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CERN Document Server 2,017 записей найдено  1 - 10следующийконец  перейти к записи: Поиск длился 0.55 секунд. 
1.
(100)
Production rates of long-lived radionuclides Be10 and Al26 under direct muon-induced spallation in granite quartz and its implications for past high-energy cosmic ray fluxes / Sakurai, H (Yamagata U.) ; Kurebayashi, Y (Yamagata U.) ; Suzuki, S (Yamagata U.) ; Horiuchi, K (Hirosaki U.) ; Takahashi, Y (Yamagata U.) ; Doshita, N (Yamagata U.) ; Kikuchi, S (Yamagata U.) ; Tokanai, F (Yamagata U.) ; Iwata, N (Yamagata U.) ; Tajima, Y (Yamagata U.) et al.
This study measured the Be10 and Al26 production cross sections of muon-induced long-lived radionuclides to investigate the long-term variations in high-energy cosmic ray muon yields and high-energy galactic cosmic rays over a few million years. We exposed targets consisting of synthetic silica plates and quartz samples in a 1-m-long granite core to a beam containing 8.79×1012 positive muons over ∼120  days with an energy of 160 GeV extracted at the COMPASS experiment line at CERN-SPS. [...]
2024 - 18 p. - Published in : Phys. Rev. D 109 (2024) 102005
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2.
(91)
High energy muon induced radioactive nuclides in nickel plate and its use for 2-D muon-beam image profile / Kurebayashi, Y (Yamagata U.) ; Sakurai, H (Yamagata U.) ; Takahashi, Y (Yamagata U.) ; Doshita, N (Yamagata U.) ; Kikuchi, S (Yamagata U.) ; Tokanai, F (Yamagata U.) ; Horiuchi, K (Hirosaki U.) ; Tajima, Y (Yamagata U.) ; Oe, T (Yamagata U.) ; Sato, T (Yamagata U.) et al.
Target materials were exposed to a muon beam with an energy of 160 GeV/c at the COMPASS experiment line in CERN-SPS to measure the production cross-sections for muon-induced radionuclides. A muon imager containing four nickel plates, each measuring 100 mm×100 mm, exposed to the IP plate successfully detected the muon beam image during an irradiation period of 33 days. [...]
ScienceDirect, 2015 - 5 p. - Published in : Nucl. Instrum. Methods Phys. Res., A 799 (2015) 54-58
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3.
(67)
Muon-induced fission / Polikanov, S M
CERN-EP-81-160.- Geneva : CERN, 1980 - 4 p. Fulltext: PDF;
In : 2nd International Symposium on Physics and Chemistry of Fission, Julich, Germany, 14 - 18 May 1979, pp.3-11 - CERN library copies
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4.
(53)
Study of muon-induced neutron production, propagation and energy spectrum with the LVD detector at LNGS / Agafonova, N Y
2005 Published version: PDF;
In : 29th International Cosmic Ray Conference, Pune, India, 3 - 10 Aug 2005, pp.37 (v.9)
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5.
(48)
Muon-induced fission of ?Np, ?Pu, and ?Pu / Aleksandrov, B M ; Buklanov, G V ; Fromm, W D ; Ganzorig, J ; Krivokhatskij, A S ; Krogulski, T ; Polikanov, S M ; Sabirov, B M
JINR-E15-8628. - 1975. - 8 p.
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6.
(48)
Scaling violation in high energy muon-induced reactions / Feltesse, Joel
DPhPE-79-25. - 1979. - 67 p.
CERN library copies
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7.
(42)
 Determination of Cross-Sections of Fast-Muon-Induced Reactions to Cosmogenic Radionuclides / Neumaier, Sinstitute et al.
Approved: 20 April 1995.-
Status: Finished
Fulltext: JPG;
Experiment: NA54
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8.
(41)
Particle-induced Amorphization Of Complex Ceramics. Final Report / Ewing, R C
DOE-ER-45498-T-3. - 1998.
Records from U.S. DOE Office of Scientific and Technical Information
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9.
(38)
Study of muon-induced fission with the photoemulsion-method / Belovitsky, G E ; Suhov, L V ; Petitjean, C
PR-82-02 ; SIN-PR-82-02. - 1982. - 11 p.
CERN library copies
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10.
(37)
Geological isotope anomalies as signatures of nearby supernovae / Ellis, John R. (CERN) ; Fields, Brian D. (Paris, Inst. Astrophys.) ; Schramm, David N. (CERN ; Chicago U.)
Nearby supernova explosions may cause geological isotope anomalies via the direct deposition of debris or by cosmic-ray spallation in the earth's atmosphere. We estimate the mass of material deposited terrestrially by these two mechanisms, showing the dependence on the supernova distance. [...]
astro-ph/9605128; FERMILAB-PUB-95-157-A; CERN-TH-95-64; CERN-TH-95-64; FERMILAB-PUB-95-157.- Geneva : CERN, 1996 - 28 p. - Published in : Astrophys. J. 470 (1996) 1227-1236 Access to fulltext document: PDF; Fulltext: PDF; External link: Fermilab Library Server (fulltext available) - Please contact the library if you need to access this document.
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