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1. Integration and qualification of the Mini-EUSO telescope on board the ISS

Author: Francesca Capel, Eva Reali, Enzo Reali, T. Napolitano, L. Marcelli, Pavel Klimov, Lech Wiktor Piotrowski, Maria Teresa Ricci, A. Franceschi, Alexander S. Belov, Alberto Franceschi, P. Klimov, Marco Ricci, M. Casolino, F. Capel, Andrei S. Belov, Piergiorgio Picozza, L.W. Piotrowski, P. Picozza, Marco Casolino, and G. Cambiè
Subjects: Physics, Photomultiplier, business.industry, Detector, FOS: Physical sciences, Photon counting, law.invention, Telescope, Silicon photomultiplier, Optics, law, International Space Station, Satellite, Image sensor, business, Astrophysics - Instrumentation and Methods for Astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM)
Abstract: Mini-EUSO is a new space-based experiment designed primarily to observe showers that develop in atmosphere due to the interaction between molecular nitrogen and Ultra High Energy Cosmic particles (above 1021 eV) crossing by. It belongs to the JEM-EUSO program, which includes several past experiments all devoted to develop new larger size satellite detectors like K-EUSO and POEMMA for future UHEC Rays study from space. Mini-EUSO is a multiwavelenght telescope launched on August 2019 with the unmanned Soyuz MS-14 rocket to the International Space Station and currently operating on board the Russian Zvezda module, facing a UV-transparent window watching Earth in Nadir direction. The telescope optics comprise a main detection system employing two double-sided Fresnel lenses focusing UV (300–400 nm) light onto an array of 36 Hamamatsu Multi-Anode PhotoMultiplier Tubes, each of 64 channels for a total of 2304 pixels working in single photon counting mode, providing a wide field of view (44°) correpsonding to a ground area of 263 x 263 km2 with a highly fast time resolution up to few microseconds. Mini-EUSO includes also multiple ancillary sensors such as visible (400–780 nm) and NIR (1500–1600 nm) cameras covering a wide range of radiation wavelenght as well as a 64 channels Multi-Pixel Photon Counter Silicon PhotoMultiplier array which will increase the Technology Readiness Level of this ultrafast imaging sensor. Beside the primary objective, the mission aims to study different event such as meteoroids, Transient Luminous Event, search for Strange Quark matter and thanks to its space-time resolution is capable to provide UV Earth maps over the surface covered during ISS orbits. In this work we will present the detector integration, the qualification measurements on ground and some preliminary data.
Published: 2022

2. The EUSO@Turlab Project: Tests of Mini-EUSO Engineering Model

Author: A. Franceschi, L. Marcelli, G. Contino, Maria Teresa Ricci, A. Djakonow, Marco Mignone, Lech Wiktor Piotrowski, A. Murashov, J. Szabelski, M.E Bertaina, Naoto Sakaki, Pavel Klimov, W. Marszał, Matteo Battisti, F. Bisconti, Alexander S. Belov, A. Poroshin, K. Shinozaki, S. Blin-Bondil, Daniele Gardiol, Francesca Capel, Francesco Fenu, Enzo Reali, M. Przybylak, A. Cellino, E. Parizot, P. Picozza, M. I. Panasyuk, G. Suino, M. Bertaina, S. Turriziani, Toshikazu Ebisuzaki, Federico Fausti, Marco Casolino, Claudio Fornaro, Guillaume Prévôt, G. Cambiè, I. Churilo, P. Gorodetzky, F. Kajino, M. Traïche, F. Cafagna, Y. Takizawa, Z. Plebaniak, G. Osteria, Christer Fuglesang, R. Bonino, T. Napolitano, Rossella Caruso, G. Cotto, Organisation de Micro-Électronique Générale Avancée (OMEGA), École polytechnique (X)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), JEM-EUSO, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-École polytechnique (X)-Centre National de la Recherche Scientifique (CNRS), and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)
Subjects: Brightness, business.industry, Detector, Cosmic ray, Field of view, Rotating tank, law.invention, Telescope, law, Environmental science, Focal surface, Aerospace engineering, business, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Space debris
Abstract: International audience; The TurLab facility is a laboratory, equipped with a 5 m diameter and 1 m depth rotating tank, located in the Physics Department of the University of Turin. Originally, it was mainly built to study systems of different scales where rotation plays a key role in the fluid behaviour such as in atmospheric and oceanic flows. In the past few years the TurLab facility has been used to perform experiments related to the observation of Extreme Energy Cosmic Rays (EECRs) from space using the fluorescence technique. For example, in the case of the JEM-EUSO mission, where the diffuse night brightness and artificial light sources can vary significantly in time and space inside the Field of View of the telescope. The Focal Surface of Mini-EUSO Engineering Model (Mini-EUSO EM) with the level 1 (L1) and 2 (L2) trigger logics implemented in the Photo-Detector Module (PDM) has been tested at TurLab. Tests related to the possibility of using an EUSO-like detector for other type of applications such as Space Debris (SD) monitoring and imaging detector have also been pursued. The tests and results obtained within the EUSO@TurLab Project on these different topics are presented.
Published: 2019

3. The POEMMA (Probe of Extreme Multi-Messenger Astrophysics) mission

Author: A. Neronov, Francesco Fenu, Mark Christl, S. Mackovjak, Alessandro Liberatore, J. S. Perkins, P. Bertone, Mauricio Bustamante, F. Bisconti, T. Paul, E. Hays, James H. Adams, Guillaume Prévôt, R. D. Young, E. G. Judd, C. Guepin, Patrick J. Reardon, F. W. Stecker, Roberto Aloisio, K. Shinozaki, Angela V. Olinto, M. E. Bertaina, Luis A. Anchordoqui, Mary Hall Reno, Tonia M. Venters, John F. Krizmanic, E. Kuznetsov, E. Parizot, Julie McEnery, J. W. Mitchell, Foteini Oikonomou, M. Unger, Marco Casolino, Johannes Eser, I. DeMitri, Douglas Bergman, J.F. Soriano, R. Diesing, L. R. Wiencke, F. Sarazin, Maria Teresa Ricci, A. N. Otte, Y. Takizawa, Ralf Ulrich, Austin Cummings, Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)
Subjects: Astrophysics and Astronomy, media_common.quotation_subject, Astrophysics::High Energy Astrophysical Phenomena, satellite, FOS: Physical sciences, Cosmic ray, 7. Clean energy, 01 natural sciences, High Energy Physics - Experiment, law.invention, High Energy Physics - Experiment (hep-ex), law, 0103 physical sciences, ultraviolet, optical, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], surface, Cherenkov, ddc:530, cosmic radiation: UHE, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], 010306 general physics, Instrumentation and Methods for Astrophysics (astro-ph.IM), Cherenkov radiation, media_common, Physics, astro-ph.HE, High Energy Astrophysical Phenomena (astro-ph.HE), COSMIC cancer database, hybrid, 010308 nuclear & particles physics, hep-ex, formation, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy, Photometer, messenger, Sky, Focal surface, fluorescence, Neutrino, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Ultrashort pulse, Particle Physics - Experiment, astro-ph.IM
Abstract: 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. The hybrid focal surface includes a fast (1 ${\mu}$s) ultraviolet camera for fluorescence observations and an ultrafast (10 ns) optical camera for Cherenkov observations. POEMMA will provide new multi-messenger windows onto the most energetic events in the universe, enabling the study of new astrophysics and particle physics at these otherwise inaccessible energies., Comment: 8 pages, 6 figures, presented in 36th International Cosmic Ray Conference (Madison). arXiv admin note: substantial text overlap with arXiv:1907.06217
Published: 2019

4. Mini-EUSO engineering model: tests in open-sky condition

Author: Christer Fuglesang, S. Turriziani, Toshikazu Ebisuzaki, Federico Fausti, Lech Wiktor Piotrowski, Z. Plebaniak, J. Szabelski, G. Osteria, A. Djakonow, Naoto Sakaki, P. Gorodetzky, W. Marszał, G. Cotto, A. Belov, A. Murashov, A. Cellino, G. Suino, Matteo Battisti, Marco Casolino, Claudio Fornaro, Daniele Gardiol, Dario Barghini, Y. Takizawa, P. Picozza, Francesca Capel, G. Cambiè, I. Churilo, S. Blin-Bondil, T. Napolitano, F. Bisconti, K. Shinozaki, Hiroko Miyamoto, A. Poroshin, Maria Teresa Ricci, Enzo Reali, A. Franceschi, L. Marcelli, Guillaume Prévôt, Francesco Fenu, F. Kajino, E. Parizot, M. Traïche, M. Przybylak, F. Cafagna, Marco Mignone, M. E. Bertaina, Pavel Klimov, M. I. Panasyuk, Organisation de Micro-Électronique Générale Avancée (OMEGA), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-École polytechnique (X), AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), JEM-EUSO, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-École polytechnique (X)-Centre National de la Recherche Scientifique (CNRS), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), École polytechnique (X)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP)
Subjects: media_common.quotation_subject, Astrophysics::High Energy Astrophysical Phenomena, Night sky, FOS: Physical sciences, Cosmic ray, law.invention, Atmosphere, Telescope, Planet, law, International Space Station, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Instrumentation and Methods for Astrophysics (astro-ph.IM), media_common, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), Meteoroid, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy, 13. Climate action, Sky, Physics::Space Physics, Astrophysics::Earth and Planetary Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract: Mini-EUSO is a UV telescope that will look downwards to the Earth's atmosphere onboard the International Space Station. With the design of the ultra-high energy cosmic ray fluorescence detectors belonging to the JEM-EUSO program, it will make the first UV map of the Earth by observing atmospheric phenomena such as transient luminous events, sprites and lightning, as well as meteors and bioluminescence from earth. Diffused light from laser shots from the ground, which mimic the fluorescence light emitted by Nitrogen molecules when extensive air showers pass through the atmosphere, can be used to verify the capability of this kind of detector to observe ultra-high energy cosmic rays. To validate the electronics and the trigger algorithms developed for Mini-EUSO, a scaled down version of the telescope with 1:9 of the original focal surface and a lens of 2.5 cm diameter has been built. Tests of the Mini-EUSO engineering model have been made in laboratory and in open sky condition. In this paper, we report results of observations of the night sky, which include the detection of stars, meteors, a planet and a rocket body reflecting the sunlight. Interesting results of the observation of city lights are also reported., Comment: presented at the 36th ICRC (Madison, WI; 2019)
Published: 2019
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5. Sharp increasing of positron to electron fluxes ratio below 2 GV measured by the PAMELA

Author: Alfonso Monaco, A. N. Kvashnin, M. Merge, V. V. Mikhailov, P. Carlson, A. G. Mayorov, G. I. Vasiliev, R. Sparvoli, N. De Simone, G. Zampa, Beatrice Panico, M. Simon, N. Zampa, Sergey Koldashov, G. A. Bazilevskaya, Yu. T. Yurkin, C. De Santis, Yu. I. Stozhkov, V. V. Malakhov, S. Yu. Krutkov, P. Picozza, Roberto Bellotti, Mark Pearce, S. B. Ricciarini, F. Palma, A. M. Galper, P. Papini, Giuseppe Osteria, E. Vannuccini, Matteo Martucci, S. A. Koldobsky, E. Mocchiutti, F. Cafagna, A. V. Karelin, Mirko Boezio, D. Campana, S. Bottai, Maria Teresa Ricci, S. A. Voronov, Marco Casolino, C. De Donato, Nicola Mori, E. A. Bogomolov, Riccardo Munini, M. Bongi, P. Spillantini, O. Adriani, W. Menn, V. Di Felice, V. Bonvicini, G. C. Barbarino, G. Castellini, L. Marcelli, A. Vacchi, A. Bruno, Alexey Leonov, Mikhailov, V. V., Adriani, O., Barbarino, G., Bazilevskaya, G. A., Bellotti, R., Boezio, M., Bogomolov, E. A., Bongi, M., Bonvicini, V., Bottai, S., Bruno, A., Cafagna, F. S., Campana, D., Carlson, P., Casolino, M., Castellini, G., De Donato, C., De Santis, C., De Simone, N., Di Felice, V., Galper, A. M., Karelin, A. V., Koldashov, S. V., Koldobsky, S., Krutkov, S. Y., Kvashnin, A. N., Leonov, A. A., Malakhov, V. V., Marcelli, L., Martucci, M., Mayorov, A. G., Menn, W., Merge, M., Mocchiutti, E., Monaco, A., Mori, N., Munini, R., Osteria, G., Papini, P., Palma, F., Panico, B., Pearce, M., Picozza, P., Ricci, M., Ricciarini, S. B., Simon, M., Sparvoli, R., Spillantini, P., Stozhkov, Y. I., Vacchi, A., Vannuccini, E., Vasiliev, G. I., Voronov, S. A., Yurkin, Y. T., Zampa, G., and Zampa, N.
Subjects: Physics, Settore FIS/01, History, Antiparticle, PAMELA detector, Spectrometer, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, Polar orbit, Cosmic ray, Astrophysics, Electron, Cosmology, Electrons, Magnetic polarity, Orbits, Positrons, Computer Science Applications, Education, law.invention, Physics and Astronomy (all), Positron, law, Physics::Space Physics, Satellite, Astrophysics::Earth and Planetary Astrophysics
Abstract: Magnetic spectrometer PAMELA was launched onboard a satellite Resurs-DK1 into low-Earth polar orbit with altitude 350-600 km to study cosmic ray antiparticle fluxes in a wide energy range from ~ 100 MeV to hundreds GeV. This paper presents the results of observations of temporal variations of the positron and electron fluxes in the 2006-2015. The ratio of the positron and electron fluxes below 2 GV shows sharp increasing since 2014 due to changing of the polarity of the solar magnetic field.
Published: 2017

