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41 results on '"De Santis, C."'

1. Multispacecraft Observations of Protons and Helium Nuclei in Some Solar Energetic Particle Events toward the Maximum of Cycle 25.

Author

Bartocci, S., Battiston, R., Benella, S., Beolè, S., Burger, W. J., Cipollone, P., Contin, A., Cristoforetti, M., De Donato, C., De Santis, C., Di Luca, A., Follega, F. M., Gebbia, G., Iuppa, R., Laurenza, M., Lega, A., Lolli, M., Martucci, M., Masciantonio, G., and Mergè, M.

Subjects
SOLAR energetic particles, SPACE environment, PARTICLE physics, SUN, PARTICLE detectors
Abstract

The intricate behavior of particle acceleration and transport mechanisms complicates the overall efforts in formulating a comprehensive understanding of solar energetic particle (SEP) events; these efforts include observations of low-energy particles (from tens of keV to hundreds of MeV) by space-borne instruments and measurements by the ground-based neutron monitors of the secondary particles generated in the Earth atmosphere by SEPs in the GeV range. Numerous space-borne missions provided good data on the nature/characteristics of these solar particles in past solar cycles, but more recently—concurrently with the rise toward the maximum of solar cycle 25—the High-Energy Particle Detector (HEPD-01) proved to be well suited for the study of solar physics and space weather. Its nominal 30–300 MeV energy range for protons can enlarge the detection capabilities of solar particles at low Earth orbit, closer to the injection limit of many SEP events. In this work, we characterize three SEP events within the first six months of 2022 through spectral and velocity dispersion analysis, assessing the response of HEPD-01 to >M1 events. [ABSTRACT FROM AUTHOR]

Published
2024
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2. Real-time signal processing and data acquisition for the Electric Field Detector (EFD-02) on the CSES-02 satellite

Author

Ammendola, R., primary, Badoni, D., additional, De Santis, C., additional, Rebustini, G., additional, Alunno Camelia, E., additional, Bertello, I., additional, Cipollone, P., additional, De Angelis, F., additional, Diego, P., additional, Fiorenza, E., additional, Masciantonio, G., additional, Nuccilli, F., additional, Parmentier, A., additional, Papini, E., additional, Picozza, P., additional, Piersanti, M., additional, Russi, A., additional, Sparvoli, R., additional, Ubertini, P., additional, and Vertolli, N., additional

Published
2024
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3. Helium fluxes measured by the PAMELA experiment from the minimum to the maximum solar activity for solar cycle 24

Author

Marcelli, N. (N.), Boezio, M. (M.), Lenni, A. (A.), Menn, W. (W.), Munini, R. (R.), Aslam, O. P. (O. P. M.), Bisschoff, D. (D.), Ngobeni, M. D. (M. D.), Potgieter, M. S. (M. S.), Adriani, O. (O.), Barbarino, G. C. (G. C.), Bazilevskaya, G. A. (G. A.), Bellotti, R. (R.), Bogomolov, E. A. (E. A.), Bongi, M. (M.), Bonvicini, V. (V.), Bruno, A. (A.), Cafagna, F. (F.), Campana, D. (D.), Carlson, P. (P.), M. C. (M. Casolino), Castellini, G. (G.), De Santis, C. (C.), Galper, A. M. (A. M.), Koldashov, S. V. (S. V.), Koldobskiy, S. (S.), Kvashnin, A. N. (A. N.), Leonov, A. A. (A. A.), Malakhov, V. V. (V. V.), Marcelli, L. (L.), Martucci, M. (M.), Mayorov, A. G. (A. G.), Mergè, M. (M.), Mocchiutti, E. (E.), Monaco, A. (A.), Mori, N. (N.), Mikhailov, V. V. (V. V.), Osteria, G. (G.), Panico, B. (B.), Papini, P. (P.), Pearce, M. (M.), Picozza, P. (P.), Ricci, M. (M.), Ricciarini, S. B. (S. B.), Simon, M. (M.), Sotgiu, A. (A.), Sparvoli, R. (R.), Spillantini, P. (P.), Stozhkov, Y. I. (Y. I.), Vacchi, A. (A.), Vannuccini, E. (E.), Vasilyev, G. I. (G. I.), Voronov, S. A. (S. A.), Yurkin, Y. T. (Y. T.), Zampa, G. (G.), Zampa, N. (N.), Marcelli, N. (N.), Boezio, M. (M.), Lenni, A. (A.), Menn, W. (W.), Munini, R. (R.), Aslam, O. P. (O. P. M.), Bisschoff, D. (D.), Ngobeni, M. D. (M. D.), Potgieter, M. S. (M. S.), Adriani, O. (O.), Barbarino, G. C. (G. C.), Bazilevskaya, G. A. (G. A.), Bellotti, R. (R.), Bogomolov, E. A. (E. A.), Bongi, M. (M.), Bonvicini, V. (V.), Bruno, A. (A.), Cafagna, F. (F.), Campana, D. (D.), Carlson, P. (P.), M. C. (M. Casolino), Castellini, G. (G.), De Santis, C. (C.), Galper, A. M. (A. M.), Koldashov, S. V. (S. V.), Koldobskiy, S. (S.), Kvashnin, A. N. (A. N.), Leonov, A. A. (A. A.), Malakhov, V. V. (V. V.), Marcelli, L. (L.), Martucci, M. (M.), Mayorov, A. G. (A. G.), Mergè, M. (M.), Mocchiutti, E. (E.), Monaco, A. (A.), Mori, N. (N.), Mikhailov, V. V. (V. V.), Osteria, G. (G.), Panico, B. (B.), Papini, P. (P.), Pearce, M. (M.), Picozza, P. (P.), Ricci, M. (M.), Ricciarini, S. B. (S. B.), Simon, M. (M.), Sotgiu, A. (A.), Sparvoli, R. (R.), Spillantini, P. (P.), Stozhkov, Y. I. (Y. I.), Vacchi, A. (A.), Vannuccini, E. (E.), Vasilyev, G. I. (G. I.), Voronov, S. A. (S. A.), Yurkin, Y. T. (Y. T.), Zampa, G. (G.), and Zampa, N. (N.)

Abstract

Time-dependent energy spectra of galactic cosmic rays (GCRs) carry fundamental information regarding their origin and propagation. When observed at the Earth, these spectra are significantly affected by the solar wind and the embedded solar magnetic field that permeates the heliosphere, changing significantly over an 11 yr solar cycle. Energy spectra of GCRs measured during different epochs of solar activity provide crucial information for a thorough understanding of solar and heliospheric phenomena. The PAMELA experiment collected data for almost 10 years (2006 June 15–2016 January 23), including the minimum phase of solar cycle 23 and the maximum phase of solar cycle 24. In this paper, we present new spectra for helium nuclei measured by the PAMELA instrument from 2010 January to 2014 September over a three-Carrington-rotation time basis. These data are compared to the PAMELA spectra measured during the previous solar minimum, providing a picture of the time dependence of the helium-nuclei fluxes over a nearly full solar cycle. Time and rigidity dependencies are observed in the proton-to-helium flux ratios. The force-field approximation of the solar modulation was used to relate these dependencies to the shapes of the local interstellar proton and helium-nuclei spectra.

