Testing the prototype of the NUCLEON setup on the pion beam of the SPS accelerator (CERN)
Abstract A technique for determining the energy of primary cosmic rays in the range of $ 10^{12} $–$ 10^{15} $ eV has been developed. The idea behind this technique consists in measuring the spatial flux density of secondary particles produced in the first act of inelastic nuclear interaction inside...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Voronin, A. G. [verfasserIn] |
|---|
| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2007 |
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| Anmerkung: |
© Pleiades Publishing, Ltd. 2007 |
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| Übergeordnetes Werk: |
Enthalten in: Instruments and experimental techniques - Nauka/Interperiodica, 1959, 50(2007), 2 vom: März, Seite 176-186 |
|---|---|
| Übergeordnetes Werk: |
volume:50 ; year:2007 ; number:2 ; month:03 ; pages:176-186 |
| Links: |
|---|
| DOI / URN: |
10.1134/S0020441207020029 |
|---|
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OLC203414564X |
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| 520 | |a Abstract A technique for determining the energy of primary cosmic rays in the range of $ 10^{12} $–$ 10^{15} $ eV has been developed. The idea behind this technique consists in measuring the spatial flux density of secondary particles produced in the first act of inelastic nuclear interaction inside a target and passed through a thin converter layer in which the electromagnetic component (photons from decays of neutral pions) is multiplied. This technique has been developed by generalizing the well-known Castagnoli method (for measuring the angular characteristics of tracks of secondary particles produced in the first act of inelastic nuclear interaction inside a target), and its application offers a chance to design instruments for scientific studies such that their mass is relatively low while their luminosity is high. It is proposed to use this technique in a satellite-based NUCLEON experiment. The technique has been tested on charged particle beams of the SPS accelerator at CERN. Results of these tests confirm that, using this method, it is possible to measure the particle energy and, therefore, perform an orbital scientific experiment with the proposed equipment. | ||
| 700 | 1 | |a Grebenyuk, V. M. |4 aut | |
| 700 | 1 | |a Karmanov, D. E. |4 aut | |
| 700 | 1 | |a Korotkova, N. A. |4 aut | |
| 700 | 1 | |a Krumshtein, Z. V. |4 aut | |
| 700 | 1 | |a Merkin, M. M. |4 aut | |
| 700 | 1 | |a Pakhomov, A. Yu. |4 aut | |
| 700 | 1 | |a Podorozhnyi, D. M. |4 aut | |
| 700 | 1 | |a Sadovskii, A. B. |4 aut | |
| 700 | 1 | |a Sveshnikova, L. G. |4 aut | |
| 700 | 1 | |a Tkachev, L. G. |4 aut | |
| 700 | 1 | |a Turundaevskii, A. N. |4 aut | |
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10.1134/S0020441207020029 doi (DE-627)OLC203414564X (DE-He213)S0020441207020029-p DE-627 ger DE-627 rakwb eng 620 VZ 11 ssgn Voronin, A. G. verfasserin aut Testing the prototype of the NUCLEON setup on the pion beam of the SPS accelerator (CERN) 2007 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2007 Abstract A technique for determining the energy of primary cosmic rays in the range of $ 10^{12} $–$ 10^{15} $ eV has been developed. The idea behind this technique consists in measuring the spatial flux density of secondary particles produced in the first act of inelastic nuclear interaction inside a target and passed through a thin converter layer in which the electromagnetic component (photons from decays of neutral pions) is multiplied. This technique has been developed by generalizing the well-known Castagnoli method (for measuring the angular characteristics of tracks of secondary particles produced in the first act of inelastic nuclear interaction inside a target), and its application offers a chance to design instruments for scientific studies such that their mass is relatively low while their luminosity is high. It is proposed to use this technique in a satellite-based NUCLEON experiment. The technique has been tested on charged particle beams of the SPS accelerator at CERN. Results of these tests confirm that, using this method, it is possible to measure the particle energy and, therefore, perform an orbital scientific experiment with the proposed equipment. Grebenyuk, V. M. aut Karmanov, D. E. aut Korotkova, N. A. aut Krumshtein, Z. V. aut Merkin, M. M. aut Pakhomov, A. Yu. aut Podorozhnyi, D. M. aut Sadovskii, A. B. aut Sveshnikova, L. G. aut Tkachev, L. G. aut Turundaevskii, A. N. aut Enthalten in Instruments and experimental techniques Nauka/Interperiodica, 1959 50(2007), 2 vom: März, Seite 176-186 (DE-627)129603007 (DE-600)241643-8 (DE-576)015096815 0020-4412 nnns volume:50 year:2007 number:2 month:03 pages:176-186 https://doi.org/10.1134/S0020441207020029 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY GBV_ILN_40 GBV_ILN_70 AR 50 2007 2 03 176-186 |