6. Solar modulation of galactic cosmic rays during 2006-2015 based on PAMELA and ARINA data

Author: Alfonso Monaco, S. Bottai, A. G. Mayorov, P. Picozza, M. Merge, Maria Teresa Ricci, Sergey Koldobskiy, G. C. Barbarino, P. Yu. Naumov, A. V. Karelin, P. Spillantini, Alexey Leonov, R. Sparvoli, Mark Pearce, S. B. Ricciarini, Nicola Mori, S. A. Voronov, M. Simon, P. Papini, E. Vannuccini, N. Zampa, G. A. Bazilevskaya, L. Marcelli, E. A. Bogomolov, G. Osteria, D. Campana, A. Vacchi, Laura Rossetto, V. V. Malakhov, Yu. T. Yurkin, A. Bruno, V. V. Mikhailov, O. Adriani, M. A. Mayorova, Marco Casolino, Roberto Bellotti, A. M. Galper, Matteo Martucci, W. Menn, G. I. Vasilyev, V. Di Felice, A. A. Kvashnin, Mirko Boezio, G. Castellini, G. Zampa, Beatrice Panico, Riccardo Munini, C. De Santis, S. A. Rodenko, F. Cafagna, M. Bongi, Per Carlson, V. Bonvicini, Y. Stozhkov, Sergey Aleksandrin, E. Mocchiutti, and S. V. Koldashov
Subjects: Settore FIS/01, Physics, History, Scintillation, PAMELA detector, Spectrometer, Cosmic rays, Cosmology, Magnetic polarity, Modulation, Solar energy, Spectrometers Galactic cosmic rays, Magnetic spectrometers, Solar activity, Solar magnetic fields, Solar modulation, Transient periods, Astrophysics::High Energy Astrophysical Phenomena, Cosmic ray, Astrophysics, Computer Science Applications, Education, Magnetic field, law.invention, Physics and Astronomy (all), law, Physics::Space Physics, Nuclear Experiment
Abstract: Solar modulation of galactic protons with energies from 50 MeV up to dozens of GeV during July '06 - January '16 studied based on a data of the magnetic spectrometer PAMELA and scintillation spectrometer ARINA. This period is interesting because it covers the end of 23rd and current 24th cycles of solar activity, including the abnormally long transient period and change of the polarity of solar magnetic field. © Published under licence by IOP Publishing Ltd.
Published: 2017

7. The PAMELA experiment: A decade of Cosmic Ray Physics in space

Author: P. Spillantini, Matteo Martucci, Yu. T. Yurkin, Nicola Mori, M. Bongi, Riccardo Munini, S. Y. Krutkov, Per Carlson, G. Zampa, A. V. Karelin, Beatrice Panico, A. N. Kvashnin, R. Sparvoli, C. De Santis, C. De Donato, V. V. Malakhov, O. Adriani, P. Picozza, W. Menn, A. G. Mayorov, S. A. Voronov, M. Merge, G. A. Bazilevskaya, Sergey Koldobskiy, G. C. Barbarino, M. Simon, G. Osteria, G. I. Vasilyev, V. Di Felice, V. Bonvicini, S. Bottai, A. Bruno, Y. I. Stozhkov, N. Zampa, Maria Teresa Ricci, F. Cafagna, E. A. Bogomolov, Roberto Bellotti, E. Mocchiutti, V. V. Mikhailov, A. M. Galper, Mark Pearce, S. B. Ricciarini, P. Papini, E. Vannuccini, L. Marcelli, A. Vacchi, F. Palma, Mirko Boezio, Alexey Leonov, G. Castellini, Sergey Koldashov, D. Campana, Marco Casolino, Galper, A. M., Sparvoli, R., Adriani, O., Barbarino, G., Bazilevskaya, G. A., Bellotti, R., Boezio, M., Bogomolov, E. A., Bongi, M., Bonvicini, V., Bottai, S., Bruno, A., Cafagna, F., Campana, D., Carlson, P., Casolino, M., Castellini, G., De Donato, C., De Santis, C., Di Felice, V., Karelin, A. V., Koldashov, S. V., Koldobskiy, S. A., Krutkov, S. Y., Kvashnin, A. N., Leonov, A. A., Malakhov, V. V., Marcelli, L., Martucci, M., Mayorov, A. G., Menn, W., Merge, M., Mikhailov, V. V., Mocchiutti, E., Mori, N., Munini, R., Osteria, G., Palma, F., Panico, B., Papini, P., Pearce, M., Picozza, P., Ricci, M., Ricciarini, S. B., Simon, M., Spillantini, P., Stozhkov, Y. I., Vacchi, A., Vannuccini, E., Vasilyev, G. I., Voronov, S. A., Yurkin, Y. T., Zampa, G., and Zampa, N.
Subjects: Physics, Settore FIS/01, History, COSMIC cancer database, 010504 meteorology & atmospheric sciences, PAMELA detector, Astronomy, Cosmic ray, Astrophysics, Space (mathematics), Carbon, Cosmology, Earth (planet), High energy physics, Positrons, Radiation belts, Solar energy Continuous data, Elemental compositions, Heliospheres, Measurements of, Quark matter, Radiation environments, Solar activity, Solar modulation, 01 natural sciences, Computer Science Applications, Education, law.invention, On board, Physics and Astronomy (all), law, 0103 physical sciences, Satellite, 010306 general physics, 0105 earth and related environmental sciences
Abstract: The PAMELA detector was launched on June 15 th of 2006 on board the Russian Resurs-DK1 satellite and during ten years of continuous data-taking it has observed very interesting features in cosmic rays, especially in the fluxes of protons, helium and electrons. Moreover, PAMELA measurements of cosmic antiproton and positron fluxes and positron-to-all-electron ratio have set strong constraints to the nature of Dark Matter. Measurements of boron, carbon, lithium and beryllium (together with the isotopic fraction) have also shed new light on the elemental composition of the cosmic radiation. Search for signatures of more exotic processes (such as the ones involving Strange Quark Matter) has also been pursued. Furthermore, over the years the instrument has allowed a constant monitoring of the solar activity and a prolonged study of the solar modulation, improving the comprehension of the heliosphere mechanisms. PAMELA has also measured the radiation environment around the Earth, and detected for the first time the presence of an antiproton radiation belt surrounding our planet. In this highlight paper PAMELA main results will be reviewed.
Published: 2017

8. Solar modulation of galactic cosmic rays electrons and positrons over the 23rd solar minimum with the PAMELA experiment

Author: M. S. Potgieter, A. G. Mayorov, S. Bottai, E. Mocchiutti, M. Merge, G. Castellini, Sergey Koldobskiy, G. A. Bazilevskaya, G. C. Barbarino, N. Zampa, V. V. Mikhailov, Mirko Boezio, C. De Santis, G. Zampa, Beatrice Panico, Maria Teresa Ricci, V. Bonvicini, Ritabrata Sarkar, C. De Donato, L. Marcelli, A. Vacchi, S. Y. Krutkov, Matteo Martucci, A. Bruno, Y. I. Stozhkov, V. Formato, A. M. Galper, A. Leonov, A. V. Karelin, S. V. Koldashov, André Monaco, S. A. Voronov, Nicola Mori, F. Palma, V. V. Malakhov, E. A. Bogomolov, V. Di Felice, M. Simon, P. Picozza, F. Cafagna, Etienne Vos, P. Spillantini, G. Osteria, Riccardo Munini, D. Campana, G. I. Vasilyev, N. De Simone, Marco Casolino, Valentina Scotti, R. Sparvoli, Per Carlson, Y. T. Yurkin, Roberto Bellotti, O. Adriani, W. Menn, M. Bongi, Mark Pearce, S. B. Ricciarini, P. Papini, E. Vannuccini, and A. N. Kvashnin
Subjects: Solar minimum, Physics, Positron, PAMELA detector, Modulation, law, Astronomy, Cosmic ray, Electron, Astrophysics, law.invention
Abstract: The satellite-borne PAMELA experiment has been continuously collecting data since 15th June 2006, when it was launched from the Baikonur cosmodrome to detect the charged component of cosmic rays ov ...
Published: 2016

9. Features of re-entrant albedo deuteron trajectories in near Earth orbit with PAMELA experiment

Author: A. V. Karelin, V. Formato, S. A. Voronov, Yu. T. Yurkin, M. Merge, S. Y. Krutkov, P. Picozza, Sergey Koldashov, G. Osteria, R. Sparvoli, E. A. Bogomolov, V. V. Mikhailov, Per Carlson, Andrea Vacchi, O. Adriani, Mirko Boezio, Massimo Bongi, W. Menn, V. Di Felice, L. Marcelli, Roberto Bellotti, A. M. Galper, G. Zampa, Beatrice Panico, A. Bruno, V. V. Malakhov, Matteo Martucci, A. N. Kvashnin, D. Campana, Sergey Koldobskiy, G. C. Barbarino, N. Zampa, V. Bonvicini, Valentina Scotti, G. A. Bazilevskaya, Riccardo Munini, Y. I. Stozhkov, N. De Simone, Piero Spillantini, Marco Casolino, F. Cafagna, A. G. Mayorov, G. Castellini, F. Palma, Mark Pearce, S. B. Ricciarini, P. Papini, E. Vannuccini, Maria Teresa Ricci, C. De Donato, Ritabrata Sarkar, E. Mocchiutti, M. Simon, A. A. Leonov, S. Bottai, G. I. Vasilyev, Nicola Mori, C. De Santis, Alfonso Monaco, Koldobskiy, S. A., Adriani, O., Barbarino, G. C., Bazilevskaya, G. A., Bellotti, R., Boezio, M., Bogomolov, E. A., Bongi, M., Bonvicini, V., Bottai, S., Bruno, A., Cafagna, F., Campana, D., Carlson, P., Casolino, M., Castellini, G., De Donato, C., De Santis, C., De Simone, N., Felice, V. D., Formato, V., Galper, A. M., Karelin, A. V., Koldashov, S. V., Krutkov, S. Y., Kvashnin, A. N., Leonov, A., Malakhov, V., Marcelli, L., Martucci, M., Mayorov, A. G., Menn, W., Mergè, M., Mikhailov, V. V., Mocchiutti, E., Monaco, A., Mori, N., Munini, R., Osteria, G., Palma, F., Panico, B., Papini, P., Pearce, M., Picozza, P., Ricci, M., Ricciarini, S. B., Sarkar, R., Scotti, V., Simon, M., Sparvoli, R., Spillantini, P., Stozhkov, Y. I., Vacchi, A., Vannuccini, E., Vasilyev, G., Voronov, S. A., Yurkin, Y. T., Zampa, G., and Zampa, N.
Subjects: Physics, History, Earth's orbit, PAMELA detector, Settore FIS/04, Astrophysics::High Energy Astrophysical Phenomena, Nuclear Theory, Astrophysics, Cosmic ray measurement, Cosmology, Deuterium, Orbits, Solar radiation Cosmic-ray particles, Albedo, Computer Science Applications, Education, law.invention, Nuclear physics, Physics and Astronomy (all), law, Re entrant, Nuclear Experiment, Trajectory (fluid mechanics)
Abstract: The results of trajectory reconstruction for re-entrant albedo deuteron fluxes obtained in the PAMELA experiment are presented in this work. PAMELA is an international experiment aimed on measurements of cosmic ray particle fluxes in wide energy range. In particular, analysis of PAMELA data gives possibility to identify deuterons. Classification of re-entrant albedo deuterons with energies from 70 to 400 MeV/nucleon depending on theirs reconstructed lifetimes and generation zones is presented here at first time.
Published: 2016

10. Time variations of proton flux in Earth inner radiation belt during 23/24 solar cycles based on the PAMELA and the ARINA data

Author: Yu. T. Yurkin, Mark Pearce, S. B. Ricciarini, V. Di Felice, Roberta Sparvoli, G. Zampa, Beatrice Panico, P. Papini, E. Vannuccini, D. Campana, G. C. Barbarino, Valentina Scotti, Valerio Formato, Yu. I. Stozhkov, A. M. Galper, Mirko Boezio, S. Yu. Krutkov, Alexey Leonov, N. Zampa, G. A. Bazilevskaya, S. Bottai, A. G. Mayorov, A. N. Kvashnin, Ritabrata Sarkar, M. A. Mayorova, Marco Casolino, P. Spillantini, V. V. Mikhailov, A. V. Karelin, E. Mocchuuitti, M. Simon, V. V. Malakhov, Sergey Koldashov, Riccardo Munini, G. Osteria, G. Castellini, Matteo Martucci, F. Palma, A. A. Kvashnin, Massimo Bongi, O. Adriani, L. Marcelli, F. Cafagna, W. Menn, N. De Simone, A. Bruno, Maria Teresa Ricci, P. Picozza, V. Bonvicini, Per Carlson, A. Vacci, S. A. Voronov, E. A. Bogomolov, S. Yu. Aleksandrin, G. I. Vasilyev, C. De Santis, C. De Donato, Alfonso Monaco, M. Merge, Nicola Mori, Malakhov, V. V, Koldashov, S. V, Mayorov, A. G, Mayorova, M. A, Mikhailov, V. V, Aleksandrin, S. Yu, Adriani, O, Barbarino, Giancarlo, Bazilevskaya, G. A, Boezio, M, Bogomolov, E. A, Bongi, M, Bonvicini, V, Bottai, S, Bruno, A, Cafagna, F, Campana, D, Carlson, P, Casolino, M, Castellini, G, De Donato, C, De Santis, C, De Simone, N, Di Felice, V, Formato, V, Galper, A. M, Karelin, A. V, Krutkov, S. Yu, Kvashnin, A. A, Kvashnin, A. N, Leonov, A. A, Marcelli, L, Martucci, M, Menn, W, Merge, M, Mocchuuitti, E, Monaco, A, Mori, N, Munini, R, Osteria, G, Palma, F, Panico, B, Papini, P, Pearce, M, Picozza, P, Ricci, M, Ricciarini, S. B, Sarkar, R, Scotti, V, Simon, M, Sparvoli, R, Spillantini, P, Stozhkov, Yu I, Vacci, A, Vannuccini, E, Vasilyev, G. I, Voronov, S. A, Yurkin, Yu T, Zampa, G, Zampa, N., V., Malakhov, S. V., Koldashov, A. G., Mayorov, M. A., Mayorova, V. V., Mikhailov, Aleksandrin, S. Y. u., O., Adriani, G. C., Barbarino, G. A., Bazilevskaya, M., Boezio, E. A., Bogomolov, M., Bongi, V., Bonvicini, S., Bottai, A., Bruno, F., Cafagna, D., Campana, P., Carlson, M., Casolino, G., Castellini, C., De Donato, C., De Santi, N., De Simone, V., Di Felice, V., Formato, A. M., Galper, A. V., Karelin, S. Y., Krutkov, A. A., Kvashnin, A. N., Kvashnin, A., Leonov, L., Marcelli, M., Martucci, W., Menn, M., Mergé, E., Mocchiutti, A., Monaco, N., Mori, Munini, Riccardo, G., Osteria, F., Palma, B., Panico, P., Papini, M., Pearce, P., Picozza, M., Ricci, S. B., Ricciarini, R., Sarkar, V., Scotti, M., Simon, R., Sparvoli, P., Spillantini, Y. I., Stozhkov, A., Vacchi, E., Vannuccini, G. I., Vasilyev, S. A., Voronov, Y. T., Yurkin, G., Zampa, and N., Zampa
Subjects: History, High energy, Astrophysics::High Energy Astrophysical Phenomena, Cosmic ray, Astrophysics, Proton flux, radiation belt, Education, law.invention, satellite experiment, symbols.namesake, law, PAMELA, Cosmic rays, radiation belt, proton, PAMELA, Cosmic rays, Physics, PAMELA detector, Settore FIS/04, Astronomy, Computer Science Applications, Proton (rocket family), Van Allen radiation belt, Physics::Space Physics, symbols, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, Satellite, Time variations, proton
Abstract: The PAMELA and the ARINA experiments are carried out on the board of satellite RESURS-DK1 since 2006 up to now. Main goal of the PAMELA instrument is measurements of high energy antiparticles in cosmic rays while the ARINA instrument is intended studying high energy charged particle bursts in the magnetosphere. Both of these experiments have a possibility to study trapped particles in the inner radiation belt. Complex of these two instruments covers proton energy range from 30 MeV up to trapping limit (E= ~2 GeV). Continuous measurements with the PAMELA and the ARINA spectrometers include falling and rising phases of 23/24 solar cycles and maximum of 24th one. In this report we present temporal profiles of proton flux in the inner zone of the radiation belt (1.11 < L < 1.18, 0.18 < B < 0.22G). Dependence of proton fluxes on a magnitude of the solar activity was studied for various phases of 23/24 solar cycles. At that it was shown that proton fluxes at the solar minimum are several times greater than at the solar maximum.
Published: 2015