Published
2022

4. Solar-cycle variations of South Atlantic anomaly proton intensities measured with the PAMELA mission

Author

Bruno, A. (A.), Martucci, M. (M.), Cafagna, F. S. (F. S.), Sparvoli, R. (R.), Adriani, O. (O.), Barbarino, G. C. (G. C.), Bazilevskaya, G. A. (G. A.), Bellotti, R. (R.), Boezio, M. (M.), Bogomolov, E. A. (E. A.), Bongi, M. (M.), Bonvicini, V. (V), Campana, D. (D.), Carlson, P. (P.), Casolino, M. (M.), Castellini, G. (G.), De Santis, C. (C.), Galper, A. M. (A. M.), Koldashov, S. V. (S., V), Koldobskiy, S. (S.), Kvashnin, A. N. (A. N.), Lenni, A. (A.), Leonov, A. A. (A. A.), Malakhov, V. V. (V. V.), Marcelli, L. (L.), Marcelli, N. (N.), Mayorov, A. G. (A. G.), Menn, W. (W.), Merge, M. (M.), Mocchiutti, E. (E.), Monaco, A. (A.), Mori, N. (N.), Mikhailov, V. V. (V. V.), Munini, R. (R.), Osteria, G. (G.), Panico, B. (B.), Papini, P. (P.), Pearce, M. (M.), Picozza, P. (P.), Ricci, M. (M.), Ricciarini, S. B. (S. B.), Simon, M. (M.), Sotgiu, A. (A.), Spillantini, P. (P.), Stozhkov, Y. I. (Y., I), Vacchi, A. (A.), Vannuccini, E. (E.), Vasilyev, G. I. (G., I), Voronov, S. A. (S. A.), Yurkin, Y. T. (Y. T.), Zampa, G. (G.), Zampa, N. (N.), Zharaspayev, T. R. (T. R.), Bruno, A. (A.), Martucci, M. (M.), Cafagna, F. S. (F. S.), Sparvoli, R. (R.), Adriani, O. (O.), Barbarino, G. C. (G. C.), Bazilevskaya, G. A. (G. A.), Bellotti, R. (R.), Boezio, M. (M.), Bogomolov, E. A. (E. A.), Bongi, M. (M.), Bonvicini, V. (V), Campana, D. (D.), Carlson, P. (P.), Casolino, M. (M.), Castellini, G. (G.), De Santis, C. (C.), Galper, A. M. (A. M.), Koldashov, S. V. (S., V), Koldobskiy, S. (S.), Kvashnin, A. N. (A. N.), Lenni, A. (A.), Leonov, A. A. (A. A.), Malakhov, V. V. (V. V.), Marcelli, L. (L.), Marcelli, N. (N.), Mayorov, A. G. (A. G.), Menn, W. (W.), Merge, M. (M.), Mocchiutti, E. (E.), Monaco, A. (A.), Mori, N. (N.), Mikhailov, V. V. (V. V.), Munini, R. (R.), Osteria, G. (G.), Panico, B. (B.), Papini, P. (P.), Pearce, M. (M.), Picozza, P. (P.), Ricci, M. (M.), Ricciarini, S. B. (S. B.), Simon, M. (M.), Sotgiu, A. (A.), Spillantini, P. (P.), Stozhkov, Y. I. (Y., I), Vacchi, A. (A.), Vannuccini, E. (E.), Vasilyev, G. I. (G., I), Voronov, S. A. (S. A.), Yurkin, Y. T. (Y. T.), Zampa, G. (G.), Zampa, N. (N.), and Zharaspayev, T. R. (T. R.)

Abstract

We present a study of the solar-cycle variations of >80 MeV proton flux intensities in the lower edge of the inner radiation belt, based on the measurements of the Payload for Antimatter Matter Exploration and Light-nuclei Astrophysics (PAMELA) mission. The analyzed data sample covers an similar to 8 yr interval from 2006 July to 2014 September, thus spanning from the decaying phase of the 23rd solar cycle to the maximum of the 24th cycle. We explored the intensity temporal variations as a function of drift shell and proton energy, also providing an explicit investigation of the solar modulation effects at different equatorial pitch angles. PAMELA observations offer new important constraints for the modeling of low-altitude particle radiation environment at the highest trapping energies.

Published
2021

5. Time dependence of the proton and helium flux measured by PAMELA

Author

Panico, B., Campana, D., Osteria, G., Barbarino, G. C., Adriani, O., Bongi, M., Spillantini, P., Mori, N., Papini, P., Vannuccini, E., Bazilevskaya, G. A., Kvashnin, A. N., Stozhkov, Y. I., Bellotti, R., Monaco, A., Bruno, A., Cafagna, F., Boezio, M., Bonvicini, V., Mocchiutti, E., Munini, R., Zampa, G., Zampa, N., Vacchi, A., Bogomolov, E. A., Krutkov, S. Y., Vasilyev, G. I., Carlson, Per, Pearce, Mark, Casolino, M., Castellini, G., De Santis, C., Marcelli, L., Mergé, M., Picozza, P., Sparvoli, R., Di Felice, V., Galper, A. M., Karelin, A. V., Koldashov, S. V., Koldobskiy, S., Yurkin, Y. T., Malakhov, V., Leonov, A., Mayorov, A. G., Mikhailov, V. V., Voronov, S. A., Martucci, M., Menn, W., Simon, M., Ricci, M., Ricciarini, S. B., Panico, B., Campana, D., Osteria, G., Barbarino, G. C., Adriani, O., Bongi, M., Spillantini, P., Mori, N., Papini, P., Vannuccini, E., Bazilevskaya, G. A., Kvashnin, A. N., Stozhkov, Y. I., Bellotti, R., Monaco, A., Bruno, A., Cafagna, F., Boezio, M., Bonvicini, V., Mocchiutti, E., Munini, R., Zampa, G., Zampa, N., Vacchi, A., Bogomolov, E. A., Krutkov, S. Y., Vasilyev, G. I., Carlson, Per, Pearce, Mark, Casolino, M., Castellini, G., De Santis, C., Marcelli, L., Mergé, M., Picozza, P., Sparvoli, R., Di Felice, V., Galper, A. M., Karelin, A. V., Koldashov, S. V., Koldobskiy, S., Yurkin, Y. T., Malakhov, V., Leonov, A., Mayorov, A. G., Mikhailov, V. V., Voronov, S. A., Martucci, M., Menn, W., Simon, M., Ricci, M., and Ricciarini, S. B.

Abstract

The energy spectra of galactic cosmic rays carry fundamental information regarding their origin and propagation, but, near Earth, cosmic rays are significantly affected by the solar magnetic field which changes over time. The time dependence of proton and electron spectra were measured from July 2006 to December 2009 by PAMELA experiment, that is a ballooon-borne experiment collecting data since 15 June 2006. These studies allowed to obtain a more complete description of the cosmic radiation, providing fundamental information about the transport and modulation of cosmic rays inside the heliosphere. The study of the time dependence of the cosmic-ray protons and helium nuclei from the unusual 23rd solar minimum through the following period of solar maximum activity is presented., QC 20210907

Published
2020
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6. Cosmic Rays Investigation by the PAMELA experiment

Author

Panico, B., Campana, D., Osteria, G., Barbarino, G. C., Adriani, O., Bongi, M., Spillantini, P., Mori, N., Papini, P., Vannuccini, E., Bazilevskaya, G. A., Kvashnin, A. N., Stozhkov, Y. I., Bellotti, R., Monaco, A., Bruno, A., Cafagna, F., Boezio, M., Bonvicini, V., Mocchiutti, E., Munini, R., Zampa, G., Zampa, N., Vacchi, A., Bogomolov, E. A., Krutkov, S. Y., Vasilyev, G. I., Carlson, Per, Pearce, Mark, Casolino, M., Castellini, G., De Santis, C., Marcelli, L., Mergé, M., Picozza, P., Sparvoli, R., Di Felice, V., Galper, A. M., Karelin, A. V., Koldashov, S. V., Koldobskiy, S., Yurkin, Y. T., Malakhov, V., Leonov, A., Mayorov, A. G., Mikhailov, V. V., Voronov, S. A., Martucci, M., Menn, W., Simon, M., Ricci, M., Ricciarini, S. B., Panico, B., Campana, D., Osteria, G., Barbarino, G. C., Adriani, O., Bongi, M., Spillantini, P., Mori, N., Papini, P., Vannuccini, E., Bazilevskaya, G. A., Kvashnin, A. N., Stozhkov, Y. I., Bellotti, R., Monaco, A., Bruno, A., Cafagna, F., Boezio, M., Bonvicini, V., Mocchiutti, E., Munini, R., Zampa, G., Zampa, N., Vacchi, A., Bogomolov, E. A., Krutkov, S. Y., Vasilyev, G. I., Carlson, Per, Pearce, Mark, Casolino, M., Castellini, G., De Santis, C., Marcelli, L., Mergé, M., Picozza, P., Sparvoli, R., Di Felice, V., Galper, A. M., Karelin, A. V., Koldashov, S. V., Koldobskiy, S., Yurkin, Y. T., Malakhov, V., Leonov, A., Mayorov, A. G., Mikhailov, V. V., Voronov, S. A., Martucci, M., Menn, W., Simon, M., Ricci, M., and Ricciarini, S. B.

