CERN Accelerating science

CERN Document Server Намерени са 74 записа  1 - 10следващкрай  отиване на запис: Търсенето отне 0.71 секунди. 
1.
The Alpha Magnetic Spectrometer (AMS) on the International Space Station. I: Results from the test flight on the space shuttle / AMS Collaboration
The Alpha Magnetic Spectrometer (AMS) was flown on the space shuttle Discovery during flight STS-91 (June 1998) in a 51.7° orbit at altitudes between 320 and 390 km . A search for antihelium nuclei in the rigidity range 1– 140 GV was performed. [...]
2002 - 75 p. - Published in : Phys. Rep. 366 (2002) 331-405
- Published in : Phys. Rep. 380 (2003) 97-98
2.
Isotopic Composition of Light Nuclei in Cosmic Rays: Results from AMS-01 / AMS-01 Collaboration
The variety of isotopes in cosmic rays allows us to study different aspects of the processes that cosmic rays undergo between the time they are produced and the time of their arrival in the heliosphere. In this paper, we present measurements of the isotopic ratios $^2$H/$^4$He, $^3$He/$^4$He, $^6$Li/$7$Li, $7$Be/($^9$Be+$^{10}$Be), and $^{10}$B/$^{11}$B in the range 0.2-1.4 GeV of kinetic energy per nucleon. [...]
arXiv:1106.2269.- 2011 - 12 p. - Published in : Astrophys. J. 736 (2011) 105 Fulltext: PDF; External link: Preprint
3.
Relative Composition and Energy Spectra of Light Nuclei in Cosmic Rays. Results from AMS-01 / AMS-01 Collaboration
Measurement of the chemical and isotopic composition of cosmic rays is essential for the precise understanding of their propagation in the galaxy. While the model parameters are mainly determined using the B/C ratio, the study of extended sets of ratios can provide stronger constraints on the propagation models. [...]
arXiv:1008.5051.- 2010 - 13 p. - Published in : Astrophys. J. 724 (2010) 329-340 Fulltext: PDF; External link: Preprint
4.
Cosmic-ray positron fraction measurement from 1 to 30 GeV with AMS-01 / AMS-01 Collaboration
A measurement of the cosmic ray positron fraction e+/(e+ + e-) in the energy range of 1-30 GeV is presented. The measurement is based on data taken by the AMS-01 experiment during its 10 day Space Shuttle flight in June 1998. [...]
astro-ph/0703154.- 2007 - 20 p. - Published in : Phys. Lett. B 646 (2007) 145-154 Access to fulltext document: PDF; Fulltext: S0370269307001104 - XML; arXiv:astro-ph_0703154 - PDF;
5.
A$_{1}$ and A$_{2}$ production at 40 GeV/c / Antipov, Yu ; Ascoli, G ; Busnello, R ; Damgaard, G ; Kienzle-Focacci, M N ; Kienzle, W ; Klanner, Robert ; Lebedev, A A ; Lechanoine-Leluc, C ; Lecomte, P et al.
1972
In : 3rd International Conference on Experimental Meson Spectroscopy : Festschrift Julius Halpern, 1912-1972, Philadelphia, PN, USA, 28 - 29 Apr 1972, pp.164-183
6.
AMS - A magnetic spectrometer on the International Space Station / Lechanoine-Leluc, C
2005 Published version: PDF;
In : 29th International Cosmic Ray Conference, Pune, India, 3 - 10 Aug 2005, pp.381 (v.3)
7.
Letter of Intention : A multipurpose experiment on mass-spectra and decay analysis of various resonances / Kienzle, W ; Maglic, Bogdan C (CERN) ; Focacci, M N ; Chikovani, G E ; Levrat, B ; Martin, M ; Grieder, P ; Schübelin, P ; Fayolle, J C ; Cotteron, J et al.
CERN-PH-I-COM-66-54.
- 1966. - 2 p.
Fulltext
8.
Proposal for an experiment : Experiment to determine spin and parity of the $A_{2}$ meson / Chikovani, G E ; Dubal, L ; Grieder, P ; Kienzle, W ; Lechanoine-Leluc, C ; Levrat, B ; Maglic, Bogdan C (CERN) ; Martin, M ; Schübelin, P
CERN-PH-I-COM-66-43.
- 1966. - 3 p.
Fulltext
9.
Dalitz plot of the $A_{2}$ meson region obtained with wire spark chambers / Martin, M (CERN) ; Schübelin, P (CERN) ; Chikovani, G E (CERN) ; Focacci, M N (CERN) ; Kienzle, W (CERN) ; Kruse, U (CERN) ; Lechanoine-Leluc, C (CERN) ; Levrat, B (CERN)
1967.
10.
Letter of Intent : Magnetic meson spectrometer for singly and doubly charged states (I = 1 and 2) and masses up to 4 GeV / Kienzle, W ; Zavattini, E ; Maglic, Bogdan C (CERN) ; Chikovani, G E ; Focacci, M N ; Levrat, B ; Martin, M ; Schübelin, P ; Lechanoine-Leluc, C ; Fayolle, J C et al.
CERN-PH-I-COM-67-3.
- 1967. - 3 p.
Fulltext

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