11. Solar modulation of GCR electrons over the 23rd solar minimum with PAMELA

Author: L. Marcelli, A. Vacchi, S. Bottai, A. Bruno, E. Mocchiutti, D. Campana, Mirko Boezio, Maria Teresa Ricci, Marco Casolino, F. Cafagna, A. V. Karelin, Riccardo Munini, Etienne Vos, G. Osteria, M. S. Potgieter, O. Adriani, Massimo Bongi, Matteo Martucci, Alexey Leonov, W. Menn, V. V. Mikhailov, V. Formato, Valentina Scotti, N. Zampa, G. A. Bazilevskaya, C. De Santis, Roberto Bellotti, A. M. Galper, Sergey Koldashov, A. N. Kvashnin, Mark Pearce, S. B. Ricciarini, P. Papini, E. Vannuccini, V. Bonvicini, Y. I. Stozhkov, A. G. Mayorov, M. Simon, Sergey Koldobskiy, F. Palma, G. C. Barbarino, V. Di Felice, Nicola Mori, V. V. Malakhov, C. De Donato, G. I. Vasilyev, Roberta Sparvoli, S. Y. Krutkov, P. Picozza, P. Spillantini, Alfonso Monaco, M. Merge, Ritabrata Sarkar, S. A. Voronov, E. A. Bogomolov, N. De Simone, G. Castellini, Per Carlson, Yu. T. Yurkin, G. Zampa, Beatrice Panico, Munini, R, Di Felice, V, Adriani, O, Barbarino, Giancarlo, Bazilevskaya, G. A, Bellotti, R, Boezio, M, Bogomolov, E. A, Bongi, M, Bonvicini, V, Bottai, S, Bruno, A, Cafagna, F, Campana, D, Carlson, P, Casolino, M, Castellini, G, De Donato, C, De Santis, C, De Simone, N, Formato, V, Galper, A. M, Karelin, A. V, Koldashov, S. V, Koldobskiy, S, Krutkov, S. Y, Kvashnin, A. N, Leonov, A, Malakhov, V, Marcelli, L, Martucci, M, Mayorov, A. G, Menn, W, Merge, M, Mikhailov, V. V, Mocchiutti, E, Monaco, A, Mori, N, Osteria, G, Palma, F, Panico, B, Papini, P, Pearce, M, Picozza, P, Ricci, M, Ricciarini, S. B, Sarkar, R, Scotti, V, Simon, M, Sparvoli, R, Spillantini, P, Stozhkov, Y. I, Vacchi, A, Vannuccini, E, Vasilyev, G, Voronov, S. A, Yurkin, Y. T, Zampa, G, Zampa, N, Potgieter, M. S, Vos, E. E., Munini, Riccardo, V., Di Felice, O., Adriani, G. C., Barbarino, G. A., Bazilevskaya, R., Bellotti, M., Boezio, E. A., Bogomolov, M., Bongi, V., Bonvicini, S., Bottai, A., Bruno, F., Cafagna, D., Campana, P., Carlson, M., Casolino, G., Castellini, C., De Donato, C., De Santi, N., De Simone, V., Formato, A. M., Galper, A. V., Karelin, S. V., Koldashov, S., Koldobskiy, S. Y., Krutkov, A. N., Kvashnin, A., Leonov, V., Malakhov, L., Marcelli, M., Martucci, A. G., Mayorov, W., Menn, M., Mergé, V. V., Mikhailov, E., Mocchiutti, A., Monaco, N., Mori, G., Osteria, F., Palma, B., Panico, P., Papini, M., Pearce, P., Picozza, M., Ricci, S. B., Ricciarini, R., Sarkar, V., Scotti, M., Simon, R., Sparvoli, P., Spillantini, Y. I., Stozhkov, A., Vacchi, E., Vannuccini, G. I., Vasilyev, S. A., Voronov, Y. T., Yurkin, G., Zampa, N., Zampa, M. S., Potgieter, and E. E., Vos
Subjects: Solar minimum, electron, History, Antiparticle, Astrophysics::High Energy Astrophysical Phenomena, solar minimum, Solar cycle 23, Cosmic ray, Astrophysics, Solar Modulation, electron, solar minimum, PAMELA, Education, law.invention, Physics and Astronomy (all), law, PAMELA, Cosmology, Modulation, Solar energy Apparatus design, Charged components, Electron spectrum, Galactic cosmic rays, Solar minima, Solar modulation, Solar modulation effects, Coronal mass ejection, Physics, PAMELA detector, Settore FIS/04, Computer Science Applications, Solar cycle, Solar Modulation, Antimatter, Physics::Space Physics, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING
Abstract: The satellite-borne PAMELA experiment has been continuously collecting data since 15th June 2006, when it was launched from the Baikonur cosmodrome to detect the charged component of cosmic rays over a wide energy range and with unprecedented statistics. The apparatus design is particularly suited for particle and antiparticle identification. The PAMELA experiment has measured the electron spectrum at Earth in great detail, extending up to about 100 GeV and down to about 200 MeV. The galactic cosmic ray electron spectra for 2007 and 2009, i.e. measured during the A
Published: 2015

12. PAMELA measurements of the boron and carbon spectra

Author: Alexey Leonov, A. G. Mayorov, Ritabrata Sarkar, G. Zampa, Beatrice Panico, S. Y. Krutkov, Yu. T. Yurkin, A. V. Karelin, C. De Santis, N. Zampa, G. A. Bazilevskaya, P. Picozza, P. Spillantini, Valerio Formato, C. De Donato, G. Osteria, Riccardo Munini, D. Campana, R. Carbone, O. Adriani, Alfonso Monaco, Sergey Koldobskiy, V. Di Felice, G. C. Barbarino, W. Menn, V. Bonvicini, V. V. Malakhov, Marco Casolino, Roberto Bellotti, Valentina Scotti, G. Castellini, A. M. Galper, L. Marcelli, Y. I. Stozhkov, A. Vacchi, S. Bottai, A. Bruno, M. Merge, N. De Simone, M. Bongi, A. N. Kvashnin, Mark Pearce, S. B. Ricciarini, Sergey Koldashov, Nicola Mori, P. Papini, Matteo Martucci, E. Vannuccini, Mirko Boezio, S. A. Voronov, G. I. Vasilyev, Per Carlson, E. A. Bogomolov, F. Palma, V. V. Mikhailov, Maria Teresa Ricci, F. Cafagna, M. Simon, Roberta Sparvoli, E. Mocchiutti, N., Mori, O., Adriani, G. C., Barbarino, G. A., Bazilevskaya, R., Bellotti, M., Boezio, E. A., Bogomolov, M., Bongi, V., Bonvicini, S., Bottai, A., Bruno, F., Cafagna, D., Campana, R., Carbone, P., Carlson, M., Casolino, G., Castellini, C., De Donato, C., De Santi, N., De Simone, V., Di Felice, V., Formato, A. M., Galper, A. V., Karelin, S. V., Koldashov, S., Koldobskiy, S. Y., Krutkov, A. N., Kvashnin, A., Leonov, V., Malakhov, L., Marcelli, M., Martucci, A. G., Mayorov, W., Menn, M., Mergé, V. V., Mikhailov, E., Mocchiutti, A., Monaco, Munini, Riccardo, G., Osteria, F., Palma, B., Panico, P., Papini, M., Pearce, P., Picozza, M., Ricci, S. B., Ricciarini, R., Sarkar, V., Scotti, M., Simon, R., Sparvoli, P., Spillantini, Y. I., Stozhkov, A., Vacchi, E., Vannuccini, G. I., Vasilyev, S. A., Voronov, Y. T., Yurkin, G., Zampa, N., Zampa, Mori, N, Adriani, O, Barbarino, Giancarlo, Bazilevskaya, G. A, Bellotti, R, Boezio, M, Bogomolov, E. A, Bongi, M, Bonvicini, V, Bottai, S, Bruno, A, Cafagna, F, Campana, D, Carbone, R, Carlson, P, Casolino, M, Castellini, G, De Donato, C, De Santis, C, De Simone, N, Felice, V. Di, Formato, V, Galper, A. M, Karelin, A. V, Koldashov, S. V, Koldobskiy, S, Krutkov, S. Y, Kvashnin, A. N, Leonov, A, Malakhov, V, Marcelli, L, Martucci, M, Mayorov, A. G, Menn, W, Mergé, M, Mikhailov, V. V, Mocchiutti, E, Monaco, A, Munini, R, Osteria, G, Palma, F, Panico, B, Papini, P, Pearce, M, Picozza, P, Ricci, M, Ricciarini, S. B, Sarkar, R, Scotti, V, Simon, M, Sparvoli, R, Spillantini, P, Stozhkov, Y. I, Vacchi, A, Vannuccini, E, Vasilyev, G. I, Voronov, S. A, Yurkin, Y. T, Zampa, G, and Zampa, N.
Subjects: History, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, chemistry.chemical_element, Cosmic ray, Spectral line, Education, law.invention, Nuclear physics, Physics and Astronomy (all), cosmic rays, law, PAMELA, Boron, Cosmic ray measurement, Cosmology, High energy physics Anticoincidence systems, Boron and carbons, Cosmic ray spectra, Data analysis techniques, Electromagnetic calorimeter, Injection spectra, Magnetic spectrometers, Time of flight systems, Neutron detection, Physics, carbon boron, Spectrometer, PAMELA detector, Settore FIS/04, PAMELA, cosmic rays, carbon boron, fluxes, fluxes, Computer Science Applications, chemistry, Antimatter, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, Carbon
Abstract: The satellite-borne PAMELA experiment is aimed at precision measurements of the charged light component of the cosmic-ray spectrum, with a particular focus on antimatter. It consists of a magnetic spectrometer, a time-of-flight system, an electromagnetic calorimeter with a tail catcher scintillating layer, an anticoincidence system and a neutron detector. PAMELA has measured the absolute fluxes of boron and carbon and the B/C ratio, which plays a central role in galactic propagation studies in order to derive the injection spectra at sources from measurements at Earth. In this paper, the data analysis techniques and the final results are presented.
Published: 2015

13. Measurement of electron-positron spectrum in high-energy cosmic rays in the PAMELA experiment

Author: S. Bottai, Roberta Sparvoli, Sergey Koldobskiy, A. V. Karelin, G. C. Barbarino, Alfonso Monaco, Yu. T. Yurkin, D. Campana, G. Osteria, Riccardo Munini, M. Merge, L. Marcelli, A. Vacchi, Per Carlson, Marco Casolino, A. Bruno, F. Palma, V. V. Malakhov, S. Y. Krutkov, Sergey Koldashov, Massimo Bongi, S. A. Voronov, Roberto Bellotti, G. Zampa, Beatrice Panico, R. Carbone, A. M. Galper, E. A. Bogomolov, N. Zampa, G. A. Bazilevskaya, Valentina Scotti, A. N. Kvashnin, P. Picozza, G. Castellini, Laura Rossetto, Mirko Boezio, Mark Pearce, S. B. Ricciarini, Alexey Leonov, N. De Simone, P. Papini, E. Vannuccini, Ritabrata Sarkar, Valerio Formato, V. V. Mikhailov, M. Simon, O. Adriani, W. Menn, Matteo Martucci, F. Cafagna, Maria Teresa Ricci, Piero Spillantini, A. G. Mayorov, G. I. Vasilyev, C. De Santis, C. De Donato, Nicola Mori, E. Mocchiutti, V. Di Felice, V. Bonvicini, A. V., Karelin, O., Adriani, G. C., Barbarino, G. A., Bazilevskaya, R., Bellotti, M., Boezio, E. A., Bogomolov, M., Bongi, V., Bonvicini, S., Bottai, A., Bruno, F., Cafagna, D., Campana, R., Carbone, P., Carlson, M., Casolino, G., Castellini, C., De Donato, C., De Santi, N., De Simone, V., Di Felice, V., Formato, A. M., Galper, S. V., Koldashov, S., Koldobskiy, S. Y., Krutkov, A. N., Kvashnin, A., Leonov, A. G., Mayorov, V., Malakhov, L., Marcelli, M., Martucci, W., Menn, M., Mergé, V. V., Mikhailov, E., Mocchiutti, A., Monaco, N., Mori, Munini, Riccardo, G., Osteria, F., Palma, B., Panico, P., Papini, M., Pearce, P., Picozza, M., Ricci, S. B., Ricciarini, R., Sarkar, V., Scotti, L., Rossetto, M., Simon, R., Sparvoli, P., Spillantini, A., Vacchi, E., Vannuccini, G. I., Vasilyev, S. A., Voronov, Y. T., Yurkin, G., Zampa, N., Zampa, Karelin, A. V, Adriani, O, Barbarino, Giancarlo, Bazilevskaya, G. A, Bellotti, R, Boezio, M, Bogomolov, E. A, Bongi, M, Bonvicini, V, Bottai, S, Bruno, A, Cafagna, F, Campana, D, Carbone, R, Carlson, P, Casolino, M, Castellini, G, De Donato, C, De Santis, C, De Simone, N, Felice, V. Di, Formato, V., Galper, A. M, Koldashov, S. V, Koldobskiy, S. A, Krutkov, S. Y, Kvashnin, A. N, Leonov, A. A, Mayorov, A. G, Malakhov, V. V, Marcelli, L, Martucci, M., Menn, W, Merge, M., Mikhailov, V. V, Mocchiutti, E, Monaco, A, Mori, N, Munini, R., Osteria, G, Palma, F, Panico, B., Papini, P, Pearce, M, Picozza, P, Ricci, M, Ricciarini, S. B, Sarkar, R, Scotti, V., Rossetto, L, Simon, M, Sparvoli, R, Spillantini, P, Vacchi, A, Vannuccini, E, Vasilyev, G. I, Voronov, S. A, Yurkin, Y. T, Zampa, G, and Zampa, N.
Subjects: electron, History, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Cosmic rays, positron, electron, PAMELA, Cosmic ray, Particle detector, Education, law.invention, Nuclear physics, Physics and Astronomy (all), Positron, law, PAMELA, Neutron detection, Ultra-high-energy cosmic ray, Cosmic rays, Physics, Calorimeter (particle physics), PAMELA detector, Settore FIS/04, Computer Science Applications, Antimatter, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, positron, High Energy Physics::Experiment, Calorimeters, Cosmic ray measurement, Cosmology, Electron energy levels, Positrons, Tellurium compounds Cosmic ray electrons, Energy ranges, High-energy cosmic rays, High-energy electron, High-energy range
Abstract: At present the existing data on the cosmic ray electron energy spectra in the high energy range are fragmented, and the situation is exacerbated by their small number. In the satellite PAMELA experiment measurements at high energies are carried out by the calorimeter. The experimental data accumulated for more than 8 years of measurements, with the information of the calorimeter, the neutron detector and the scintillation counters made it possible to obtain the total spectrum of high-energy electrons and positrons in energy range 0.3-3 TeV.
Published: 2015

