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Featured researches published by U. Bravar.


The Astrophysical Journal | 1996

Measurement of the positron to electron ratio in the cosmic rays above 5-GeV

R. L. Golden; S.J. Stochaj; S. A. Stephens; F. Aversa; G. Barbiellini; M. Boezio; U. Bravar; A. Colavita; F. Fratnik; P. Schiavon; A. Vacchi; N. Zampa; J. W. Mitchell; J.F. Ormes; R. E. Streitmatter; R. Bellotti; F. Cafagna; M. Castellano; M. Circella; G. de Cataldo; C. De Marzo; N. Giglietto; B. Marangelli; A. Rain; P. Spinelli; M. Bocciolini; N. Finetti; P. Papini; A. Perego; S. Piccardi

As part of a series of experiments to search for antimatter in cosmic rays, the New Mexico State University balloon-borne magnet spectrometer was configured for a flight to study positrons. Two completely new instruments, a transition radiation detector and a silicon-tungsten imaging calorimeter, were added to the magnet spectrometer. These two detectors provided a proton rejection factor better than 3 × 104. This instrument was flown from Fort Sumner, New Mexico, at an average depth of 4.5 g cm-2 of residual atmosphere for a period of 25 hr. We report here the measured fraction of positrons e+/(e+ + e-) from ~5 to 60 GeV at the top of the atmosphere. Our measurements do not show any compelling evidence for an increase in this ratio with energy, and our results are consistent with a constant fraction of 0.078 ± 0.016 over the entire energy region.


Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 1995

WiZard SiW imaging calorimeter: a preliminary study on its particle identification capability during a balloon flight in 1993

F. Aversa; G. Barbiellini; M. Boezio; U. Bravar; A. Colavita; F. Fratnik; P. Schiavon; A. Vacchi; N. Zampa; V. Bidoli; M. Candusso; M. Casolino; M. P. De Pascale; A. Morselli; P. Picozza; Roberta Sparvoli; M. Bocciolini; F. Celletti; N. Finetti; M. Grandi; P. Papini; A. Perego; S. Piccardi; P. Spillantini; G. Basini; F.M. Brancaccio; G. Mazzenga; M. Ricci; R. Bellotti; F. Cafagna

Abstract The WiZard Collaboration is engaged in a program to study the antimatter components of the cosmic rays. A silicon-tungsten (Wiue5f8W) imaging calorimeter has been developed as part of this program. We present its performance and preliminary results, obtained during a balloon flight on September 8, 1993. The flight was dedicated to the measurement of the positron spectrum in the energy range 4–50 GeV and took place from Ft. Sumner, New Mexico.


Astroparticle Physics | 1996

Identification of cosmic ray electrons and positrons by neural networks

F. Aversa; G. Barbiellini; G. Basini; R. Bellotti; V. Bidoli; M. Bocciolini; U. Bravar; M. Boezio; F. Cafagna; M. Candusso; M. Casolino; M. Castellano; M. Circella; A. Colavita; G. de Cataldo; C. De Marzo; M. P. De Pascale; N. Finetti; F. Fratnik; N. Giglietto; R. L. Golden; C. Grimani; M. Hof; B. Marangelli; F. Massimo Brancaccio; W. Menn; J. W. Mitchell; A. Morselli; P. Papini; A. Perego

Abstract A data analysis based on artificial neural network classifiers has been done to identify cosmic ray electrons and positrons detected with the balloon-borne NMSU/Wizard-TS93 experiment. The information is provided by two ancillary and independent particle detectors: a transition radiation detector and a silicon-tungsten imaging calorimeter. Electrons and positrons measured during the flight have been identified with background rejection factors of 80 ± 3 and 500 ± 37 at signal efficiencies of 72 ± 3% and 86 ± 2% for the transition radiation detector and silicon-tungsten imaging calorimeter, respectively. The ability of the artificial neural network classifiers to perform a careful multidimensional analysis surpasses the results achieved by conventional methods.


