The Plasma Wave Experiment (PWE) on board the Arase (ERG) satellite

Abstract The Exploration of energization and Radiation in Geospace (ERG) project aims to study acceleration and loss mechanisms of relativistic electrons around the Earth. The Arase (ERG) satellite was launched on December 20, 2016, to explore in the heart of the Earth’s radiation belt. In the prese...

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Main Authors: Yoshiya Kasahara, Yasumasa Kasaba, Hirotsugu Kojima, Satoshi Yagitani, Keigo Ishisaka, Atsushi Kumamoto, Fuminori Tsuchiya, Mitsunori Ozaki, Shoya Matsuda, Tomohiko Imachi, Yoshizumi Miyoshi, Mitsuru Hikishima, Yuto Katoh, Mamoru Ota, Masafumi Shoji, Ayako Matsuoka, Iku Shinohara
Format: Article
Language:English
Published: SpringerOpen 2018-05-01
Series:Earth, Planets and Space
Subjects:
Online Access:http://link.springer.com/article/10.1186/s40623-018-0842-4
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author Yoshiya Kasahara
Yasumasa Kasaba
Hirotsugu Kojima
Satoshi Yagitani
Keigo Ishisaka
Atsushi Kumamoto
Fuminori Tsuchiya
Mitsunori Ozaki
Shoya Matsuda
Tomohiko Imachi
Yoshizumi Miyoshi
Mitsuru Hikishima
Yuto Katoh
Mamoru Ota
Masafumi Shoji
Ayako Matsuoka
Iku Shinohara
author_facet Yoshiya Kasahara
Yasumasa Kasaba
Hirotsugu Kojima
Satoshi Yagitani
Keigo Ishisaka
Atsushi Kumamoto
Fuminori Tsuchiya
Mitsunori Ozaki
Shoya Matsuda
Tomohiko Imachi
Yoshizumi Miyoshi
Mitsuru Hikishima
Yuto Katoh
Mamoru Ota
Masafumi Shoji
Ayako Matsuoka
Iku Shinohara
author_sort Yoshiya Kasahara
collection DOAJ
description Abstract The Exploration of energization and Radiation in Geospace (ERG) project aims to study acceleration and loss mechanisms of relativistic electrons around the Earth. The Arase (ERG) satellite was launched on December 20, 2016, to explore in the heart of the Earth’s radiation belt. In the present paper, we introduce the specifications of the Plasma Wave Experiment (PWE) on board the Arase satellite. In the inner magnetosphere, plasma waves, such as the whistler-mode chorus, electromagnetic ion cyclotron wave, and magnetosonic wave, are expected to interact with particles over a wide energy range and contribute to high-energy particle loss and/or acceleration processes. Thermal plasma density is another key parameter because it controls the dispersion relation of plasma waves, which affects wave–particle interaction conditions and wave propagation characteristics. The DC electric field also plays an important role in controlling the global dynamics of the inner magnetosphere. The PWE, which consists of an orthogonal electric field sensor (WPT; wire probe antenna), a triaxial magnetic sensor (MSC; magnetic search coil), and receivers named electric field detector (EFD), waveform capture and onboard frequency analyzer (WFC/OFA), and high-frequency analyzer (HFA), was developed to measure the DC electric field and plasma waves in the inner magnetosphere. Using these sensors and receivers, the PWE covers a wide frequency range from DC to 10 MHz for electric fields and from a few Hz to 100 kHz for magnetic fields. We produce continuous ELF/VLF/HF range wave spectra and ELF range waveforms for 24 h each day. We also produce spectral matrices as continuous data for wave direction finding. In addition, we intermittently produce two types of waveform burst data, “chorus burst” and “EMIC burst.” We also input raw waveform data into the software-type wave–particle interaction analyzer (S-WPIA), which derives direct correlation between waves and particles. Finally, we introduce our PWE observation strategy and provide some initial results.