14. A method to detect positron anisotropies with Pamela data

Author: R. Carbone, Sergey Koldobskiy, G. C. Barbarino, V. Di Felice, P. Spillantini, A. M. Galper, M. Simon, Roberto Bellotti, A. A. Leonov, V. G. Zverev, Per Carlson, E. Mocchiutti, Riccardo Munini, A. N. Kvashnin, A. G. Mayorov, S. Y. Krutkov, N. Zampa, G. A. Bazilevskaya, V. V. Malakhov, Maria Teresa Ricci, V. Bonvicini, Y. I. Stozhkov, Valerio Formato, S. B. Ricciarini, Roberta Sparvoli, C. Pizzolotto, S. A. Voronov, P. Picozza, Alfonso Monaco, G. Zampa, Beatrice Panico, Mark Pearce, E. A. Bogomolov, Y. T. Yurkin, A. V. Karelin, F. Palma, S. Bottai, M. Merge, G. Castellini, G. Osteria, Mirko Boezio, P. Papini, E. Vannuccini, Ritabrata Sarkar, Matteo Martucci, V. V. Mikhailov, N. De Simone, F. Cafagna, C. De Donato, Nicola Mori, G. I. Vasilyev, C. De Santis, O. Adriani, W. Menn, M. Bongi, L. Marcelli, A. Vacchi, A. Bruno, D. Campana, Marco Casolino, Sergey Koldashov, V. Scotti, Ugo Giaccari, Panico, B., Adriani, O., Barbarino, G. C., Bazilevskaya, G. A., Bellotti, R., Boezio, M., Bogomolov, E. A., Bongi, M., Bonvicini, V., Bottai, S., Bruno, A., Cafagna, F., Campana, D., Carbone, R., Carlson, P., Casolino, M., Castellini, G., De Donato, C., De Santis, C., De Simone, N., Di Felice, V., Formato, V., Galper, A. M., Giaccari, U., Karelin, A. V., Koldashov, S. V., Koldobskiy, S., Krutkov, S. Y., Kvashnin, A. N., Leonov, A., Malakhov, V., Marcelli, L., Martucci, M., Mayorov, A. G., Menn, W., Merge, M., Mikhailov, V. V., Mocchiutti, E., Monaco, A., Mori, N., Munini, R., Osteria, G., Palma, F., Papini, P., Pearce, M., Picozza, P., Pizzolotto, C., Ricci, M., Ricciarini, S. B., Sarkar, R., Scotti, V., Simon, M., Sparvoli, R., Spillantini, P., Stozhkov, Y. I., Vacchi, A., Vannuccini, E., Vasilyev, G. I., Voronov, S. A., Yurkin, Y. T., Zampa, G., Zampa, N., Zverev, V. G., and Munini, Riccardo
Subjects: Physics, PAMELA, cosmic ray, anisotropy, positron, electrons, Nuclear and High Energy Physics, Annihilation, PAMELA detector, Astrophysics::High Energy Astrophysical Phenomena, Dark matter, Flux, Cosmic ray, Astrophysics, Electron, Atomic and Molecular Physics, and Optics, law.invention, Nuclear physics, Positron, Pulsar, law, Atomic and Molecular Physics, Anisotropy, Electrons, and Optics
Abstract: The PAMELA experiment is collecting data since 2006; its results indicate the presence of a large flux of positron with respect to electrons in the CR spectrum above 10 GeV. This excess might also be originated in objects such as pulsars and microquasars or through dark matter annihilation. Here the electrons and positrons events collected by PAMELA have been analized searching for anisotropies. The analysis is performed at different angular scales and results will be presented at the conference. © 2014 Elsevier B.V.
Published: 2014

15. Solar modulation of galactic protons and helium with the PAMELA experiment

Author: V. Formato, S. A. Voronov, V. Bonvicini, E. A. Bogomolov, Mark Pearce, S. B. Ricciarini, P. Papini, E. Vannuccini, A. Bruno, Y. I. Stozhkov, S. V. Koldashov, A. N. Kvashnin, C. De Donato, Nicola Mori, A. M. Galper, S. Y. Krutkov, V. G. Zverev, C. De Santis, M. Merge, M. Simon, C. Pizzolotto, E. Mocchiutti, G. Castellini, A. A. Leonov, A. G. Mayorov, V. Di Felice, V. V. Malakhov, N. Zampa, O. Adriani, N. De Simone, Riccardo Munini, G. I. Vasilyev, R. Sparvoli, W. Menn, P. Picozza, M. P. De Pascale, D. Campana, G. Zampa, Matteo Martucci, Marco Casolino, Piero Spillantini, André Monaco, Maria Teresa Ricci, Valentina Scotti, Ritabrata Sarkar, G. A. Bazilevskaya, S. Bottai, R. Carbone, G. C. Barbarino, F. Palma, V. V. Mikhailov, Mirko Boezio, P. Carlson, L. Marcelli, A. Vacchi, F. Cafagna, Massimo Bongi, Y. T. Yurkin, Roberto Bellotti, A. V. Karelin, G. Osteria, Formato, V., Boezio, M., Bonvicini, V., Carbone, R., Mocchiutti, E., Munini, Riccardo, Sarkar, R., Vacchi, A., Zampa, G., Zampa, N., Casolino, M., Donato, C. DE, Simone, N. DE, Pascale, M. P. DE, Santis, C. DE, Felice, V. DI, Marcelli, L., Martucci, M., Merg, M., Palma, F., Picozza, P., Sparvoli, R., Adriani, O., Bongi, M., Bottai, S., Mori, N., Papini, P., Ricciarini, S. B., Spillantini, P., Vannuccini, E., Barbarino, G. C., Campana, D., Osteria, G., Scotti, V., Bazilevskaya, G. A., Kvashnin, A. N., Stozhkov, Y. I., Bellotti, R., Bruno, A., Cafagna, F., Monaco, A., Bogomolov, E. A., Krutkov, S. Y., Vasilyev, G., Carlson, P., Pearce, M., Castellini, G., Galper, A. M., Karelin, A. V., Koldashov, S. V., Leonov, A., Malakhov, V., Mayorov, A. G., Mikhailov, V. V., Voronov, S. A., Yurkin, Y. T., Zverev, V. G., Pizzolotto, C., Ricci, M., Menn, W., and Simon, M.
Subjects: Solar minimum, Physics, Proton, PAMELA detector, Spectrometer, Physics::Instrumentation and Detectors, solar modulation, Astrophysics::High Energy Astrophysical Phenomena, Solar cycle 23, chemistry.chemical_element, Cosmic ray, Astrophysics, Charged particle, law.invention, PAMELA, cosmic rays, proton, solar modulation, chemistry, cosmic rays, law, PAMELA, Astrophysics::Earth and Planetary Astrophysics, Helium, proton
Abstract: PAMELA has been orbiting the Earth for more than six years, gathering data on solar, galactic and trapped cosmic rays during the time of the last solar minimum. The apparatus comprises a time-of-flight system, a silicon-microstrip magnetic spectrometer, a silicon-tungsten electromagnetic calorimeter, an anticoincidence system, a shower tail catcher scintillator and a neutron detector. The combination of these devices allows charged particle and antiparticle identification over a wide energy range and with an unprecedented precision. The quasi-polar orbit of the instrument, with an inclination of 70 degrees, makes it possible to measure low energy particles starting from about 100 MeV/n. In this work we present the time and rigidity dependence of the galactic proton and helium fluxes over the first 4 years of operation during the A < 0 solar minimum of solar cycle 23.
Published: 2014

16. PRECISE COSMIC RAYS MEASUREMENTS WITH PAMELA

Author: S. V. Borisov, G. Zampa, S. A. Voronov, N. De Simone, P. Spillantini, E. A. Bogomolov, A. V. Karelin, C. De Santis, William Gillard, Giovanna Jerse, L. Marcelli, A. G. Mayorov, A. Vacchi, Laura Rossetto, V. V. Mikhailov, V. G. Zverev, G. C. Barbarino, G. Osteria, F. Palma, O. Adriani, R. Carbone, S. Bottai, V. Di Felice, N. N. Nikonov, W. Menn, L. Consiglio, Alfonso Monaco, Juan Wu, Roberta Sparvoli, N. Zampa, G. A. Bazilevskaya, S. Y. Krutkov, M. D. Kheymits, L. A. Grishantseva, M. Bongi, V. V. Malakhov, C. Pizzolotto, M. P. De Pascale, Nicola Mori, V. Bonvicini, Y. T. Yurkin, D. Campana, F. Cafagna, A. Bruno, Y. I. Stozhkov, Maria Teresa Ricci, P. Picozza, Roberto Bellotti, Per Carlson, Mirko Boezio, Marco Casolino, E. Mocchiutti, G. I. Vasilyev, A. N. Kvashnin, M. Simon, S. V. Koldashov, A. A. Leonov, A. M. Galper, Ritabrata Sarkar, G. Castellini, Mark Pearce, S. B. Ricciarini, P. Papini, E. Vannuccini, A., Bruno, O. c., Adriani, Barbarino, Giancarlo, G., Bazilevskaya, R. g., Bellotti, M., Boezio, E., Bogomolov, M., Bongi, V., Bonvicini, S. k., L., S., Bottai, F., Cafagna, D., Campana, R. k., Carbone, P., Carlson, M., Casolino, G., Castellini, Consiglio, Lucia, M. k., De, C. k., De, N. k., De, V. D., Felice, A., Galper, W., Gillard, L., Grishantseva, G. o., Jerse, A., Karelin, M., Kheymit, S., Koldashov, S., Krutkov, A., Kvashnin, A., Leonov, V., Malakhov, L., Marcelli, A., Mayorov, W., Menn, V., Mikhailov, E., Mocchiutti, A. c., Monaco, N. c., Mori, N. j., K., Osteria, Giuseppe, F. k., Palma, P., Papini, M., Pearce, P. k., Picozza, C., Pizzolotto, M., Ricci, S., Ricciarini, L., Rossetto, R., Sarkar, M., Simon, R. k., Sparvoli, P. c., Spillantini, Y., Stozhkov, A., Vacchi, E., Vannuccini, G., Vasilyev, S., Voronov, Y., Yurkin, J., Wu, G., Zampa, N., Zampa, and V., Zverev
Subjects: Physics, Antimatter, Cosmic rays, Dark matter, Solar modulation, Trapped radiation, Engineering (all), PAMELA detector, Astrophysics::High Energy Astrophysical Phenomena, General Engineering, Astronomy, Magnetosphere, Cosmic ray, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Galaxy, law.invention, Positron, Antiproton, law, lcsh:TA1-2040, lcsh:Engineering (General). Civil engineering (General)
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. �� Czech Technical University in Prague, 2013.
Published: 2013