Abstract

PAMELA (Payload for Antimatter Matter Exploration and Light-nuclei Astrophysics) is a satellite-borne experiment. It was launched on June 15th 2006 from the Baikonur space centre on board the Russian Resurs-DK1 satellite. For about 10 years PAMELA took data, giving a fundamental contribution to the cosmic ray physics. It made high-precision measurements of the charged component of the cosmic radiation challenging the standard model of the mechanisms of production, acceleration and propagation of cosmic rays in the galaxy and in the heliosphere. PAMELA gave results on different topics on a very wide range of energy. Moreover, the long PAMELA life gives the possibility to study the variation of the proton, electron and positron spectra during the last solar minimum. The time dependence of the cosmic-ray proton and helium nuclei from the solar minimum through the following period of solar maximum activity is currently being studied. Low energy particle spectra were accurately measured also for various solar events that occurred during the PAMELA mission. In this paper a review of main PAMELA results will be reported., QC 20210909

Published
2020
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7. Cosmic Rays Investigation by the PAMELA experiment

Author

Panico, Beatrice, primary, Campana, D., additional, Osteria, G., additional, Barbarino, G. C., additional, Adriani, O., additional, Bongi, M., additional, Spillantini, P., additional, Mori, N., additional, Papini, P., additional, Vannuccini, E., additional, Bazilevskaya, G. A., additional, Kvashnin, A. N., additional, Stozhkov, Y. I., additional, Bellotti, R., additional, Monaco, A., additional, Bruno, A., additional, Cafagna, F., additional, Boezio, M., additional, Bonvicini, V., additional, Mocchiutti, E., additional, Munini, R., additional, Zampa, G., additional, Zampa, N., additional, Vacchi, A., additional, Bogomolov, E. A., additional, Krutkov, S. Y., additional, Vasilyev, G. I., additional, Carlson, P., additional, Pearce, M., additional, Casolino, M., additional, Castellini, G., additional, De Santis, C., additional, Marcelli, L., additional, Mergé, M., additional, Picozza, P., additional, Sparvoli, R., additional, Di Felice, V., additional, Galper, A. M., additional, Karelin, A. V., additional, Koldashov, S. V., additional, Koldobskiy, S., additional, Yurkin, Y. T., additional, Malakhov, V., additional, Leonov, A., additional, Mayorov, A. G., additional, Mikhailov, V. V., additional, Voronov, S. A., additional, Martucci, M., additional, Menn, W., additional, Simon, M., additional, Ricci, M., additional, and Ricciarini, S. B., additional

Published
2020
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8. The HEPD apparatus for the CSES mission

Author

Panico, Beatrice, primary, Osteria, G., additional, Perfetto, F., additional, Scotti, V., additional, Cipollone, P., additional, De Donato, C., additional, De Santis, C., additional, Marcelli, L., additional, Masciantonio, G., additional, Mergè, M., additional, Palma, F., additional, Picozza, P., additional, Sotgiu, A., additional, Sparvoli, R., additional, Contin, A., additional, Guadalini, C., additional, Laurenti, G., additional, Lolli, M., additional, Palmonari, F., additional, Patrizii, L., additional, Pozzato, M., additional, Ricci, M., additional, Spataro, B., additional, Burger, W.J., additional, Battiston, R., additional, Follega, F.M., additional, Iuppa, R., additional, Lazzizzera, I., additional, Manea, C., additional, Rashevskaya, I., additional, Ricci, E., additional, Vitale, V., additional, Ambrosi, G., additional, Ionica, M., additional, Sposito, M., additional, Bartocci, S., additional, Conti, L., additional, Castellini, G., additional, Pacini, L., additional, and Ricciarini, S.B., additional

Published
2020
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9. Time dependence of the proton and helium flux measured by PAMELA

Author

Panico, Beatrice, primary, Campana, D., additional, Osteria, G., additional, Barbarino, G. C., additional, Adriani, O., additional, Bongi, M., additional, Spillantini, P., additional, Mori, N., additional, Papini, P., additional, Vannuccini, E., additional, Bazilevskaya, G. A., additional, Kvashnin, A. N., additional, Stozhkov, Y. I., additional, Bellotti, R., additional, Monaco, A., additional, Bruno, A., additional, Cafagna, F., additional, Boezio, M., additional, Bonvicini, V., additional, Mocchiutti, E., additional, Munini, R., additional, Zampa, G., additional, Zampa, N., additional, Vacchi, A., additional, Bogomolov, E. A., additional, Krutkov, S. Y., additional, Vasilyev, G. I., additional, Carlson, P., additional, Pearce, M., additional, Casolino, M., additional, Castellini, G., additional, De Santis, C., additional, Marcelli, L., additional, Mergè, M., additional, Picozza, P., additional, Sparvoli, R., additional, Di Felice, V., additional, Galper, A. M., additional, Karelin, A. V., additional, Koldashov, S. V., additional, Koldobskiy, S., additional, Yurkin, Y. T., additional, Malakhov, V., additional, Leonov, A., additional, Mayorov, A. G., additional, Mikhailov, V. V., additional, Voronov, S. A., additional, Martucci, M., additional, Menn, W., additional, Simon, M., additional, Ricci, M., additional, and Ricciarini, S. B., additional

Published
2020
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11. Cosmic ray electrons and positrons over decade with the PAMELA experiment

Author

Mikhailov, V V, primary, Adriani, O, additional, Barbarino, G, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Boezio, M, additional, Bogomolov, E A, additional, Bongi, M, additional, Bonvicini, V, additional, Bruno, A, additional, Cafagna, F S, additional, Campana, D, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, De Santis, C, additional, Di Felice, V, additional, Galper, A M, additional, Karelin, A V, additional, Kleymenova, S O, additional, Koldashov, S V, additional, Koldobskiy, S, additional, Krutkov, S Yu, additional, Kvashnin, A N, additional, Leonov, A A, additional, Malakhov, V V, additional, Marcelli, L, additional, Martucci, M, additional, Mayorova, A G, additional, Menn, W, additional, Merge, M, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N., additional, Munini, R, additional, Osteria, G, additional, Papini, P, additional, Panico, B, additional, Pearce, M, additional, Picozza, P, additional, Ricci, M, additional, Ricciarini, S B, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Yu I, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasiliev, G I, additional, Voronov, S A, additional, Yurkin, Yu T, additional, Zampa, G, additional, and Zampa, N, additional

Published
2019
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12. Galactic Cosmic-Ray Hydrogen Spectra in the 40–250 MeV Range Measured by the High-energy Particle Detector (HEPD) on board the CSES-01 Satellite between 2018 and 2020.