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spelling doaj.art-fc00b0c6b86e43a5b5b609b9ebe961592022-12-21T18:52:05ZengSpringerOpenEarth, Planets and Space1880-59812018-05-0170112810.1186/s40623-018-0842-4The Plasma Wave Experiment (PWE) on board the Arase (ERG) satelliteYoshiya Kasahara0Yasumasa Kasaba1Hirotsugu Kojima2Satoshi Yagitani3Keigo Ishisaka4Atsushi Kumamoto5Fuminori Tsuchiya6Mitsunori Ozaki7Shoya Matsuda8Tomohiko Imachi9Yoshizumi Miyoshi10Mitsuru Hikishima11Yuto Katoh12Mamoru Ota13Masafumi Shoji14Ayako Matsuoka15Iku Shinohara16Graduate School of Natural Science and Technology, Kanazawa UniversityGraduate School of Science, Tohoku UniversityResearch Institute for Sustainable Humanosphere, Kyoto UniversityGraduate School of Natural Science and Technology, Kanazawa UniversityToyama Prefectural UniversityGraduate School of Science, Tohoku UniversityGraduate School of Science, Tohoku UniversityGraduate School of Natural Science and Technology, Kanazawa UniversityNagoya UniversityGraduate School of Natural Science and Technology, Kanazawa UniversityNagoya UniversityISAS, JAXAGraduate School of Science, Tohoku UniversityGraduate School of Natural Science and Technology, Kanazawa UniversityNagoya UniversityISAS, JAXAISAS, JAXAAbstract The Exploration of energization and Radiation in Geospace (ERG) project aims to study acceleration and loss mechanisms of relativistic electrons around the Earth. The Arase (ERG) satellite was launched on December 20, 2016, to explore in the heart of the Earth’s radiation belt. In the present paper, we introduce the specifications of the Plasma Wave Experiment (PWE) on board the Arase satellite. In the inner magnetosphere, plasma waves, such as the whistler-mode chorus, electromagnetic ion cyclotron wave, and magnetosonic wave, are expected to interact with particles over a wide energy range and contribute to high-energy particle loss and/or acceleration processes. Thermal plasma density is another key parameter because it controls the dispersion relation of plasma waves, which affects wave–particle interaction conditions and wave propagation characteristics. The DC electric field also plays an important role in controlling the global dynamics of the inner magnetosphere. The PWE, which consists of an orthogonal electric field sensor (WPT; wire probe antenna), a triaxial magnetic sensor (MSC; magnetic search coil), and receivers named electric field detector (EFD), waveform capture and onboard frequency analyzer (WFC/OFA), and high-frequency analyzer (HFA), was developed to measure the DC electric field and plasma waves in the inner magnetosphere. Using these sensors and receivers, the PWE covers a wide frequency range from DC to 10 MHz for electric fields and from a few Hz to 100 kHz for magnetic fields. We produce continuous ELF/VLF/HF range wave spectra and ELF range waveforms for 24 h each day. We also produce spectral matrices as continuous data for wave direction finding. In addition, we intermittently produce two types of waveform burst data, “chorus burst” and “EMIC burst.” We also input raw waveform data into the software-type wave–particle interaction analyzer (S-WPIA), which derives direct correlation between waves and particles. Finally, we introduce our PWE observation strategy and provide some initial results.http://link.springer.com/article/10.1186/s40623-018-0842-4Plasma waveRadiation beltGeospaceInner magnetosphereChorus
spellingShingle Yoshiya Kasahara
Yasumasa Kasaba
Hirotsugu Kojima
Satoshi Yagitani
Keigo Ishisaka
Atsushi Kumamoto
Fuminori Tsuchiya
Mitsunori Ozaki
Shoya Matsuda
Tomohiko Imachi
Yoshizumi Miyoshi
Mitsuru Hikishima
Yuto Katoh
Mamoru Ota
Masafumi Shoji
Ayako Matsuoka
Iku Shinohara
The Plasma Wave Experiment (PWE) on board the Arase (ERG) satellite
Earth, Planets and Space
Plasma wave
Radiation belt
Geospace
Inner magnetosphere
Chorus
title The Plasma Wave Experiment (PWE) on board the Arase (ERG) satellite
title_full The Plasma Wave Experiment (PWE) on board the Arase (ERG) satellite
title_fullStr The Plasma Wave Experiment (PWE) on board the Arase (ERG) satellite
title_full_unstemmed The Plasma Wave Experiment (PWE) on board the Arase (ERG) satellite
title_short The Plasma Wave Experiment (PWE) on board the Arase (ERG) satellite
title_sort plasma wave experiment pwe on board the arase erg satellite
topic Plasma wave
Radiation belt
Geospace
Inner magnetosphere
Chorus
url http://link.springer.com/article/10.1186/s40623-018-0842-4
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