17. The PAMELA experiment: light-nuclei selection with stand-alone detectors

Author: V. Malvezzi, C. Pizzolotto, P. Spillantini, E. Mocchiutti, C. De Santis, S. Y. Krutkov, V. Di Felice, Matteo Martucci, Ugo Giaccari, Juan Wu, N. Zampa, G. A. Bazilevskaya, V. Bonvicini, P. Picozza, Y. I. Stozhkov, S. V. Koldashov, A. G. Mayorov, Mark Pearce, S. B. Ricciarini, Alfonso Monaco, G. Castellini, G. I. Vasilyev, Lorenzo Bonechi, V. V. Malakhov, M. Simon, A. A. Leonov, P. Papini, E. Vannuccini, Riccardo Munini, L. A. Grishantseva, O. Adriani, Ritabrata Sarkar, W. Menn, M. P. De Pascale, Nicola Mori, Giovanna Jerse, A. Bianco, Maria Teresa Ricci, S. A. Voronov, Valerio Formato, A. M. Galper, D. Campana, M. Bongi, N. N. Nikonov, F. Cafagna, N. De Simone, Marco Casolino, E. A. Bogomolov, V. V. Mikhailov, Laura Rossetto, Y. T. Yurkin, S. V. Borisov, A. V. Karelin, Mirko Boezio, R. Carbone, G. C. Barbarino, G. Osteria, Per Carlson, Roberto Bellotti, A. N. Kvashnin, F. Palma, Andrea Vacchi, L. Marcelli, A. Bruno, V. G. Zverev, S. Bottai, Roberta Sparvoli, M. D. Kheymits, G. Zampa, A D Erlykin, R P Kokoulin, A S Lidvansky, L I Meroshnichenko, M I Panasyuk, A D Panov A W Wolfendale, R., Carbone, O., Adriani, G. C., Barbarino, G. A., Bazilevskaya, R., Bellotti, A., Bianco, M., Boezio, E. A., Bogomolov, L., Bonechi, M., Bongi, V., Bonvicini, S., Borisov, S., Bottai, A., Bruno, F., Cafagna, D., Campana, P., Carlson, M., Casolino, G., Castellini, M. P., De Pascale, C., De Santi, N., De Simone, V., Di Felice, Formato, Valerio, A. M., Galper, U., Giaccari, L., Grishantseva, Jerse, Giovanna, A. V., Karelin, M. D., Kheymit, S. V., Koldashov, S. Y., Krutkov, A. N., Kvashnin, A., Leonov, V., Malakhov, V., Malvezzi, L., Marcelli, M., Martucci, A. G., Mayorov, W., Menn, V. V., Mikhailov, Mocchiutti, Emiliano, A., Monaco, N., Mori, Munini, Riccardo, N., Nikonov, G., Osteria, F., Palma, P., Papini, M., Pearce, P., Picozza, C., Pizzolotto, M., Ricci, S. B., Ricciarini, L., Rossetto, R., Sarkar, M., Simon, R., Sparvoli, P., Spillantini, Y. I., Stozhkov, Vacchi, Andrea, E., Vannuccini, G., Vasilyev, S. A., Voronov, J., Wu, Y. T., Yurkin, G., Zampa, N., Zampa, V. G., Zverev, O. c., Adriani, Barbarino, Giancarlo, G., Bazilevskaya, R. h., Bellotti, A. i., Bianco, E., Bogomolov, S. l., M, A. h., Bruno, M. l., De, C. D., Santi, N. D., Simone, V. D., Felice, V. i., Formato, A., Galper, G. i., Jerse, A., Karelin, M., Kheymit, S., Koldashov, S., Krutkov, A., Kvashnin, M. p., Martucci, A., Mayorov, V., Mikhailov, E., Mocchiutti, A. h., Monaco, R. i. n, N. k. l, Osteria, Giuseppe, F. l., Palma, P. l., Picozza, C. r., S, S., Ricciarini, R. l., Sparvoli, P. c., Spillantini, Y., Stozhkov, A., Vacchi, S., Voronov, Y., Yurkin, and V., Zverev
Subjects: Physics, History, Analysis strategies, Dark matter, Energy ranges, Light nuclei, Magnetic spectrometers, Measurements of, Precise measurements, Propagation models, Space experiments, Time-of-flight system, COSMIC cancer database, Spectrometer, PAMELA detector, Astrophysics::High Energy Astrophysical Phenomena, Dark matter, Cosmic ray, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, Galaxy, Cosmic Rays, Settore FIS/04 - Fisica Nucleare e Subnucleare, Computer Science Applications, Education, law.invention, Nuclear physics, Cosmic ray measurement, Positron, Antiproton, law, Nuclear Experiment, Cosmic rays, Detectors, Experiments, Galaxies, Isotope
Abstract: Launched on the 15th of June 2006, the space experiment PAMELA 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. In addition, PAMELA measurements of cosmic antiproton and positron fluxes are setting strong constraints to the nature of Dark Matter. PAMELA is also testing cosmic rays acceleration and propagation models through precise measurements of light nuclei and their isotopes. The determination of fluxes and secondary-to-primary ratios is possible for nuclei up to Oxygen in the energy range 200MeV/n – 150 GeV/n. To investigate this important item, PAMELA can use measurements from three main detectors: the magnetic spectrometer, the calorimeter and the Time-of-Flight system. Analysis strategy and performance for nuclei studies using the detectors in stand-alone configuration will be discussed in this work.
Published: 2013

18. Cosmic ray electron and positron spectra measured with PAMELA

Author: Alfonso Monaco, S. A. Voronov, Maria Teresa Ricci, V. Bonvicini, G. I. Vasiliev, Y. I. Stozhkov, Roberta Sparvoli, E. A. Bogomolov, P. Picozza, Per Carlson, Laura Rossetto, Giovanna Jerse, L. Consiglio, Ritabrata Sarkar, P. Spillantini, S. V. Borisov, V. V. Malakhov, C. Pizzolotto, V. Di Felice, S. Bottai, Mark Pearce, S. B. Ricciarini, V. Malvezzi, V. G. Zverev, Lorenzo Bonechi, R. Carbone, C. De Santis, M. P. De Pascale, S. Yu. Krutkov, G. C. Barbarino, F. Cafagna, L. Marcelli, A. Vacchi, A. G. Mayorov, G. Zampa, D. Campana, N. De Simone, P. Papini, A. Bruno, Marco Casolino, E. Vannuccini, V. V. Mikhailov, G. Castellini, Juan Wu, Y. T. Yurkin, A. V. Karelin, Giuseppe Osteria, F. Palma, M. Simon, A. A. Leonov, M. Bongi, N. Zampa, G. A. Bazilevskaya, Roberto Bellotti, A. M. Galper, A. N. Kvashnin, O. Adriani, W. Menn, S. A. Koldobsky, Mirko Boezio, Nicola Mori, S. V. Koldashov, E. Mocchiutti, V., Mikhailov, O., Adriani, Barbarino, Giancarlo, G., Bazilevskaya, R., Bellotti, M., Boezio, E., Bogomolov, L., Bonechi, M., Bongi, V., Bonvicini, S., Borisov, S., Bottai, A., Bruno, F., Cafagna, D., Campana, R., Carbone, P., Carlson, M., Casolino, G., Castellini, Consiglio, Lucia, M. m., De, C. D., Santi, N. D., Simone, V. D., Felice, A., Galper, G., Jerse, A., Karelin, S., Koldashov, S., Koldobsky, S. Y., Krutkov, A., Kvashnin, A., Leonov, V., Malakhov, V., Malvezzi, L., Marcelli, A., Mayorov, W., Menn, E., Mocchiutti, A., Monaco, N., Mori, Osteria, Giuseppe, P., Papini, F. m., Palma, M., Pearce, P. m., Picozza, C., Pizzolotto, M., Ricci, S., Ricciarini, L., Rossetto, R., Sarkar, M., Simon, R. m., Sparvoli, P., Spillantini, Y., Stozhkov, A., Vacchi, E., Vannuccini, G., Vasiliev, S., Voronov, J., Wu, Y., Yurkin, G., Zampa, N., Zampa, and V., Zverev
Subjects: Physics, History, Antiparticle, PAMELA detector, Spectrometer, Astrophysics::High Energy Astrophysical Phenomena, Polar orbit, Cosmic ray, Astrophysics, Electrons, Positrons, Tungsten, Particle detector, Cosmic ray electrons, Electromagnetic calorimeter, Magnetic spectrometers, Polar orbit, Propagation models, Wide energy range, Settore FIS/04 - Fisica Nucleare e Subnucleare, Computer Science Applications, Education, law.invention, Nuclear physics, Physics and Astronomy (all), Positron, law, Antimatter, Cosmic rays
Abstract: The PAMELA experiment is carried out on board of the satellite Resurs DK1 launched on June 15th 2006 on polar orbit (the inclination is 70, the altitude is 350-600 km). The instrument which consists of magnetic spectrometer, silicon-tungsten imaging electromagnetic calorimeter gives a possibility to measure electron and positron fluxes over wide energy range from hundreds MeVs to hundreds GeVs. Measurements made in June 2006- January 2010 are presented and compared with other results and models. Positron spectrum appears to be harder than standard diffusive propagation models predict.
Published: 2013

19. Search for cosmic ray electron-positron anisotropies with the Pamela data

Author: Riccardo Munini, S. Y. Krutkov, A. V. Karelin, G. Osteria, D. Campana, V. Malvezzi, Marco Casolino, A. Bianco, Alfonso Monaco, A. M. Galper, V. G. Zverev, M. P. De Pascale, Mark Pearce, S. B. Ricciarini, S. V. Koldashov, P. Picozza, P. Papini, E. Vannuccini, Roberta Sparvoli, L. Marcelli, A. Bruno, Y. T. Yurkin, Roberto Bellotti, A. N. Kvashnin, Maria Teresa Ricci, P. Spillantini, V. Di Felice, F. Cafagna, V. Bonvicini, Y. I. Stozhkov, Matteo Martucci, Lorenzo Bonechi, Juan Wu, M. Simon, A. A. Leonov, F. Palma, E. Mocchiutti, V. V. Malakhov, Ugo Giaccari, C. De Santis, S. Bottai, M. D. Kheymits, N. Zampa, C. Pizzolotto, G. A. Bazilevskaya, V. V. Mikhailov, N. N. Nikonov, Andrea Vacchi, Mirko Boezio, Giovanna Jerse, A. G. Mayorov, M. Bongi, R. Carbone, G. C. Barbarino, G. Zampa, L. A. Grishantseva, O. Adriani, W. Menn, G. I. Vasilyev, Nicola Mori, S. V. Borisov, S. A. Voronov, E. A. Bogomolov, Laura Rossetto, Ritabrata Sarkar, Valerio Formato, G. Castellini, Per Carlson, N. De Simone, D., Campana, U., Giaccari, O. c., Adriani, Barbarino, Giancarlo, G., Bazilevskaya, R. g., Bellotti, A. i., Bianco, M., Boezio, E., Bogomolov, L., Bonechi, M., Bongi, V., Bonvicini, S. l., M, S., Bottai, A. g., Bruno, F., Cafagna, R., Carbone, P., Carlson, M., Casolino, G., Castellini, M. l., De, C. D., Santi, N. D., Simone, V. D., Felice, V. i., Formato, A., Galper, L., Grishantseva, G. i., Jerse, A., Karelin, M., Kheymit, S., Koldashov, S., Krutkov, A., Kvashnin, A., Leonov, V., Malakhov, V., Malvezzi, L., Marcelli, M. p., Martucci, A., Mayorov, W., Menn, V., Mikhailov, E., Mocchiutti, A. g., Monaco, N., Mori, R. i. n, N. k. l, Osteria, Giuseppe, F. l., Palma, P., Papini, M., Pearce, P. l., Picozza, C. r., S, M., Ricci, S., Ricciarini, L., Rossetto, R., Sarkar, M., Simon, R. l., Sparvoli, P. c., Spillantini, Y., Stozhkov, A., Vacchi, E., Vannuccini, G., Vasilyev, S., Voronov, J., Wu, Y., Yurkin, G., Zampa, N., Zampa, V., Zverev, A D Erlykin, R P Kokoulin, A S Lidvansky, L I Meroshnichenko, M I Panasyuk, A D Panov and A W Wolfendale, O., Adriani, G. C., Barbarino, G. A., Bazilevskaya, R., Bellotti, A., Bianco, E. A., Bogomolov, S., Borisov, A., Bruno, M. P., De Pascale, C., De Santi, N., De Simone, V., Di Felice, Formato, Valerio, A. M., Galper, Jerse, Giovanna, A. V., Karelin, M. D., Kheymit, S. V., Koldashov, S. Y., Krutkov, A. N., Kvashnin, M., Martucci, A. G., Mayorov, V. V., Mikhailov, Mocchiutti, Emiliano, A., Monaco, Munini, Riccardo, N., Nikonov, G., Osteria, F., Palma, P., Picozza, C., Pizzolotto, S. B., Ricciarini, R., Sparvoli, P., Spillantini, Y. I., Stozhkov, Vacchi, Andrea, S. A., Voronov, Y. T., Yurkin, and V. G., Zverev
Subjects: Physics, History, Angular distribution, Anisotropy, Positron, PAMELA detector, Astrophysics::High Energy Astrophysical Phenomena, Isotropy, Flux, Cosmic ray, Electron, Astrophysics, Cosmic Rays, Settore FIS/04 - Fisica Nucleare e Subnucleare, Computer Science Applications, Education, law.invention, Angular scale, Arrival direction, Cosmic ray electrons, Directional Analysis, Strong anisotropy, Nuclear physics, Positron, law, Anisotropy, Directional analysis
Abstract: Using data taken by the Pamela experiment during 5 years of operation we studied the anisotropy in the arrival direction of cosmic ray electrons and positrons with energy above 40 GeV. We report on a study of anisotropy in the e�� flux at different angular scales extending from 30��up to 90��, furthermore a directional analysis has been performed around the Sun direction. The observed distribution of arrival directions is consistent with the isotropic expectation at any angular scale used in this study and no significant evidence of strong anisotropies has been observed, also the analysis around the Sun direction did not show any significant excess.
Published: 2013

