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 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. Ausführliche Beschreibung

Gespeichert in:

Autor*in:	Kasahara, Yoshiya [verfasserIn] Kasaba, Yasumasa Kojima, Hirotsugu Yagitani, Satoshi Ishisaka, Keigo Kumamoto, Atsushi Tsuchiya, Fuminori Ozaki, Mitsunori Matsuda, Shoya Imachi, Tomohiko Miyoshi, Yoshizumi Hikishima, Mitsuru Katoh, Yuto Ota, Mamoru Shoji, Masafumi Matsuoka, Ayako Shinohara, Iku

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2018

Schlagwörter:	Plasma wave Radiation belt Geospace Inner magnetosphere Chorus

Anmerkung:	© The Author(s) 2018

Übergeordnetes Werk:	Enthalten in: Earth, planets and space - Heidelberg : Springer, 1998, 70(2018), 1 vom: 21. Mai
Übergeordnetes Werk:	volume:70 ; year:2018 ; number:1 ; day:21 ; month:05

Links:	Volltext

DOI / URN:	10.1186/s40623-018-0842-4

Katalog-ID:	SPR036929468

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allfields	10.1186/s40623-018-0842-4 doi (DE-627)SPR036929468 (SPR)s40623-018-0842-4-e DE-627 ger DE-627 rakwb eng Kasahara, Yoshiya verfasserin (orcid)0000-0002-9304-8235 aut The Plasma Wave Experiment (PWE) on board the Arase (ERG) satellite 2018 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2018 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. Plasma wave (dpeaa)DE-He213 Radiation belt (dpeaa)DE-He213 Geospace (dpeaa)DE-He213 Inner magnetosphere (dpeaa)DE-He213 Chorus (dpeaa)DE-He213 Kasaba, Yasumasa aut Kojima, Hirotsugu aut Yagitani, Satoshi aut Ishisaka, Keigo aut Kumamoto, Atsushi aut Tsuchiya, Fuminori aut Ozaki, Mitsunori aut Matsuda, Shoya aut Imachi, Tomohiko aut Miyoshi, Yoshizumi aut Hikishima, Mitsuru aut Katoh, Yuto aut Ota, Mamoru aut Shoji, Masafumi aut Matsuoka, Ayako aut Shinohara, Iku aut Enthalten in Earth, planets and space Heidelberg : Springer, 1998 70(2018), 1 vom: 21. Mai (DE-627)353898597 (DE-600)2087663-4 1880-5981 nnns volume:70 year:2018 number:1 day:21 month:05 https://dx.doi.org/10.1186/s40623-018-0842-4 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 70 2018 1 21 05
spelling	10.1186/s40623-018-0842-4 doi (DE-627)SPR036929468 (SPR)s40623-018-0842-4-e DE-627 ger DE-627 rakwb eng Kasahara, Yoshiya verfasserin (orcid)0000-0002-9304-8235 aut The Plasma Wave Experiment (PWE) on board the Arase (ERG) satellite 2018 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2018 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. Plasma wave (dpeaa)DE-He213 Radiation belt (dpeaa)DE-He213 Geospace (dpeaa)DE-He213 Inner magnetosphere (dpeaa)DE-He213 Chorus (dpeaa)DE-He213 Kasaba, Yasumasa aut Kojima, Hirotsugu aut Yagitani, Satoshi aut Ishisaka, Keigo aut Kumamoto, Atsushi aut Tsuchiya, Fuminori aut Ozaki, Mitsunori aut Matsuda, Shoya aut Imachi, Tomohiko aut Miyoshi, Yoshizumi aut Hikishima, Mitsuru aut Katoh, Yuto aut Ota, Mamoru aut Shoji, Masafumi aut Matsuoka, Ayako aut Shinohara, Iku aut Enthalten in Earth, planets and space Heidelberg : Springer, 1998 70(2018), 1 vom: 21. Mai (DE-627)353898597 (DE-600)2087663-4 1880-5981 nnns volume:70 year:2018 number:1 day:21 month:05 https://dx.doi.org/10.1186/s40623-018-0842-4 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 70 2018 1 21 05
