Neutron flux generated by cosmic-ray muons at 5200 hg/cm2s.r. underground. Depth-neutron intensity curve
- Author
- AGLIETTA, M1 ; BADINO, G; DADYKIN, V. L; KHALCHUKOV, F. F; KORTCHAGUIN, V. B; KORTCHAGUIN, P. V; KUDRYAVTSEV, V. A; MALGUIN, A. S; RYASNY, V. G; RYAZHSKAYA, O. G; YAKUSHEV, V. F; ZATSEPIN, G. T; BOLOGNA, C; CASTAGNOLI, C; CASTELLINA, A; FULGIONE, W; GALEOTTI, P; SAAVEDRA, O; TRINCHERO, G; VERNETTO, S
[1] CNR, ist. gosmogeofisica, Torino, Italy - Source
Nuovo cimento della società italiana di fisica. C. 1989, Vol 12, Num 4, pp 469-477 ; ref : dissem
- ISSN
- 0390-5551
- Scientific domain
- Astronomy earth cosmic environment; Geophysics
- Publisher
- Compositori, Bologna
- Publication country
- Italy
- Document type
- Article
- Language
- English
- Keyword (fr)
- Distribution temporelle Détecteur particule Mesure souterraine Multiplicité Muon Neutron Rayonnement cosmique
- Keyword (en)
- Time distribution Particle detector Underground measurement Multiplicity Muon Neutrons Cosmic ray
- Keyword (es)
- Distribución temporal Detector partícula Medida subterránea Multiplicidad Muón Neutrón Radiación cósmica
- Classification
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03B Solar system / 001E03B40 Cosmic rays
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 6688648
Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS
Access to the document
Install on your browser
DOI
10.1007/BF02525079 
https://dx.doi.org/10.1007/BF02525079
"O:13:\"PanistOpenUrl\":36:{s:10:\"\u0000*\u0000openUrl\";N;s:6:\"\u0000*\u0000idc\";N;s:6:\"\u0000*\u0000fmt\";s:7:\"journal\";s:6:\"\u0000*\u0000doi\";s:18:\"10.1007\/BF02525079\";s:6:\"\u0000*\u0000pii\";s:0:\"\";s:7:\"\u0000*\u0000pmid\";s:0:\"\";s:9:\"\u0000*\u0000atitle\";s:104:\"Neutron flux generated by cosmic-ray muons at 5200 hg\/cm2s.r. underground. Depth-neutron intensity curve\";s:9:\"\u0000*\u0000jtitle\";s:50:\"Nuovo cimento della societ\u00e0 italiana di fisica. C\";s:9:\"\u0000*\u0000stitle\";s:32:\"Nuovo cimento