20. Measurement of antiproton flux in primary cosmic radiation with PAMELA experiment

Author: S. Bottai, C. Pizzolotto, S. V. Borisov, S. A. Voronov, Sergey Koldobskiy, D. Campana, Roberto Bellotti, G. C. Barbarino, S. Y. Krutkov, V. G. Zverev, Marco Casolino, G. Castellini, E. A. Bogomolov, A. N. Kvashnin, E. Mocchiutti, Roberta Sparvoli, Laura Rossetto, V. Di Felice, M. Simon, Mark Pearce, S. B. Ricciarini, N. Zampa, G. A. Bazilevskaya, Alfonso Monaco, P. Picozza, A. A. Leonov, N. N. Nikonov, Ritabrata Sarkar, O. Adriani, P. Spillantini, P. Papini, R. Carbone, Lorenzo Bonechi, V. V. Malakhov, W. Menn, Per Carlson, E. Vannuccini, Giovanna Jerse, V. V. Mikhailov, N. De Simone, M. Bongi, S. V. Koldashov, V. Bonvicini, Y. I. Stozhkov, Maria Teresa Ricci, M. P. De Pascale, Y. T. Yurkin, A. V. Karelin, F. Cafagna, G. Osteria, A. G. Mayorov, L. Consiglio, William Gillard, A. M. Galper, L. Marcelli, A. Vacchi, M. D. Kheymits, A. Bruno, G. Zampa, G. I. Vasilyev, Juan Wu, Nicola Mori, C. De Santis, F. Palma, Mirko Boezio, A., Mayorov, O. b., Adriani, G, Barbarino, Giancarlo, Bazilevskaya, R. g., Bellotti, M., Boezio, E., Bogomolov, L. b., Bonechi, M., Bongi, V., Bonvicini, S. k., L., S., Bottai, A. g., Bruno, F., Cafagna, D., Campana, R. k., Carbone, P., Carlson, M. r., Casolino, G., Castellini, L., Consiglio, M. k., De, C. k., De, N. k., De, V. D., Felice, A., Galper, W., Gillard, G. o., Jerse, A., Karelin, M., Kheymit, S., Koldashov, S., Koldobskiy, S., Krutkov, A., Kvashnin, A., Leonov, V., Malakhov, L., Marcelli, W., Menn, V., Mikhailov, E., Mocchiutti, A., Monaco, N. b., Mori, N. j., K., Osteria, Giuseppe, F. k., Palma, P., Papini, M., Pearce, P. k., Picozza, C., Pizzolotto, M., Ricci, S., Ricciarini, R., Sarkar, L., Rossetto, M., Simon, R. k., Sparvoli, P. b., Spillantini, Y., Stozhkov, A., Vacchi, E., Vannuccini, G., Vasilyev, S., Voronov, J., Wu, Y., Yurkin, G., Zampa, N., Zampa, and V., Zverev
Subjects: Physics, History, Antiparticle, Experiments, Intelligent systems, Proton, Calorimeter (particle physics), PAMELA detector, Astrophysics::High Energy Astrophysical Phenomena, Antiproton flux, Classification algorithm, Energy ranges, Galactic cosmic radiations, Monte Carlo Simulation, Training sample, Cosmic ray, Particle detector, Particle identification, Settore FIS/04 - Fisica Nucleare e Subnucleare, Computer Science Applications, Education, law.invention, Nuclear physics, Physics and Astronomy (all), law, Antiproton, Antimatter, Nuclear Experiment, Cosmic rays
Abstract: The new method based on the classification algorithms was developed to separate antiprotons and electrons in the PAMELA experiment. Training samples based on Monte-Carlo simulation of particle's interactions in the PAMELA imaging Si/W calorimeter were used to achieve rejection factor and to keep high antiproton efficiency. With comparison to the previous publication the number of events was increased 1.5 times. Information collected from the mission start in 2006 till January 2010 was used in the analysis. 2800 events were found in the energy range from 60 MeV to 350 GeV. The flux of antiprotons in galactic cosmic radiation obtained with new method is presented.
Published: 2013

21. Cosmic ray study with the PAMELA experiment

Author: N. De Simone, P. Spillantini, M. D. Kheymits, Nicola Mori, S. Bottai, Alfonso Monaco, Giovanna Jerse, A. G. Mayorov, Roberto Bellotti, G. Zampa, Mark Pearce, S. B. Ricciarini, A. M. Galper, R. Carbone, S. A. Voronov, P. Papini, E. Vannuccini, O. Adriani, D. Campana, W. Menn, G. C. Barbarino, A. N. Kvashnin, V. V. Malakhov, E. A. Bogomolov, A. V. Karelin, L. Marcelli, A. Vacchi, A. Bruno, S. V. Borisov, G. I. Vasilyev, S. Y. Krutkov, C. Pizzolotto, F. Palma, E. Mocchiutti, Laura Rossetto, M. Bongi, N. N. Nikonov, Roberta Sparvoli, Marco Casolino, V. V. Mikhailov, P. Carlson, G. Osteria, Juan Wu, C. De Santis, S. V. Koldashov, V. Di Felice, V. Bonvicini, G. Castellini, Y. I. Stozhkov, L. A. Grishantseva, Mirko Boezio, F. Cafagna, M. P. De Pascale, Y. T. Yurkin, P. Picozza, Ritabrata Sarkar, V. G. Zverev, N. Zampa, G. A. Bazilevskaya, Maria Teresa Ricci, M. Simon, A. A. Leonov, P. b., Picozza, L., Marcelli, O. d., Adriani, Barbarino, Giancarlo, G., Bazilevskaya, R. i., Bellotti, M., Boezio, E., Bogomolov, M., Bongi, V., Bonvicini, S. b., L, S., Bottai, A. i., Bruno, F., Cafagna, D., Campana, R., Carbone, P., Carlson, M. b., N, G., Castellini, M. b., De, C. b., De, N. D., Simone, V. D., Felice, A., Galper, L., Grishantseva, G. q., Jerse, A., Karelin, M., Kheymit, S., Koldashov, S., Krutkov, A., Kvashnin, A., Leonov, V., Malakhov, A., Mayorov, W., Menn, V., Mikhailov, E., Mocchiutti, A. i., Monaco, N., Mori, N. b., K, Osteria, Giuseppe, F. b., Palma, P., Papini, M., Pearce, C., Pizzolotto, M., Ricci, S., Ricciarini, R., Sarkar, L., Rossetto, M., Simon, R. b., Sparvoli, P. d., Spillantini, Y., Stozhkov, A., Vacchi, E., Vannuccini, G., Vasilyev, S., Voronov, Y., Yurkin, J., Wu, G., Zampa, N., Zampa, and V., Zverev
Subjects: History, Astrophysics::High Energy Astrophysical Phenomena, Dark matter, Cosmic ray, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, Settore FIS/04 - Fisica Nucleare e Subnucleare, Education, law.invention, symbols.namesake, Physics and Astronomy (all), Positron, law, Experiments, Galaxies, Protons, Radiation belts, Solar energy, Cosmic rays, Physics, COSMIC cancer database, PAMELA detector, Astronomy, Computer Science Applications, Dark matter, Data collection, Heliospheres, Measurements of, Particle detection, Radiation environments, Solar activity, Solar modulation, Antiproton, Van Allen radiation belt, Physics::Space Physics, symbols, Heliosphere
Abstract: In six years of data collection years in space, the experiment PAMELA has discovered very interesting features in cosmic rays, namely in the fluxes of protons, helium, electrons, that might change our basic vision of the mechanisms of production, acceleration and propagation of cosmic rays in the Galaxy. In addition, PAMELA measurements of cosmic antiproton and positron fluxes are setting strong constraints to the nature of Dark Matter. The continuous particle detection is allowing a constant monitoring of the solar activity and detailed study of the solar modulation for a long period, giving important improvements to the comprehension of the heliosphere mechanisms. PAMELA is also measuring the radiation environment around the Earth, and has recently discovered an antiproton radiation belt.
Published: 2013

22. La 'cortegiania' y la 'cortesana filosofía': B. Castiglione y B. Gracián

Author: Maria Teresa Ricci
Subjects: Literature, Elegance, business.industry, media_common.quotation_subject, Human life, Philosophy, Sign (semiotics), Prudence, Discretion, The arts, Law, Strategic behavior, HERO, business, media_common
Abstract: El artículo explora el concepto de « cortesanía » en Castiglione y en Gracián. El héroe de Gracián aprende el arte de la « cortesanía » de Castiglione, sin por eso ser un « cortesano ». Gracián emplea la palabra « cortesano » en un sentido mucho más amplio. La cortesanía en Castiglione es una suerte de metadisciplina que contiene en sí todas las artes y se funda sobre la regla universal de la « gracia ». El artículo muestra cómo la teoría de la gracia de Castiglione, a través de la cual el conde habría sabido conciliar dos exigencias, el éxito en la corte y una vida orientada bajo el signo de la elegancia, pierde su intensidad en Gracián, quien insiste más en el comportamiento estratégico, fundado más bien sobre la prudencia y la discreción que sobre la gracia. La filosofía cortesana de Gracián es entendida como un discurso sobre la vida. No se trata de una losofía de la corte, si se entiende a la corte como el espacio cerrado en el cual vive el cortesano de Castiglione, sino que de una filosofía de la vida humana. La corte de Gracián es la plaza del mundo.
Published: 2015

23. Results from PAMELA

Author: Alfonso Monaco, A. V. Karelin, William Gillard, Mirko Boezio, L. Marcelli, D. Campana, A. Vacchi, Per Carlson, Marco Casolino, N. N. Nikonov, A. Bruno, G. Osteria, V. V. Malakhov, V. G. Zverev, M. F. Runtso, S. V. Borisov, R. Carbone, Lorenzo Bonechi, F. Cafagna, O. Adriani, L. A. Grishantseva, S. A. Voronov, W. Menn, Roberto Bellotti, G. Zampa, A. M. Galper, N. Zampa, G. A. Bazilevskaya, A. N. Kvashnin, E. A. Bogomolov, Roberta Sparvoli, S. Bottai, Mark Pearce, S. B. Ricciarini, P. Papini, Laura Rossetto, E. Vannuccini, M. Bongi, M. P. De Pascale, G. C. Barbarino, L. Consiglio, F. Palma, G. Castellini, C. Pizzolotto, Giovanna Jerse, Y. T. Yurkin, G. I. Vasilyev, V. V. Mikhailov, C. De Santis, N. De Simone, O. Maksumov, Ritabrata Sarkar, Juan Wu, Nicola Mori, A. G. Mayorov, M. Simon, A. A. Leonov, Maria Teresa Ricci, S. Y. Krutkov, P. Picozza, P. Spillantini, V. Malvezzi, E. Mocchiutti, S. V. Koldashov, V. Di Felice, V. Bonvicini, Y. I. Stozhkov, E., Mocchiutti, O., Adriani, Barbarino, Giancarlo, G. A., Bazilevskaya, R., Bellotti, M., Boezio, E. A., Bogomolov, L., Bonechi, M., Bongi, V., Bonvicini, S., Borisov, S., Bottai, A., Bruno, F., Cafagna, D., Campana, R., Carbone, P., Carlson, M., Casolino, G., Castellini, L., Consiglio, M. P., De Pascale, C., De Santi, N., De Simone, V., Di Felice, A. M., Galper, W., Gillard, L., Grishantseva, G., Jerse, A. V., Karelin, S. V., Koldashov, S. Y., Krutkov, A. N., Kvashnin, A., Leonov, O., Maksumov, V., Malakhov, V., Malvezzi, L., Marcelli, A. G., Mayorov, W., Menn, A., Monaco, V. V., Mikhailov, N., Mori, N. N., Nikonov, G., Osteria, F., Palma, P., Papini, M., Pearce, P., Picozza, C., Pizzolotto, M., Ricci, S. B., Ricciarini, L., Rossetto, M., Runtso, R., Sarkar, M., Simon, R., Sparvoli, P., Spillantini, Y. I., Stozhkov, A., Vacchi, E., Vannuccini, G., Vasilyev, S. A., Voronov, J., Wu, Y. T., Yurkin, G., Zampa, N., Zampa, and V. G., Zverev
Subjects: Physics, Nuclear and High Energy Physics, genetic structures, Spectrometer, Calorimeter (particle physics), PAMELA detector, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics, Atomic and Molecular Physics, and Optics, law.invention, Settore FIS/04 - Fisica Nucleare e Subnucleare, Nuclear physics, Low earth orbit, law, Magnet, Atomic and Molecular Physics, Physics::Space Physics, Satellite, Astrophysics::Earth and Planetary Astrophysics, and Optics
Abstract: The PAMELA satellite experiment was launched into low earth orbit on June 15(th) 2006. The combination of a permanent magnet silicon strip spectrometer and a silicon-tungsten imaging calorimeter al ...
Published: 2011

24. Latest results from PAMELA

Author: G. Zampa, O. Adriani, W. Menn, V. G. Zverev, M. Bongi, E. Mocchiutti, G. I. Vasilyev, R. Carbone, Roberta Sparvoli, M. P. De Pascale, Lorenzo Bonechi, D. Campana, Nicola Mori, Maria Teresa Ricci, S. V. Borisov, Mark Pearce, S. B. Ricciarini, C. Pizzolotto, Marco Casolino, S. V. Koldashov, N. N. Nikonov, V. Malvezzi, P. Papini, M. Simon, A. A. Leonov, E. Vannuccini, A. M. Galper, V. Di Felice, G. C. Barbarino, V. Bonvicini, Per Carlson, S. Bottai, Y. I. Stozhkov, Roberto Bellotti, N. De Simone, Sarkar Ritabrata, Juan Wu, A. N. Kvashnin, G. Osteria, N. Zampa, G. A. Bazilevskaya, Y. T. Yurkin, William Gillard, P. Spillantini, L. Marcelli, A. Vacchi, A. Bruno, S. Y. Krutkov, Giovanna Jerse, P. Picozza, L. A. Grishantseva, F. Cafagna, V. V. Mikhailov, S. A. Voronov, E. A. Bogomolov, Mirko Boezio, Laura Rossetto, Petter Hofverberg, G. Castellini, P., Papini, Barbarino, Giancarlo, D., Campana, R., Carbone, and Osteria, Giuseppe
Subjects: Physics, Antiparticle, Nuclear and High Energy Physics, Spectrometer, PAMELA detector, Physics::Instrumentation and Detectors, Detector, Cosmic ray, Atomic and Molecular Physics, and Optics, Charged particle, Particle identification, Settore FIS/04 - Fisica Nucleare e Subnucleare, law.invention, Nuclear physics, Rigidity (electromagnetism), law, Atomic and Molecular Physics, and Optics
Abstract: The PAMELA experiment is a satellite-borne apparatus designed to study charged particles in the cosmic radiation, with a particular focus on antiparticles. The detector is housed on the Resurs-DK1 satellite and it is taking data since June 2006. The main parts of the apparatus are a magnetic spectrometer, which is equipped with a silicon-microstrip tracking system and which is used to measure the rigidity and the charge of particles, and a silicon/tungsten electromagnetic calorimeter which provides particle identification. The main results about the antiparticles component of cosmic rays obtained during the first 500 days of data taking are summarized here.
Published: 2009