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10.1134/S0020441207020029 doi (DE-627)OLC203414564X (DE-He213)S0020441207020029-p DE-627 ger DE-627 rakwb eng 620 VZ 11 ssgn Voronin, A. G. verfasserin aut Testing the prototype of the NUCLEON setup on the pion beam of the SPS accelerator (CERN) 2007 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2007 Abstract A technique for determining the energy of primary cosmic rays in the range of $ 10^{12} $–$ 10^{15} $ eV has been developed. The idea behind this technique consists in measuring the spatial flux density of secondary particles produced in the first act of inelastic nuclear interaction inside a target and passed through a thin converter layer in which the electromagnetic component (photons from decays of neutral pions) is multiplied. This technique has been developed by generalizing the well-known Castagnoli method (for measuring the angular characteristics of tracks of secondary particles produced in the first act of inelastic nuclear interaction inside a target), and its application offers a chance to design instruments for scientific studies such that their mass is relatively low while their luminosity is high. It is proposed to use this technique in a satellite-based NUCLEON experiment. The technique has been tested on charged particle beams of the SPS accelerator at CERN. Results of these tests confirm that, using this method, it is possible to measure the particle energy and, therefore, perform an orbital scientific experiment with the proposed equipment. Grebenyuk, V. M. aut Karmanov, D. E. aut Korotkova, N. A. aut Krumshtein, Z. V. aut Merkin, M. M. aut Pakhomov, A. Yu. aut Podorozhnyi, D. M. aut Sadovskii, A. B. aut Sveshnikova, L. G. aut Tkachev, L. G. aut Turundaevskii, A. N. aut Enthalten in Instruments and experimental techniques Nauka/Interperiodica, 1959 50(2007), 2 vom: März, Seite 176-186 (DE-627)129603007 (DE-600)241643-8 (DE-576)015096815 0020-4412 nnns volume:50 year:2007 number:2 month:03 pages:176-186 https://doi.org/10.1134/S0020441207020029 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY GBV_ILN_40 GBV_ILN_70 AR 50 2007 2 03 176-186 |
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10.1134/S0020441207020029 doi (DE-627)OLC203414564X (DE-He213)S0020441207020029-p DE-627 ger DE-627 rakwb eng 620 VZ 11 ssgn Voronin, A. G. verfasserin aut Testing the prototype of the NUCLEON setup on the pion beam of the SPS accelerator (CERN) 2007 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2007 Abstract A technique for determining the energy of primary cosmic rays in the range of $ 10^{12} $–$ 10^{15} $ eV has been developed. The idea behind this technique consists in measuring the spatial flux density of secondary particles produced in the first act of inelastic nuclear interaction inside a target and passed through a thin converter layer in which the electromagnetic component (photons from decays of neutral pions) is multiplied. This technique has been developed by generalizing the well-known Castagnoli method (for measuring the angular characteristics of tracks of secondary particles produced in the first act of inelastic nuclear interaction inside a target), and its application offers a chance to design instruments for scientific studies such that their mass is relatively low while their luminosity is high. It is proposed to use this technique in a satellite-based NUCLEON experiment. The technique has been tested on charged particle beams of the SPS accelerator at CERN. Results of these tests confirm that, using this method, it is possible to measure the particle energy and, therefore, perform an orbital scientific experiment with the proposed equipment. Grebenyuk, V. M. aut Karmanov, D. E. aut Korotkova, N. A. aut Krumshtein, Z. V. aut Merkin, M. M. aut Pakhomov, A. Yu. aut Podorozhnyi, D. M. aut Sadovskii, A. B. aut Sveshnikova, L. G. aut Tkachev, L. G. aut Turundaevskii, A. N. aut Enthalten in Instruments and experimental techniques Nauka/Interperiodica, 1959 50(2007), 2 vom: März, Seite 176-186 (DE-627)129603007 (DE-600)241643-8 (DE-576)015096815 0020-4412 nnns volume:50 year:2007 number:2 month:03 pages:176-186 https://doi.org/10.1134/S0020441207020029 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY GBV_ILN_40 GBV_ILN_70 AR 50 2007 2 03 176-186 |