Soc. ital. fis., C\";s:7:\"\u0000*\u0000date\";s:4:\"1989\";s:9:\"\u0000*\u0000volume\";s:2:\"12\";s:8:\"\u0000*\u0000issue\";s:1:\"4\";s:8:\"\u0000*\u0000spage\";s:3:\"469\";s:8:\"\u0000*\u0000epage\";s:3:\"477\";s:8:\"\u0000*\u0000pages\";s:0:\"\";s:7:\"\u0000*\u0000issn\";s:9:\"0390-5551\";s:8:\"\u0000*\u0000eissn\";s:0:\"\";s:9:\"\u0000*\u0000aulast\";s:8:\"AGLIETTA\";s:10:\"\u0000*\u0000aufirst\";s:1:\"M\";s:9:\"\u0000*\u0000auinit\";s:0:\"\";s:10:\"\u0000*\u0000auinitm\";s:0:\"\";s:5:\"\u0000*\u0000au\";a:19:{i:0;s:9:\"BADINO, G\";i:1;s:13:\"DADYKIN, V. L\";i:2;s:16:\"KHALCHUKOV, F. F\";i:3;s:17:\"KORTCHAGUIN, V. B\";i:4;s:17:\"KORTCHAGUIN, P. V\";i:5;s:17:\"KUDRYAVTSEV, V. A\";i:6;s:13:\"MALGUIN, A. S\";i:7;s:12:\"RYASNY, V. G\";i:8;s:16:\"RYAZHSKAYA, O. G\";i:9;s:14:\"YAKUSHEV, V. F\";i:10;s:14:\"ZATSEPIN, G. T\";i:11;s:10:\"BOLOGNA, C\";i:12;s:13:\"CASTAGNOLI, C\";i:13;s:13:\"CASTELLINA, A\";i:14;s:11:\"FULGIONE, W\";i:15;s:11:\"GALEOTTI, P\";i:16;s:11:\"SAAVEDRA, O\";i:17;s:12:\"TRINCHERO, G\";i:18;s:11:\"VERNETTO, S\";}s:9:\"\u0000*\u0000aucorp\";s:0:\"\";s:7:\"\u0000*\u0000isbn\";s:0:\"\";s:8:\"\u0000*\u0000coden\";s:0:\"\";s:8:\"\u0000*\u0000genre\";s:7:\"article\";s:7:\"\u0000*\u0000part\";s:0:\"\";s:9:\"\u0000*\u0000btitle\";s:0:\"\";s:8:\"\u0000*\u0000title\";s:104:\"Neutron flux generated by cosmic-ray muons at 5200 hg\/cm2s.r. underground. Depth-neutron intensity curve\";s:8:\"\u0000*\u0000place\";s:7:\"Bologna\";s:6:\"\u0000*\u0000pub\";s:11:\"Compositori\";s:10:\"\u0000*\u0000edition\";s:0:\"\";s:9:\"\u0000*\u0000tpages\";s:0:\"\";s:9:\"\u0000*\u0000series\";s:0:\"\";s:8:\"\u0000*\u0000proxy\";s:30:\"http:\/\/proxyout.inist.fr:8080\/\";s:12:\"\u0000*\u0000integrite\";b:1;}"
Panist access
"O:12:\"IstexOpenUrl\":35:{s:10:\"\u0000*\u0000openUrl\";N;s:6:\"\u0000*\u0000fmt\";s:7:\"journal\";s:6:\"\u0000*\u0000doi\";s:18:\"10.1007\/BF02525079\";s:6:\"\u0000*\u0000pii\";s:0:\"\";s:7:\"\u0000*\u0000pmid\";s:0:\"\";s:9:\"\u0000*\u0000atitle\";s:104:\"Neutron flux generated by cosmic-ray muons at 5200 hg\/cm2s.r. underground. Depth-neutron intensity curve\";s:9:\"\u0000*\u0000jtitle\";s:50:\"Nuovo cimento della societ\u00e0 italiana di fisica. C\";s:9:\"\u0000*\u0000stitle\";s:32:\"Nuovo cimento Soc. ital. fis., C\";s:7:\"\u0000*\u0000date\";s:4:\"1989\";s:9:\"\u0000*\u0000volume\";s:2:\"12\";s:8:\"\u0000*\u0000issue\";s:1:\"4\";s:8:\"\u0000*\u0000spage\";s:3:\"469\";s:8:\"\u0000*\u0000epage\";s:3:\"477\";s:8:\"\u0000*\u0000pages\";s:0:\"\";s:7:\"\u0000*\u0000issn\";s:9:\"0390-5551\";s:8:\"\u0000*\u0000eissn\";s:0:\"\";s:9:\"\u0000*\u0000aulast\";s:8:\"AGLIETTA\";s:10:\"\u0000*