PRECISE COSMIC RAYS MEASUREMENTS WITH PAMELA

Authors

  • A. Bruno INFN, Sezione di Bari, I-70126 Bari
  • O. Adriani University of Florence, Department of Physics, I-50019 Sesto Fiorentino, Florence; INFN, Sezione di Florence, I-50019 Sesto Fiorentino, Florence
  • G. C. Barbarino University of Naples “Federico II”, Department of Physics, I-80126 Naples; INFN, Sezione di Naples, I-80126 Naples
  • G. A. Bazilevskaya Lebedev Physical Institute, RU-119991, Moscow
  • R. Bellotti INFN, Sezione di Bari, I-70126 Bari; University of Bari, Department of Physics, I-70126 Bari
  • M. Boezio INFN, Sezione di Trieste, I-34149 Trieste
  • E. A. Bogomolov Ioffe Physical Technical Institute, RU-194021 St. Petersburg
  • M. Bongi INFN, Sezione di Florence, I-50019 Sesto Fiorentino, Florence
  • V. Bonvicini INFN, Sezione di Trieste, I-34149 Trieste
  • S. Borisov INFN, Sezione di Rome “Tor Vergata”, I-00133 Rome; University of Rome “Tor Vergata”, Department of Physics, I-00133 Rome
  • S. Bottai INFN, Sezione di Florence, I-50019 Sesto Fiorentino, Florence
  • F. Cafagna INFN, Sezione di Bari, I-70126 Bari
  • D. Campana INFN, Sezione di Naples, I-80126 Naples
  • R. Carbone INFN, Sezione di Naples, I-80126 Naples; University of Rome “Tor Vergata”, Department of Physics, I-00133 Rome
  • P. Carlson mKTH, Department of Physics, and the Oskar Klein Centre for Cosmoparticle Physics, AlbaNova University Centre, SE-10691 Stockholm
  • M. Casolino INFN, Sezione di Rome “Tor Vergata”, I-00133 Rome
  • G. Castellini IFAC, I-50019 Sesto Fiorentino, Florence
  • L. Consiglio INFN, Sezione di Naples, I-80126 Naples
  • M. P. De Pascale INFN, Sezione di Rome “Tor Vergata”, I-00133 Rome; University of Rome “Tor Vergata”, Department of Physics, I-00133 Rome
  • C. De Santis INFN, Sezione di Rome “Tor Vergata”, I-00133 Rome; University of Rome “Tor Vergata”, Department of Physics, I-00133 Rome
  • N. De Simone INFN, Sezione di Rome “Tor Vergata”, I-00133 Rome; University of Rome “Tor Vergata”, Department of Physics, I-00133 Rome
  • V. Di Felice INFN, Sezione di Rome “Tor Vergata”, I-00133 Rome
  • A. M. Galper NRNU MEPhI, RU-115409 Moscow
  • W. Gillard mKTH, Department of Physics, and the Oskar Klein Centre for Cosmoparticle Physics, AlbaNova University Centre, SE-10691 Stockholm
  • L. Grishantseva NRNU MEPhI, RU-115409 Moscow
  • G. Jerse INFN, Sezione di Trieste, I-34149 Trieste; University of Trieste, Department of Physics, I-34147 Trieste
  • A. V. Karelin NRNU MEPhI, RU-115409 Moscow
  • M. D. Kheymits NRNU MEPhI, RU-115409 Moscow
  • S. V. Koldashov NRNU MEPhI, RU-115409 Moscow
  • S. Y. Krutkov Ioffe Physical Technical Institute, RU-194021 St. Petersburg
  • A. N. Kvashnin Lebedev Physical Institute, RU-119991, Moscow
  • A. Leonov NRNU MEPhI, RU-115409 Moscow
  • V. Malakhov NRNU MEPhI, RU-115409 Moscow
  • L. Marcelli INFN, Sezione di Rome “Tor Vergata”, I-00133 Rome
  • A. G. Mayorov NRNU MEPhI, RU-115409 Moscow
  • W. Menn Universitat Siegen, Department of Physics, D-57068 Siegen
  • V. V. Mikhailov NRNU MEPhI, RU-115409 Moscow
  • E. Mocchiutti INFN, Sezione di Trieste, I-34149 Trieste, Italy
  • A. Monaco INFN, Sezione di Bari, I-70126 Bari, Italy; INFN, Sezione di Florence, I-50019 Sesto Fiorentino, Florence, Italy
  • N. Mori University of Florence, Department of Physics, I-50019 Sesto Fiorentino, Florence, Italy; INFN, Sezione di Florence, I-50019 Sesto Fiorentino, Florence, Italy
  • N. Nikonov Ioffe Physical Technical Institute, RU-194021 St. Petersburg, Russia; INFN, Sezione di Rome “Tor Vergata”, I-00133 Rome, Italy; University of Rome “Tor Vergata”, Department of Physics, I-00133 Rome, Italy
  • G. Osteria INFN, Sezione di Florence, I-50019 Sesto Fiorentino, Florence, Italy
  • F. Palma j INFN, Sezione di Rome “Tor Vergata”, I-00133 Rome, Italy; k University of Rome “Tor Vergata”, Department of Physics, I-00133 Rome, Italy
  • P. Papini INFN, Sezione di Florence, I-50019 Sesto Fiorentino, Florence, Italy
  • M. Pearce mKTH, Department of Physics, and the Oskar Klein Centre for Cosmoparticle Physics, AlbaNova University Centre, SE-10691 Stockholm,
  • P. Picozza INFN, Sezione di Rome “Tor Vergata”, I-00133 Rome, Italy; k University of Rome “Tor Vergata”, Department of Physics, I-00133 Rome, Italy
  • C. Pizzolotto INFN, Sezione di Trieste, I-34149 Trieste, Italy
  • M. Ricci INFN, Laboratori Nazionali di Frascati, Via Enrico Fermi 40, I-00044 Frascati, Italy
  • S. B. Ricciarini INFN, Sezione di Florence, I-50019 Sesto Fiorentino, Florence, Italy
  • L. Rossetto KTH, Department of Physics, and the Oskar Klein Centre for Cosmoparticle Physics, AlbaNova University Centre, SE-10691 Stockholm, Sweden
  • R. Sarkar INFN, Sezione di Trieste, I-34149 Trieste, Italy
  • M. Simon Universitat Siegen, Department of Physics, D-57068 Siegen, Germany
  • R. Sparvoli INFN, Sezione di Rome “Tor Vergata”, I-00133 Rome, Italy; k University of Rome “Tor Vergata”, Department of Physics, I-00133 Rome, Italy
  • P. Spillantini University of Florence, Department of Physics, I-50019 Sesto Fiorentino, Florence, Italy; c INFN, Sezione di Florence, I-50019 Sesto Fiorentino, Florence, Italy
  • Y. I. Stozhkov Lebedev Physical Institute, RU-119991, Moscow, Russia
  • A. Vacchi INFN, Sezione di Trieste, I-34149 Trieste, Italy
  • E. Vannuccini INFN, Sezione di Florence, I-50019 Sesto Fiorentino, Florence, Italy
  • G. Vasilyev Ioffe Physical Technical Institute, RU-194021 St. Petersburg, Russia
  • S. A. Voronov NRNU MEPhI, RU-115409 Moscow, Russia
  • Y. T. Yurkin NRNU MEPhI, RU-115409 Moscow, Russia
  • J. Wu KTH, Department of Physics, and the Oskar Klein Centre for Cosmoparticle Physics, AlbaNova University Centre, SE-10691 Stockholm, Sweden
  • G. Zampa INFN, Sezione di Trieste, I-34149 Trieste, Italy
  • N. Zampa INFN, Sezione di Trieste, I-34149 Trieste, Italy
  • V. G. Zverev NRNU MEPhI, RU-115409 Moscow, Russia

