CERN Accelerating science

CERN Document Server Pronađeno je 31 zapisa  1 - 10slijedećikraj  idi na zapis: Pretraživanje je potrajalo 0.60 sekundi 
1.
The POEMMA (Probe of Extreme Multi-Messenger Astrophysics) mission / Olinto, A.V. (Chicago U.) ; Adams, J.H. (Alabama U., Huntsville) ; Aloisio, R. (GSSI, Aquila) ; Anchordoqui, L.A. (Lehman Coll.) ; Bergman, D.R. (Utah U.) ; Bertaina, M.E. (Turin U.) ; Bertone, P. (NASA, Marshall) ; Bisconti, F. (Turin U.) ; Bustamante, M. (Bohr Inst. ; DARK Cosmology Ctr.) ; Casolino, M. (Wako, RIKEN) et al.
The Probe Of Extreme Multi-Messenger Astrophysics (POEMMA) is designed to observe cosmic neutrinos (CNs) above 20 PeV and ultra-high energy cosmic rays (UHECRs) above 20 EeV over the full sky. The POEMMA mission calls for two identical satellites flying in loose formation, each comprised of a 4-meter wide field-of-view (45 degrees) Schmidt photometer. [...]
arXiv:1909.09466.- 2019 - 8 p. - Published in : PoS: ICRC2019 (2019) , pp. 378
Fulltext: PDF;
In : 36th International Cosmic Ray Conference, Madison, WI, USA, 24 Jul - 1 Aug 2019, pp.378
2.
Search for Ultra-High Energy Photons with the Pierre Auger Observatory / Pierre Auger Collaboration
One of key scientific objectives of the Pierre Auger Observatory is the search for ultra-high energy photons. [...]
arXiv:1804.05613 ; FERMILAB-CONF-18-152-ND-PPD-TD.
- 2018. - 7 p.
Preprint
3.
Radar reflection off extensive air showers / Stasielak, J (Cracow, INP) ; Baur, S (Karlsruhe U.) ; Bertaina, M (INFN, Turin) ; Blümer, J (Karlsruhe U.) ; Chiavassa, A (INFN, Turin) ; Engel, R (Karlsruhe U.) ; Haungs, A (Karlsruhe U.) ; Huege, T (Karlsruhe U.) ; Kampert, K -H (Wuppertal U.) ; Klages, H (Karlsruhe U.) et al.
We investigate the possibility of detecting extensive air showers by the radar technique. [...]
arXiv:1210.1427.
- 2012. - 6 p.
Preprint
4.
A measurement of the proton, helium and CNO fluxes at E<sub>0</sub>~100 TeV from the EAS- TOP (Cherenkov) and MACRO (TeV Muon) data at the Gran Sasso Laboratories / Bertaina, M
2005 Published version: PDF;
In : 29th International Cosmic Ray Conference, Pune, India, 3 - 10 Aug 2005, pp.41 (v.6)
5.
The longitudinal development of showers induced by high-energy hadrons in an iron-sampling calorimeter / Milke, J ; Antoni, T ; Apel, W D ; Badea, F ; Bekk, K ; Bercuci, A ; Bertaina, M ; Blümer, H ; Bozdog, H ; Büttner, C et al.
Occasionally cosmic-ray induced air showers result in single, unaccompanied hadrons at ground level. Such events are investigated with the 300 m2 hadron calorimeter of the KASCADE-Grande experiment. [...]
2005 - Published in : Nucl. Phys. B, Proc. Suppl. 151 (2005) 325-328
In : 20th International Symposium on Lattice Field Theory, Cambridge, MA, USA, 24 - 29 Jun 2002, pp.325-328
6.
The cosmic ray proton, helium and CNO fluxes in the 100 TeV energy region from TeV muons and EAS atmospheric Cherenkov light observations of MACRO and EAS-TOP / Aglietta, M ; Alessandro, B ; Ambrosio, M ; Antolini, R ; Antonioli, P ; Arneodo, F ; Baldini, A ; Barbarino, G C ; Barish, B C ; Battistoni, G et al.
The primary cosmic ray (CR) proton, helium and CNO fluxes in the energy range 80-300 TeV are studied at the National Gran Sasso Laboratories by means of EAS-TOP (Campo Imperatore, 2005 m a.s.l.) and MACRO (deep underground, 3100 m w.e., the surface energy threshold for a muon reaching the detector being E/sub mu //sup th/ approximately=1.3 TeV). The measurement is based on: (a) the selection of primaries based on their energy/nucleon (i.e., with energy/nucleon sufficient to produce a muon with energy larger than 1.3 TeV) and the reconstruction of the shower geometry by means of the muons recorded by MACRO in the deep underground laboratories; (b) the detection of the associated atmospheric Cherenkov light (C.l.) signals by means of the C.l. [...]
2004 - Published in : Astropart. Phys. 21 (2004) 223-40
7.
The cosmic ray primary composition between $10^{15}$ and $10^{16}$ ev from Extensive Air Showers electromagnetic and TeV muon data / Aglietta, M ; Alessandro, B ; Ambrosio, M ; Antolini, R ; Antonioli, P ; Arneodo, F ; Baldini, A ; Barbarino, G C ; Barish, B C ; Battistoni, G et al.
The cosmic ray primary composition in the energy range between 10/sup 15/ and 10/sup 16/ eV, i.e., around the "knee" of the primary spectrum, has been studied through the combined measurements of the EAS-TOP air shower array (2005 m a.s.l., 10/sup 5/ m/sup 2/ collecting area) and the MACRO underground detector (963 m a.s.l., 3100 m w.e. of minimum rock overburden, 920 m/sup 2/ effective area) at the National Gran Sasso Laboratories. [...]
2004 - Published in : Astropart. Phys. 20 (2004) 641-52
8.
Recent results from L3+COSMICS at CERN L3 collaboration / Bertaina, M
11x10 sup 9 cosmic ray muon events above 20 GeV have been collected with the L3+C detector at LEP, CERN, in 1999 and 2000. During the last year the energy, core position and direction of the air showers causing the observed muons could be derived for part of the data. [...]
2002 - Published in : Nucl. Phys. B, Proc. Suppl. 110 (2002) 469-471
9.
Study of jet production in p-N interactions at $sqrt{s} \approx 500 GeV$ in EAS multicore events / EAS-TOP Collaboration
The cross section for large p/sub t/ jet production for transverse momentum 10<or=p/sub t/<or=20 GeV/c and rapidity 1.6<or= eta <or=2.6 in p-N (p-`air') interactions is studied from the analysis of multicore extensive air showers recorded in the EAS-TOP calorimeter. The projectiles are the leading particles interacting at atmospheric depths between 250 and 480 cm/sup -2/, the CMS energy of interaction being square root (s) approximately=500 GeV. [...]
1999 - Published in : Phys. Lett. B 460 (1999) 474-83
10.
The hadron calorimeter of EAS-TOP : operation, calibration and resolution / Adinolfi-Falcone, R ; Aglietta, M ; Alessandro, B ; Antonioli, P ; Arneodo, F ; Bergamasco, L ; Bertaina, M ; Bertoni, R ; Campos-Fauth, A ; Cini-Castagnoli, G et al.
INFN-AE-98-22.
- 1998. - 23 p.
Access to fulltext document - Access to fulltext document

CERN Document Server : Pronađeno je 31 zapisa   1 - 10slijedećikraj  idi na zapis:
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