Author

Bartocci, S., Battiston, R., Burger, W. J., Campana, D., Carfora, L., Castellini, G., Conti, L., Contin, A., De Donato, C., De Persio, F., De Santis, C., Diego, P., Follega, F. M., Iuppa, R., Lazzizzera, I., Marcelli, N., Martucci, M., Masciantonio, G., Mergé, M., and Osteria, G.

Subjects
PARTICLE detectors, HYDROGEN as fuel, HYDROGEN, ARTIFICIAL satellites
Abstract

The High-energy Particle Detector (HEPD) on board the China Seismo-Electromagnetic Satellite (CSES-01)—launched on 2018 February 2—is a light and compact payload suitable for measuring electrons (3–100 MeV), protons (30–250 MeV), and light nuclei (up to a few hundreds of MeV). The Sun-synchronous orbit and large acceptance allow HEPD to measure cosmic-ray particles near the ±65° latitude limit for a fair amount of time per day. In this work, three semiannual galactic hydrogen energy spectra between ∼40 and 250 MeV are presented, including a comparison with theoretical spectra from HelMod, a 2D Monte Carlo model developed to simulate the solar modulation of cosmic rays throughout the heliosphere. To our knowledge, these are the first hydrogen energy spectra below 250 MeV measured at 1 au between 2018 and 2020. [ABSTRACT FROM AUTHOR]

Published
2020
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13. Sharp increasing of positron to electron fluxes ratio below 2 GV measured by the PAMELA

Author

Mikhailov, V V, primary, Adriani, O, additional, Barbarino, G, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Boezio, M, additional, Bogomolov, E A, additional, Bongi, M, additional, Bonvicini, V, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F S, additional, Campana, D, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, De Donato, C., additional, De Santis, C, additional, De Simone, N, additional, Di Felice, V., additional, Galper, A M, additional, Karelin, A V, additional, Koldashov, S V, additional, Koldobsky, S, additional, Krutkov, S Yu, additional, Kvashnin, A N, additional, Leonov, A A, additional, Malakhov, V V, additional, Marcelli, L, additional, Martucci, M, additional, Mayorov, A G, additional, Menn, W, additional, Merge, M, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N., additional, Munini, R, additional, Osteria, G, additional, Papini, P, additional, Palma, F, additional, Panico, B, additional, Pearce, M, additional, Picozza, P, additional, Ricci, M, additional, Ricciarini, S B, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Yu I, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasiliev, G I, additional, Voronov, S A, additional, Yurkin, Yu T, additional, Zampa, G, additional, and Zampa, N, additional

Published
2017
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14. Solar modulation of galactic cosmic rays during 2006-2015 based on PAMELA and ARINA data

Author

Mayorov, A G, primary, Adriani, O, additional, Aleksandrin, S Y, additional, Barbarino, G C, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Boezio, M, additional, Bogomolov, E A, additional, Bongi, M, additional, Bonvicini, V, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F, additional, Campana, D, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, De Santis, C, additional, Di Felice, V, additional, Galper, A M, additional, Karelin, A V, additional, Koldashov, S V, additional, Koldobskiy, S A, additional, Kvashnin, A A, additional, Leonov, A A, additional, Malakhov, V V, additional, Marcelli, L, additional, Martucci, M, additional, Mayorova, M A, additional, Menn, W, additional, Merge’, M, additional, Mikhailov, V V, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N, additional, Munini, R, additional, Naumov, P Yu, additional, Osteria, G, additional, Panico, B, additional, Papini, P, additional, Pearce, M, additional, Picozza, P, additional, Ricci, M, additional, Ricciarini, S B, additional, Rodenko, S A, additional, Rossetto, L, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Y, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasilyev, G I, additional, Voronov, S A, additional, Yurkin, Y T, additional, Zampa, G, additional, and Zampa, N, additional

Published
2017
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15. The PAMELA experiment: a decade of Cosmic Ray Physics in space

Author

Galper, A M, primary, Sparvoli, R, additional, Adriani, O, additional, Barbarino, G, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Boezio, M, additional, Bogomolov, E A, additional, Bongi, M, additional, Bonvicini, V, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F, additional, Campana, D, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, De Donato, C, additional, De Santis, C, additional, Di Felice, V, additional, Karelin, A V, additional, Koldashov, S V, additional, Koldobskiy, S A, additional, Krutkov, S Y, additional, Kvashnin, A N, additional, Leonov, A A, additional, Malakhov, V V, additional, Marcelli, L, additional, Martucci, M, additional, Mayorov, A G, additional, Menn, W, additional, Mergè, M, additional, Mikhailov, V V, additional, Mocchiutti, E, additional, Mori, N, additional, Munini, R, additional, Osteria, G, additional, Palma, F, additional, Panico, B, additional, Papini, P, additional, Pearce, M, additional, Picozza, P, additional, Ricci, M, additional, Ricciarini, S B, additional, Simon, M, additional, Spillantini, P, additional, Stozhkov, Y I, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasilyev, G I, additional, Voronov, S A, additional, Yurkin, Y T, additional, Zampa, G, additional, and Zampa, N, additional

Published
2017
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16. The measurement of the dipole anisotropy of protons and helium cosmic rays with the PAMELA experiment

Author

Karelin, A V, primary, Adriani, O, additional, Barbarino, G C, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Boezio, M, additional, Bogomolov, E A, additional, Bongi, M, additional, Bonvicini, V, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F, additional, Campana, D, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, De Donato, C, additional, De Santis, C, additional, De Simone, N, additional, Felice, V Di, additional, Formato, V, additional, Galper, A M, additional, Koldobskiy, S A, additional, Koldashov, S V, additional, Krutkov, S Y, additional, Kvashnin, A N, additional, Leonov, AA, additional, Malakhov, V, additional, Marcelli, L, additional, Martucci, M, additional, Mayorov, A G, additional, Menn, W, additional, Mergè, M, additional, Mikhailov, V V, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N, additional, Munini, R, additional, Osteria, G, additional, Palma, F, additional, Panico, B, additional, Papini, P, additional, Pearce, M, additional, Picozza, P, additional, Ricci, M, additional, Ricciarini, S B, additional, Sarkar, R, additional, Scotti, V, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Y I, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasilyev, GI, additional, Voronov, S A, additional, Yurkin, Y T, additional, Zampa, G, additional, and Zampa, N, additional

Published
2016
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17. H, He, Li and Be Isotopes in the PAMELA-Experiment

Author

Menn, W, primary, Adriani, O, additional, Barbarino, G C, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Boezio, M, additional, Bogomolov, E A, additional, Bongi, M, additional, Bonvicini, V., additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F, additional, Campana, D, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, De Donato, C, additional, De Santis, C, additional, De Simone, N, additional, di Felice, V, additional, Formato, V, additional, Galper, A M, additional, Karelin, A V, additional, Koldashov, S V, additional, Koldobskiy, S, additional, Krutkov, S Y, additional, Kvashnin, A N, additional, Leonov, A, additional, Malakhov, V, additional, Marcelli, L, additional, Martucci, M, additional, Mayorov, A G, additional, Mergè, M, additional, Mikhailov, V, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N, additional, Munini, R, additional, Osteria, G, additional, Palma, F, additional, Panico, B, additional, Papini, P, additional, Pearce, M, additional, Picozza, P, additional, Ricci, M, additional, Ricciarini, S B, additional, Sarkar, R, additional, Scotti, V., additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Y I, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasilyev, G, additional, Voronov, S A, additional, Yurkin, Y T, additional, Zampa, G, additional, Zampa, N, additional, Potgieter, M S, additional, and Vos, E E, additional

Published
2016
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18. The May 17, 2012 solar event: back-tracing analysis and flux reconstruction with PAMELA

