Software-type Wave–Particle Interaction Analyzer on board the Arase satellite
Abstract 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 install...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Katoh, Yuto [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2018 |
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| Schlagwörter: |
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| Anmerkung: |
© The Author(s) 2018 |
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| Übergeordnetes Werk: |
Enthalten in: Earth, planets and space - Heidelberg : Springer, 1998, 70(2018), 1 vom: 08. Jan. |
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| Übergeordnetes Werk: |
volume:70 ; year:2018 ; number:1 ; day:08 ; month:01 |
| Links: |
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| DOI / URN: |
10.1186/s40623-017-0771-7 |
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| Katalog-ID: |
SPR036928739 |
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| 520 | |a Abstract 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. | ||
| 650 | 4 | |a Radiation belts |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Magnetosphere |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Whistler-mode chorus |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Wave–particle interactions |7 (dpeaa)DE-He213 | |
| 700 | 1 | |a Kojima, Hirotsugu |4 aut | |
| 700 | 1 | |a Hikishima, Mitsuru |4 aut | |
| 700 | 1 | |a Takashima, Takeshi |4 aut | |
| 700 | 1 | |a Asamura, Kazushi |4 aut | |
| 700 | 1 | |a Miyoshi, Yoshizumi |4 aut | |
| 700 | 1 | |a Kasahara, Yoshiya |4 aut | |
| 700 | 1 | |a Kasahara, Satoshi |4 aut | |
| 700 | 1 | |a Mitani, Takefumi |4 aut | |
| 700 | 1 | |a Higashio, Nana |4 aut | |
| 700 | 1 | |a Matsuoka, Ayako |4 aut | |
| 700 | 1 | |a Ozaki, Mitsunori |4 aut | |
| 700 | 1 | |a Yagitani, Satoshi |4 aut | |
| 700 | 1 | |a Yokota, Shoichiro |4 aut | |
| 700 | 1 | |a Matsuda, Shoya |4 aut | |
| 700 | 1 | |a Kitahara, Masahiro |4 aut | |
| 700 | 1 | |a Shinohara, Iku |4 aut | |
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10.1186/s40623-017-0771-7 doi (DE-627)SPR036928739 (SPR)s40623-017-0771-7-e DE-627 ger DE-627 rakwb eng Katoh, Yuto verfasserin (orcid)0000-0002-4318-0633 aut Software-type Wave–Particle Interaction Analyzer on board the Arase satellite 2018 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2018 Abstract 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. Radiation belts (dpeaa)DE-He213 Magnetosphere (dpeaa)DE-He213 Whistler-mode chorus (dpeaa)DE-He213 Wave–particle interactions (dpeaa)DE-He213 Kojima, Hirotsugu aut Hikishima, Mitsuru aut Takashima, Takeshi aut Asamura, Kazushi aut Miyoshi, Yoshizumi aut Kasahara, Yoshiya aut Kasahara, Satoshi aut Mitani, Takefumi aut Higashio, Nana aut Matsuoka, Ayako aut Ozaki, Mitsunori aut Yagitani, Satoshi aut Yokota, Shoichiro aut Matsuda, Shoya aut Kitahara, Masahiro aut Shinohara, Iku aut Enthalten in Earth, planets and space Heidelberg : Springer, 1998 70(2018), 1 vom: 08. Jan. (DE-627)353898597 (DE-600)2087663-4 1880-5981 nnns volume:70 year:2018 number:1 day:08 month:01 https://dx.doi.org/10.1186/s40623-017-0771-7 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 08 01 |
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10.1186/s40623-017-0771-7 doi (DE-627)SPR036928739 (SPR)s40623-017-0771-7-e DE-627 ger DE-627 rakwb eng Katoh, Yuto verfasserin (orcid)0000-0002-4318-0633 aut Software-type Wave–Particle Interaction Analyzer on board the Arase satellite 2018 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2018 Abstract 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. Radiation belts (dpeaa)DE-He213 Magnetosphere (dpeaa)DE-He213 Whistler-mode chorus (dpeaa)DE-He213 Wave–particle interactions (dpeaa)DE-He213 Kojima, Hirotsugu aut Hikishima, Mitsuru aut Takashima, Takeshi aut Asamura, Kazushi aut Miyoshi, Yoshizumi aut Kasahara, Yoshiya aut Kasahara, Satoshi aut Mitani, Takefumi aut Higashio, Nana aut Matsuoka, Ayako aut Ozaki, Mitsunori aut Yagitani, Satoshi aut Yokota, Shoichiro aut Matsuda, Shoya aut Kitahara, Masahiro aut Shinohara, Iku aut Enthalten in Earth, planets and space Heidelberg : Springer, 1998 70(2018), 1 vom: 08. Jan. (DE-627)353898597 (DE-600)2087663-4 1880-5981 nnns volume:70 year:2018 number:1 day:08 month:01 https://dx.doi.org/10.1186/s40623-017-0771-7 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 08 01 |