allfields_unstemmed	10.1186/s40623-018-0842-4 doi (DE-627)SPR036929468 (SPR)s40623-018-0842-4-e DE-627 ger DE-627 rakwb eng Kasahara, Yoshiya verfasserin (orcid)0000-0002-9304-8235 aut The Plasma Wave Experiment (PWE) on board the Arase (ERG) satellite 2018 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2018 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. Plasma wave (dpeaa)DE-He213 Radiation belt (dpeaa)DE-He213 Geospace (dpeaa)DE-He213 Inner magnetosphere (dpeaa)DE-He213 Chorus (dpeaa)DE-He213 Kasaba, Yasumasa aut Kojima, Hirotsugu aut Yagitani, Satoshi aut Ishisaka, Keigo aut Kumamoto, Atsushi aut Tsuchiya, Fuminori aut Ozaki, Mitsunori aut Matsuda, Shoya aut Imachi, Tomohiko aut Miyoshi, Yoshizumi aut Hikishima, Mitsuru aut Katoh, Yuto aut Ota, Mamoru aut Shoji, Masafumi aut Matsuoka, Ayako aut Shinohara, Iku aut Enthalten in Earth, planets and space Heidelberg : Springer, 1998 70(2018), 1 vom: 21. Mai (DE-627)353898597 (DE-600)2087663-4 1880-5981 nnns volume:70 year:2018 number:1 day:21 month:05 https://dx.doi.org/10.1186/s40623-018-0842-4 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 70 2018 1 21 05
allfieldsGer	10.1186/s40623-018-0842-4 doi (DE-627)SPR036929468 (SPR)s40623-018-0842-4-e DE-627 ger DE-627 rakwb eng Kasahara, Yoshiya verfasserin (orcid)0000-0002-9304-8235 aut The Plasma Wave Experiment (PWE) on board the Arase (ERG) satellite 2018 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2018 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. Plasma wave (dpeaa)DE-He213 Radiation belt (dpeaa)DE-He213 Geospace (dpeaa)DE-He213 Inner magnetosphere (dpeaa)DE-He213 Chorus (dpeaa)DE-He213 Kasaba, Yasumasa aut Kojima, Hirotsugu aut Yagitani, Satoshi aut Ishisaka, Keigo aut Kumamoto, Atsushi aut Tsuchiya, Fuminori aut Ozaki, Mitsunori aut Matsuda, Shoya aut Imachi, Tomohiko aut Miyoshi, Yoshizumi aut Hikishima, Mitsuru aut Katoh, Yuto aut Ota, Mamoru aut Shoji, Masafumi aut Matsuoka, Ayako aut Shinohara, Iku aut Enthalten in Earth, planets and space Heidelberg : Springer, 1998 70(2018), 1 vom: 21. Mai (DE-627)353898597 (DE-600)2087663-4 1880-5981 nnns volume:70 year:2018 number:1 day:21 month:05 https://dx.doi.org/10.1186/s40623-018-0842-4 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 70 2018 1 21 05
allfieldsSound	10.1186/s40623-018-0842-4 doi (DE-627)SPR036929468 (SPR)s40623-018-0842-4-e DE-627 ger DE-627 rakwb eng Kasahara, Yoshiya verfasserin (orcid)0000-0002-9304-8235 aut The Plasma Wave Experiment (PWE) on board the Arase (ERG) satellite 2018 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2018 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. Plasma wave (dpeaa)DE-He213 Radiation belt (dpeaa)DE-He213 Geospace (dpeaa)DE-He213 Inner magnetosphere (dpeaa)DE-He213 Chorus (dpeaa)DE-He213 Kasaba, Yasumasa aut Kojima, Hirotsugu aut Yagitani, Satoshi aut Ishisaka, Keigo aut Kumamoto, Atsushi aut Tsuchiya, Fuminori aut Ozaki, Mitsunori aut Matsuda, Shoya aut Imachi, Tomohiko aut Miyoshi, Yoshizumi aut Hikishima, Mitsuru aut Katoh, Yuto aut Ota, Mamoru aut Shoji, Masafumi aut Matsuoka, Ayako aut Shinohara, Iku aut Enthalten in Earth, planets and space Heidelberg : Springer, 1998 70(2018), 1 vom: 21. Mai (DE-627)353898597 (DE-600)2087663-4 1880-5981 nnns volume:70 year:2018 number:1 day:21 month:05 https://dx.doi.org/10.1186/s40623-018-0842-4 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 70 2018 1 21 05
language	English
source	Enthalten in Earth, planets and space 70(2018), 1 vom: 21. Mai volume:70 year:2018 number:1 day:21 month:05
sourceStr	Enthalten in Earth, planets and space 70(2018), 1 vom: 21. Mai volume:70 year:2018 number:1 day:21 month:05
format_phy_str_mv	Article
institution	findex.gbv.de
topic_facet	Plasma wave Radiation belt Geospace Inner magnetosphere Chorus