Author

Bruno, A, primary, Adriani, O, additional, Barbarino, G C, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Boezio, M, additional, Bogomolov, E A., additional, Bongi, M, additional, Bonvicini, V, additional, Bottai, S, additional, Bravar, U, additional, Cafagna, F, additional, Campana, D, additional, Carbone, R, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, Christian, E C, additional, De Donato, C, additional, de Nolfo, G A, additional, De Santis, C, additional, De Simone, N, additional, Felice, V Di, additional, Formato, V, additional, Galper, A M, additional, Karelin, A V, additional, Koldashov, S V, additional, Koldobskiy, S, additional, Krutkov, S Y, additional, Kvashnin, A N, additional, Lee, M, additional, Leonov, A, additional, Malakhov, V, additional, Marcelli, L, additional, Martucci, M, additional, Mayorov, A G, additional, Menn, W, additional, Mergè, M, additional, Mikhailov, V V, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N, additional, Munini, R, additional, Osteria, G, additional, Palma, F, additional, Panico, B, additional, Papini, P, additional, Pearce, M, additional, Picozza, P, additional, Ricci, M, additional, Ricciarini, S B, additional, Ryan, J M, additional, Sarkar, R, additional, Scotti, V, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stochaj, S, additional, Stozhkov, Y I, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasilyev, G I, additional, Voronov, S A, additional, Yurkin, Y T, additional, Zampa, G, additional, Zampa, N, additional, and Zverev, V G, additional

Published
2016
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19. Features of re-entrant albedo deuteron trajectories in near Earth orbit with PAMELA experiment

Author

Koldobskiy, S A, primary, Adriani, O, additional, Barbarino, G C, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Boezio, M, additional, Bogomolov, E A, additional, Bongi, M, additional, Bonvicini, V, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F, additional, Campana, D, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, De Donato, C, additional, De Santis, C, additional, De Simone, N, additional, Felice, V Di, additional, Formato, V, additional, Galper, A M, additional, Karelin, A V, additional, Koldashov, S V, additional, Krutkov, S Y, additional, Kvashnin, A N, additional, Leonov, AA, additional, Malakhov, V, additional, Marcelli, L, additional, Martucci, M, additional, Mayorov, A G, additional, Menn, W, additional, Mergè, M, additional, Mikhailov, V V, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N, additional, Munini, R, additional, Osteria, G, additional, Palma, F, additional, Panico, B, additional, Papini, P, additional, Pearce, M, additional, Picozza, P, additional, Ricci, M, additional, Ricciarini, S B, additional, Sarkar, R, additional, Scotti, V, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Y I, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasilyev, GI, additional, Voronov, S A, additional, Yurkin, Y T, additional, Zampa, G, additional, and Zampa, N, additional

Published
2016
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20. Trapped positrons observed by PAMELA experiment

Author

Mikhailov, V V, primary, Adriani, O, additional, Barbarino, G, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Boezio, M, additional, Bogomolov, E A, additional, Bongi, M, additional, Bonvicini, V, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F S, additional, Campana, D, additional, Carbone, R, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, Consiglio, L, additional, De Santis, C, additional, De Simone, N, additional, Felice, V. Di, additional, Galper, A M, additional, Karelin, A V, additional, Koldashov, S V, additional, Koldobsky, S, additional, Krutkov, S Yu, additional, Kvashnin, A N, additional, Leonov, A A, additional, Malakhov, V V, additional, Marcelli, L, additional, Martucci, M, additional, Mayorov, A G, additional, Menn, W, additional, Merge, M, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N., additional, Munini, R, additional, Osteria, G, additional, Papini, P, additional, Palma, F, additional, Panico, B, additional, Pearce, M, additional, Picozza, P, additional, Ricci, M, additional, Ricciarini, S B, additional, Sarkar, R, additional, Scotti, V, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Yu I, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasiliev, G I, additional, Voronov, S A, additional, Yurkin, Yu T, additional, Zampa, G, additional, and Zampa, N, additional

Published
2016
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21. Study of deuteron spectra under radiation belt with PAMELA instrument

Author

Koldobskiy, S A, primary, Adriani, O, additional, Barbarino, G C, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Boezio, M, additional, Bogomolov, E A, additional, Bongi, M, additional, Bonvicini, V, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F, additional, Campana, D, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, De Donato, C, additional, De Santis, C, additional, De Simone, N, additional, Felice, V Di, additional, Formato, V, additional, Galper, A M, additional, Karelin, A V, additional, Koldashov, S V, additional, Krutkov, S Y, additional, Kvashnin, A A, additional, Kvashnin, A N, additional, Leonov, A A, additional, Malakhov, V V, additional, Marcelli, L, additional, Martucci, M, additional, Mayorov, A G, additional, Menn, W, additional, Merge’, M, additional, Mikhailov, V V, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N, additional, Munini, R, additional, Osteria, G, additional, Palma, F, additional, Panico, B, additional, Papini, P, additional, Pearce, M, additional, Picozza, P, additional, Ricci, M, additional, Ricciarini, S B, additional, Sarkar, R, additional, Scotti, V, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Y I, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasilyev, G I, additional, Voronov, S A, additional, Yurkin, Y T, additional, Zampa, G, additional, and Zampa, N, additional

Published
2015
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22. Measurement of electron-positron spectrum in high-energy cosmic rays in the PAMELA experiment

Author

Karelin, A V, primary, Adriani, O, additional, Barbarino, G C, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Boezio, M, additional, Bogomolov, E A, additional, Bongi, M, additional, Bonvicini, V, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F, additional, Campana, D, additional, Carbone, R, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, De Donato, C, additional, De Santis, C, additional, De Simone, N, additional, Felice, V Di, additional, Formato, V., additional, Galper, A M, additional, Koldashov, S V, additional, Koldobskiy, S A, additional, Krutkov, S Y, additional, Kvashnin, A N, additional, Leonov, A A, additional, Mayorov, A G, additional, Malakhov, V V, additional, Marcelli, L, additional, Martucci, M., additional, Menn, W, additional, Merge, M., additional, Mikhailov, V V, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N, additional, Munini, R., additional, Osteria, G, additional, Palma, F, additional, Panico, B., additional, Papini, P, additional, Pearce, M, additional, Picozza, P, additional, Ricci, M, additional, Ricciarini, S B, additional, Sarkar, R, additional, Scotti, V., additional, Rossetto, L, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasilyev, G I, additional, Voronov, S A, additional, Yurkin, Y T, additional, Zampa, G, additional, and Zampa, N, additional

Published
2015
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23. PAMELA measurements of the boron and carbon spectra

Author

Mori, N, primary, Adriani, O, additional, Barbarino, G C, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Boezio, M, additional, Bogomolov, E A, additional, Bongi, M, additional, Bonvicini, V, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F, additional, Campana, D, additional, Carbone, R, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, De Donato, C, additional, De Santis, C, additional, De Simone, N, additional, Felice, V Di, additional, Formato, V, additional, Galper, A M, additional, Karelin, A V, additional, Koldashov, S V, additional, Koldobskiy, S, additional, Krutkov, S Y, additional, Kvashnin, A N, additional, Leonov, A, additional, Malakhov, V, additional, Marcelli, L, additional, Martucci, M, additional, Mayorov, A G, additional, Menn, W, additional, Mergé, M, additional, Mikhailov, V V, additional, Mocchiutti, E, additional, Monaco, A, additional, Munini, R, additional, Osteria, G, additional, Palma, F, additional, Panico, B, additional, Papini, P, additional, Pearce, M, additional, Picozza, P, additional, Ricci, M, additional, Ricciarini, S B, additional, Sarkar, R, additional, Scotti, V, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Y I, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasilyev, G I, additional, Voronov, S A, additional, Yurkin, Y T, additional, Zampa, G, additional, and Zampa, N, additional

Published
2015
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24. Solar modulation of GCR electrons over the 23rd solar minimum with PAMELA

