The proton-air cross-section at $ 10^{16} $ eV
Summary A study of the Čerenkov light lateral distribution function for cosmic-ray showers with energies of about $ 10^{16} $ eV has been used to determine the distribution of depths of shower maximum at these energies. This distribution has an exponential tail due to fluctuations in the depths of e...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Dawson, B. R. [verfasserIn] |
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| Format: |
Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
1986 |
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| Anmerkung: |
© Società Italiana di Fisica 1986 |
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| Übergeordnetes Werk: |
Enthalten in: Il Nuovo Cimento C - Kluwer Academic Publishers, 1978, 9(1986), 6 vom: Nov., Seite 1125-1129 |
|---|---|
| Übergeordnetes Werk: |
volume:9 ; year:1986 ; number:6 ; month:11 ; pages:1125-1129 |
| Links: |
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| DOI / URN: |
10.1007/BF02507429 |
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| 520 | |a Summary A study of the Čerenkov light lateral distribution function for cosmic-ray showers with energies of about $ 10^{16} $ eV has been used to determine the distribution of depths of shower maximum at these energies. This distribution has an exponential tail due to fluctuations in the depths of early interactions of the proton primary component. The form of this tail may be used to infer an inelastic proton-air cross-section of (590±70) mb at ≈$ 10^{16} $ eV. | ||
| 700 | 1 | |a Clay, R. W. |4 aut | |
| 700 | 1 | |a Edwards, P. G. |4 aut | |
| 700 | 1 | |a Prescott, J. R. |4 aut | |
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10.1007/BF02507429 doi (DE-627)OLC2055367250 (DE-He213)BF02507429-p DE-627 ger DE-627 rakwb eng 530 VZ 16,13 ssgn Dawson, B. R. verfasserin aut The proton-air cross-section at $ 10^{16} $ eV 1986 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Società Italiana di Fisica 1986 Summary A study of the Čerenkov light lateral distribution function for cosmic-ray showers with energies of about $ 10^{16} $ eV has been used to determine the distribution of depths of shower maximum at these energies. This distribution has an exponential tail due to fluctuations in the depths of early interactions of the proton primary component. The form of this tail may be used to infer an inelastic proton-air cross-section of (590±70) mb at ≈$ 10^{16} $ eV. Clay, R. W. aut Edwards, P. G. aut Prescott, J. R. aut Enthalten in Il Nuovo Cimento C Kluwer Academic Publishers, 1978 9(1986), 6 vom: Nov., Seite 1125-1129 (DE-627)129367362 (DE-600)161886-6 (DE-576)014741970 1124-1896 nnns volume:9 year:1986 number:6 month:11 pages:1125-1129 https://doi.org/10.1007/BF02507429 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-GEO SSG-OLC-AST SSG-OPC-GGO SSG-OPC-GEO SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_24 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_130 GBV_ILN_2012 GBV_ILN_4046 GBV_ILN_4103 GBV_ILN_4155 GBV_ILN_4319 GBV_ILN_4323 AR 9 1986 6 11 1125-1129 |
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10.1007/BF02507429 doi (DE-627)OLC2055367250 (DE-He213)BF02507429-p DE-627 ger DE-627 rakwb eng 530 VZ 16,13 ssgn Dawson, B. R. verfasserin aut The proton-air cross-section at $ 10^{16} $ eV 1986 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Società Italiana di Fisica 1986 Summary A study of the Čerenkov light lateral distribution function for cosmic-ray showers with energies of about $ 10^{16} $ eV has been used to determine the distribution of depths of shower maximum at these energies. This distribution has an exponential tail due to fluctuations in the depths of early interactions of the proton primary component. The form of this tail may be used to infer an inelastic proton-air cross-section of (590±70) mb at ≈$ 10^{16} $ eV. Clay, R. W. aut Edwards, P. G. aut Prescott, J. R. aut Enthalten in Il Nuovo Cimento C Kluwer Academic Publishers, 1978 9(1986), 6 vom: Nov., Seite 1125-1129 (DE-627)129367362 (DE-600)161886-6 (DE-576)014741970 1124-1896 nnns volume:9 year:1986 number:6 month:11 pages:1125-1129 https://doi.org/10.1007/BF02507429 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-GEO SSG-OLC-AST SSG-OPC-GGO SSG-OPC-GEO SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_24 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_130 GBV_ILN_2012 GBV_ILN_4046 GBV_ILN_4103 GBV_ILN_4155 GBV_ILN_4319 GBV_ILN_4323 AR 9 1986 6 11 1125-1129 |
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10.1007/BF02507429 doi (DE-627)OLC2055367250 (DE-He213)BF02507429-p DE-627 ger DE-627 rakwb eng 530 VZ 16,13 ssgn Dawson, B. R. verfasserin aut The proton-air cross-section at $ 10^{16} $ eV 1986 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Società Italiana di Fisica 1986 Summary A study of the Čerenkov light lateral distribution function for cosmic-ray showers with energies of about $ 10^{16} $ eV has been used to determine the distribution of depths of shower maximum at these energies. This distribution has an exponential tail due to fluctuations in the depths of early interactions of the proton primary component. The form of this tail may be used to infer an inelastic proton-air cross-section of (590±70) mb at ≈$ 10^{16} $ eV. Clay, R. W. aut Edwards, P. G. aut Prescott, J. R. aut Enthalten in Il Nuovo Cimento C Kluwer Academic Publishers, 1978 9(1986), 6 vom: Nov., Seite 1125-1129 (DE-627)129367362 (DE-600)161886-6 (DE-576)014741970 1124-1896 nnns volume:9 year:1986 number:6 month:11 pages:1125-1129 https://doi.org/10.1007/BF02507429 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-GEO SSG-OLC-AST SSG-OPC-GGO SSG-OPC-GEO SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_24 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_130 GBV_ILN_2012 GBV_ILN_4046 GBV_ILN_4103 GBV_ILN_4155 GBV_ILN_4319 GBV_ILN_4323 AR 9 1986 6 11 1125-1129 |
