A
A. Bianco
Researcher at University of Trieste
Publications - 5
Citations - 360
A. Bianco is an academic researcher from University of Trieste. The author has contributed to research in topics: Cosmic ray & PAMELA detector. The author has an hindex of 3, co-authored 5 publications receiving 333 citations.
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Journal ArticleDOI
Cosmic-Ray Positron Energy Spectrum Measured by PAMELA
O. Adriani,G. C. Barbarino,G. A. Bazilevskaya,Roberto Bellotti,A. Bianco,Mirko Boezio,E. A. Bogomolov,M. Bongi,V. Bonvicini,S. Bottai,A. Bruno,F. Cafagna,D. Campana,R. Carbone,P. Carlson,Marco Casolino,G. Castellini,C. De Donato,C. De Santis,N. De Simone,V. Di Felice,Valerio Formato,A. M. Galper,A. V. Karelin,S. V. Koldashov,Sergey Koldobskiy,S. Y. Krutkov,A. N. Kvashnin,A. A. Leonov,V. V. Malakhov,L. Marcelli,Matteo Martucci,A. G. Mayorov,W. Menn,M. Merge,V. V. Mikhailov,E. Mocchiutti,André Monaco,Nicola Mori,Riccardo Munini,G. Osteria,F. Palma,P. Papini,Mark Pearce,P. Picozza,C. Pizzolotto,Marco Ricci,S. B. Ricciarini,Laura Rossetto,Ritabrata Sarkar,Valentina Scotti,M. Simon,Roberta Sparvoli,Piero Spillantini,Steven Stochaj,J. C. Stockton,Y. I. Stozhkov,Andrea Vacchi,E. Vannuccini,G. I. Vasilyev,S. A. Voronov,Y. T. Yurkin,G. Zampa,N. Zampa,V. G. Zverev +64 more
TL;DR: The satellite-borne experiment PAMELA has been used to make a new measurement of the cosmic-ray positron flux and fraction that extends previously published measurements up to 300 GeV in kinetic energy.
Journal ArticleDOI
Anisotropy studies in the cosmic ray proton flux with the PAMELA experiment
Ugo Giaccari,O. Adriani,G. C. Barbarino,G. A. Bazilevskaya,Roberto Bellotti,A. Bianco,Mirko Boezio,E. A. Bogomolov,Lorenzo Bonechi,M. Bongi,V. Bonvicini,S. V. Borisov,S. Bottai,A. Bruno,F. Cafagna,D. Campana,R. Carbone,Per Carlson,Marco Casolino,G. Castellini,M. P. De Pascale,C. De Santis,N. De Simone,V. Di Felice,Valerio Formato,A. M. Galper,L. A. Grishantseva,Giovanna Jerse,A. V. Karelin,M. D. Kheymits,S. V. Koldashov,S. Y. Krutkov,A. N. Kvashnin,A. A. Leonov,V. V. Malakhov,V. Malvezzi,L. Marcelli,Matteo Martucci,A. G. Mayorov,W. Menn,V. V. Mikhailov,E. Mocchiutti,Alfonso Monaco,Nicola Mori,Riccardo Munini,Riccardo Munini,N. N. Nikonov,G. Osteria,F. Palma,P. Papini,Mark Pearce,P. Picozza,C. Pizzolotto,Maria Teresa Ricci,S. B. Ricciarini,Laura Rossetto,Ritabrata Sarkar,M. Simon,Roberta Sparvoli,P. Spillantini,Y. I. Stozhkov,Andrea Vacchi,E. Vannuccini,G. I. Vasilyev,S. A. Voronov,Juan Wu,Y. T. Yurkin,G. Zampa,N. Zampa,V. G. Zverev +69 more
TL;DR: In this paper, the authors used two different and independent techniques to investigate the large and medium anisotropy patterns in the proton spectrum and found that the observed distribution of arrival directions is consistent with the isotropic expectation and no significant evidence of strong anisotropies has been observed.
