High-energy electron experiments (HEP) aboard the ERG (Arase) satellite

Abstract This paper reports the design, calibration, and operation of high-energy electron experiments (HEP) aboard the exploration of energization and radiation in geospace (ERG) satellite. HEP detects 70 keV–2 MeV electrons and generates a three-dimensional velocity distribution for these electron...
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Autor*in:	Mitani, Takefumi [verfasserIn] Takashima, Takeshi Kasahara, Satoshi Miyake, Wataru Hirahara, Masafumi

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2018

Schlagwörter:	ERG Arase Radiation belts High-energy electrons

Anmerkung:	© The Author(s) 2018

Übergeordnetes Werk:	Enthalten in: Earth, planets and space - Heidelberg : Springer, 1998, 70(2018), 1 vom: 08. Mai
Übergeordnetes Werk:	volume:70 ; year:2018 ; number:1 ; day:08 ; month:05

Links:	Volltext

DOI / URN:	10.1186/s40623-018-0853-1

Katalog-ID:	SPR036929573

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allfields	10.1186/s40623-018-0853-1 doi (DE-627)SPR036929573 (SPR)s40623-018-0853-1-e DE-627 ger DE-627 rakwb eng Mitani, Takefumi verfasserin aut High-energy electron experiments (HEP) aboard the ERG (Arase) satellite 2018 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2018 Abstract This paper reports the design, calibration, and operation of high-energy electron experiments (HEP) aboard the exploration of energization and radiation in geospace (ERG) satellite. HEP detects 70 keV–2 MeV electrons and generates a three-dimensional velocity distribution for these electrons in every period of the satellite’s rotation. Electrons are detected by two instruments, namely HEP-L and HEP-H, which differ in their geometric factor (G-factor) and range of energies they detect. HEP-L detects 70 keV–1 MeV electrons and its G-factor is 9.3 × $ 10^{−4} $ $ cm^{2} $ sr at maximum, while HEP-H observes 0.7–2 MeV electrons and its G-factor is 9.3 × $ 10^{−3} $ $ cm^{2} $ sr at maximum. The instruments utilize silicon strip detectors and application-specific integrated circuits to readout the incident charge signal from each strip. Before the launch, we calibrated the detectors by measuring the energy spectra of all strips using γ-ray sources. To evaluate the overall performance of the HEP instruments, we measured the energy spectra and angular responses with electron beams. After HEP was first put into operation, on February 2, 2017, it was demonstrated that the instruments performed normally. HEP began its exploratory observations with regard to energization and radiation in geospace in late March 2017. The initial results of the in-orbit observations are introduced briefly in this paper. ERG (dpeaa)DE-He213 Arase (dpeaa)DE-He213 Radiation belts (dpeaa)DE-He213 High-energy electrons (dpeaa)DE-He213 Takashima, Takeshi aut Kasahara, Satoshi aut Miyake, Wataru aut Hirahara, Masafumi aut Enthalten in Earth, planets and space Heidelberg : Springer, 1998 70(2018), 1 vom: 08. Mai (DE-627)353898597 (DE-600)2087663-4 1880-5981 nnns volume:70 year:2018 number:1 day:08 month:05 https://dx.doi.org/10.1186/s40623-018-0853-1 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 05
spelling	10.1186/s40623-018-0853-1 doi (DE-627)SPR036929573 (SPR)s40623-018-0853-1-e DE-627 ger DE-627 rakwb eng Mitani, Takefumi verfasserin aut High-energy electron experiments (HEP) aboard the ERG (Arase) satellite 2018 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2018 Abstract This paper reports the design, calibration, and operation of high-energy electron experiments (HEP) aboard the exploration of energization and radiation in geospace (ERG) satellite. HEP detects 70 keV–2 MeV electrons and generates a three-dimensional velocity distribution for these electrons in every period of the satellite’s rotation. Electrons are detected by two instruments, namely HEP-L and HEP-H, which differ in their geometric factor (G-factor) and range of energies they detect. HEP-L detects 70 keV–1 MeV electrons and its G-factor is 9.3 × $ 10^{−4} $ $ cm^{2} $ sr at maximum, while HEP-H observes 0.7–2 MeV electrons and its G-factor is 9.3 × $ 10^{−3} $ $ cm^{2} $ sr at maximum. The instruments utilize silicon strip detectors and application-specific integrated circuits to readout the incident charge signal from each strip. Before the launch, we calibrated the detectors by measuring the energy spectra of all strips using γ-ray sources. To evaluate