High Frequency Analyzer (HFA) of Plasma Wave Experiment (PWE) onboard the Arase spacecraft
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- Material Type
- 記事
- Author/Editor
- Atsushi KumamotoFuminori TsuchiyaYoshiya Kasahara
- Publication, Distribution, etc.
- Publication Date
- 2018-05-16
- Publication Date (W3CDTF)
- 2018-05-16
- Periodical title
- EPS : Earth, Planets and Space
- No. or year of volume/issue
- 70(82)
- Volume
- 70(82)
- ISSN (Periodical Title)
- 1880-5981
- ISSN-L (Periodical Title)
- 1343-8832
- Text Language Code
- eng
- DOI
- 10.1186/s40623-018-0854-0
- Persistent ID (NDL)
- info:ndljp/pid/11125850
- 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)
- 2018-08-10T20:26:03+09:00
- Date Captured (W3CDTF)
- 2018-08-10
- 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 High Frequency Analyzer (HFA) is a subsystem of the Plasma Wave Experiment onboard the Arase (ERG) spacecraft. The main purposes of the HFA include (1) determining the electron number density around the spacecraft from observations of upper hybrid resonance (UHR) waves, (2) measuring the electromagnetic field component of whistler-mode chorus in a frequency range above 20 kHz, and (3) observing radio and plasma waves excited in the storm-time magnetosphere. Two components of AC electric fields detected by Wire Probe Antenna and one component of AC magnetic fields detected by Magnetic Search Coils are fed to the HFA. By applying analog and digital signal processing in the HFA, the spectrograms of two electric fields (EE mode) or one electric field and one magnetic field (EB mode) in a frequency range from 10 kHz to 10 MHz are obtained at an interval of 8 s. For the observation of plasmapause, the HFA can also be operated in PP (plasmapause) mode, in which spectrograms of one electric field component below 1 MHz are obtained at an interval of 1 s. In the initial HFA operations from January to July, 2017, the following results are obtained: (1) UHR waves, auroral kilometric radiation (AKR), whistler-mode chorus, electrostatic electron cyclotron harmonic waves, and nonthermal terrestrial continuum radiation were observed by the HFA in geomagnetically quiet and disturbed conditions. (2) In the test operations of the polarization observations on June 10, 2017, the fundamental R-X and L-O mode AKR and the second-harmonic R-X mode AKR from different sources in the northern polar region were observed. (3) The semiautomatic UHR frequency identification by the computer and a human operator was applied to the HFA spectrograms. In the identification by the computer, we used an algorithm for narrowing down the candidates of UHR frequency by checking intensity and bandwidth. Then, the identified UHR frequency by the computer was checked and corrected if needed by the human operator. Electron number density derived from the determined UHR frequency will be useful for the investigation of the storm-time evolution of the plasmasphere and topside ionosphere.
- DOI
- 10.1186/s40623-018-0854-0
- 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
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- Related Material (URI)
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- 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 StationsDeep Learning Model Size Performance Evaluation for Lightning Whistler Detection on Arase Satellite DatasetTransient ionization of the mesosphere during auroral breakup: Arase satellite and ground-based conjugate observations at Syowa StationRelationship between the locations of the midlatitude trough and plasmapause using GNSS-TEC and Arase satellite observation dataData 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 eruptionOnboard software of Plasma Wave Experiment aboard Arase: instrument management and signal processing of Waveform Capture/Onboard Frequency AnalyzerVisualization of rapid electron precipitation via chorus element wave–particle interactionsPlasma 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 EquatorInvestigation of Small‐Scale Electron Density Irregularities Observed by the Arase and Van Allen Probes Satellites Inside and Outside the PlasmasphereThe 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 THEMISCollaborative 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 Distributions of Auroral Kilometric Radiation in Earth's Northern and Southern Hemispheres Observed by the Arase SatellitePropagation Mechanism of Medium Wave Broadcasting Waves Observed by the Arase Satellite: Hectometric Line SpectraPlasmasphere Control of ULF Wave Distribution at Different Geomagnetic ConditionsTemporal 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 2017Data‐Driven Simulation of Rapid Flux Enhancement of Energetic Electrons With an Upper‐Band Whistler BurstRelation of the Plasmapause to the Midlatitude Ionospheric Trough, the Sub‐Auroral Temperature Enhancement and the Distribution of Small‐Scale Field Aligned Currents as Observed in the Magnetosphere by THEMIS, RBSP, and Arase, and in the Topside Ionosphere by SwarmLocalization of Sources of Two Types of Continuum RadiationUsing Van Allen Probes and Arase Observations to Develop an Empirical Plasma Density Model in the Inner ZoneDensity Depletions Associated With Enhancements of Electron Cyclotron Harmonic Emissions: An ERG ObservationStrong Diffusion of Energetic Electrons by Equatorial Chorus Waves in the Midnight‐to‐Dawn SectorMultiple time-scale beats in aurora: precise orchestration via magnetospheric chorus wavesAn 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 SubstormA Concise Empirical Formula for the Field‐Aligned Distribution of Auroral Kilometeric Radiation Based on Arase Satellite and Van Allen ProbesObservation 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 2017Direct 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 densityChanneling of Auroral Kilometric Radiation During Geomagnetic DisturbancesCharacteristic E-Region Plasma Signature of Magnetospheric Wave-Particle InteractionsSpatial Distribution of Fine‐Structured and Unstructured EMIC Waves Observed by the Arase SatelliteArase 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 SatelliteDirect Antenna Impedance Measurement for Quantitative AC Electric Field Measurement by AraseCross-Energy Couplings from Magnetosonic Waves to Electromagnetic Ion Cyclotron Waves through Cold Ion Heating inside the PlasmasphereLatitudinal dependence of ground VLF transmitter wave power in the inner magnetosphereA Proposal for Modification of Plasmaspheric Electron Density Profiles Using Characteristics of Lightning WhistlersAlfvén velocity sudden increase as an indicator of the plasmapauseNew 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 ImagersSatellite observations and modeling of the plasmapause structure and dynamicsConjugate 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 ElementsComprehensive Observations of Substorm‐Enhanced Plasmaspheric Hiss Generation, Propagation, and DissipationAutomatic Electron Density Determination by Using a Convolutional Neural NetworkExploration 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) Plasma Wave Experiment (PWE) High Frequency Analyzer (HFA) Level-2 spectrum dataWire Probe Antenna (WPT) and Electric Field Detector (EFD) of Plasma Wave Experiment (PWE) aboard the Arase satellite : specifications and initial evaluation resultsPlasma frequency demand for mode conversion processes from slow Z-mode to LO-mode waves in an inhomogeneous plasmaThe ERG Science CenterOxygen torus and its coincidence with EMIC wave in the deep inner magnetosphere : Van Allen Probe B and Arase observationsGeospace exploration project ERGSpace-to-space very low frequency radio transmission in the magnetosphere using the DSX and Arase satellites
- References
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- 国立情報学研究所 : CiNii Research
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- Bibliographic ID (NDL)
- 11125850
- NAID
- 120006502577