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10.1186/s40623-017-0771-7 doi (DE-627)SPR036928739 (SPR)s40623-017-0771-7-e DE-627 ger DE-627 rakwb eng Katoh, Yuto verfasserin (orcid)0000-0002-4318-0633 aut Software-type Wave–Particle Interaction Analyzer on board the Arase satellite 2018 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2018 Abstract 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. Radiation belts (dpeaa)DE-He213 Magnetosphere (dpeaa)DE-He213 Whistler-mode chorus (dpeaa)DE-He213 Wave–particle interactions (dpeaa)DE-He213 Kojima, Hirotsugu aut Hikishima, Mitsuru aut Takashima, Takeshi aut Asamura, Kazushi aut Miyoshi, Yoshizumi aut Kasahara, Yoshiya aut Kasahara, Satoshi aut Mitani, Takefumi aut Higashio, Nana aut Matsuoka, Ayako aut Ozaki, Mitsunori aut Yagitani, Satoshi aut Yokota, Shoichiro aut Matsuda, Shoya aut Kitahara, Masahiro aut Shinohara, Iku aut Enthalten in Earth, planets and space Heidelberg : Springer, 1998 70(2018), 1 vom: 08. Jan. (DE-627)353898597 (DE-600)2087663-4 1880-5981 nnns volume:70 year:2018 number:1 day:08 month:01 https://dx.doi.org/10.1186/s40623-017-0771-7 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 08 01 |
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10.1186/s40623-017-0771-7 doi (DE-627)SPR036928739 (SPR)s40623-017-0771-7-e DE-627 ger DE-627 rakwb eng Katoh, Yuto verfasserin (orcid)0000-0002-4318-0633 aut Software-type Wave–Particle Interaction Analyzer on board the Arase satellite 2018 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2018 Abstract 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. Radiation belts (dpeaa)DE-He213 Magnetosphere (dpeaa)DE-He213 Whistler-mode chorus (dpeaa)DE-He213 Wave–particle interactions (dpeaa)DE-He213 Kojima, Hirotsugu aut Hikishima, Mitsuru aut Takashima, Takeshi aut Asamura, Kazushi aut Miyoshi, Yoshizumi aut Kasahara, Yoshiya aut Kasahara, Satoshi aut Mitani, Takefumi aut Higashio, Nana aut Matsuoka, Ayako aut Ozaki, Mitsunori aut Yagitani, Satoshi aut Yokota, Shoichiro aut Matsuda, Shoya aut Kitahara, Masahiro aut Shinohara, Iku aut Enthalten in Earth, planets and space Heidelberg : Springer, 1998 70(2018), 1 vom: 08. Jan. (DE-627)353898597 (DE-600)2087663-4 1880-5981 nnns volume:70 year:2018 number:1 day:08 month:01 https://dx.doi.org/10.1186/s40623-017-0771-7 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 08 01 |
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Software-type Wave–Particle Interaction Analyzer on board the Arase satellite |
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Abstract 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. © The Author(s) 2018 |
| abstractGer |
Abstract 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. © The Author(s) 2018 |
| abstract_unstemmed |
Abstract 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. © The Author(s) 2018 |
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| container_issue |
1 |
| title_short |
Software-type Wave–Particle Interaction Analyzer on board the Arase satellite |
| url |
https://dx.doi.org/10.1186/s40623-017-0771-7 |
| remote_bool |
true |
| author2 |
Kojima, Hirotsugu Hikishima, Mitsuru Takashima, Takeshi Asamura, Kazushi Miyoshi, Yoshizumi Kasahara, Yoshiya Kasahara, Satoshi Mitani, Takefumi Higashio, Nana Matsuoka, Ayako Ozaki, Mitsunori Yagitani, Satoshi Yokota, Shoichiro Matsuda, Shoya Kitahara, Masahiro Shinohara, Iku |
| author2Str |
Kojima, Hirotsugu Hikishima, Mitsuru Takashima, Takeshi Asamura, Kazushi Miyoshi, Yoshizumi Kasahara, Yoshiya Kasahara, Satoshi Mitani, Takefumi Higashio, Nana Matsuoka, Ayako Ozaki, Mitsunori Yagitani, Satoshi Yokota, Shoichiro Matsuda, Shoya Kitahara, Masahiro Shinohara, Iku |
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| doi_str |
10.1186/s40623-017-0771-7 |
| up_date |
2024-07-03T20:24:51.751Z |
| _version_ |
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