Author

Munini, R, primary, Di Felice, V, additional, Adriani, O, additional, Barbarino, G C, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Boezio, M, additional, Bogomolov, E A, additional, Bongi, M, additional, Bonvicini, V, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F, additional, Campana, D, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, De Donato, C, additional, De Santis, C, additional, De Simone, N, additional, Formato, V, additional, Galper, A M, additional, Karelin, A V, additional, Koldashov, S V, additional, Koldobskiy, S, additional, Krutkov, S Y, additional, Kvashnin, A N, additional, Leonov, A, additional, Malakhov, V, additional, Marcelli, L, additional, Martucci, M, additional, Mayorov, A G, additional, Menn, W, additional, Merge, M, additional, Mikhailov, V V, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N, additional, Osteria, G, additional, Palma, F, additional, Panico, B, additional, Papini, P, additional, Pearce, M, additional, Picozza, P, additional, Ricci, M, additional, Ricciarini, S B, additional, Sarkar, R, additional, Scotti, V, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Y I, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasilyev, G, additional, Voronov, S A, additional, Yurkin, Y T, additional, Zampa, G, additional, Zampa, N, additional, Potgieter, M S, additional, and Vos, E E, additional

Published
2015
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25. Time variations of proton flux in Earth inner radiation belt during 23/24 solar cycles based on the PAMELA and the ARINA data

Author

Malakhov, V V, primary, Koldashov, S V, additional, Mayorov, A G, additional, Mayorova, M A, additional, Mikhailov, V V, additional, Aleksandrin, S Yu, additional, Adriani, O, additional, Barbarino, G C, additional, Bazilevskaya, G A, additional, Boezio, M, additional, Bogomolov, E A, additional, Bongi, M, additional, Bonvicini, V, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F, additional, Campana, D, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, De Donato, C, additional, De Santis, C, additional, De Simone, N, additional, Di Felice, V, additional, Formato, V, additional, Galper, A M, additional, Karelin, A V, additional, Krutkov, S Yu, additional, Kvashnin, A A, additional, Kvashnin, A N, additional, Leonov, A A, additional, Marcelli, L, additional, Martucci, M, additional, Menn, W, additional, Merge, M, additional, Mocchuuitti, E, additional, Monaco, A, additional, Mori, N, additional, Munini, R, additional, Osteria, G, additional, Palma, F, additional, Panico, B, additional, Papini, P, additional, Pearce, M, additional, Picozza, P, additional, Ricci, M, additional, Ricciarini, S B, additional, Sarkar, R, additional, Scotti, V, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Yu I, additional, Vacci, A, additional, Vannuccini, E, additional, Vasilyev, G I, additional, Voronov, S A, additional, Yurkin, Yu T, additional, Zampa, G, additional, and Zampa, N, additional

Published
2015
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26. Measurement of the isotopic composition of hydrogen and helium nuclei in cosmic rays with the PAMELA experiment

Author

Adriani, O., Barbarino, G. C., Bazilevskaya, G. A., Bellotti, R., Boezio, M., Bogomolov, E. A., Bongi, M., Bonvicini, V., Borisov, S., Bottai, S., Bruno, A., Cafagna, F., Campana, D., Carbone, R., Carlson, Per, Casolino, M., Castellini, G., Danilchenko, I. A., De Pascale, M. P., De Santis, C., De Simone, N., Di Felice, V., 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., Mayorov, A. G., Menn, W., Mikhailov, V. V., Mocchiutti, E., Monaco, A., Mori, N., Nikonov, N., Osteria, G., Palma, F., Papini, P., Pearce, Mark, Picozza, P., Pizzolotto, C., Ricci, M., Ricciarini, S. B., Rossetto, Laura, Sarkar, R., Simon, M., Sparvoli, R., Spillantini, P., Stozhkov, Y. I., Vacchi, A., Vannuccini, E., Vasilyev, G., Voronov, S. A., Yurkin, Y. T., Wu, Juan, Zampa, G., Zampa, N., Zverev, V. G., Adriani, O., Barbarino, G. C., Bazilevskaya, G. A., Bellotti, R., Boezio, M., Bogomolov, E. A., Bongi, M., Bonvicini, V., Borisov, S., Bottai, S., Bruno, A., Cafagna, F., Campana, D., Carbone, R., Carlson, Per, Casolino, M., Castellini, G., Danilchenko, I. A., De Pascale, M. P., De Santis, C., De Simone, N., Di Felice, V., 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., Mayorov, A. G., Menn, W., Mikhailov, V. V., Mocchiutti, E., Monaco, A., Mori, N., Nikonov, N., Osteria, G., Palma, F., Papini, P., Pearce, Mark, Picozza, P., Pizzolotto, C., Ricci, M., Ricciarini, S. B., Rossetto, Laura, Sarkar, R., Simon, M., Sparvoli, R., Spillantini, P., Stozhkov, Y. I., Vacchi, A., Vannuccini, E., Vasilyev, G., Voronov, S. A., Yurkin, Y. T., Wu, Juan, Zampa, G., Zampa, N., and Zverev, V. G.

Abstract

The satellite-borne experiment PAMELA has been used to make new measurements of cosmic ray H and He isotopes. The isotopic composition was measured between 100 and 600 MeV /n for hydrogen and between 100 and 900 MeV /n for helium isotopes over the 23rd solar minimum from 2006 July to 2007 December. The energy spectrum of these components carries fundamental information regarding the propagation of cosmic rays in the galaxy which are competitive with those obtained from other secondary to primary measurements such as B/C., QC 20131213

Published
2013
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27. Time Dependence Of The Proton Flux Measured By Pamela During The 2006 July-2009 December Solar Minimum

Author

Adriani, O., Barbarino, G. C., Bazilevskaya, G. A., Bellotti, R., Boezio, M., Bogomolov, E. A., Bongi, M., Bonvicini, V., Borisov, S., Bottai, S., Bruno, A., Cafagna, F., Campana, D., Carbone, R., Carlson, Per, Casolino, M., Castellini, G., De Pascale, M. P., De Santis, C., De Simone, N., Di Felice, V., Formato, V., Galper, A. M., Grishantseva, L., Karelin, A. V., Koldashov, S. V., Koldobskiy, S., Krutkov, S. Y., Kvashnin, A. N., Leonov, A., Malakhov, V., Marcelli, L., Mayorov, A. G., Menn, W., Mikhailov, V. V., Mocchiutti, E., Monaco, A., Mori, N., Nikonov, N., Osteria, G., Palma, F., Papini, P., Pearce, Mark, Picozza, P., Pizzolotto, C., Ricci, M., Ricciarini, S. B., Rossetto, Laura, Sarkar, R., Simon, M., Sparvoli, R., Spillantini, P., Stozhkov, Y. I., Vacchi, A., Vannuccini, E., Vasilyev, G., Voronov, S. A., Yurkin, Y. T., Wu, Juan, Zampa, G., Zampa, N., Zverev, V. G., Potgieter, M. S., Vos, E. E., Adriani, O., Barbarino, G. C., Bazilevskaya, G. A., Bellotti, R., Boezio, M., Bogomolov, E. A., Bongi, M., Bonvicini, V., Borisov, S., Bottai, S., Bruno, A., Cafagna, F., Campana, D., Carbone, R., Carlson, Per, Casolino, M., Castellini, G., De Pascale, M. P., De Santis, C., De Simone, N., Di Felice, V., Formato, V., Galper, A. M., Grishantseva, L., Karelin, A. V., Koldashov, S. V., Koldobskiy, S., Krutkov, S. Y., Kvashnin, A. N., Leonov, A., Malakhov, V., Marcelli, L., Mayorov, A. G., Menn, W., Mikhailov, V. V., Mocchiutti, E., Monaco, A., Mori, N., Nikonov, N., Osteria, G., Palma, F., Papini, P., Pearce, Mark, Picozza, P., Pizzolotto, C., Ricci, M., Ricciarini, S. B., Rossetto, Laura, Sarkar, R., Simon, M., Sparvoli, R., Spillantini, P., Stozhkov, Y. I., Vacchi, A., Vannuccini, E., Vasilyev, G., Voronov, S. A., Yurkin, Y. T., Wu, Juan, Zampa, G., Zampa, N., Zverev, V. G., Potgieter, M. S., and Vos, E. E.

