loss by Whistler‐Mode Wave ScatteringCollaborative Research Activities of the Arase and Van Allen ProbesMulti‐Event Analysis of Magnetosphere‐Ionosphere Coupling of Nighttime Medium‐Scale Traveling Ionospheric Disturbances From the Ground and the Arase SatelliteAsymmetric Development of Auroral Surges in the Northern and Southern HemispheresPlasmasphere Control of ULF Wave Distribution at Different Geomagnetic ConditionsGiant Pulsations Excited by a Steep Earthward Gradient of Proton Phase Space Density: Arase ObservationTemporal and Spatial Variations of Storm Time Midlatitude Ionospheric Trough Based on Global GNSS‐TEC and Arase Satellite ObservationsTemporal and Spatial Correspondence of Pc1/EMIC Waves and Relativistic Electron Precipitations Observed With Ground‐Based Multi‐Instruments on 27 March 2017Tracking the Region of High Correlation Between Pulsating Aurora and Chorus: Simultaneous Observations With Arase Satellite and Ground‐Based All‐Sky Imager in RussiaData‐Driven Simulation of Rapid Flux Enhancement of Energetic Electrons With an Upper‐Band Whistler BurstPitch‐Angle Scattering of Inner Magnetospheric Electrons Caused by ECH Waves Obtained With the Arase SatelliteFirst Direct Observations of Propagation of Discrete Chorus Elements From the Equatorial Source to Higher Latitudes, Using the Van Allen Probes and Arase SatellitesStatistical Study of Approaching Strong Diffusion of Low‐Energy Electrons by Chorus and ECH Waves Based on <i>In Situ</i> ObservationsAn event of extreme relativistic and ultra-relativistic electron enhancements following the arrival of consecutive corotating interaction regions: Coordinated observations by Van Allen Probes, Arase, THEMIS and Galileo satellitesUsing Van Allen Probes and Arase Observations to Develop an Empirical Plasma Density Model in the Inner ZoneA Triggering Process for Nonlinear EMIC Waves Driven by the Compression of the Dayside MagnetosphereGlobal Distribution of ULF Waves During Magnetic Storms: Comparison of Arase, Ground Observations, and BATSRUS + CRCM SimulationDensity Depletions Associated With Enhancements of Electron Cyclotron Harmonic Emissions: An ERG ObservationMagnetosphere‐Ionosphere Connection of Storm‐Time Region‐2 Field‐Aligned Current and Ring Current: Arase and AMPERE ObservationsResponse of the Ionosphere‐Plasmasphere Coupling to the September 2017 Storm: What Erodes the Plasmasphere so Severely?Strong Diffusion of Energetic Electrons by Equatorial Chorus Waves in the Midnight‐to‐Dawn SectorAn Ephemeral Red Arc Appeared at 68° MLat at a Pseudo Breakup During Geomagnetically Quiet ConditionsField‐Aligned Electron Density Distribution of the Inner Magnetosphere Inferred From Coordinated Observations of Arase and Van Allen ProbesRelative Contribution of ULF Waves and Whistler‐Mode Chorus to the Radiation Belt Variation During the May 2017 StormEvening Side EMIC Waves and Related Proton Precipitation Induced by a SubstormObservation of Source Plasma and Field Variations of a Substorm Brightening Aurora at <i>L</i> ∼ 6 by a Ground‐Based Camera and the Arase Satellite on 12 October 2017Mesospheric ionization during substorm growth phaseDirect Observations of Energetic Electron Scattering and Precipitation Due To Whistler‐Mode Waves in the Dayside High‐Density RegionsStatistical Study of EMIC Waves and Related Proton Distributions Observed by the Arase SatelliteCorrespondence of Pi2 Pulsations, Aurora Luminosity, and Plasma Flux Fluctuation Near a Substorm Brightening Aurora: Arase ObservationsInterhemispheric ionosphere-plasmasphere system shows a high sensitivity to the exospheric neutral hydrogen density: a caution of the global reference atmospheric model hydrogen densityOn the phase difference of ECH waves obtained from the interferometry observation by the Arase satelliteCharacteristic E-Region Plasma Signature of Magnetospheric Wave-Particle InteractionsSpatial Distribution of Fine‐Structured and Unstructured EMIC Waves Observed by the Arase SatelliteSignal and Noise Separation From Satellite Magnetic Field Data Through Independent Component Analysis: Prospect of Magnetic