\u0000aufirst\";s:1:\"M\";s:9:\"\u0000*\u0000auinit\";s:0:\"\";s:10:\"\u0000*\u0000auinitm\";s:0:\"\";s:5:\"\u0000*\u0000au\";a:19:{i:0;s:9:\"BADINO, G\";i:1;s:13:\"DADYKIN, V. L\";i:2;s:16:\"KHALCHUKOV, F. F\";i:3;s:17:\"KORTCHAGUIN, V. B\";i:4;s:17:\"KORTCHAGUIN, P. V\";i:5;s:17:\"KUDRYAVTSEV, V. A\";i:6;s:13:\"MALGUIN, A. S\";i:7;s:12:\"RYASNY, V. G\";i:8;s:16:\"RYAZHSKAYA, O. G\";i:9;s:14:\"YAKUSHEV, V. F\";i:10;s:14:\"ZATSEPIN, G. T\";i:11;s:10:\"BOLOGNA, C\";i:12;s:13:\"CASTAGNOLI, C\";i:13;s:13:\"CASTELLINA, A\";i:14;s:11:\"FULGIONE, W\";i:15;s:11:\"GALEOTTI, P\";i:16;s:11:\"SAAVEDRA, O\";i:17;s:12:\"TRINCHERO, G\";i:18;s:11:\"VERNETTO, S\";}s:9:\"\u0000*\u0000aucorp\";s:0:\"\";s:7:\"\u0000*\u0000isbn\";s:0:\"\";s:8:\"\u0000*\u0000coden\";s:0:\"\";s:8:\"\u0000*\u0000genre\";s:7:\"article\";s:7:\"\u0000*\u0000part\";s:0:\"\";s:9:\"\u0000*\u0000btitle\";s:0:\"\";s:8:\"\u0000*\u0000title\";s:104:\"Neutron flux generated by cosmic-ray muons at 5200 hg\/cm2s.r. underground. Depth-neutron intensity curve\";s:8:\"\u0000*\u0000place\";s:7:\"Bologna\";s:6:\"\u0000*\u0000pub\";s:11:\"Compositori\";s:10:\"\u0000*\u0000edition\";s:0:\"\";s:9:\"\u0000*\u0000tpages\";s:0:\"\";s:9:\"\u0000*\u0000series\";s:0:\"\";s:8:\"\u0000*\u0000proxy\";s:30:\"http:\/\/proxyout.inist.fr:8080\/\";s:12:\"\u0000*\u0000integrite\";b:1;}"
Istex access
"O:16:\"UnpaywallOpenUrl\":35:{s:8:\"\u0000*\u0000email\";s:27:\"assistance-portail@inist.fr\";s:6:\"\u0000*\u0000fmt\";N;s:6:\"\u0000*\u0000doi\";s:18:\"10.1007\/BF02525079\";s:6:\"\u0000*\u0000pii\";N;s:7:\"\u0000*\u0000pmid\";N;s:9:\"\u0000*\u0000atitle\";N;s:9:\"\u0000*\u0000jtitle\";N;s:9:\"\u0000*\u0000stitle\";N;s:7:\"\u0000*\u0000date\";N;s:9:\"\u0000*\u0000volume\";N;s:8:\"\u0000*\u0000issue\";N;s:8:\"\u0000*\u0000spage\";N;s:8:\"\u0000*\u0000epage\";N;s:8:\"\u0000*\u0000pages\";N;s:7:\"\u0000*\u0000issn\";N;s:8:\"\u0000*\u0000eissn\";N;s:9:\"\u0000*\u0000aulast\";N;s:10:\"\u0000*\u0000aufirst\";N;s:9:\"\u0000*\u0000auinit\";N;s:10:\"\u0000*\u0000auinitm\";N;s:5:\"\u0000*\u0000au\";N;s:9:\"\u0000*\u0000aucorp\";N;s:7:\"\u0000*\u0000isbn\";N;s:8:\"\u0000*\u0000coden\";N;s:8:\"\u0000*\u0000genre\";N;s:7:\"\u0000*\u0000part\";N;s:9:\"\u0000*\u0000btitle\";N;s:8:\"\u0000*\u0000title\";N;s:8:\"\u0000*\u0000place\";N;s:6:\"\u0000*\u0000pub\";N;s:10:\"\u0000*\u0000edition\";N;s:9:\"\u0000*\u0000tpages\";N;s:9:\"\u0000*\u0000series\";N;s:8:\"\u0000*\u0000proxy\";s:30:\"http:\/\/proxyout.inist.fr:8080\/\";s:12:\"\u0000*\u0000integrite\";N;}"
