Trigger System of the NUCLEON Space Experiment
Abstract The NUCLEON satellite experiment is designed to investigate directly the energy spectra of galactic cosmic ray (CR) nuclei and its charge composition before the “knee”: in the energy interval from 100 GeV to 100 TeV and the charge range Z = 1–30 respectively. The “knee” energy range of $ 10...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Nurtayeva, U. M. [verfasserIn] |
|---|
| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2019 |
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| Anmerkung: |
© Pleiades Publishing, Ltd. 2019 |
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| Übergeordnetes Werk: |
Enthalten in: Physics of atomic nuclei - Pleiades Publishing, 1993, 82(2019), 6 vom: Nov., Seite 782-787 |
|---|---|
| Übergeordnetes Werk: |
volume:82 ; year:2019 ; number:6 ; month:11 ; pages:782-787 |
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| DOI / URN: |
10.1134/S1063778819660414 |
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OLC2049932111 |
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| 520 | |a Abstract The NUCLEON satellite experiment is designed to investigate directly the energy spectra of galactic cosmic ray (CR) nuclei and its charge composition before the “knee”: in the energy interval from 100 GeV to 100 TeV and the charge range Z = 1–30 respectively. The “knee” energy range of $ 10^{11} $–$ 10^{16} $ eV is a crucial region for the understanding of the cosmic-ray acceleration and propagation in the interstellar medium. The NUCLEON detector has been data taken since December, 2014. The NUCLEON trigger system and CR event selection are described, including the beam tests at the SPS CERN, flight tests in orbit and the Monte-Carlo simulation. | ||
| 700 | 1 | |a Grebenyuk, V. M. |4 aut | |
| 700 | 1 | |a Karmanov, D. M. |4 aut | |
| 700 | 1 | |a Pan, A. |4 aut | |
| 700 | 1 | |a Podorozhny, D. M. |4 aut | |
| 700 | 1 | |a Porokhovoy, S. Yu. |4 aut | |
| 700 | 1 | |a Sadovsky, A. B. |4 aut | |
| 700 | 1 | |a Tkachenko, A. V. |4 aut | |
| 700 | 1 | |a Tkachev, L. G. |4 aut | |
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10.1134/S1063778819660414 doi (DE-627)OLC2049932111 (DE-He213)S1063778819660414-p DE-627 ger DE-627 rakwb eng 530 VZ Nurtayeva, U. M. verfasserin aut Trigger System of the NUCLEON Space Experiment 2019 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2019 Abstract The NUCLEON satellite experiment is designed to investigate directly the energy spectra of galactic cosmic ray (CR) nuclei and its charge composition before the “knee”: in the energy interval from 100 GeV to 100 TeV and the charge range Z = 1–30 respectively. The “knee” energy range of $ 10^{11} $–$ 10^{16} $ eV is a crucial region for the understanding of the cosmic-ray acceleration and propagation in the interstellar medium. The NUCLEON detector has been data taken since December, 2014. The NUCLEON trigger system and CR event selection are described, including the beam tests at the SPS CERN, flight tests in orbit and the Monte-Carlo simulation. Grebenyuk, V. M. aut Karmanov, D. M. aut Pan, A. aut Podorozhny, D. M. aut Porokhovoy, S. Yu. aut Sadovsky, A. B. aut Tkachenko, A. V. aut Tkachev, L. G. aut Enthalten in Physics of atomic nuclei Pleiades Publishing, 1993 82(2019), 6 vom: Nov., Seite 782-787 (DE-627)131188437 (DE-600)1146378-8 (DE-576)032622155 1063-7788 nnns volume:82 year:2019 number:6 month:11 pages:782-787 https://doi.org/10.1134/S1063778819660414 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_70 AR 82 2019 6 11 782-787 |
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10.1134/S1063778819660414 doi (DE-627)OLC2049932111 (DE-He213)S1063778819660414-p DE-627 ger DE-627 rakwb eng 530 VZ Nurtayeva, U. M. verfasserin aut Trigger System of the NUCLEON Space Experiment 2019 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2019 Abstract The NUCLEON satellite experiment is designed to investigate directly the energy spectra of galactic cosmic ray (CR) nuclei and its charge composition before the “knee”: in the energy interval from 100 GeV to 100 TeV and the charge range Z = 1–30 respectively. The “knee” energy range of $ 10^{11} $–$ 10^{16} $ eV is a crucial region for the understanding of the cosmic-ray acceleration and propagation in the interstellar medium. The NUCLEON detector has been data taken since December, 2014. The NUCLEON trigger system and CR event selection are described, including the beam tests at the SPS CERN, flight tests in orbit and the Monte-Carlo simulation. Grebenyuk, V. M. aut Karmanov, D. M. aut Pan, A. aut Podorozhny, D. M. aut Porokhovoy, S. Yu. aut Sadovsky, A. B. aut Tkachenko, A. V. aut Tkachev, L. G. aut Enthalten in Physics of atomic nuclei Pleiades Publishing, 1993 82(2019), 6 vom: Nov., Seite 782-787 (DE-627)131188437 (DE-600)1146378-8 (DE-576)032622155 1063-7788 nnns volume:82 year:2019 number:6 month:11 pages:782-787 https://doi.org/10.1134/S1063778819660414 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_70 AR 82 2019 6 11 782-787 |