Measurements Without Boom and Noise Source InformationMeasurements of Magnetic Field Fluctuations for Plasma Wave Investigation by the Search Coil Magnetometers (SCM) Onboard Bepicolombo Mio (Mercury Magnetospheric Orbiter)Arase Observation of the Source Region of Auroral Arcs and Diffuse Auroras in the Inner MagnetosphereDetection of UHR Frequencies by a Convolutional Neural Network From Arase/PWE DataMultievent Study of Characteristics and Propagation of Naturally Occurring ELF/VLF Waves Using High‐Latitude Ground Observations and Conjunctions With the Arase SatelliteCross-Energy Couplings from Magnetosonic Waves to Electromagnetic Ion Cyclotron Waves through Cold Ion Heating inside the PlasmasphereComparative Study of Electric Currents and Energetic Particle Fluxes in a Solar Flare and Earth Magnetospheric SubstormA Proposal for Modification of Plasmaspheric Electron Density Profiles Using Characteristics of Lightning WhistlersAlfvén velocity sudden increase as an indicator of the plasmapauseDistribution of ULF Wave Power in Magnetic Latitude and Local Time Using THEMIS and Arase MeasurementsNew aspects of the upper atmospheric disturbances caused by the explosive eruption of the 2022 Hunga Tonga–Hunga Ha’apai volcanoAn Implication of Detecting the Internal Modulation in a Pulsating Aurora: A Conjugate Observation by the Arase Satellite and All‐Sky ImagersPolarization and Spatial Distribution Features of Pc4 and Pc5 Waves in the MagnetosphereConjugate Observations of Dayside and Nightside VLF Chorus and QP Emissions Between Arase (ERG) and Kannuslehto, FinlandA Systematic Study in Characteristics of Lower Band Rising‐Tone Chorus ElementsRemote Detection of Drift Resonance Between Energetic Electrons and Ultralow Frequency Waves: Multisatellite Coordinated Observation by Arase and Van Allen ProbesComprehensive Observations of Substorm‐Enhanced Plasmaspheric Hiss Generation, Propagation, and DissipationA Multi‐Instrument Approach to Determining the Source‐Region Extent of EEP‐Driving EMIC WavesAutomatic Electron Density Determination by Using a Convolutional Neural NetworkExploration of energization and Radiation in Geospace (ERG) Magnetic Field Experiment (MGF) Level-2 high-resolution (64/128/256 Hz) magnetic field dataExploration of energization and Radiation in Geospace (ERG) HEP Level-3 pitch angle sorted electron flux dataExploration of energization and Radiation in Geospace (ERG) MEP-i Level-3 3-D flux dataExploration of energization and Radiation in Geospace (ERG) LEPe Level-3 pitch angle distribution electron flux dataExploration of energization and Radiation in Geospace (ERG) Plasma Wave Experiment (PWE) High Frequency Analyzer (HFA) Level-3 electron density dataExploration of energization and Radiation in Geospace (ERG) MEP-e Level-3 pitch-angle sorted flux dataExploration of energization and Radiation in Geospace (ERG) Plasma Wave Experiment (PWE) Onboard Frequency Analyzer (OFA) Level-3 wave property dataExploration of energization and Radiation in Geospace (ERG) MEP-e Level-3 3-D flux dataExploration of energization and Radiation in Geospace (ERG) LEPe Level-3 pitch angle distribution data of electron flux based on fine channelsExploration of energization and Radiation in Geospace (ERG) MEP-i Level-3 pitch-angle sorted flux dataExploration of energization and Radiation in Geospace (ERG) Magnetic Field Experiment (MGF) Level-2 spin-averaged magnetic field dataIn situ observations of ions and magnetic field around Phobos : the mass spectrum analyzer (MSA) for the Martian Moons eXploration (MMX) missionThe ERG Science CenterERG observations of drift echoes during a unique period of the satellite missionOxygen torus and its coincidence with EMIC wave in the deep inner magnetosphere : Van Allen Probe B and Arase observationsGeospace exploration project ERGISEE_Wave : interactive plasma wave analysis tool
- References
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- 国立情報学研究所 : CiNii Research
- Original Data Provider (Database)
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- Bibliographic ID (NDL)
- 11067500
- NAID
- 120006537088