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10.1007/BF02507429 doi (DE-627)OLC2055367250 (DE-He213)BF02507429-p DE-627 ger DE-627 rakwb eng 530 VZ 16,13 ssgn Dawson, B. R. verfasserin aut The proton-air cross-section at $ 10^{16} $ eV 1986 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Società Italiana di Fisica 1986 Summary A study of the Čerenkov light lateral distribution function for cosmic-ray showers with energies of about $ 10^{16} $ eV has been used to determine the distribution of depths of shower maximum at these energies. This distribution has an exponential tail due to fluctuations in the depths of early interactions of the proton primary component. The form of this tail may be used to infer an inelastic proton-air cross-section of (590±70) mb at ≈$ 10^{16} $ eV. Clay, R. W. aut Edwards, P. G. aut Prescott, J. R. aut Enthalten in Il Nuovo Cimento C Kluwer Academic Publishers, 1978 9(1986), 6 vom: Nov., Seite 1125-1129 (DE-627)129367362 (DE-600)161886-6 (DE-576)014741970 1124-1896 nnns volume:9 year:1986 number:6 month:11 pages:1125-1129 https://doi.org/10.1007/BF02507429 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-GEO SSG-OLC-AST SSG-OPC-GGO SSG-OPC-GEO SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_24 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_130 GBV_ILN_2012 GBV_ILN_4046 GBV_ILN_4103 GBV_ILN_4155 GBV_ILN_4319 GBV_ILN_4323 AR 9 1986 6 11 1125-1129 |
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10.1007/BF02507429 doi (DE-627)OLC2055367250 (DE-He213)BF02507429-p DE-627 ger DE-627 rakwb eng 530 VZ 16,13 ssgn Dawson, B. R. verfasserin aut The proton-air cross-section at $ 10^{16} $ eV 1986 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Società Italiana di Fisica 1986 Summary A study of the Čerenkov light lateral distribution function for cosmic-ray showers with energies of about $ 10^{16} $ eV has been used to determine the distribution of depths of shower maximum at these energies. This distribution has an exponential tail due to fluctuations in the depths of early interactions of the proton primary component. The form of this tail may be used to infer an inelastic proton-air cross-section of (590±70) mb at ≈$ 10^{16} $ eV. Clay, R. W. aut Edwards, P. G. aut Prescott, J. R. aut Enthalten in Il Nuovo Cimento C Kluwer Academic Publishers, 1978 9(1986), 6 vom: Nov., Seite 1125-1129 (DE-627)129367362 (DE-600)161886-6 (DE-576)014741970 1124-1896 nnns volume:9 year:1986 number:6 month:11 pages:1125-1129 https://doi.org/10.1007/BF02507429 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-GEO SSG-OLC-AST SSG-OPC-GGO SSG-OPC-GEO SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_24 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_130 GBV_ILN_2012 GBV_ILN_4046 GBV_ILN_4103 GBV_ILN_4155 GBV_ILN_4319 GBV_ILN_4323 AR 9 1986 6 11 1125-1129 |
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the proton-air cross-section at $ 10^{16} $ ev |
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The proton-air cross-section at $ 10^{16} $ eV |
| abstract |
Summary A study of the Čerenkov light lateral distribution function for cosmic-ray showers with energies of about $ 10^{16} $ eV has been used to determine the distribution of depths of shower maximum at these energies. This distribution has an exponential tail due to fluctuations in the depths of early interactions of the proton primary component. The form of this tail may be used to infer an inelastic proton-air cross-section of (590±70) mb at ≈$ 10^{16} $ eV. © Società Italiana di Fisica 1986 |
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Summary A study of the Čerenkov light lateral distribution function for cosmic-ray showers with energies of about $ 10^{16} $ eV has been used to determine the distribution of depths of shower maximum at these energies. This distribution has an exponential tail due to fluctuations in the depths of early interactions of the proton primary component. The form of this tail may be used to infer an inelastic proton-air cross-section of (590±70) mb at ≈$ 10^{16} $ eV. © Società Italiana di Fisica 1986 |
| abstract_unstemmed |
Summary A study of the Čerenkov light lateral distribution function for cosmic-ray showers with energies of about $ 10^{16} $ eV has been used to determine the distribution of depths of shower maximum at these energies. This distribution has an exponential tail due to fluctuations in the depths of early interactions of the proton primary component. The form of this tail may be used to infer an inelastic proton-air cross-section of (590±70) mb at ≈$ 10^{16} $ eV. © Società Italiana di Fisica 1986 |
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The proton-air cross-section at $ 10^{16} $ eV |
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Clay, R. W. Edwards, P. G. Prescott, J. R. |
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