Unpaywall access
"O:16:\"EuropePMCOpenUrl\":35:{s:10:\"\u0000*\u0000openUrl\";N;s:6:\"\u0000*\u0000fmt\";s:7:\"journal\";s:6:\"\u0000*\u0000doi\";s:18:\"10.1007\/BF02525079\";s:6:\"\u0000*\u0000pii\";s:0:\"\";s:7:\"\u0000*\u0000pmid\";s:0:\"\";s:9:\"\u0000*\u0000atitle\";s:104:\"Neutron flux generated by cosmic-ray muons at 5200 hg\/cm2s.r. underground. Depth-neutron intensity curve\";s:9:\"\u0000*\u0000jtitle\";s:50:\"Nuovo cimento della societ\u00e0 italiana di fisica. C\";s:9:\"\u0000*\u0000stitle\";s:32:\"Nuovo cimento Soc. ital. fis., C\";s:7:\"\u0000*\u0000date\";s:4:\"1989\";s:9:\"\u0000*\u0000volume\";s:2:\"12\";s:8:\"\u0000*\u0000issue\";s:1:\"4\";s:8:\"\u0000*\u0000spage\";s:3:\"469\";s:8:\"\u0000*\u0000epage\";s:3:\"477\";s:8:\"\u0000*\u0000pages\";s:0:\"\";s:7:\"\u0000*\u0000issn\";s:9:\"0390-5551\";s:8:\"\u0000*\u0000eissn\";s:0:\"\";s:9:\"\u0000*\u0000aulast\";s:8:\"AGLIETTA\";s:10:\"\u0000*\u0000aufirst\";s:1:\"M\";s:9:\"\u0000*\u0000auinit\";s:0:\"\";s:10:\"\u0000*\u0000auinitm\";s:0:\"\";s:5:\"\u0000*\u0000au\";a:19:{i:0;s:9:\"BADINO, G\";i:1;s:13:\"DADYKIN, V. L\";i:2;s:16:\"KHALCHUKOV, F. F\";i:3;s:17:\"KORTCHAGUIN, V. B\";i:4;s:17:\"KORTCHAGUIN, P. V\";i:5;s:17:\"KUDRYAVTSEV, V. A\";i:6;s:13:\"MALGUIN, A. S\";i:7;s:12:\"RYASNY, V. G\";i:8;s:16:\"RYAZHSKAYA, O. G\";i:9;s:14:\"YAKUSHEV, V. F\";i:10;s:14:\"ZATSEPIN, G. T\";i:11;s:10:\"BOLOGNA, C\";i:12;s:13:\"CASTAGNOLI, C\";i:13;s:13:\"CASTELLINA, A\";i:14;s:11:\"FULGIONE, W\";i:15;s:11:\"GALEOTTI, P\";i:16;s:11:\"SAAVEDRA, O\";i:17;s:12:\"TRINCHERO, G\";i:18;s:11:\"VERNETTO, S\";}s:9:\"\u0000*\u0000aucorp\";s:0:\"\";s:7:\"\u0000*\u0000isbn\";s:0:\"\";s:8:\"\u0000*\u0000coden\";s:0:\"\";s:8:\"\u0000*\u0000genre\";s:7:\"article\";s:7:\"\u0000*\u0000part\";s:0:\"\";s:9:\"\u0000*\u0000btitle\";s:0:\"\";s:8:\"\u0000*\u0000title\";s:104:\"Neutron flux generated by cosmic-ray muons at 5200 hg\/cm2s.r. underground. Depth-neutron intensity curve\";s:8:\"\u0000*\u0000place\";s:7:\"Bologna\";s:6:\"\u0000*\u0000pub\";s:11:\"Compositori\";s:10:\"\u0000*\u0000edition\";s:0:\"\";s:9:\"\u0000*\u0000tpages\";s:0:\"\";s:9:\"\u0000*\u0000series\";s:0:\"\";s:8:\"\u0000*\u0000proxy\";s:30:\"http:\/\/proxyout.inist.fr:8080\/\";s:12:\"\u0000*\u0000integrite\";b:1;}"