the overall performance of the HEP instruments, we measured the energy spectra and angular responses with electron beams. After HEP was first put into operation, on February 2, 2017, it was demonstrated that the instruments performed normally. HEP began its exploratory observations with regard to energization and radiation in geospace in late March 2017. The initial results of the in-orbit observations are introduced briefly in this paper. ERG (dpeaa)DE-He213 Arase (dpeaa)DE-He213 Radiation belts (dpeaa)DE-He213 High-energy electrons (dpeaa)DE-He213 Takashima, Takeshi aut Kasahara, Satoshi aut Miyake, Wataru aut Hirahara, Masafumi aut Enthalten in Earth, planets and space Heidelberg : Springer, 1998 70(2018), 1 vom: 08. Mai (DE-627)353898597 (DE-600)2087663-4 1880-5981 nnns volume:70 year:2018 number:1 day:08 month:05 https://dx.doi.org/10.1186/s40623-018-0853-1 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 05
allfields_unstemmed	10.1186/s40623-018-0853-1 doi (DE-627)SPR036929573 (SPR)s40623-018-0853-1-e DE-627 ger DE-627 rakwb eng Mitani, Takefumi verfasserin aut High-energy electron experiments (HEP) aboard the ERG (Arase) satellite 2018 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2018 Abstract This paper reports the design, calibration, and operation of high-energy electron experiments (HEP) aboard the exploration of energization and radiation in geospace (ERG) satellite. HEP detects 70 keV–2 MeV electrons and generates a three-dimensional velocity distribution for these electrons in every period of the satellite’s rotation. Electrons are detected by two instruments, namely HEP-L and HEP-H, which differ in their geometric factor (G-factor) and range of energies they detect. HEP-L detects 70 keV–1 MeV electrons and its G-factor is 9.3 × $ 10^{−4} $ $ cm^{2} $ sr at maximum, while HEP-H observes 0.7–2 MeV electrons and its G-factor is 9.3 × $ 10^{−3} $ $ cm^{2} $ sr at maximum. The instruments utilize silicon strip detectors and application-specific integrated circuits to readout the incident charge signal from each strip. Before the launch, we calibrated the detectors by measuring the energy spectra of all strips using γ-ray sources. To evaluate the overall performance of the HEP instruments, we measured the energy spectra and angular responses with electron beams. After HEP was first put into operation, on February 2, 2017, it was demonstrated that the instruments performed normally. HEP began its exploratory observations with regard to energization and radiation in geospace in late March 2017. The initial results of the in-orbit observations are introduced briefly in this paper. ERG (dpeaa)DE-He213 Arase (dpeaa)DE-He213 Radiation belts (dpeaa)DE-He213 High-energy electrons (dpeaa)DE-He213 Takashima, Takeshi aut Kasahara, Satoshi aut Miyake, Wataru aut Hirahara, Masafumi aut Enthalten in Earth, planets and space Heidelberg : Springer, 1998 70(2018), 1 vom: 08. Mai (DE-627)353898597 (DE-600)2087663-4 1880-5981 nnns volume:70 year:2018 number:1 day:08 month:05 https://dx.doi.org/10.1186/s40623-018-0853-1 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 05
allfieldsGer	10.1186/s40623-018-0853-1 doi (DE-627)SPR036929573 (SPR)s40623-018-0853-1-e DE-627 ger DE-627 rakwb eng Mitani, Takefumi verfasserin aut High-energy electron experiments (HEP) aboard the ERG (Arase) satellite 2018 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2018 Abstract This paper reports the design, calibration, and operation of high-energy electron experiments (HEP) aboard the exploration of energization and radiation in geospace (ERG) satellite. HEP detects 70 keV–2 MeV electrons and generates a three-dimensional velocity distribution for these electrons in every period of the satellite’s rotation. Electrons are detected by two instruments, namely HEP-L and HEP-H, which differ in their geometric factor (G-factor) and range of energies they detect. HEP-L detects 70 keV–1 MeV electrons and its G-factor is 9.3 × $ 10^{−4} $ $ cm^{2} $ sr at maximum, while HEP-H observes 0.7–2 MeV electrons and its G-factor is 9.3 × $ 10^{−3} $ $ cm^{2} $ sr at maximum. The instruments utilize silicon strip detectors and application-specific integrated circuits to readout the incident charge signal from each strip. Before the launch, we calibrated the detectors by measuring the energy spectra of all strips using γ-ray sources. To evaluate the overall performance of the HEP instruments, we measured the energy