Zobrazeno 1 - 10
of 102
pro vyhledávání: '"M. AMBRIOLA"'
Autor:
V. Bidoli, M. Casolino, De Pascale, G. Furano, A. Iannucci, A. Morselli, P. Picozza, R. Sparvoli, A. Bakaldin, A. Galper, S. Koldashov, M. Korotkov, A. Leonov, V. Mikhailov, S. Voronov, M. Boezio, V. Bonvicini, A. Vacchi, G. Zampa, N. Zampa, M. Ambriola, F. Cafagna, M. Circella, C. De Marzo, O. Adriani, P. Papini, P. Spillantini, S. Straulino, E. Vannuccini, M. Ricci, G. Castellini
Publikováno v:
Annales Geophysicae, Vol 20, Pp 1693-1697 (2002)
In this paper we report on the energy spectrum of protons of albedo origin measured by the instruments NINA and NINA-2 at different geomagnetic locations, and the behaviour of the proton flux as a function of altitude out of the South Atlantic
Externí odkaz:
https://doaj.org/article/3fd05c5c66b84f71a218b8a58c9dfa52
Autor:
Montaruli, T., al, M. Ambriola et
We report on the results of a Monte Carlo simulation study of a km^3 scale deep underwater Cherenkov detector aimed at detecting neutrinos of astrophysical origin. This analysis has been undertaken as part of the NEMO R&D project to develop such an e
Externí odkaz:
http://arxiv.org/abs/hep-ex/9905019
Autor:
Montaruli, T., al, M. Ambriola et
We present updated results on the search for a neutrino signal from the core of the Earth and of the Sun induced by Weakly Interacting Massive Particles (WIMPs). In this paper we concentrate on neutralinos as WIMP candidates. The 971 and 642 events u
Externí odkaz:
http://arxiv.org/abs/hep-ex/9905021
Autor:
Montaruli, T., al, M. Ambriola et
We use a sample of 990 upward-going muons, induced primarily by atmospheric neutrinos, to search for neutrinos of astrophysical origin. No evidence has been found using the event direction information. Flux limits of the order of 10^-15 cm^-2 s^-1 ar
Externí odkaz:
http://arxiv.org/abs/hep-ex/9905020
Autor:
M. Ambriola, Roberta Sparvoli, C. De Marzo, Tom Francke, Peter Hansen, W. Menn, V. Bonvicini, P. Papini, D. Bergström, A. Morselli, E. Vannuccini, J. Kremer, P. Schiavon, Marco Ricci, M. Simon, John Mitchell, M. Suffert, Jonathan F. Ormes, S. J. Stochaj, Roberto Bellotti, Per Carlson, Marco Casolino, S. A. Stephens, M. P. De Pascale, F. Cafagna, M. Hof, A. Vacchi, E. Mocchiutti, S. Piccardi, R. E. Streitmatter, Piero Spillantini, F. Ciacio, M. Circella, Ulisse Bravar, P. Picozza, S. Bartalucci, Mirko Boezio, N. Zampa
Publikováno v:
The Astrophysical Journal. 615:259-274
We report the first measurement of the deuterium abundance in cosmic rays above 10 GeV nucleon � 1 of kinetic energy. The data were collected by the balloon-borne experiment CAPRICE98, which was flown on 1998 May 28–29 from Fort Sumner, New Mexic
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::362adeb9bc836015cc854288d4cf5e3d
https://doi.org/10.1086/424027
https://doi.org/10.1086/424027
Autor:
A. M. Galper, F. Cafagna, G. Vasiljev, A. V. Bakaldin, M. Ambriola, M. Nagni, O. Adriani, M. Simon, Silvio Orsi, W. Menn, Massimo Bongi, Roberta Sparvoli, G. A. Bazilevskaja, E. Taddei, S. A. Voronov, C. De Marzo, R. Y. Stozhkov, S. Y. Krutkov, Petter Hofverberg, P. Schiavon, John Mitchell, E. A. Bogomolov, R. Mukhametshin, Giuseppe Osteria, S. J. Stochaj, V. Malvezzi, S. V. Koldashov, D. Fedele, M. G. Korotkov, A. Grigorjeva, Mirko Boezio, Mark Pearce, S. B. Ricciarini, Marco Ricci, S. A. Stephens, N. Zampa, M. Albi, M. Circella, P. Papini, S. Russo, V. V. Mikhailov, E. Vannuccini, P. Carlson, A. Vacchi, G. Castellini, A. Basili, M. Boscherini, M. P. De Pascale, E. Streitmatter, F. Altamura, R. Bencardino, J. Lund, P. Picozza, V. Bonvicini, L. Marcelli, Roberto Bellotti, P. Spillantini, A. Morselli, E. Mocchiutti, M. Grandi, G. Zampa, S. Bottai, Y. T. Yurkin, D. Campana, Marco Casolino, M. Minori, Lorenzo Bonechi, J. Lundquist, G. C. Barbarino, L. Bongiorno
Publikováno v:
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment. 572:471-473
The Pamela apparatus will allow precise measurements of cosmic rays in Low Earth Orbit, mainly focusing on the antiparticles component. The apparatus is now ready for flight, and the launch is foreseen during June 2006. The paper briefly reports the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1dbd32939a8df51d071d6973c8d73d6b