Europe PubMed Central access
"O:11:\"BaseOpenUrl\":35:{s:10:\"\u0000*\u0000openUrl\";N;s:6:\"\u0000*\u0000fmt\";s:7:\"journal\";s:6:\"\u0000*\u0000doi\";s:18:\"10.1007\/BF02525079\";s:6:\"\u0000*\u0000pii\";s:0:\"\";s:7:\"\u0000*\u0000pmid\";s:0:\"\";s:9:\"\u0000*\u0000atitle\";s:104:\"Neutron flux generated by cosmic-ray muons at 5200 hg\/cm2s.r. underground. Depth-neutron intensity curve\";s:9:\"\u0000*\u0000jtitle\";s:50:\"Nuovo cimento della societ\u00e0 italiana di fisica. C\";s:9:\"\u0000*\u0000stitle\";s:32:\"Nuovo cimento Soc. ital. fis., C\";s:7:\"\u0000*\u0000date\";s:4:\"1989\";s:9:\"\u0000*\u0000volume\";s:2:\"12\";s:8:\"\u0000*\u0000issue\";s:1:\"4\";s:8:\"\u0000*\u0000spage\";s:3:\"469\";s:8:\"\u0000*\u0000epage\";s:3:\"477\";s:8:\"\u0000*\u0000pages\";s:0:\"\";s:7:\"\u0000*\u0000issn\";s:9:\"0390-5551\";s:8:\"\u0000*\u0000eissn\";s:0:\"\";s:9:\"\u0000*\u0000aulast\";s:8:\"AGLIETTA\";s:10:\"\u0000*\u0000aufirst\";s:1:\"M\";s:9:\"\u0000*\u0000auinit\";s:0:\"\";s:10:\"\u0000*\u0000auinitm\";s:0:\"\";s:5:\"\u0000*\u0000au\";a:19:{i:0;s:9:\"BADINO, G\";i:1;s:13:\"DADYKIN, V. L\";i:2;s:16:\"KHALCHUKOV, F. F\";i:3;s:17:\"KORTCHAGUIN, V. B\";i:4;s:17:\"KORTCHAGUIN, P. V\";i:5;s:17:\"KUDRYAVTSEV, V. A\";i:6;s:13:\"MALGUIN, A. S\";i:7;s:12:\"RYASNY, V. G\";i:8;s:16:\"RYAZHSKAYA, O. G\";i:9;s:14:\"YAKUSHEV, V. F\";i:10;s:14:\"ZATSEPIN, G. T\";i:11;s:10:\"BOLOGNA, C\";i:12;s:13:\"CASTAGNOLI, C\";i:13;s:13:\"CASTELLINA, A\";i:14;s:11:\"FULGIONE, W\";i:15;s:11:\"GALEOTTI, P\";i:16;s:11:\"SAAVEDRA, O\";i:17;s:12:\"TRINCHERO, G\";i:18;s:11:\"VERNETTO, S\";}s:9:\"\u0000*\u0000aucorp\";s:0:\"\";s:7:\"\u0000*\u0000isbn\";s:0:\"\";s:8:\"\u0000*\u0000coden\";s:0:\"\";s:8:\"\u0000*\u0000genre\";s:7:\"article\";s:7:\"\u0000*\u0000part\";s:0:\"\";s:9:\"\u0000*\u0000btitle\";s:0:\"\";s:8:\"\u0000*\u0000title\";s:104:\"Neutron flux generated by cosmic-ray muons at 5200 hg\/cm2s.r. underground. Depth-neutron intensity curve\";s:8:\"\u0000*\u0000place\";s:7:\"Bologna\";s:6:\"\u0000*\u0000pub\";s:11:\"Compositori\";s:10:\"\u0000*\u0000edition\";s:0:\"\";s:9:\"\u0000*\u0000tpages\";s:0:\"\";s:9:\"\u0000*\u0000series\";s:0:\"\";s:8:\"\u0000*\u0000proxy\";s:30:\"http:\/\/proxyout.inist.fr:8080\/\";s:12:\"\u0000*\u0000integrite\";b:1;}"