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10.1134/S1063778819660414 doi (DE-627)OLC2049932111 (DE-He213)S1063778819660414-p DE-627 ger DE-627 rakwb eng 530 VZ Nurtayeva, U. M. verfasserin aut Trigger System of the NUCLEON Space Experiment 2019 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2019 Abstract The NUCLEON satellite experiment is designed to investigate directly the energy spectra of galactic cosmic ray (CR) nuclei and its charge composition before the “knee”: in the energy interval from 100 GeV to 100 TeV and the charge range Z = 1–30 respectively. The “knee” energy range of $ 10^{11} $–$ 10^{16} $ eV is a crucial region for the understanding of the cosmic-ray acceleration and propagation in the interstellar medium. The NUCLEON detector has been data taken since December, 2014. The NUCLEON trigger system and CR event selection are described, including the beam tests at the SPS CERN, flight tests in orbit and the Monte-Carlo simulation. Grebenyuk, V. M. aut Karmanov, D. M. aut Pan, A. aut Podorozhny, D. M. aut Porokhovoy, S. Yu. aut Sadovsky, A. B. aut Tkachenko, A. V. aut Tkachev, L. G. aut Enthalten in Physics of atomic nuclei Pleiades Publishing, 1993 82(2019), 6 vom: Nov., Seite 782-787 (DE-627)131188437 (DE-600)1146378-8 (DE-576)032622155 1063-7788 nnns volume:82 year:2019 number:6 month:11 pages:782-787 https://doi.org/10.1134/S1063778819660414 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_70 AR 82 2019 6 11 782-787 |
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10.1134/S1063778819660414 doi (DE-627)OLC2049932111 (DE-He213)S1063778819660414-p DE-627 ger DE-627 rakwb eng 530 VZ Nurtayeva, U. M. verfasserin aut Trigger System of the NUCLEON Space Experiment 2019 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2019 Abstract The NUCLEON satellite experiment is designed to investigate directly the energy spectra of galactic cosmic ray (CR) nuclei and its charge composition before the “knee”: in the energy interval from 100 GeV to 100 TeV and the charge range Z = 1–30 respectively. The “knee” energy range of $ 10^{11} $–$ 10^{16} $ eV is a crucial region for the understanding of the cosmic-ray acceleration and propagation in the interstellar medium. The NUCLEON detector has been data taken since December, 2014. The NUCLEON trigger system and CR event selection are described, including the beam tests at the SPS CERN, flight tests in orbit and the Monte-Carlo simulation. Grebenyuk, V. M. aut Karmanov, D. M. aut Pan, A. aut Podorozhny, D. M. aut Porokhovoy, S. Yu. aut Sadovsky, A. B. aut Tkachenko, A. V. aut Tkachev, L. G. aut Enthalten in Physics of atomic nuclei Pleiades Publishing, 1993 82(2019), 6 vom: Nov., Seite 782-787 (DE-627)131188437 (DE-600)1146378-8 (DE-576)032622155 1063-7788 nnns volume:82 year:2019 number:6 month:11 pages:782-787 https://doi.org/10.1134/S1063778819660414 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_70 AR 82 2019 6 11 782-787 |
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10.1134/S1063778819660414 doi (DE-627)OLC2049932111 (DE-He213)S1063778819660414-p DE-627 ger DE-627 rakwb eng 530 VZ Nurtayeva, U. M. verfasserin aut Trigger System of the NUCLEON Space Experiment 2019 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2019 Abstract The NUCLEON satellite experiment is designed to investigate directly the energy spectra of galactic cosmic ray (CR) nuclei and its charge composition before the “knee”: in the energy interval from 100 GeV to 100 TeV and the charge range Z = 1–30 respectively. The “knee” energy range of $ 10^{11} $–$ 10^{16} $ eV is a crucial region for the understanding of the cosmic-ray acceleration and propagation in the interstellar medium. The NUCLEON detector has been data taken since December, 2014. The NUCLEON trigger system and CR event selection are described, including the beam tests at the SPS CERN, flight tests in orbit and the Monte-Carlo simulation. Grebenyuk, V. M. aut Karmanov, D. M. aut Pan, A. aut Podorozhny, D. M. aut Porokhovoy, S. Yu. aut Sadovsky, A. B. aut Tkachenko, A. V. aut Tkachev, L. G. aut Enthalten in Physics of atomic nuclei Pleiades Publishing, 1993 82(2019), 6 vom: Nov., Seite 782-787 (DE-627)131188437 (DE-600)1146378-8 (DE-576)032622155 1063-7788 nnns volume:82 year:2019 number:6 month:11 pages:782-787 https://doi.org/10.1134/S1063778819660414 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_70 AR 82 2019 6 11 782-787 |