spectra and angular responses with electron beams. After HEP was first put into operation, on February 2, 2017, it was demonstrated that the instruments performed normally. HEP began its exploratory observations with regard to energization and radiation in geospace in late March 2017. The initial results of the in-orbit observations are introduced briefly in this paper. ERG (dpeaa)DE-He213 Arase (dpeaa)DE-He213 Radiation belts (dpeaa)DE-He213 High-energy electrons (dpeaa)DE-He213 Takashima, Takeshi aut Kasahara, Satoshi aut Miyake, Wataru aut Hirahara, Masafumi aut Enthalten in Earth, planets and space Heidelberg : Springer, 1998 70(2018), 1 vom: 08. Mai (DE-627)353898597 (DE-600)2087663-4 1880-5981 nnns volume:70 year:2018 number:1 day:08 month:05 https://dx.doi.org/10.1186/s40623-018-0853-1 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 05
allfieldsSound	10.1186/s40623-018-0853-1 doi (DE-627)SPR036929573 (SPR)s40623-018-0853-1-e DE-627 ger DE-627 rakwb eng Mitani, Takefumi verfasserin aut High-energy electron experiments (HEP) aboard the ERG (Arase) satellite 2018 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2018 Abstract This paper reports the design, calibration, and operation of high-energy electron experiments (HEP) aboard the exploration of energization and radiation in geospace (ERG) satellite. HEP detects 70 keV–2 MeV electrons and generates a three-dimensional velocity distribution for these electrons in every period of the satellite’s rotation. Electrons are detected by two instruments, namely HEP-L and HEP-H, which differ in their geometric factor (G-factor) and range of energies they detect. HEP-L detects 70 keV–1 MeV electrons and its G-factor is 9.3 × $ 10^{−4} $ $ cm^{2} $ sr at maximum, while HEP-H observes 0.7–2 MeV electrons and its G-factor is 9.3 × $ 10^{−3} $ $ cm^{2} $ sr at maximum. The instruments utilize silicon strip detectors and application-specific integrated circuits to readout the incident charge signal from each strip. Before the launch, we calibrated the detectors by measuring the energy spectra of all strips using γ-ray sources. To evaluate the overall performance of the HEP instruments, we measured the energy spectra and angular responses with electron beams. After HEP was first put into operation, on February 2, 2017, it was demonstrated that the instruments performed normally. HEP began its exploratory observations with regard to energization and radiation in geospace in late March 2017. The initial results of the in-orbit observations are introduced briefly in this paper. ERG (dpeaa)DE-He213 Arase (dpeaa)DE-He213 Radiation belts (dpeaa)DE-He213 High-energy electrons (dpeaa)DE-He213 Takashima, Takeshi aut Kasahara, Satoshi aut Miyake, Wataru aut Hirahara, Masafumi aut Enthalten in Earth, planets and space Heidelberg : Springer, 1998 70(2018), 1 vom: 08. Mai (DE-627)353898597 (DE-600)2087663-4 1880-5981 nnns volume:70 year:2018 number:1 day:08 month:05 https://dx.doi.org/10.1186/s40623-018-0853-1 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 05
language	English
source	Enthalten in Earth, planets and space 70(2018), 1 vom: 08. Mai volume:70 year:2018 number:1 day:08 month:05
sourceStr	Enthalten in Earth, planets and space 70(2018), 1 vom: 08. Mai volume:70 year:2018 number:1 day:08 month:05
format_phy_str_mv	Article
institution	findex.gbv.de
topic_facet	ERG Arase Radiation belts High-energy electrons
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container_title	Earth, planets and space
authorswithroles_txt_mv	Mitani, Takefumi @@aut@@ Takashima, Takeshi @@aut@@ Kasahara, Satoshi @@aut@@ Miyake, Wataru @@aut@@ Hirahara, Masafumi @@aut@@
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topic_title	High-energy electron experiments (HEP) aboard the ERG (Arase) satellite ERG (dpeaa)DE-He213 Arase (dpeaa)DE-He213 Radiation belts (dpeaa)DE-He213 High-energy electrons (dpeaa)DE-He213
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title	High-energy electron experiments (HEP) aboard the ERG (Arase) satellite
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title_sort	high-energy electron experiments (hep) aboard the erg (arase) satellite
title_auth	High-energy electron experiments (HEP) aboard the ERG (Arase) satellite