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10.1134/S0020441207020029 doi (DE-627)OLC203414564X (DE-He213)S0020441207020029-p DE-627 ger DE-627 rakwb eng 620 VZ 11 ssgn Voronin, A. G. verfasserin aut Testing the prototype of the NUCLEON setup on the pion beam of the SPS accelerator (CERN) 2007 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2007 Abstract A technique for determining the energy of primary cosmic rays in the range of $ 10^{12} $–$ 10^{15} $ eV has been developed. The idea behind this technique consists in measuring the spatial flux density of secondary particles produced in the first act of inelastic nuclear interaction inside a target and passed through a thin converter layer in which the electromagnetic component (photons from decays of neutral pions) is multiplied. This technique has been developed by generalizing the well-known Castagnoli method (for measuring the angular characteristics of tracks of secondary particles produced in the first act of inelastic nuclear interaction inside a target), and its application offers a chance to design instruments for scientific studies such that their mass is relatively low while their luminosity is high. It is proposed to use this technique in a satellite-based NUCLEON experiment. The technique has been tested on charged particle beams of the SPS accelerator at CERN. Results of these tests confirm that, using this method, it is possible to measure the particle energy and, therefore, perform an orbital scientific experiment with the proposed equipment. Grebenyuk, V. M. aut Karmanov, D. E. aut Korotkova, N. A. aut Krumshtein, Z. V. aut Merkin, M. M. aut Pakhomov, A. Yu. aut Podorozhnyi, D. M. aut Sadovskii, A. B. aut Sveshnikova, L. G. aut Tkachev, L. G. aut Turundaevskii, A. N. aut Enthalten in Instruments and experimental techniques Nauka/Interperiodica, 1959 50(2007), 2 vom: März, Seite 176-186 (DE-627)129603007 (DE-600)241643-8 (DE-576)015096815 0020-4412 nnns volume:50 year:2007 number:2 month:03 pages:176-186 https://doi.org/10.1134/S0020441207020029 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY GBV_ILN_40 GBV_ILN_70 AR 50 2007 2 03 176-186 |
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10.1134/S0020441207020029 doi (DE-627)OLC203414564X (DE-He213)S0020441207020029-p DE-627 ger DE-627 rakwb eng 620 VZ 11 ssgn Voronin, A. G. verfasserin aut Testing the prototype of the NUCLEON setup on the pion beam of the SPS accelerator (CERN) 2007 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2007 Abstract A technique for determining the energy of primary cosmic rays in the range of $ 10^{12} $–$ 10^{15} $ eV has been developed. The idea behind this technique consists in measuring the spatial flux density of secondary particles produced in the first act of inelastic nuclear interaction inside a target and passed through a thin converter layer in which the electromagnetic component (photons from decays of neutral pions) is multiplied. This technique has been developed by generalizing the well-known Castagnoli method (for measuring the angular characteristics of tracks of secondary particles produced in the first act of inelastic nuclear interaction inside a target), and its application offers a chance to design instruments for scientific studies such that their mass is relatively low while their luminosity is high. It is proposed to use this technique in a satellite-based NUCLEON experiment. The technique has been tested on charged particle beams of the SPS accelerator at CERN. Results of these tests confirm that, using this method, it is possible to measure the particle energy and, therefore, perform an orbital scientific experiment with the proposed equipment. Grebenyuk, V. M. aut Karmanov, D. E. aut Korotkova, N. A. aut Krumshtein, Z. V. aut Merkin, M. M. aut Pakhomov, A. Yu. aut Podorozhnyi, D. M. aut Sadovskii, A. B. aut Sveshnikova, L. G. aut Tkachev, L. G. aut Turundaevskii, A. N. aut Enthalten in Instruments and experimental techniques Nauka/Interperiodica, 1959 50(2007), 2 vom: März, Seite 176-186 (DE-627)129603007 (DE-600)241643-8 (DE-576)015096815 0020-4412 nnns volume:50 year:2007 number:2 month:03 pages:176-186 https://doi.org/10.1134/S0020441207020029 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY GBV_ILN_40 GBV_ILN_70 AR 50 2007 2 03 176-186 |
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Testing the prototype of the NUCLEON setup on the pion beam of the SPS accelerator (CERN) |
| author_sort |
Voronin, A. G. |
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Instruments and experimental techniques |
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Instruments and experimental techniques |
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eng |
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600 - Technology |
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2007 |
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176 |
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Voronin, A. G. Grebenyuk, V. M. Karmanov, D. E. Korotkova, N. A. Krumshtein, Z. V. Merkin, M. M. Pakhomov, A. Yu. Podorozhnyi, D. M. Sadovskii, A. B. Sveshnikova, L. G. Tkachev, L. G. Turundaevskii, A. N. |
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50 |
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620 VZ 11 ssgn |