Abstract

The energy spectra of galactic cosmic rays carry fundamental information regarding their origin and propagation. These spectra, when measured near Earth, are significantly affected by the solar magnetic field. A comprehensive description of the cosmic radiation must therefore include the transport and modulation of cosmic rays inside the heliosphere. During the end of the last decade, the Sun underwent a peculiarly long quiet phase well suited to study modulation processes. In this paper we present proton spectra measured from 2006 July to 2009 December by PAMELA. The large collected statistics of protons allowed the time variation to be followed on a nearly monthly basis down to 400 MV. Data are compared with a state-of-the-art three-dimensional model of solar modulation., QC 20130408

Published
2013
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28. Galactic deuteron spectrum measured in PAMELA experiment

Author

Koldobskiy, S. A., Adriani, O., Barbarino, G. C., Bazilevskaya, G. A., Bellotti, R., Boezio, M., Bogomolov, E. A., Bonechi, L., Bongi, M., Bonvicini, V., Borisov, S. V., Bottai, S., Bruno, A., Cafagna, F., Campana, D., Carbone, R., Carlson, P., Casolino, M., Castellini, G., Consiglio, L., De Pascale, M. P., De Santis, C., De Simone, N., Di Felice, V., Galper, A. M., Gillard, William, Jerse, G., Karelin, A. V., Kheymits, M. D., Koldashov, S. V., Krutkov, S. Y., Kvashnin, A. N., Leonov, A. A., Malakhov, V. V., Marcelli, L., Mayorov, A. G., Menn, W., Mikhailov, V. V., Mocchiutti, E., Monaco, A., Mori, N., Nikonov, N., Osteria, G., Palma, F., Papini, P., Pearce, M., Picozza, P., Pizzolotto, C., Ricci, M., Ricciarini, S. B., Sarkar, R., Rossetto, Laura, Simon, M., Sparvoli, R., Spillantini, P., Stozhkov, Y. I., Vacchi, A., Vannuccini, E., Vasilyev, G. I., Voronov, S. A., Wu, Juan, Yurkin, Y. T., Zampa, G., Zampa, N., Zverev, V. G., Koldobskiy, S. A., Adriani, O., Barbarino, G. C., Bazilevskaya, G. A., Bellotti, R., Boezio, M., Bogomolov, E. A., Bonechi, L., Bongi, M., Bonvicini, V., Borisov, S. V., Bottai, S., Bruno, A., Cafagna, F., Campana, D., Carbone, R., Carlson, P., Casolino, M., Castellini, G., Consiglio, L., De Pascale, M. P., De Santis, C., De Simone, N., Di Felice, V., Galper, A. M., Gillard, William, Jerse, G., Karelin, A. V., Kheymits, M. D., Koldashov, S. V., Krutkov, S. Y., Kvashnin, A. N., Leonov, A. A., Malakhov, V. V., Marcelli, L., Mayorov, A. G., Menn, W., Mikhailov, V. V., Mocchiutti, E., Monaco, A., Mori, N., Nikonov, N., Osteria, G., Palma, F., Papini, P., Pearce, M., Picozza, P., Pizzolotto, C., Ricci, M., Ricciarini, S. B., Sarkar, R., Rossetto, Laura, Simon, M., Sparvoli, R., Spillantini, P., Stozhkov, Y. I., Vacchi, A., Vannuccini, E., Vasilyev, G. I., Voronov, S. A., Wu, Juan, Yurkin, Y. T., Zampa, G., Zampa, N., and Zverev, V. G.

Abstract

Results of galactic deuteron spectrum measurement by means of PAMELA apparatus are described. PAMELA is an international experiment developed for antimatter search and measurement of p, He, electron and positron spectra in wide energy range. In addition, PAMELA allows to identify and measure deuteron spectrum at low energies. In this paper deuteron-to-proton ratio and deuteron spectrum are presented., QC 20211111

Published
2013
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29. Relative nuclear abundance from C to Fe and integrated flux inside the Russian part of the ISS with the Sileye-3/Alteino experiment

Author

Larsson, O, primary, Benghin, V V, additional, Casolino, M, additional, Chernikch, I V, additional, Fino, L di, additional, Fuglesang, C, additional, Larosa, M, additional, Lund-Jensen, B, additional, Narici, L, additional, Nikolaev, I V, additional, Petrov, V M, additional, Picozza, P, additional, de Santis, C, additional, and Zaconte, V, additional

Published
2013
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30. The PAMELA experiment: light-nuclei selection with stand-alone detectors

Author

Carbone, R, primary, Adriani, O, additional, Barbarino, G C, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Bianco, A, additional, Boezio, M, additional, Bogomolov, E A, additional, Bonechi, L, additional, Bongi, M, additional, Bonvicini, V, additional, Borisov, S, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F, additional, Campana, D, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, De Pascale, M P, additional, De Santis, C, additional, De Simone, N, additional, Di Felice, V, additional, Formato, V, additional, Galper, A M, additional, Giaccari, U, additional, Grishantseva, L, additional, Jerse, G, additional, Karelin, A V, additional, Kheymits, M D, additional, Koldashov, S V, additional, Krutkov, S Y, additional, Kvashnin, A N, additional, Leonov, A, additional, Malakhov, V, additional, Malvezzi, V, additional, Marcelli, L, additional, Martucci, M, additional, Mayorov, A G, additional, Menn, W, additional, Mikhailov, V V, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N, additional, Munini, R, additional, Nikonov, N, additional, Osteria, G, additional, Palma, F, additional, Papini, P, additional, Pearce, M, additional, Picozza, P, additional, Pizzolotto, C, additional, Ricci, M, additional, Ricciarini, S B, additional, Rossetto, L, additional, Sarkar, R, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Y I, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasilyev, G, additional, Voronov, S A, additional, Wu, J, additional, Yurkin, Y T, additional, Zampa, G, additional, Zampa, N, additional, and Zverev, V G, additional

Published
2013
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31. A search algorithm for finding Cosmic-Ray anisotropy with the PAMELA calorimeter

Author

Karelin, A V, primary, Adriani, O, additional, Barbarino, G C, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Boezio, M, additional, Bogomolov, E A, additional, Bonechi, L, additional, Bongi, M, additional, Bonvicini, V, additional, Borisov, S V, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F, additional, Campana, D, additional, Carbone, R, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, Consiglio, L, additional, De Pascale, M P, additional, De Santis, C, additional, De Simone, N, additional, Di Felice, V, additional, Galper, A M, additional, Gillard, W, additional, Jerse, G, additional, Kheymits, M D, additional, Koldashov, S V, additional, Koldobskiy, S A, additional, Krutkov, S Y, additional, Kvashnin, A N, additional, Leonov, A A, additional, Mayorov, A G, additional, Malakhov, V V, additional, Marcelli, L, additional, Menn, W, additional, Mikhailov, V V, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N, additional, Nikonov, N, additional, Osteria, G, additional, Palma, F, additional, Papini, P, additional, Pearce, M, additional, Picozza, P, additional, Pizzolotto, C, additional, Ricci, M, additional, Ricciarini, S B, additional, Sarkar, R, additional, Rossetto, L, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Y I, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasilyev, G I, additional, Voronov, S A, additional, Wu, J, additional, Yurkin, Y T, additional, Zampa, G, additional, Zampa, N, additional, and Zverev, V G, additional