abstract	Abstract This paper reports the design, calibration, and operation of high-energy electron experiments (HEP) aboard the exploration of energization and radiation in geospace (ERG) satellite. HEP detects 70 keV–2 MeV electrons and generates a three-dimensional velocity distribution for these electrons in every period of the satellite’s rotation. Electrons are detected by two instruments, namely HEP-L and HEP-H, which differ in their geometric factor (G-factor) and range of energies they detect. HEP-L detects 70 keV–1 MeV electrons and its G-factor is 9.3 × $ 10^{−4} $ $ cm^{2} $ sr at maximum, while HEP-H observes 0.7–2 MeV electrons and its G-factor is 9.3 × $ 10^{−3} $ $ cm^{2} $ sr at maximum. The instruments utilize silicon strip detectors and application-specific integrated circuits to readout the incident charge signal from each strip. Before the launch, we calibrated the detectors by measuring the energy spectra of all strips using γ-ray sources. To evaluate the overall performance of the HEP instruments, we measured the energy spectra and angular responses with electron beams. After HEP was first put into operation, on February 2, 2017, it was demonstrated that the instruments performed normally. HEP began its exploratory observations with regard to energization and radiation in geospace in late March 2017. The initial results of the in-orbit observations are introduced briefly in this paper. © The Author(s) 2018
abstractGer	Abstract This paper reports the design, calibration, and operation of high-energy electron experiments (HEP) aboard the exploration of energization and radiation in geospace (ERG) satellite. HEP detects 70 keV–2 MeV electrons and generates a three-dimensional velocity distribution for these electrons in every period of the satellite’s rotation. Electrons are detected by two instruments, namely HEP-L and HEP-H, which differ in their geometric factor (G-factor) and range of energies they detect. HEP-L detects 70 keV–1 MeV electrons and its G-factor is 9.3 × $ 10^{−4} $ $ cm^{2} $ sr at maximum, while HEP-H observes 0.7–2 MeV electrons and its G-factor is 9.3 × $ 10^{−3} $ $ cm^{2} $ sr at maximum. The instruments utilize silicon strip detectors and application-specific integrated circuits to readout the incident charge signal from each strip. Before the launch, we calibrated the detectors by measuring the energy spectra of all strips using γ-ray sources. To evaluate the overall performance of the HEP instruments, we measured the energy spectra and angular responses with electron beams. After HEP was first put into operation, on February 2, 2017, it was demonstrated that the instruments performed normally. HEP began its exploratory observations with regard to energization and radiation in geospace in late March 2017. The initial results of the in-orbit observations are introduced briefly in this paper. © The Author(s) 2018
abstract_unstemmed	Abstract This paper reports the design, calibration, and operation of high-energy electron experiments (HEP) aboard the exploration of energization and radiation in geospace (ERG) satellite. HEP detects 70 keV–2 MeV electrons and generates a three-dimensional velocity distribution for these electrons in every period of the satellite’s rotation. Electrons are detected by two instruments, namely HEP-L and HEP-H, which differ in their geometric factor (G-factor) and range of energies they detect. HEP-L detects 70 keV–1 MeV electrons and its G-factor is 9.3 × $ 10^{−4} $ $ cm^{2} $ sr at maximum, while HEP-H observes 0.7–2 MeV electrons and its G-factor is 9.3 × $ 10^{−3} $ $ cm^{2} $ sr at maximum. The instruments utilize silicon strip detectors and application-specific integrated circuits to readout the incident charge signal from each strip. Before the launch, we calibrated the detectors by measuring the energy spectra of all strips using γ-ray sources. To evaluate the overall performance of the HEP instruments, we measured the energy spectra and angular responses with electron beams. After HEP was first put into operation, on February 2, 2017, it was demonstrated that the instruments performed normally. HEP began its exploratory observations with regard to energization and radiation in geospace in late March 2017. The initial results of the in-orbit observations are introduced briefly in this paper. © The Author(s) 2018
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title_short	High-energy electron experiments (HEP) aboard the ERG (Arase) satellite
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High-energy electron experiments (HEP) aboard the ERG (Arase) satellite

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