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Aufsätze |
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Voronin, A. G. |
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10.1134/S0020441207020029 |
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620 |
| title_sort |
testing the prototype of the nucleon setup on the pion beam of the sps accelerator (cern) |
| title_auth |
Testing the prototype of the NUCLEON setup on the pion beam of the SPS accelerator (CERN) |
| abstract |
Abstract A technique for determining the energy of primary cosmic rays in the range of $ 10^{12} $–$ 10^{15} $ eV has been developed. The idea behind this technique consists in measuring the spatial flux density of secondary particles produced in the first act of inelastic nuclear interaction inside a target and passed through a thin converter layer in which the electromagnetic component (photons from decays of neutral pions) is multiplied. This technique has been developed by generalizing the well-known Castagnoli method (for measuring the angular characteristics of tracks of secondary particles produced in the first act of inelastic nuclear interaction inside a target), and its application offers a chance to design instruments for scientific studies such that their mass is relatively low while their luminosity is high. It is proposed to use this technique in a satellite-based NUCLEON experiment. The technique has been tested on charged particle beams of the SPS accelerator at CERN. Results of these tests confirm that, using this method, it is possible to measure the particle energy and, therefore, perform an orbital scientific experiment with the proposed equipment. © Pleiades Publishing, Ltd. 2007 |
| abstractGer |
Abstract A technique for determining the energy of primary cosmic rays in the range of $ 10^{12} $–$ 10^{15} $ eV has been developed. The idea behind this technique consists in measuring the spatial flux density of secondary particles produced in the first act of inelastic nuclear interaction inside a target and passed through a thin converter layer in which the electromagnetic component (photons from decays of neutral pions) is multiplied. This technique has been developed by generalizing the well-known Castagnoli method (for measuring the angular characteristics of tracks of secondary particles produced in the first act of inelastic nuclear interaction inside a target), and its application offers a chance to design instruments for scientific studies such that their mass is relatively low while their luminosity is high. It is proposed to use this technique in a satellite-based NUCLEON experiment. The technique has been tested on charged particle beams of the SPS accelerator at CERN. Results of these tests confirm that, using this method, it is possible to measure the particle energy and, therefore, perform an orbital scientific experiment with the proposed equipment. © Pleiades Publishing, Ltd. 2007 |
| abstract_unstemmed |
Abstract A technique for determining the energy of primary cosmic rays in the range of $ 10^{12} $–$ 10^{15} $ eV has been developed. The idea behind this technique consists in measuring the spatial flux density of secondary particles produced in the first act of inelastic nuclear interaction inside a target and passed through a thin converter layer in which the electromagnetic component (photons from decays of neutral pions) is multiplied. This technique has been developed by generalizing the well-known Castagnoli method (for measuring the angular characteristics of tracks of secondary particles produced in the first act of inelastic nuclear interaction inside a target), and its application offers a chance to design instruments for scientific studies such that their mass is relatively low while their luminosity is high. It is proposed to use this technique in a satellite-based NUCLEON experiment. The technique has been tested on charged particle beams of the SPS accelerator at CERN. Results of these tests confirm that, using this method, it is possible to measure the particle energy and, therefore, perform an orbital scientific experiment with the proposed equipment. © Pleiades Publishing, Ltd. 2007 |
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| title_short |
Testing the prototype of the NUCLEON setup on the pion beam of the SPS accelerator (CERN) |
| url |
https://doi.org/10.1134/S0020441207020029 |
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Grebenyuk, V. M. Karmanov, D. E. Korotkova, N. A. Krumshtein, Z. V. Merkin, M. M. Pakhomov, A. Yu Podorozhnyi, D. M. Sadovskii, A. B. Sveshnikova, L. G. Tkachev, L. G. Turundaevskii, A. N. |
| author2Str |
Grebenyuk, V. M. Karmanov, D. E. Korotkova, N. A. Krumshtein, Z. V. Merkin, M. M. Pakhomov, A. Yu Podorozhnyi, D. M. Sadovskii, A. B. Sveshnikova, L. G. Tkachev, L. G. Turundaevskii, A. N. |
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