25. The PAMELA space mission

Author: Roberta Sparvoli, Maria Teresa Ricci, G. Zampa, V. Malvezzi, Mark Pearce, S. B. Ricciarini, P. Papini, E. Vannuccini, Mirko Boezio, M. Simon, N. De Simone, Y. T. Yurkin, A. A. Leonov, P. Spillantini, O. Adriani, V. G. Zverev, Roberto Bellotti, V. Di Felice, V. V. Mikhailov, V. Bonvicini, P. Carlson, D. Campana, S. A. Voronov, E. Mocchiutti, A. Bruno, Y. I. Stozhkov, A. N. Kvashnin, G. C. Barbarino, A. M. Galper, S. Orsi, W. Menn, S. Y. Krutkov, G. De Rosa, E. A. Bogomolov, S. V. Koldashov, Marco Casolino, Petter Hofverberg, P. Picozza, F. Cafagna, N. Zampa, Lorenzo Bonechi, M. Bongi, G. A. Bazilevskaja, G. I. Vasilyev, Giuseppe Osteria, M. P. De Pascale, L. Marcelli, A. Vacchi, G. Castellini, Barbarino, Giancarlo, Russo, Stefano, DE ROSA, Gianfranca, D., Campana, and G., Osteria
Subjects: Physics, Nuclear and High Energy Physics, PAMELA detector, Payload, Astronomy, Space (mathematics), Atomic and Molecular Physics, and Optics, law.invention, Settore FIS/04 - Fisica Nucleare e Subnucleare, law, Atomic and Molecular Physics, Satellite, and Optics
Abstract: The PAMELA (a Payload for Antimatter-Matter Exploration and Light-nuclei Astrophysics) space mission has been launched on-board the Resurs-DK1 satellite on June 15(th) 2006 from the Baikonur cosmod ...
Published: 2009

26. Study of deuteron spectra under radiation belt with PAMELA instrument

Author: S. A. Voronov, L. Marcelli, A. Vacchi, A. Bruno, Valerio Formato, Roberta Sparvoli, E. A. Bogomolov, P. Spillantini, S. Y. Krutkov, P. Picozza, A. A. Kvashnin, Mirko Boezio, N. De Simone, Nicola Mori, D. Campana, G. Castellini, A. G. Mayorov, N. Zampa, G. A. Bazilevskaya, Alexey Leonov, Yu. T. Yurkin, C. De Santis, Per Carlson, Marco Casolino, C. De Donato, Ritabrata Sarkar, S. Bottai, O. Adriani, V. Di Felice, F. Palma, Roberto Bellotti, Riccardo Munini, W. Menn, A. M. Galper, Sergey Koldashov, G. Zampa, Mark Pearce, S. B. Ricciarini, Beatrice Panico, A. N. Kvashnin, Maria Teresa Ricci, Sergey Koldobskiy, M. Bongi, V. V. Malakhov, G. C. Barbarino, G. I. Vasilyev, Valentina Scotti, P. Papini, E. Vannuccini, Alfonso Monaco, M. Simon, A. V. Karelin, G. Osteria, M. Merge, Matteo Martucci, F. Cafagna, V. V. Mikhailov, V. Bonvicini, Y. I. Stozhkov, E. Mocchiutti, Koldobskiy, S. A, Adriani, O, Barbarino, Giancarlo, Bazilevskaya, G. A, Bellotti, R, Boezio, M, Bogomolov, E. A, Bongi, M, Bonvicini, V, Bottai, S, Bruno, A, Cafagna, F, Campana, D, Carlson, P, Casolino, M, Castellini, G, De Donato, C, De Santis, C, De Simone, N, Felice, V. Di, Formato, V, Galper, A. M, Karelin, A. V, Koldashov, S. V, Krutkov, S. Y, Kvashnin, A. A, Kvashnin, A. N, Leonov, A. A, Malakhov, V. V, Marcelli, L, Martucci, M, Mayorov, A. G, Menn, W, Merge’, M, Mikhailov, V. V, Mocchiutti, E, Monaco, A, Mori, N, Munini, R, Osteria, G, Palma, F, Panico, B, Papini, P, Pearce, M, Picozza, P, Ricci, M, Ricciarini, S. B, Sarkar, R, Scotti, V, Simon, M, Sparvoli, R, Spillantini, P, Stozhkov, Y. I, Vacchi, A, Vannuccini, E, Vasilyev, G. I, Voronov, S. A, Yurkin, Y. T, Zampa, G, Zampa, N., S., Koldobskiy, O., Adriani, G. C., Barbarino, G. A., Bazilevskaya, R., Bellotti, M., Boezio, E. A., Bogomolov, M., Bongi, V., Bonvicini, S., Bottai, A., Bruno, F., Cafagna, D., Campana, P., Carlson, M., Casolino, G., Castellini, C., De Donato, C., De Santi, N., De Simone, V., Di Felice, V., Formato, A. M., Galper, A. V., Karelin, S. V., Koldashov, S. Y., Krutkov, A. A., Kvashnin, A. N., Kvashnin, A., Leonov, V., Malakhov, L., Marcelli, M., Martucci, A. G., Mayorov, W., Menn, M., Mergé, V. V., Mikhailov, E., Mocchiutti, A., Monaco, N., Mori, Munini, Riccardo, G., Osteria, F., Palma, B., Panico, P., Papini, M., Pearce, P., Picozza, M., Ricci, S. B., Ricciarini, R., Sarkar, V., Scotti, M., Simon, R., Sparvoli, P., Spillantini, Y. I., Stozhkov, A., Vacchi, E., Vannuccini, G. I., Vasilyev, S. A., Voronov, Y. T., Yurkin, G., Zampa, and N., Zampa
Subjects: deuteron, History, Proton, Astrophysics::High Energy Astrophysical Phenomena, Nuclear Theory, Cosmology, Deuterium, Geomagnetism, Radiation belts, Solar radiation Cosmic-ray particles, Energy ranges, High-precision, Measurements of, Proton flux, Wide energy range, Cosmic ray, Astrophysics, radiation belt, Radiation, Spectral line, Education, law.invention, Nuclear physics, Physics and Astronomy (all), symbols.namesake, cosmic rays, PAMELA, law, PAMELA, cosmic rays, deuteron, radiation belt, Nuclear Experiment, Settore FIS/01, Physics, PAMELA detector, Albedo, Computer Science Applications, Van Allen radiation belt, Physics::Space Physics, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, symbols, Astrophysics::Earth and Planetary Astrophysics
Abstract: This paper presents the results of measurements of proton and deuteron fluxes of albedo radiation in the Earth vicinity, obtained in the PAMELA experiment. PAMELA is an international experiment meant to study cosmic rays. PAMELA is carried out on board the satellite Resurs-DK1. High-precision equipment of the experiment allows registration and identification of cosmic ray particles of different varieties in a wide energy range. The albedo deuteron spectrum and albedo deuteron-to-proton fluxes ratio in the energy range 70 – 600 MeV/nucleon at altitude of 350 – 600 km for different geomagnetic latitudes is presented.
Published: 2015

27. THE SATELLITE TELESCOPE NINA FOR NUCLEAR AND ISOTOPIC INVESTIGATIONS IN SPACE

Author: P. Spillantini, A. Vacchi, Maria Teresa Ricci, Guido Barbiellini, A. Murashov, P. Schiavon, A. Morselli, A. V. Bakaldin, S. Piccardi, S. A. Voronov, N. Zampa, M. Ambriola, S. Bartalucci, Gianluca Furano, A. Scoscini, P. Picozza, S. V. Koldashov, F. Ciacio, A. Batishev, M. Circella, R. Cirami, P. Papini, C. De Marzo, R. Sparvoli, Mirko Boezio, A. M. Galper, V. V. Mikhailov, S. Giuntoli, Marco Casolino, V. Bidoli, F. Cafagna, W. Bonvicini, Roberto Bellotti, and M. P. De Pascale
Subjects: Physics, Telescope, law, Astronomy, Satellite, Astrophysics, Space (mathematics), law.invention
Published: 2000

28. Solar energetic particle events in 2006-2012 in the PAMELA experiment data

Author: S. A. Voronov, S. Bottai, E. A. Bogomolov, L. Consiglio, Mark Pearce, S. B. Ricciarini, Laura Rossetto, Roberta Sparvoli, Maria Teresa Ricci, P. Papini, Mirko Boezio, Alfonso Monaco, N. De Simone, G. C. Barbarino, A. V. Karelin, E. Vannuccini, M. Bongi, V. V. Malakhov, V. G. Zverev, S. Y. Krutkov, C. Pizzolotto, G. Osteria, V. Di Felice, A. M. Galper, V. Bonvicini, M. Simon, Y. I. Stozhkov, M. P. De Pascale, W. Menn, A. A. Leonov, A. G. Mayorov, Adriani, N. Zampa, G. A. Bazilevskaya, Giovanna Jerse, V. V. Mikhailov, G. Zampa, P. Picozza, E. Mocchiutti, Y. T. Yurkin, Ritabrata Sarkar, P. Spillantini, Roberto Bellotti, Juan Wu, S. V. Koldashov, A. N. Kvashnin, William Gillard, G. Castellini, L. Marcelli, A. Vacchi, Per Carlson, A. Bruno, F. Cafagna, R. Carbone, Lorenzo Bonechi, D. Campana, Marco Casolino, Nicola Mori, C. De Santis, G. I. Vasilyev, F. Palma, G. A., Bazilevskaya, A. G., Mayorov, V. V., Malakhov, V. V., Mikhailov, Adriani, Barbarino, Giancarlo, R., Bellotti, M., Boezio, E. A., Bogomolov, L., Bonechi, M., Bongi, V., Bonvicini, S., Bottai, A., Bruno, F., Cafagna, D., Campana, R., Carbone, P., Carlson, M., Casolino, G., Castellini, L., Consiglio, M. P., De Pascale, C., De Santi, N., De Simone, V., Di Felice, A. M., Galper, W., Gillard, G., Jerse, A. V., Karelin, S. V., Koldashov, S. Y., Krutkov, A. N., Kvashnin, A., Leonov, L., Marcelli, W., Menn, E., Mocchiutti, A., Monaco, N., Mori, Osteria, Giuseppe, F., Palma, P., Papini, M., Pearce, P., Picozza, C., Pizzolotto, M., Ricci, S. B., Ricciarini, R., Sarkar, L., Rossetto, M., Simon, R., Sparvoli, P., Spillantini, A., Vacchi, E., Vannuccini, G., Vasilyev, S. A., Voronov, J., Wu, Y. T., Yurkin, G., Zampa, N., Zampa, and V. G., Zverev
Subjects: Physics, History, Earth's orbit, Solar energetic particles, Spectrometer, PAMELA detector, Astrophysics::High Energy Astrophysical Phenomena, Astronomy, Astrophysics, Settore FIS/04 - Fisica Nucleare e Subnucleare, Computer Science Applications, Education, Solar cycle, law.invention, Physics and Astronomy (all), law, Physics::Space Physics, Solar particle event, Astrophysics::Solar and Stellar Astrophysics, Particle, Astrophysics::Earth and Planetary Astrophysics
Abstract: The PAMELA magnetic spectrometer launched in June 2006 has observed the last strong energetic solar particle event of the 23rd solar cycle in December 2006. Subsequent long minimum of solar activity and weak development of the 24th solar cycle led to a deficit in the solar energetic particle events on the Earth orbit. As a result, only few events with protons accelerated above 100 MeV occurred in 2010-2012. The paper gives the preliminary results on energetic solar particles in the beginning of the 24th solar circle as measured with the PAMELA instrument.
Published: 2013

29. Study of solar modulation of galactic cosmic rays with the PAMELA and ARINA spectrometers in 2006-2012

Author: S. Bottai, E. Mocchiutti, P. Spillantini, M. Simon, A. A. Leonov, Alfonso Monaco, S. V. Koldashov, C. Pizzolotto, V. Bonvicini, Y. I. Stozhkov, S. Y. Krutkov, Giovanna Jerse, V. G. Zverev, V. V. Mikhailov, V. V. Malakhov, Maria Teresa Ricci, Per Carlson, P. Picozza, V. Di Felice, Roberta Sparvoli, R. Carbone, Lorenzo Bonechi, Ritabrata Sarkar, S. V. Borisov, Sergey Koldobskiy, G. C. Barbarino, F. Cafagna, Y. T. Yurkin, Mark Pearce, S. B. Ricciarini, N. Zampa, G. A. Bazilevskaya, A. A. Ulitin, A. V. Karelin, P. Papini, E. Vannuccini, D. Campana, N. De Simone, Marco Casolino, D. S. Losev, G. Osteria, G. Castellini, Roberto Bellotti, M. P. De Pascale, A. N. Kvashnin, A. V. Sidorov, S. A. Voronov, E. A. Bogomolov, Laura Rossetto, L. Consiglio, G. Zampa, O. Adriani, W. Menn, M. Bongi, William Gillard, L. Marcelli, Juan Wu, A. Vacchi, A. Bruno, C. De Santis, A. M. Galper, A. G. Mayorov, N. N. Nikonov, Nicola Mori, M. A. Bzheumikhova, G. I. Vasilyev, F. Palma, Mirko Boezio, M. A., Bzheumikhova, O., Adriani, Barbarino, Giancarlo, G. A., Bazilevskaya, R., Bellotti, M., Boezio, E. A., Bogomolov, L., Bonechi, M., Bongi, V., Bonvicini, S., Borisov, S., Bottai, A., Bruno, F., Cafagna, D., Campana, R., Carbone, P., Carlson, M., Casolino, G., Castellini, Consiglio, Lucia, M. P., De Pascale, C., De Santi, N., De Simone, V., Di Felice, A. M., Galper, W., Gillard, G., Jerse, A. V., Karelin, S. V., Koldashov, S. A., Koldobskiy, S. Y., Krutkov, A. N., Kvashnin, A., Leonov, D. S., Losev, V., Malakhov, L., Marcelli, A. G., Mayorov, W., Menn, V. V., Mikhailov, E., Mocchiutti, A., Monaco, N., Mori, N., Nikonov, Osteria, Giuseppe, F., Palma, P., Papini, M., Pearce, P., Picozza, C., Pizzolotto, M., Ricci, S. B., Ricciarini, R., Sarkar, A. V., Sidorov, L., Rossetto, M., Simon, R., Sparvoli, P., Spillantini, Y. I., Stozhkov, A. A., Ulitin, A., Vacchi, E., Vannuccini, G., Vasilyev, S. A., Voronov, J., Wu, Y. T., Yurkin, G., Zampa, N., Zampa, and V. G., Zverev
Subjects: Physics, History, PAMELA detector, Astrophysics::High Energy Astrophysical Phenomena, Flux, Astronomy, Cosmic ray, Astrophysics, Settore FIS/04 - Fisica Nucleare e Subnucleare, Computer Science Applications, Education, Solar cycle, law.invention, Physics and Astronomy (all), Solar wind, law, Physics::Space Physics, Astrophysics::Solar and Stellar Astrophysics, Forbush decrease, Astrophysics::Earth and Planetary Astrophysics, Heliospheric current sheet, Interplanetary magnetic field
Abstract: Spectrometers PAMELA and ARINA, mounted on the spacecraft Resurs-DK1, carried out precision measurements of galactic cosmic ray (GCR) flux near the Earth from 2006 to present. Combining these instruments gives the possibility to study the effect of solar modulation in the energy range from 30 MeV to dozens of GeV. This report presents experimental results concerning the time interval from the end of the 23rd solar cycle (noted by an prolonged minimum) to the beginning of the 24th cycle. The cosmic ray flux raised up to the end of 2009, then it began to decline, which is in coincidence with the sunspot number and evidence of the solar activity increasing. Some additional features were noted in the time profile of galactic cosmic ray flux, which, as shown by analysis of the correlation, correspond to a change of such heliospheric parameters as the tilt angle of the heliospheric current sheet (HCS), the solar wind velocity and the intensity of interplanetary magnetic field (IMF).
Published: 2013

30. Science of Mini-EUSO detector on board the International Space Station

Author: M. I. Panasyuk, Piergiorgio Picozza, Pavel Klimov, Toshikazu Ebisuzaki, Maria Teresa Ricci, A. Belov, Francesca Capel, M. E. Bertaina, Marco Casolino, and G. Cambiè
Subjects: Astrophysics::High Energy Astrophysical Phenomena, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Uv spectrum, Astronomy, law.invention, On board, Telescope, Atmosphere, Space experiment, law, Physics::Space Physics, International Space Station, Space program, Environmental science, Astrophysics::Earth and Planetary Astrophysics
Abstract: The Mini-EUSO space experiment ("UV atmosphere" in Russian Space Program) is a telescope designed to perform observations of night-time Earth in the UV spectrum. The instrument comprises a compact ...