isfreeaccess_bool	true
container_title	Earth, planets and space
authorswithroles_txt_mv	Kasahara, Yoshiya @@aut@@ Kasaba, Yasumasa @@aut@@ Kojima, Hirotsugu @@aut@@ Yagitani, Satoshi @@aut@@ Ishisaka, Keigo @@aut@@ Kumamoto, Atsushi @@aut@@ Tsuchiya, Fuminori @@aut@@ Ozaki, Mitsunori @@aut@@ Matsuda, Shoya @@aut@@ Imachi, Tomohiko @@aut@@ Miyoshi, Yoshizumi @@aut@@ Hikishima, Mitsuru @@aut@@ Katoh, Yuto @@aut@@ Ota, Mamoru @@aut@@ Shoji, Masafumi @@aut@@ Matsuoka, Ayako @@aut@@ Shinohara, Iku @@aut@@
publishDateDaySort_date	2018-05-21T00:00:00Z
hierarchy_top_id	353898597
id	SPR036929468
language_de	englisch
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author	Kasahara, Yoshiya
spellingShingle	Kasahara, Yoshiya misc Plasma wave misc Radiation belt misc Geospace misc Inner magnetosphere misc Chorus The Plasma Wave Experiment (PWE) on board the Arase (ERG) satellite
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topic_title	The Plasma Wave Experiment (PWE) on board the Arase (ERG) satellite Plasma wave (dpeaa)DE-He213 Radiation belt (dpeaa)DE-He213 Geospace (dpeaa)DE-He213 Inner magnetosphere (dpeaa)DE-He213 Chorus (dpeaa)DE-He213
topic	misc Plasma wave misc Radiation belt misc Geospace misc Inner magnetosphere misc Chorus
topic_unstemmed	misc Plasma wave misc Radiation belt misc Geospace misc Inner magnetosphere misc Chorus
topic_browse	misc Plasma wave misc Radiation belt misc Geospace misc Inner magnetosphere misc Chorus
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title	The Plasma Wave Experiment (PWE) on board the Arase (ERG) satellite
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title_full	The Plasma Wave Experiment (PWE) on board the Arase (ERG) satellite
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author_browse	Kasahara, Yoshiya Kasaba, Yasumasa Kojima, Hirotsugu Yagitani, Satoshi Ishisaka, Keigo Kumamoto, Atsushi Tsuchiya, Fuminori Ozaki, Mitsunori Matsuda, Shoya Imachi, Tomohiko Miyoshi, Yoshizumi Hikishima, Mitsuru Katoh, Yuto Ota, Mamoru Shoji, Masafumi Matsuoka, Ayako Shinohara, Iku
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title_sort	plasma wave experiment (pwe) on board the arase (erg) satellite
title_auth	The Plasma Wave Experiment (PWE) on board the Arase (ERG) satellite
abstract	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. © The Author(s) 2018
abstractGer	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. © The Author(s) 2018
abstract_unstemmed	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. © The Author(s) 2018
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title_short	The Plasma Wave Experiment (PWE) on board the Arase (ERG) satellite
url	https://dx.doi.org/10.1186/s40623-018-0842-4
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author2	Kasaba, Yasumasa Kojima, Hirotsugu Yagitani, Satoshi Ishisaka, Keigo Kumamoto, Atsushi Tsuchiya, Fuminori Ozaki, Mitsunori Matsuda, Shoya Imachi, Tomohiko Miyoshi, Yoshizumi Hikishima, Mitsuru Katoh, Yuto Ota, Mamoru Shoji, Masafumi Matsuoka, Ayako Shinohara, Iku
author2Str	Kasaba, Yasumasa Kojima, Hirotsugu Yagitani, Satoshi Ishisaka, Keigo Kumamoto, Atsushi Tsuchiya, Fuminori Ozaki, Mitsunori Matsuda, Shoya Imachi, Tomohiko Miyoshi, Yoshizumi Hikishima, Mitsuru Katoh, Yuto Ota, Mamoru Shoji, Masafumi Matsuoka, Ayako Shinohara, Iku
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The Plasma Wave Experiment (PWE) on board the Arase (ERG) satellite

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