Journal ArticleDOI
Search for cosmic ray electron-positron anisotropies with the Pamela data
D. Campana,Ugo Giaccari,O. Adriani,G. C. Barbarino,G. A. Bazilevskaya,Roberto Bellotti,A. Bianco,Mirko Boezio,E. A. Bogomolov,Lorenzo Bonechi,M. Bongi,V. Bonvicini,S. V. Borisov,S. Bottai,A. Bruno,F. Cafagna,R. Carbone,Per Carlson,Marco Casolino,G. Castellini,M. P. De Pascale,C. De Santis,N. De Simone,V. Di Felice,Valerio Formato,A. M. Galper,L. A. Grishantseva,Giovanna Jerse,A. V. Karelin,M. D. Kheymits,S. V. Koldashov,S. Y. Krutkov,A. N. Kvashnin,A. A. Leonov,V. V. Malakhov,V. Malvezzi,L. Marcelli,Matteo Martucci,A. G. Mayorov,W. Menn,V. V. Mikhailov,E. Mocchiutti,Alfonso Monaco,Nicola Mori,Riccardo Munini,Riccardo Munini,N. N. Nikonov,G. Osteria,F. Palma,P. Papini,Mark Pearce,P. Picozza,C. Pizzolotto,Maria Teresa Ricci,S. B. Ricciarini,Laura Rossetto,Ritabrata Sarkar,M. Simon,Roberta Sparvoli,P. Spillantini,Y. I. Stozhkov,Andrea Vacchi,E. Vannuccini,G. I. Vasilyev,S. A. Voronov,Juan Wu,Y. T. Yurkin,G. Zampa,N. Zampa,V. G. Zverev +69 more
TL;DR: In this article, the authors studied the anisotropy in the arrival direction of cosmic ray electrons and positrons with energy above 40 GeV using data taken by the Pamela experiment during 5 years of operation.
Posted Content
Cosmic-Ray Positron Identification with the PAMELA experiment
O. Adriani,G. C. Barbarino,G. A. Bazilevskaya,Roberto Bellotti,A. Bianco,Mirko Boezio,E. A. Bogomolov,M. Bongi,V. Bonvicini,S. Bottai,A. Bruno,F. Cafagna,D. Campana,R. Carbone,P. Carlson,Marco Casolino,G. Castellini,C. De Santis,M. P. De Pascale,C. De Donato,N. De Simone,V. Di Felice,V. Formato,A. M. Galper,A. V. Karelin,S. V. Koldashov,Sergey Koldobskiy,S. Yu. Krutkov,A. N. Kvashnin,A. A. Leonov,V. V. Malakhov,L. Marcelli,Matteo Martucci,A. G. Mayorov,W. Menn,M. Merge,V. V. Mikhailov,E. Mocchiutti,André Monaco,Nicola Mori,Riccardo Munini,G. Osteria,F. Palma,P. Papini,Mark Pearce,P. Picozza,C. Pizzolotto,Marco Ricci,S. B. Ricciarini,Laura Rossetto,Ritabrata Sarkar,M. Simon,Valentina Scotti,R. Sparvoli,P. Spillantini,S. J. Stochaj,J. C. Stockton,Y. I. Stozhkov,A. Vacchi,E. Vannuccini,G. I. Vasilyev,S. A. Voronov,Y. T. Yurkin,G. Zampa,N. Zampa,V. G. Zverev +65 more
TL;DR: The PAMELA satellite borne experiment is designed to study cosmic rays with great accuracy in a wide energy range as mentioned in this paper, which is the main goal of the experiment, including the study of the antimatter component of cosmic rays.
Journal ArticleDOI
The PAMELA experiment: light-nuclei selection with stand-alone detectors
R. Carbone,O. Adriani,G. C. Barbarino,G. A. Bazilevskaya,Roberto Bellotti,A. Bianco,Mirko Boezio,E. A. Bogomolov,Lorenzo Bonechi,M. Bongi,V. Bonvicini,S. V. Borisov,S. Bottai,A. Bruno,F. Cafagna,D. Campana,Per Carlson,Marco Casolino,G. Castellini,M. P. De Pascale,C. De Santis,N. De Simone,V. Di Felice,Valerio Formato,A. M. Galper,Ugo Giaccari,L. A. Grishantseva,Giovanna Jerse,A. V. Karelin,M. D. Kheymits,S. V. Koldashov,S. Y. Krutkov,A. N. Kvashnin,A. A. Leonov,V. V. Malakhov,V. Malvezzi,L. Marcelli,Matteo Martucci,A. G. Mayorov,W. Menn,V. V. Mikhailov,E. Mocchiutti,Alfonso Monaco,Nicola Mori,Riccardo Munini,Riccardo Munini,N. N. Nikonov,G. Osteria,F. Palma,P. Papini,Mark Pearce,P. Picozza,C. Pizzolotto,Maria Teresa Ricci,S. B. Ricciarini,Laura Rossetto,Ritabrata Sarkar,M. Simon,Roberta Sparvoli,P. Spillantini,Y. I. Stozhkov,Andrea Vacchi,E. Vannuccini,G. I. Vasilyev,S. A. Voronov,Juan Wu,Y. T. Yurkin,G. Zampa,N. Zampa,V. G. Zverev +69 more
TL;DR: The PAMELA space experiment as mentioned in this paper is providing data showing interesting features in cosmic rays that might change our basic vision of the mechanisms of production, acceleration and propagation of cosmic rays in the galaxy.