31. The pamela experiment: Five years of cosmic rays investigation

Author: A. N. Kvashnin, O. Maksumov, Roberta Sparvoli, A. G. Mayorov, V. Di Felice, Mark Pearce, S. B. Ricciarini, G. Zampa, A. V. Karelin, V. Malvezzi, P. Papini, E. Vannuccini, V. Bonvicini, S. Y. Krutkov, A. Bruno, Y. I. Stozhkov, G. Osteria, S. Bottai, R. Carbone, O. Adriani, W. Menn, V. G. Zverev, F. Palma, M. P. DePascale, Mirko Boezio, C. Pizzolotto, Roberto Bellotti, N. N. Nikonov, L. Consiglio, P. Picozza, M. Simon, A. A. Leonov, V. V. Malakhov, A. M. Galper, S. V. Koldashov, Nicola Mori, P. Spillantini, G. C. Barbarino, L. A. Grishantseva, Juan Wu, M. Bongi, Maria Teresa Ricci, C. De Santis, V. Formato, M. F. Runtso, Giovanna Jerse, S. A. Voronov, L. Marcelli, A. Vacchi, G. A. Bazilevskaya, E. A. Bogomolov, Laura Rossetto, Y. T. Yurkin, E. Mocchiutti, N. Zampa, V. V. Mikhailov, P. Carlson, F. Cafagna, G. I. Vasilyev, Lorenzo Bonechi, D. Campana, S. V. Borisov, Marco Casolino, Alfonso Monaco, N. De Simone, Ritabrata Sarkar, and G. Castellini
Subjects: Physics, PAMELA detector, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Dark matter, Astronomy, Cosmic ray, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, CR composition, Settore FIS/04 - Fisica Nucleare e Subnucleare, law.invention, Energy spectra and interactions, Spaceborne and space research instruments, law, Physics::Accelerator Physics, Cosmic rays
Abstract: In five years of data taking in space, the PAMELA experiment collected very interesting data on the charged cosmic radiation over a wide energy range (from 100 MeV up to 1 TeV, depending from the species) with unprecedent statistics. The apparatus comprises a time-of-flight system, a silicon-microstrip magnetic spectrometer, a silicon-tungsten electromagnetic calorimeter, an anticoincidence system, a shower tail counter scintillator and a neutron detector. PAMELA is providing fundamental data not only to search for dark matter signals but also to better understand cosmic-ray propagation models. Main results after five years of data taking will be presented.

32. Space debris detection and tracking with the techniques of cosmic ray physics

Author: Y. Takizawa, Z. Plebaniak, P. Picozza, Guillaume Prévôt, F. Kajino, T. Napolitano, A. Cellino, G. Cotto, Lech Wiktor Piotrowski, Marco Mignone, Francesco Fenu, G. Osteria, A. Murashov, A. Poroshin, R. Bonino, Pavel Klimov, Matteo Battisti, J. Szabelski, Naoto Sakaki, S. Turriziani, G. Suino, Alexander S. Belov, Marco Casolino, Claudio Fornaro, M. Bertaina, F. Bisconti, G. Cambiè, E. Parizot, I. Churilo, Daniele Gardiol, Francesca Capel, S. Blin-Bondil, A. Franceschi, L. Marcelli, M. I. Panasyuk, W. Marszał, Maria Teresa Ricci, H. Miyamoto, Enzo Reali, A. Djakonow, M. Przybylak, M. Traïche, F. Cafagna, Toshikazu Ebisuzaki, Federico Fausti, P. Gorodetzky, Kenji Shinozaki, C. Fugelsang, Organisation de Micro-Électronique Générale Avancée (OMEGA), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-École polytechnique (X), AstroParticule et Cosmologie (APC (UMR_7164)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), JEM-EUSO, École polytechnique (X)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-École polytechnique (X)-Centre National de la Recherche Scientifique (CNRS), and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)
Subjects: Physics, business.product_category, Spacecraft, Meteoroid, business.industry, Detector, FOS: Physical sciences, Tracking (particle physics), 7. Clean energy, law.invention, Telescope, Rocket, law, International Space Station, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], business, Astrophysics - Instrumentation and Methods for Astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), Remote sensing, Space debris
Abstract: International audience; Space Debris (SD) consist of non-operational artificial objects orbiting around the Earth, which could possibly damage space vehicles, such as the International Space Station (ISS) or other manned spacecrafts. The vast majority of such objects are cm-sized, not catalogued and usually the tracking data are not precise enough. Here we present the feasibility study of SD detection and tracking with techniques usually employed in cosmic-ray physics. For this purpose, we have evaluated the possibility of using Mini-EUSO, a space-borne fluorescence telescope to be deployed on the ISS, to track SD illuminated by the Sun. By means of ESAF (EUSO Simulation and analysis Framework) simulation and by developing the trigger algorithms, we estimated the minimum size and maximum distances of detectable SD. We then studied the number of possible SD detections using an ESA software called MASTER (Meteoroid and SD Terrestrial Environment Reference). With the Mini-EUSO Engineering Model (Mini-EUSO EM), we performed some measurements to estimate the reflectance of the most common SD materials and to demonstrate the ability of Mini-EUSO to detect SD events. We also performed some tests in open-sky conditions, identifying and tracking fast-moving objects. In particular, the detection of a rocket body allowed us to confirm the simulation outcomes predictions and the expected performance of the detector.

33. Study on the high energy particle detector calorimeter

Author: Cinzia De Donato, I. Rashevskaya, Ignazio Lazzizzera, Giuseppe Osteria, Alessandro Sotgiu, S. Bartocci, L. Patrizii, Maria Ionica, Roberto Iuppa, William J. Burger, C. Manea, Roberta Sparvoli, G. Masciantonio, Giovanni Ambrosi, Michele Sposito, Ester Ricci, Maria Teresa Ricci, Vincenzo Vitale, G. Castellini, Roberto Battiston, S. B. Ricciarini, F. Palmonari, M. Lolli, Livio Conti, Francesco Palma, L. Marcelli, Andrea Contin, Cristian De Santis, M. Merge, M. Pozzato, Cristina Guadalini, Beatrice Panico, Francesco Maria Follega, Valentina Scotti, F. Perfetto, Bruno Spataro, P. Cipollone, L. Pacini, G. Laurenti, and Piergiorgio Picozza
Subjects: Settore FIS/01, Physics, High energy particle, Proton, Calorimeter (particle physics), Nuclear Theory, Cyclotron, Cosmic ray, Electron, Particle detector, law.invention, Nuclear physics, symbols.namesake, law, Van Allen radiation belt, symbols, Physics::Accelerator Physics, Nuclear Experiment
Abstract: The High-Energy Particle Detector (HEPD) is one of the payloads of the CSES space mission, built by the Italian “Limadou” collaboration. It will study the temporal stability of the inner Van Allen radiation belts, the precipitation of trapped particles in the atmosphere and the low energy component of the cosmic rays (5 - 100 MeV for electrons and 15 - 300 MeV for protons). Results of the test beams held at the Beam Test Facility of the INFN National Laboratory of Frascati, for electrons, and at the Proton Cyclotron of Trento, for protons, will be presented. The performance of the apparatus both on the energy reconstruction and in the lepton/hadron separation will be shown.

34. The hepd apparatus for the cses mission

Author: Beatrice Panico, Maria Teresa Ricci, Matteo Sposito, C. De Donato, Livio Conti, S. Bartocci, Roberto Iuppa, Ester Ricci, Maria Ionica, Francesco Maria Follega, Andrea Contin, W. J. Burger, M. Merge, V. Vitale, G. Laurenti, C. Manea, G. Ambrosi, Valentina Scotti, M. Lolli, C. Guadalini, G. Masciantonio, M. Pozzato, L. Patrizii, R. Sparvoli, L. Pacini, G. Castellini, Roberto Battiston, P. Picozza, C. De Santis, F. Palma, I. Rashevskaya, Alessandro Sotgiu, F. Perfetto, Bruno Spataro, P. Cipollone, Ignazio Lazzizzera, F. Palmonari, L. Marcelli, G. Osteria, S. B. Ricciarini, Panico, B., Osteria, G., Perfetto, F., Scotti, V., Cipollone, P., De Donato, C., De Santis, C., Marcelli, L., Masciantonio, G., Mergè, M., Palma, F., Picozza, P., Sotgiu, A., Sparvoli, R., Contin, A., Guadalini, C., Laurenti, G., Lolli, M., Palmonari, F., Patrizii, L., Pozzato, M., Ricci, M., Spataro, B., Burger, W. J., Battiston, R., Follega, F. M., Iuppa, R., Lazzizzera, I., Manea, C., Rashevskaya, I., Ricci, E., Vitale, V., Ambrosi, G., Ionica, M., Sposito, M., Bartocci, S., Conti, L., Castellini, G., Pacini, L., Ricciarini, S. B., and Merge, M.
Subjects: History, High energy particle, Proton, Nuclear Theory, Cyclotron, Cosmic ray, Electron, Particle detector, Education, Physics::Geophysics, law.invention, Nuclear physics, Atmosphere, symbols.namesake, law, Aerospace engineering, Nuclear Experiment, Trapped particle, Low-energy components, Physics, Settore FIS/01, business.industry, Radiation belts, Computer Science Applications, Magnetic field, Van Allen radiation belt, Physics::Space Physics, symbols, Physics::Accelerator Physics, Environmental science, Satellite, business, Beam (structure)
Abstract: The High-Energy Particle Detector (HEPD) is one of the payloads of the CSES space mission. The HEPD is built by the Italian Limadou collaboration and has different goals. It will study the temporal stability of the inner Van Allen radiation belts, the precipitation of trapped particles in the atmosphere and the low energy component of the cosmic rays (5-100 MeV for electrons and 15 - 300 MeV for protons). It has been tested at the Beam Test Facility of the INFN National Laboratory of Frascati, for electrons, and at the Proton Cyclotron of Trento, for protons. Here is presented a study of the performance of the apparatus to separate electrons and protons and identify nuclei up to iron.

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34 results on '"Maria Teresa Ricci"'

1. Integration and qualification of the Mini-EUSO telescope on board the ISS

2. The EUSO@Turlab Project: Tests of Mini-EUSO Engineering Model

3. The POEMMA (Probe of Extreme Multi-Messenger Astrophysics) mission

4. Mini-EUSO engineering model: tests in open-sky condition

5. Sharp increasing of positron to electron fluxes ratio below 2 GV measured by the PAMELA

6. Solar modulation of galactic cosmic rays during 2006-2015 based on PAMELA and ARINA data

7. The PAMELA experiment: A decade of Cosmic Ray Physics in space

8. Solar modulation of galactic cosmic rays electrons and positrons over the 23rd solar minimum with the PAMELA experiment

9. Features of re-entrant albedo deuteron trajectories in near Earth orbit with PAMELA experiment

10. Time variations of proton flux in Earth inner radiation belt during 23/24 solar cycles based on the PAMELA and the ARINA data

11. Solar modulation of GCR electrons over the 23rd solar minimum with PAMELA

12. PAMELA measurements of the boron and carbon spectra

13. Measurement of electron-positron spectrum in high-energy cosmic rays in the PAMELA experiment

14. A method to detect positron anisotropies with Pamela data

15. Solar modulation of galactic protons and helium with the PAMELA experiment

16. PRECISE COSMIC RAYS MEASUREMENTS WITH PAMELA

17. The PAMELA experiment: light-nuclei selection with stand-alone detectors

18. Cosmic ray electron and positron spectra measured with PAMELA

19. Search for cosmic ray electron-positron anisotropies with the Pamela data

20. Measurement of antiproton flux in primary cosmic radiation with PAMELA experiment

21. Cosmic ray study with the PAMELA experiment

22. La 'cortegiania' y la 'cortesana filosofía': B. Castiglione y B. Gracián

23. Results from PAMELA

24. Latest results from PAMELA

25. The PAMELA space mission

26. Study of deuteron spectra under radiation belt with PAMELA instrument

27. THE SATELLITE TELESCOPE NINA FOR NUCLEAR AND ISOTOPIC INVESTIGATIONS IN SPACE

28. Solar energetic particle events in 2006-2012 in the PAMELA experiment data

29. Study of solar modulation of galactic cosmic rays with the PAMELA and ARINA spectrometers in 2006-2012

30. Science of Mini-EUSO detector on board the International Space Station

31. The pamela experiment: Five years of cosmic rays investigation

32. Space debris detection and tracking with the techniques of cosmic ray physics

33. Study on the high energy particle detector calorimeter

34. The hepd apparatus for the cses mission

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34 results on '"Maria Teresa Ricci"'

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