DOI:

https://doi.org/10.14311/AP.2013.53.0712

Abstract

The PAMELA experiment was launched on board the Resurs-DK1 satellite on June 15th 2006. The apparatus was designed to conduct precision studies of charged cosmic radiation over a wide energy range, from tens of MeV up to several hundred GeV, with unprecedented statistics. In five years of continuous data taking in space, PAMELA accurately measured the energy spectra of cosmic ray antiprotons and positrons, as well as protons, electrons and light nuclei, sometimes providing data in unexplored energetic regions. These important results have shed new light in several astrophysical fields like: an indirect search for Dark Matter, a search for cosmological antimatter (anti-Helium), and the validation of acceleration, transport and secondary production models of cosmic rays in the Galaxy. Some of the most important items of Solar and Magnetospheric physics were also investigated. Here we present the most recent results obtained by the PAMELA experiment.

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Published

2013-12-18

Issue

Vol. 53 (2013): Supplement

Section

Articles

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How to Cite

Bruno, A., Adriani, O., Barbarino, G. C., Bazilevskaya, G. A., Bellotti, R., Boezio, M., Bogomolov, E. A., Bongi, M., Bonvicini, V., Borisov, S., Bottai, S., Cafagna, F., Campana, D., Carbone, R., Carlson, P., Casolino, M., Castellini, G., Consiglio, L., De Pascale, M. P., … Zverev, V. G. (2013). PRECISE COSMIC RAYS MEASUREMENTS WITH PAMELA. Acta Polytechnica, 53(A), 712-717. https://doi.org/10.14311/AP.2013.53.0712