Published
2013
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32. Cosmic ray electron and positron spectra measured with PAMELA

Author

Mikhailov, Vladimir, primary, Adriani, O, additional, Barbarino, G, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Boezio, M, additional, Bogomolov, E A, additional, Bonechi, L, additional, Bongi, M, additional, Bonvicini, V, additional, Borisov, S V, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F S, additional, Campana, D, additional, Carbone, R, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, Consiglio, L, additional, De Pascale, M P, additional, De Santis, C, additional, De Simone, N, additional, Di Felice, V, additional, Galper, A M, additional, Jerse, G, additional, Karelin, A V, additional, Koldashov, S V, additional, Koldobsky, S, additional, Yu Krutkov, S, additional, Kvashnin, A N, additional, Leonov, A A, additional, Malakhov, V V, additional, Malvezzi, V, additional, Marcelli, L, additional, Mayorov, A G, additional, Menn, W, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N, additional, Osteria, G, additional, Papini, P, additional, Palma, F, additional, Pearce, M, additional, Picozza, P, additional, Pizzolotto, C, additional, Ricci, M, additional, Ricciarini, S B, additional, Rossetto, L, additional, Sarkar, R, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Yu I, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasiliev, G I, additional, Voronov, S A, additional, Wu, J, additional, Yurkin, Yu T, additional, Zampa, G, additional, Zampa, N, additional, and Zverev, V G, additional

Published
2013
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33. Measurement of antiproton flux in primary cosmic radiation with PAMELA experiment

Author

Mayorov, A G, primary, Adriani, O, additional, Barbarino, G C, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Boezio, M, additional, Bogomolov, E A, additional, Bonechi, L, additional, Bongi, M, additional, Bonvicini, V, additional, Borisov, S V, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F, additional, Campana, D, additional, Carbone, R, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, Consiglio, L, additional, De Pascale, M P, additional, De Santis, C, additional, De Simone, N, additional, Di Felice, V, additional, Galper, A M, additional, Gillard, W, additional, Jerse, G, additional, Karelin, A V, additional, Kheymits, M D, additional, Koldashov, S V, additional, Koldobskiy, S A, additional, Krutkov, S Y, additional, Kvashnin, A N, additional, Leonov, A A, additional, Malakhov, V V, additional, Marcelli, L, additional, Menn, W, additional, Mikhailov, V V, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N, additional, Nikonov, N N, additional, Osteria, G, additional, Palma, F, additional, Papini, P, additional, Pearce, M, additional, Picozza, P, additional, Pizzolotto, C, additional, Ricci, M, additional, Ricciarini, S B, additional, Sarkar, R, additional, Rossetto, L, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Y I, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasilyev, G I, additional, Voronov, S A, additional, Wu, J, additional, Yurkin, Y T, additional, Zampa, G, additional, Zampa, N, additional, and Zverev, V G, additional

Published
2013
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34. Cosmic Ray Study with the PAMELA Experiment

Author

Picozza, P, primary, Marcelli, L, additional, Adriani, O, additional, Barbarino, G C, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Boezio, M, additional, Bogomolov, E A, additional, Bongi, M, additional, Bonvicini, V, additional, Borisov, S, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F, additional, Campana, D, additional, Carbone, R, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, De Pascale, M P, additional, De Santis, C, additional, De Simone, N, additional, Di Felice, V, additional, Galper, A M, additional, Grishantseva, L, additional, Jerse, G, additional, Karelin, A V, additional, Kheymits, M D, additional, Koldashov, S V, additional, Krutkov, S Y, additional, Kvashnin, A N, additional, Leonov, A, additional, Malakhov, V, additional, Mayorov, A G, additional, Menn, W, additional, Mikhailov, V V, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N, additional, Nikonov, N, additional, Osteria, G, additional, Palma, F, additional, Papini, P, additional, Pearce, M, additional, Pizzolotto, C, additional, Ricci, M, additional, Ricciarini, S B, additional, Sarkar, R, additional, Rossetto, L, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Y I, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasilyev, G, additional, Voronov, S A, additional, Yurkin, Y T, additional, Wu, J, additional, Zampa, G, additional, Zampa, N, additional, and Zverev, V G, additional

Published
2013
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35. Search for cosmic ray electron-positron anisotropies with the Pamela data

Author

Campana, D, primary, Giaccari, U, additional, Adriani, O, additional, Barbarino, G C, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Bianco, A, additional, Boezio, M, additional, Bogomolov, E A, additional, Bonechi, L, additional, Bongi, M, additional, Bonvicini, V, additional, Borisov, S, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F, additional, Carbone, R, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, De Pascale, M P, additional, De Santis, C, additional, De Simone, N, additional, Di Felice, V, additional, Formato, V, additional, Galper, A M, additional, Grishantseva, L, additional, Jerse, G, additional, Karelin, A V, additional, Kheymits, M D, additional, Koldashov, S V, additional, Krutkov, S Y, additional, Kvashnin, A N, additional, Leonov, A, additional, Malakhov, V, additional, Malvezzi, V, additional, Marcelli, L, additional, Martucci, M, additional, Mayorov, A G, additional, Menn, W, additional, Mikhailov, V V, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N, additional, Munini, R, additional, Nikonov, N, additional, Osteria, G, additional, Palma, F, additional, Papini, P, additional, Pearce, M, additional, Picozza, P, additional, Pizzolotto, C, additional, Ricci, M, additional, Ricciarini, S B, additional, Rossetto, L, additional, Sarkar, R, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Y I, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasilyev, G, additional, Voronov, S A, additional, Wu, J, additional, Yurkin, Y T, additional, Zampa, G, additional, Zampa, N, additional, and Zverev, V G, additional

Published
2013
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36. Galactic deuteron spectrum measured in PAMELA experiment

Author

Koldobskiy, S A, primary, Adriani, O, additional, Barbarino, G C, additional, Bazilevskaya, G A, additional, Bellotti, R, additional, Boezio, M, additional, Bogomolov, E A, additional, Bonechi, L, additional, Bongi, M, additional, Bonvicini, V, additional, Borisov, S V, additional, Bottai, S, additional, Bruno, A, additional, Cafagna, F, additional, Campana, D, additional, Carbone, R, additional, Carlson, P, additional, Casolino, M, additional, Castellini, G, additional, Consiglio, L, additional, De Pascale, M P, additional, De Santis, C, additional, De Simone, N, additional, Di Felice, V, additional, Galper, A M, additional, Gillard, W, additional, Jerse, G, additional, Karelin, A V, additional, Kheymits, M D, additional, Koldashov, S V, additional, Krutkov, S Y, additional, Kvashnin, A N, additional, Leonov, A A, additional, Malakhov, V V, additional, Marcelli, L, additional, Mayorov, A G, additional, Menn, W, additional, Mikhailov, Y V, additional, Mocchiutti, E, additional, Monaco, A, additional, Mori, N, additional, Nikonov, N, additional, Osteria, G, additional, Palma, F, additional, Papini, P, additional, Pearce, M, additional, Picozza, P, additional, Pizzolotto, C, additional, Ricci, M, additional, Ricciarini, S B, additional, Sarkar, R, additional, Rossetto, L, additional, Simon, M, additional, Sparvoli, R, additional, Spillantini, P, additional, Stozhkov, Y I, additional, Vacchi, A, additional, Vannuccini, E, additional, Vasilyev, G I, additional, Voronov, S A, additional, Wu, J, additional, Yurkin, Y T, additional, Zampa, G, additional, Zampa, N, additional, and Zverev, V G, additional

Published
2013
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41. 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

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