Electron hybrid code simulation of whistler-mode chorus generation with real parameters in the Earth's inner magnetosphere
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DOI[10.1186/s40623-016-0568-0]to the data of the same series
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- Material Type
- 記事
- Author/Editor
- Yuto KatohYoshiharu Omura
- Publication, Distribution, etc.
- Publication Date
- 2016-11-25
- Publication Date (W3CDTF)
- 2016-11-25
- Periodical title
- EPS : Earth, Planets and Space
- No. or year of volume/issue
- 68(192)
- Volume
- 68(192)
- ISSN (Periodical Title)
- 1880-5981
- ISSN-L (Periodical Title)
- 1343-8832
- Text Language Code
- eng
- DOI
- 10.1186/s40623-016-0568-0
- Persistent ID (NDL)
- info:ndljp/pid/10267463
- 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)
- 2017-01-25T12:55:04+09:00
- Date Captured (W3CDTF)
- 2017-01-13
- 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/9963599
- 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.
- We carry out a self-consistent simulation of the generation process of whistler-mode chorus by a spatially one-dimensional electron hybrid code, by assuming the magnetic field inhomogeneity corresponding to L = 4 of the dipole field. Chorus emissions with rising tones are reproduced in the simulation result, while the frequency range, sweep rate, and the amplitude profiles in the spectra of the reproduced elements are consistently explained by the nonlinear wave growth theory. We compare the simulation results with the observation by the Cluster spacecraft (Santolik et al. in J Geophys Res 108:1278, 2003, doi:10.1029/2002JA009791; Santolik in Nonlinear Process Geophys 15:621–630, 2008) and reveal similarities of the spectral fine structure of reproduced chorus elements with the observation. On the other hand, there is no gap at half the gyrofrequency in the spectra of the reproduced chorus elements, which is evident in the observation. This difference implies that the mechanism of a gap at half the gyrofrequency is governed by the process that is not described by the spatially one-dimensional simulation treating purely parallel propagating electromagnetic waves.
- DOI
- 10.1186/s40623-016-0568-0
- Access Restrictions
- インターネット公開
- Rights (production)
- © The Author(s) 2016. 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 (URI)
- Is Referenced By
- The Plasma Wave Experiment (PWE) on board the Arase (ERG) satelliteDependence of Generation of Whistler Mode Chorus Emissions on the Temperature Anisotropy and Density of Energetic Electrons in the Earth's Inner MagnetosphereSoftware-type Wave–Particle Interaction Analyzer on board the Arase satelliteTheory, Modeling, and Integrated studies in the Arase (ERG) projectSpace RadiationFine Structure of Chorus Wave Packets: Comparison Between Observations and Wave Generation ModelsMeasurability of the Nonlinear Response of Electron Distribution Function to Chorus Emissions in the Earth's Radiation BeltAdvanced numerical techniques for time integration of relativistic equations of motion for charged particlesDiffuse and Pulsating AuroraPSTEP : project for solar–terrestrial environment predictionNonlinear wave growth theory of whistler-mode chorus and hiss emissions in the magnetosphere
- References
- Nonlinear mechanisms of lower-band and upper-band VLF chorus emissions in the inner magnetosphereAmplitude dependence of frequency sweep rates of whistler mode chorus emissionsSignificance of Wave-Particle Interaction Analyzer for direct measurements of nonlinear wave-particle interactionsTriggering process of whistler mode chorus emissions in the magnetosphereNonlinear wave growth theory of coherent hiss emissions in the plasmasphereComputer simulation of chorus wave generation in the Earth's inner magnetosphereSource regions of banded chorusA computational and theoretical investigation of nonlinear wave‐particle interactions in oblique whistlersEffect of the background magnetic field inhomogeneity on generation processes of whistler‐mode chorus and broadband hiss‐like emissionsThe Energization and Radiation in Geospace (ERG) ProjectScattering by chorus waves as the dominant cause of diffuse auroral precipitationGeotail observation of upper band and lower band chorus elements in the outer magnetosphereNonlinear interaction of energetic electrons with large amplitude chorusGeneration Processes of Whistler Mode Chorus Emissions: Current Status of Nonlinear Wave Growth TheoryTheory and simulation of the generation of whistler‐mode chorusA study of generation mechanism of VLF triggered emission by self‐consistent particle codeSpatio‐temporal structure of storm‐time chorusComparison of pitch angle diffusion by turbulent and monochromatic whistler wavesEffects of cold electron number density variation on whistler-mode wave growthNew results of investigations of whistler-mode chorus emissionsAcceleration of relativistic electrons due to resonant scattering by whistler mode waves generated by temperature anisotropy in the inner magnetosphereObservations of the relationship between frequency sweep rates of chorus wave packets and plasma densityFine structure of large‐amplitude chorus wave packetsA Numerical Study on the Resonant Scattering Process of Relativistic Electrons Via Whistler-Mode Waves in the Outer Radiation BeltPitch angle transport of electrons due to cyclotron interactions with the coherent chorus subelementsNumerical simulation of resonant scattering of energetic electrons in the outer radiation beltFull particle simulation of whistler‐mode rising chorus emissions in the magnetosphereEvaluation of waveform data processing in Wave-Particle Interaction AnalyzerA simulation study of the propagation of whistler-mode chorus in the Earth’s inner magnetosphere
- Data Provider (Database)
- 国立情報学研究所 : CiNii Research
- Original Data Provider (Database)
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- NAID
- 120005997860