Physical Review D | 2003

Energy spectra of atmospheric muons measured with the CAPRICE98 balloon experiment

M. Boezio; Bonvicini; P. Schiavon; A. Vacchi; N. Zampa; D. Bergström; P. Carlson; T. Francke; P. Hansen; E. Mocchiutti; M. Suffert; M. Hof; J. Kremer; W. Menn; M. Simon; M. Ambriola; R. Bellotti; F. Cafagna; F. Ciacio; M. Circella; C. De Marzo; P. Papini; S. Piccardi; P. Spillantini; E. Vannuccini; S. Bartalucci; M. Ricci; M. Casolino; M. P. De Pascale; A. Morselli


Archive | 1995

The Magnetic Spectrometer PAMELA for the Study of Cosmic Antimatter in Space

Oscar Adriani; Behcet Alpat; G. Barbiellini; Louis M. Barbier; S. Bartalucci; R. Bellotti; G. Basini; M. Bocciolini; M. Boezio; F. Massimo Brancaccio; U. Bravar; F. Cafagna; M. Candusso; R. Cardarelli; Per Carlson; M. Casolino; Maria Gabriella Castellano; Giovanni Castellini; M. Circella; Eric R. Christian; Andrew Davis; G. de Cataldo; C. De Marzo; M. P. De Pascale; E. Fiandrini; N. Finetti; T. Francke; Chr. Fuglesang; A. M. Galper; Franco Giannini


Archive | 2003

Composition of Cosmic Ray Particles in the Atmosphere as Measured by the CAPRICE98 Balloon Borne Apparatus

E. Mocchiutti; M. Ambriola; S. Bartalucci; R. Bellotti; D. Bergström; M. Boezio; V. Bonvicini; U. Bravar; F. Cafagna; P. Carlson; M. Casolino; F. Ciacio; M. Circella; C. De Marzo; M. P. De Pascale; T. Francke; P. Hansen; M. Hof; J. Kremer; W. Menn; J. W. Mitchell; A. Morselli; J.F. Ormes; P. Papini; S. Piccardi; P. Picozza; M. Ricci; P. Schiavon; M. Simon; R. Sparvoli


Archive | 1999

CAPRICE98: A balloon borne magnetic spectrometer to study cosmic ray at different atmospheric depths

M. Ambriola; G. Barbiellini; S. Bartalucci; M. Bocciolini; M. Boezio; U. Bravar; F. Cafagna; P. Carlson; M. Casolino; M. Castellano; F. Ciacio; M. Circella; C. De Marzo; M. P. De Pascale; N. Finetti; T. Francke; S. Grinstein; M. Hof; F. Kalchukov; J. Kremer; W. Menn; J. W. Mitchell; A. Morselli; J.F. Ormes; P. Papini; A. Perego; S. Piccardi; P. Picozza; M. Ricci; P. Schiavon


Prepared for | 1997

Status of the PAMELA experiment for the study of cosmic antimatter in space

O. Adriani; S. V. Koldashov; M. Ricci; Andrew Davis; Chr. Fuglesang; John F. Krizmanic; R. Bellotti; P. Spillantini; M. Hof; U. Bravar; N. Zampa; N. Mirizzi; R. E. Streitmatter; A. A. Moiseev; Stephen M. Schindler; P. Carlson; T. Francke; J.F. Ormes; G. Basini; B. Marangelli; N. Giglietto; G. Barbiellini; A. Morselli; V. V. Mikhailov; S. Piccardi; S. A. Voronov; P. Spinelli; S. A. Stephens; R.A. Mewaldt; E. R. Christian


Archive | 1999

The study of antiprotons and positrons in cosmic rays with the PAMELA spectrometer - presented by R. D'Alessandro

O. Adriani; M. Ambriola; G. Barbiellini; Louis M. Barbier; S. Bartalucci; G. Basini; R. Bellotti; Daniel Brian Bergstrom; M. Boezio; V. Bonvicini; M. Boscherini; U. Bravar; F. Cafagna; R. Cardarelli; Per Carlson; M. Casolino; Maria Gabriella Castellano; Giovanni Castellini; Eric R. Christian; F. Ciacio; M. Circella; Raffaello D'Alessandro; Andrew Davis; G. de Cataldo; C. De Marzo; M. P. De Pascale; T. Francke; Chr. Fuglesang; L. Gradi; A. M. Galper


Archive | 1999

A new measurement of the muon component in the atmosphere

He; M. Circella; G. Barbiellini; S. Bartalucci; R. Bellotti; D. Bergström; M. Boezio; U. Bravar; F. Cafagna; P. Carlson; M. Casolino; M. Castellano; F. Ciacio; C. De Marzo; M.P. De; Pascale; N. Finetti; T. Francke; S. Grinstein; M. Hof; F. Khalchukov; J. Kremer; W. Menn; J. W. Mitchell; A. Morselli; J.F. Ormes; P. Papini; S. Piccardi; P. Picozza; M. Ricci

Collaboration


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M. Boezio

University of Trieste

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M. Casolino

Sapienza University of Rome

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M. P. De Pascale

Istituto Nazionale di Fisica Nucleare

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N. Finetti

University of Florence

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T. Francke

Royal Institute of Technology

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