Software-type Wave–Particle Interaction Analyzer on board the Arase satellite

• Material Type: 記事
• Title: Software-type Wave–Particle Interaction Analyzer on board the Arase satellite
• Author/Editor: Yuto Katoh; Hirotsugu Kojima; Mitsuru Hikishima
• Publication, Distribution, etc.: 日本 : Springer Nature
• Publication Date: 2018-01-08
• Publication Date (W3CDTF): 2018-01-08
• Periodical title: EPS : Earth, Planets and Space
• No. or year of volume/issue: 70(4)
• Volume: 70(4)
• ISSN (Periodical Title): 1880-5981
• ISSN-L (Periodical Title): 1343-8832
• Text Language Code: eng
• DOI: 10.1186/s40623-017-0771-7; https://doi.org/10.1186/s40623-017-0771-7
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• Date Accepted (W3CDTF): 2018-04-12T16:47:48+09:00
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• Summary, etc.: We describe the principles of the Wave–Particle Interaction Analyzer (WPIA) and the implementation of the Software-type WPIA (S-WPIA) on the Arase satellite. The WPIA is a new type of instrument for the direct and quantitative measurement of wave–particle interactions. The S-WPIA is installed on the Arase satellite as a software function running on the mission data processor. The S-WPIA on board the Arase satellite uses an electromagnetic field waveform that is measured by the waveform capture receiver of the plasma wave experiment (PWE), and the velocity vectors of electrons detected by the medium-energy particle experiment–electron analyzer (MEP-e), the high-energy electron experiment (HEP), and the extremely high-energy electron experiment (XEP). The prime objective of the S-WPIA is to measure the energy exchange between whistler-mode chorus emissions and energetic electrons in the inner magnetosphere. It is essential for the S-WPIA to synchronize instruments to a relative time accuracy better than the time period of the plasma wave oscillations. Since the typical frequency of chorus emissions in the inner magnetosphere is a few kHz, a relative time accuracy of better than 10 μs is required in order to measure the relative phase angle between the wave and velocity vectors. In the Arase satellite, a dedicated system has been developed to realize the time resolution required for inter-instrument communication. Here, both the time index distributed over all instruments through the satellite system and an S-WPIA clock signal are used, that are distributed from the PWE to the MEP-e, HEP, and XEP through a direct line, for the synchronization of instruments within a relative time accuracy of a few μs. We also estimate the number of particles required to obtain statistically significant results with the S-WPIA and the expected accumulation time by referring to the specifications of the MEP-e and assuming a count rate for each detector.
• DOI: 10.1186/s40623-017-0771-7; https://doi.org/10.1186/s40623-017-0771-7
• 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: Software-type Wave-Particle Interaction Analyzer on board the Arase satellite; https://cir.nii.ac.jp/crid/2120589364336569344
• Related Material (URI): http://hdl.handle.net/2433/234669; http://id.ndl.go.jp/digimeta/11067460; https://dl.ndl.go.jp/pid/11067460; http://link.springer.com/content/pdf/10.1186/s40623-017-0771-7.pdf; http://link.springer.com/article/10.1186/s40623-017-0771-7/fulltext.html
• Is Referenced By: The Plasma Wave Experiment (PWE) on board the Arase (ERG) satellite; https://cir.nii.ac.jp/crid/1050001338207686400; Magnetic Search Coil (MSC) of Plasma Wave Experiment (PWE) aboard the Arase (ERG) satellite; https://cir.nii.ac.jp/crid/1050001338207688576; Dependence of Generation of Whistler Mode Chorus Emissions on the Temperature Anisotropy and Density of Energetic Electrons in the Earth's Inner Magnetosphere; https://cir.nii.ac.jp/crid/1050012570393777152; High frequency analyzer (HFA) of plasma wave experiment (PWE) onboard the Arase spacecraft, Earth; https://cir.nii.ac.jp/crid/1050282813184324224; Theory, Modeling, and Integrated studies in the Arase (ERG) project; https://cir.nii.ac.jp/crid/1050564288161077632; Data processing in Software-type Wave–Particle Interaction Analyzer onboard the Arase satellite; https://cir.nii.ac.jp/crid/1050564288161139456; Onboard software of Plasma Wave Experiment aboard Arase: instrument management and signal processing of Waveform Capture/Onboard Frequency Analyzer; https://cir.nii.ac.jp/crid/1050845763137853440; Energy Transfer Between Hot Protons and Electromagnetic Ion Cyclotron Waves in Compressional Pc5 Ultra‐low Frequency Waves; https://cir.nii.ac.jp/crid/1050857669062676608; Space Radiation; https://cir.nii.ac.jp/crid/1360021389796891392; The Radio & Plasma Wave Investigation (RPWI) for the JUpiter