https://doi.org/10.1016/j.nima.2006.10.316
https://doi.org/10.1016/j.nima.2006.10.316
Autor:
S. Orsi, M. Ambriola, Roberta Sparvoli, A. Morselli, E. Taddei, Yu. I. Stozhkov, S. Russo, Mirko Boezio, D. Campana, A. N. Kvashnin, O. Maksumov, S. V. Koldashov, Marco Ricci, V. Bonvicini, O. Adriani, W. Menn, Marco Casolino, Petter Hofverberg, Gianluigi Zampa, Andrea Vacchi, A. Bruno, M. Minori, N. De Simone, M. Simon, N. N. Nikonov, Giuseppe Osteria, E. Mocchiutti, S. Misin, D. Fedele, Lorenzo Bonechi, F. Cafagna, L. Marcelli, M. Bongi, V. Malvezzi, A. M. Galper, G. De Rosa, V. G. Zverev, M. F. Runtso, Piero Spillantini, S. A. Voronov, E. A. Bogomolov, J. Lundquist, V. V. Mikhailov, G. I. Vasilyev, G. Castellini, N. Zampa, Mark Pearce, S. B. Ricciarini, G. C. Barbarino, P. Picozza, C. De Marzo, P. Papini, E. Vannuccini, G. A. Bazilevskaja, V. Di Felice, Y. T. Yurkin, A. Basili, M. P. De Pascale, S. Yu. Krutkov, Per Carlson
Publikováno v:
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment. 588:243-246
PAMELA is a satellite-borne experiment designed to make long duration measurements of the cosmic radiation in Low Earth Orbit. It is devoted to the detection of the cosmic-ray spectra in the 100 MeV 300 GeV range with primary scientific goal the meas
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bb5d369690289811e078b6061277db8d
https://doi.org/10.1016/j.nima.2008.01.046
https://doi.org/10.1016/j.nima.2008.01.046
Autor:
P. Spinelli, G. Rossi, J. Lundquist, N. Zampa, M. Romita, Alessandra Menicucci, V. V. Mikhailov, R. E. Streitmatter, P. Carlson, M. G. Korotkov, M. Ambriola, M. P. De Pascale, S. Straulino, C. De Marzo, F. Taccetti, Roberta Sparvoli, Mark Pearce, S. B. Ricciarini, O. Adriani, S. V. Koldashov, S. A. Voronov, Marco Ricci, M. Circella, Silvio Orsi, W. Menn, A. V. Bakaldin, R. Wischnewski, P. Papini, E. Vannuccini, N. Mirizzi, E. A. Bogomolov, F. Cafagna, P. Spillantini, G. Vasiljev, P. Schiavon, V. I. Logachev, M. Boscherini, M. Minori, Giuseppe Osteria, N. Giglietto, S. Russo, G. Castellini, Vladimir Makhmutov, Mirko Boezio, Y. T. Yurkin, John Mitchell, S. J. Stochaj, S. Y. Krutkov, M. Simon, P. Picozza, A. M. Galper, R. Bencardino, J. Lund, E. Mocchiutti, G. A. Bazilevskaja, Massimo Bongi, Lorenzo Bonechi, A. Basili, Yu. I. Stozhkov, Roberto Bellotti, A. Morselli, A. N. Kvashnin, D. Campana, Gianluigi Zampa, Marco Casolino, M. Bonvicini, L. Bongiorno, O. Maksumov, Gianluca Furano, G. C. Barbarino, Andrea Vacchi
Publikováno v:
Advances in Space Research. 37:1841-1847
PAMELA is a satellite-borne experiment which will measure the antiparticle component of cosmic rays over an extended energy range and with unprecedented accuracy. The apparatus consists of a perman ...
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::241b49415f3dd6366ef3e439bcb81a43
https://doi.org/10.1016/j.asr.2005.05.100
https://doi.org/10.1016/j.asr.2005.05.100
Autor:
M. Ambriola, P. Spinelli, M. Romita, N. Giglietto, M. Circella, B. Marangelli, F. Cafagna, N. Mirizzi, C. De Marzo, Roberto Bellotti
Publikováno v:
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment. 522:77-80
PAMELA space mission objective is to flight a satellite-borne magnetic spectrometer built to fulfill the primary scientific goals of detecting antiparticles (antiprotons and positrons) and to measure spectra of particles in cosmic rays. The PAMELA te
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::547c2650457e3d3c2af36869790290b1
https://doi.org/10.1016/j.nima.2004.01.022
https://doi.org/10.1016/j.nima.2004.01.022
Publikováno v:
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment. 510:362-370
Support vector machines (SVMs) provide an interesting computational paradigm for the classification of data from high-energy physics and particle astrophysics experiments. In this study, the classification power of SVMs is compared with those from st
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3572af0000f47b5aef1d7183d7795901
https://doi.org/10.1016/s0168-9002(03)01926-0
https://doi.org/10.1016/s0168-9002(03)01926-0