Base Search access
"O:12:\"ArXivOpenUrl\":35:{s:10:\"\u0000*\u0000openUrl\";N;s:6:\"\u0000*\u0000fmt\";s:7:\"journal\";s:6:\"\u0000*\u0000doi\";s:18:\"10.1007\/BF02525079\";s:6:\"\u0000*\u0000pii\";s:0:\"\";s:7:\"\u0000*\u0000pmid\";s:0:\"\";s:9:\"\u0000*\u0000atitle\";s:104:\"Neutron flux generated by cosmic-ray muons at 5200 hg\/cm2s.r. underground. Depth-neutron intensity curve\";s:9:\"\u0000*\u0000jtitle\";s:50:\"Nuovo cimento della societ\u00e0 italiana di fisica. C\";s:9:\"\u0000*\u0000stitle\";s:32:\"Nuovo cimento Soc. ital. fis., C\";s:7:\"\u0000*\u0000date\";s:4:\"1989\";s:9:\"\u0000*\u0000volume\";s:2:\"12\";s:8:\"\u0000*\u0000issue\";s:1:\"4\";s:8:\"\u0000*\u0000spage\";s:3:\"469\";s:8:\"\u0000*\u0000epage\";s:3:\"477\";s:8:\"\u0000*\u0000pages\";s:0:\"\";s:7:\"\u0000*\u0000issn\";s:9:\"0390-5551\";s:8:\"\u0000*\u0000eissn\";s:0:\"\";s:9:\"\u0000*\u0000aulast\";s:8:\"AGLIETTA\";s:10:\"\u0000*\u0000aufirst\";s:1:\"M\";s:9:\"\u0000*\u0000auinit\";s:0:\"\";s:10:\"\u0000*\u0000auinitm\";s:0:\"\";s:5:\"\u0000*\u0000au\";a:19:{i:0;s:9:\"BADINO, G\";i:1;s:13:\"DADYKIN, V. L\";i:2;s:16:\"KHALCHUKOV, F. F\";i:3;s:17:\"KORTCHAGUIN, V. B\";i:4;s:17:\"KORTCHAGUIN, P. V\";i:5;s:17:\"KUDRYAVTSEV, V. A\";i:6;s:13:\"MALGUIN, A. S\";i:7;s:12:\"RYASNY, V. G\";i:8;s:16:\"RYAZHSKAYA, O. G\";i:9;s:14:\"YAKUSHEV, V. F\";i:10;s:14:\"ZATSEPIN, G. T\";i:11;s:10:\"BOLOGNA, C\";i:12;s:13:\"CASTAGNOLI, C\";i:13;s:13:\"CASTELLINA, A\";i:14;s:11:\"FULGIONE, W\";i:15;s:11:\"GALEOTTI, P\";i:16;s:11:\"SAAVEDRA, O\";i:17;s:12:\"TRINCHERO, G\";i:18;s:11:\"VERNETTO, S\";}s:9:\"\u0000*\u0000aucorp\";s:0:\"\";s:7:\"\u0000*\u0000isbn\";s:0:\"\";s:8:\"\u0000*\u0000coden\";s:0:\"\";s:8:\"\u0000*\u0000genre\";s:7:\"article\";s:7:\"\u0000*\u0000part\";s:0:\"\";s:9:\"\u0000*\u0000btitle\";s:0:\"\";s:8:\"\u0000*\u0000title\";s:104:\"Neutron flux generated by cosmic-ray muons at 5200 hg\/cm2s.r. underground. Depth-neutron intensity curve\";s:8:\"\u0000*\u0000place\";s:7:\"Bologna\";s:6:\"\u0000*\u0000pub\";s:11:\"Compositori\";s:10:\"\u0000*\u0000edition\";s:0:\"\";s:9:\"\u0000*\u0000tpages\";s:0:\"\";s:9:\"\u0000*\u0000series\";s:0:\"\";s:8:\"\u0000*\u0000proxy\";s:30:\"http:\/\/proxyout.inist.fr:8080\/\";s:12:\"\u0000*\u0000integrite\";b:1;}"
arXiv access