ICy moons Explorer (JUICE); https://cir.nii.ac.jp/crid/1360306906067633664; A Calibration Method of Short‐Time Waveform Signals Passed Through Linear Time‐Invariant Systems: 1. Methodology and Simple Examples; https://cir.nii.ac.jp/crid/1360580232168582016; Anomalous Trapping of Low Pitch Angle Electrons by Coherent Whistler Mode Waves; https://cir.nii.ac.jp/crid/1361131418080036864; A Systematic Study in Characteristics of Lower Band Rising‐Tone Chorus Elements; https://cir.nii.ac.jp/crid/1361131418080147072; Plasma frequency demand for mode conversion processes from slow Z-mode to LO-mode waves in an inhomogeneous plasma; https://cir.nii.ac.jp/crid/2050025942143161856; The ERG Science Center; https://cir.nii.ac.jp/crid/2050307417106079872; High-energy electron experiments (HEP) aboard the ERG (Arase) satellite; https://cir.nii.ac.jp/crid/2050588892082787328; Design of a mission network system using SpaceWire for scientific payloads onboard the Arase spacecraft; https://cir.nii.ac.jp/crid/2050870367059496704; Medium-energy particle experiments : electron analyzer (MEP-e) for the exploration of energization and radiation in geospace (ERG) mission; https://cir.nii.ac.jp/crid/2051151842036207104; Geospace exploration project ERG; https://cir.nii.ac.jp/crid/2051151842036212992; The extremely high-energy electron experiment (XEP) onboard the Arase (ERG) satellite; https://cir.nii.ac.jp/crid/2051996266972566912
• References: Nonlinear mechanisms of lower-band and upper-band VLF chorus emissions in the inner magnetosphere; https://cir.nii.ac.jp/crid/1050001201692749824; Amplitude dependence of frequency sweep rates of whistler mode chorus emissions; https://cir.nii.ac.jp/crid/1050001335745167360; Significance of Wave-Particle Interaction Analyzer for direct measurements of nonlinear wave-particle interactions; https://cir.nii.ac.jp/crid/1050001335802556416; Electron hybrid code simulation of whistler-mode chorus generation with real parameters in the Earth's inner magnetosphere; https://cir.nii.ac.jp/crid/1050001335841204224; A new instrument for the study of wave-particle interactions in space: One-chip Wave-Particle Interaction Analyzer; https://cir.nii.ac.jp/crid/1360011142931396352; Computer simulation of chorus wave generation in the Earth's inner magnetosphere; https://cir.nii.ac.jp/crid/1360011142935387008; Relativistic turning acceleration of resonant electrons by coherent whistler mode waves in a dipole magnetic field; https://cir.nii.ac.jp/crid/1360011142939459456; Effect of the background magnetic field inhomogeneity on generation processes of whistler‐mode chorus and broadband hiss‐like emissions; https://cir.nii.ac.jp/crid/1360283689562348288; Method for direct detection of pitch angle scattering of energetic electrons caused by whistler mode chorus emissions; https://cir.nii.ac.jp/crid/1360285704780915968; Relativistic theory of wave‐particle resonant diffusion with application to electron acceleration in the magnetosphere; https://cir.nii.ac.jp/crid/1360292617907729920; Rebuilding process of the outer radiation belt during the 3 November 1993 magnetic storm: NOAA and Exos‐D observations; https://cir.nii.ac.jp/crid/1360292617913682432; Ion hole formation and nonlinear generation of electromagnetic ion cyclotron waves: THEMIS observations; https://cir.nii.ac.jp/crid/1360848654737999104; Theory and simulation of the generation of whistler‐mode chorus; https://cir.nii.ac.jp/crid/1360855567862120320; Ultra‐relativistic acceleration of electrons in planetary magnetospheres; https://cir.nii.ac.jp/crid/1360855571434724224; Acceleration of relativistic electrons due to resonant scattering by whistler mode waves generated by temperature anisotropy in the inner magnetosphere; https://cir.nii.ac.jp/crid/1361981468955048320; Langmuir wave growth and electron bunching: Results from a wave‐particle correlator; https://cir.nii.ac.jp/crid/1361981470380606848; Correlator measurements of megahertz wave‐particle interactions during electron beam operations on STS; https://cir.nii.ac.jp/crid/1361981470955406720; Phase sorting wave‐particle correlator; https://cir.nii.ac.jp/crid/1364233269329240448; Evaluation of waveform data processing in Wave-Particle Interaction Analyzer; https://cir.nii.ac.jp/crid/2050025942186664192; A simulation study of the propagation of whistler-mode chorus in the Earth’s inner magnetosphere; https://cir.nii.ac.jp/crid/2050307417163363072
• References (URI): https://cir.nii.ac.jp/crid/1370004236852853129; https://cir.nii.ac.jp/crid/1370567186806296070
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• Bibliographic ID (NDL): 11067460; http://id.ndl.go.jp/bib/11067460
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