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Abstract The NUCLEON satellite experiment is designed to investigate directly the energy spectra of galactic cosmic ray (CR) nuclei and its charge composition before the “knee”: in the energy interval from 100 GeV to 100 TeV and the charge range Z = 1–30 respectively. The “knee” energy range of $ 10^{11} $–$ 10^{16} $ eV is a crucial region for the understanding of the cosmic-ray acceleration and propagation in the interstellar medium. The NUCLEON detector has been data taken since December, 2014. The NUCLEON trigger system and CR event selection are described, including the beam tests at the SPS CERN, flight tests in orbit and the Monte-Carlo simulation. © Pleiades Publishing, Ltd. 2019 |
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Abstract The NUCLEON satellite experiment is designed to investigate directly the energy spectra of galactic cosmic ray (CR) nuclei and its charge composition before the “knee”: in the energy interval from 100 GeV to 100 TeV and the charge range Z = 1–30 respectively. The “knee” energy range of $ 10^{11} $–$ 10^{16} $ eV is a crucial region for the understanding of the cosmic-ray acceleration and propagation in the interstellar medium. The NUCLEON detector has been data taken since December, 2014. The NUCLEON trigger system and CR event selection are described, including the beam tests at the SPS CERN, flight tests in orbit and the Monte-Carlo simulation. © Pleiades Publishing, Ltd. 2019 |
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Abstract The NUCLEON satellite experiment is designed to investigate directly the energy spectra of galactic cosmic ray (CR) nuclei and its charge composition before the “knee”: in the energy interval from 100 GeV to 100 TeV and the charge range Z = 1–30 respectively. The “knee” energy range of $ 10^{11} $–$ 10^{16} $ eV is a crucial region for the understanding of the cosmic-ray acceleration and propagation in the interstellar medium. The NUCLEON detector has been data taken since December, 2014. The NUCLEON trigger system and CR event selection are described, including the beam tests at the SPS CERN, flight tests in orbit and the Monte-Carlo simulation. © Pleiades Publishing, Ltd. 2019 |
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<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">OLC2049932111</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230504110744.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">200820s2019 xx ||||| 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1134/S1063778819660414</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC2049932111</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-He213)S1063778819660414-p</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">530</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Nurtayeva, U. M.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Trigger System of the NUCLEON Space Experiment</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2019</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">ohne Hilfsmittel zu benutzen</subfield><subfield code="b">n</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Band</subfield><subfield code="b">nc</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">© Pleiades Publishing, Ltd. 2019</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract The NUCLEON satellite experiment is designed to investigate directly the energy spectra of galactic cosmic ray (CR) nuclei and its charge composition before the “knee”: in the energy interval from 100 GeV to 100 TeV and the charge range Z = 1–30 respectively. The “knee” energy range of $ 10^{11} $–$ 10^{16} $ eV is a crucial region for the understanding of the cosmic-ray acceleration and propagation in the interstellar medium. The NUCLEON detector has been data taken since December, 2014. The NUCLEON trigger system and CR event selection are described, including the beam tests at the SPS CERN, flight tests in orbit and the Monte-Carlo simulation.</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Grebenyuk, V. M.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Karmanov, D. M.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Pan, A.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Podorozhny, D. 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