13 results on '"Krutkov, S.Yu."'
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2. Cosmic ray measurements with Pamela experiment
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Casolino, M., De Simone, N., De Pascale, M.P., Di Felice, V., Marcelli, L., Minori, M., Picozza, P., Sparvoli, R., Castellini, G., Adriani, O., Bonechi, L., Bongi, M., Bottai, S., Fedele, D., Papini, P., Ricciarini, S., Spillantini, P., Taddei, E., Vannuccini, E., Barbarino, G., Campana, D., Carbone, R., De Rosa, G., Osteria, G., Boezio, M., Bonvicini, V., Mocchiutti, E., Vacchi, A., Zampa, G., Zampa, N., Bruno, A., Cafagna, F.S., Ricci, Marco, Hofverberg, Petter, Pearce, Mark, Carlson, Per, Bogomolov, Edward, Krutkov, S.Yu., Nikonov, N.N., Vasilyev, G.I., Menn, Wolfgang, Simon, Manfred, Galper, Arkady M., Grishantseva, Lubov, Koldashov, Sergey, Leonov, Alexey, Mikhailov, Vladimir V., Voronov, Sergey A., Yurkin, Yuri T., Zverev, Valeri G., Bazilevskaya, Galina A., Kvashnin, Alexander N., Maksumov, Osman, and Stozhkov, Yuri
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- 2009
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3. In-flight performances of the PAMELA satellite experiment
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Papini, P., Adriani, O., Ambriola, M., Barbarino, G.C., Basili, A., Bazilevskaja, G.A., Boezio, M., Bogomolov, E.A., Bonechi, L., Bongi, M., Bongiorno, L., Bonvicini, V., Bruno, A., Cafagna, F., Campana, D., Carlson, P., Casolino, M., Castellini, G., Conrad, J., De Marzo, C., De Pascale, M.P., De Rosa, G., Di Felice, V., Fedele, D., Galper, A.M., Hofverberg, P., Koldashov, S.V., Krutkov, S.Yu., Kvashnin, A.N., Lund, J., Lundquist, J., Maksumov, O., Malvezzi, V., Marcelli, L., Menn, W., Mikhailov, V.V., Minori, M., Misin, S., Mocchiutti, E., Morselli, A., Nikonov, N.N., Orsi, S., Osteria, G., Pearce, M., Picozza, P., Ricci, M., Ricciarini, S.B., Runtso, M.F., Russo, S., Simon, M., Sparvoli, R., Spillantini, P., Stozhkov, Yu.I., Taddei, E., Vacchi, A., Vannuccini, E., Voronov, S.A., Yurkin, Y.T., Zampa, G., Zampa, N., and Zverev, V.G.
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- 2008
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4. Magnetospheric and solar physics observations with the PAMELA experiment
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Casolino, M., Adriani, O., Ambriola, M., Barbarino, G.C., Basili, A., Bazilevskaja, G.A., Boezio, M., Bogomolov, E.A., Bonechi, L., Bongi, M., Bonvicini, V., Bruno, A., Cafagna, F., Campana, D., Carlson, P., Castellini, G., De Marzo, C., De Pascale, M.P., De Rosa, G., De Simone, N., Di Felice, V., Fedele, D., Galper, A.M., Hofverberg, P., Koldashov, S.V., Krutkov, S.Yu., Kvashnin, A.N., Lundquist, J., Maksumov, O., Malvezzi, V., Marcelli, L., Menn, W., Mikhailov, V.V., Minori, M., Misin, S., Mocchiutti, E., Morselli, A., Nikonov, N.N., Orsi, S., Osteria, G., Papini, P., Pearce, M., Picozza, P., Ricci, M., Ricciarini, S.B., Runtso, M.F., Russo, S., Simon, M., Sparvoli, R., Spillantini, P., Stozhkov, Yu.I., Taddei, E., Vacchi, A., Vannuccini, E., Vasilyev, G.I., Voronov, S.A., Yurkin, Y.T., Zampa, G., Zampa, N., and Zverev, V.G.
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- 2008
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5. PAMELA – A payload for antimatter matter exploration and light-nuclei astrophysics
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Picozza, P., Galper, A.M., Castellini, G., Adriani, O., Altamura, F., Ambriola, M., Barbarino, G.C., Basili, A., Bazilevskaja, G.A., Bencardino, R., Boezio, M., Bogomolov, E.A., Bonechi, L., Bongi, M., Bongiorno, L., Bonvicini, V., Cafagna, F., Campana, D., Carlson, P., Casolino, M., De Marzo, C., De Pascale, M.P., De Rosa, G., Fedele, D., Hofverberg, P., Koldashov, S.V., Krutkov, S.Yu., Kvashnin, A.N., Lund, J., Lundquist, J., Maksumov, O., Malvezzi, V., Marcelli, L., Menn, W., Mikhailov, V.V., Minori, M., Misin, S., Mocchiutti, E., Morselli, A., Nikonov, N.N., Orsi, S., Osteria, G., Papini, P., Pearce, M., Ricci, M., Ricciarini, S.B., Runtso, M.F., Russo, S., Simon, M., Sparvoli, R., Spillantini, P., Stozhkov, Yu.I., Taddei, E., Vacchi, A., Vannuccini, E., Voronov, S.A., Yurkin, Y.T., Zampa, G., Zampa, N., and Zverev, V.G.
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- 2007
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6. PAMELA mission: heralding a new era in cosmic ray physics
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Ricciarini S. 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 Pascale M.P., De Santis C., De Simone N., Di Felice V., Formato V., Galper A.M., Karelin A.V., Kheymits M.D., Koldashov S.V., Koldobskiy S., Krutkov S.Yu., 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., Pizzolotto C., Ricci M., Sarkar R., Simon M., Scotti V., Sparvoli R., Spillantini P., Stozhkov Y.I., Vacchi A., Vannuccini E., Vasilyev G.I., Voronov S.A., Yurkin Y.T., Zampa G., Zampa N., and Zverev V.G.
- Subjects
Physics ,QC1-999 - Abstract
After seven years of data taking in space, the experiment PAMELA is showing 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.
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- 2014
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7. Antiprotons of galactic cosmic radiation in the PAMELA experiment
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Mayorov, A. G., Adriani, O., Barbarino, G., Bazilevskaia, G. A., Belotti, 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, Per, Casolino, M., Castellini, G., Consiglio, L., Danilchenko, I. A., De Pascale, M. P., De Santis, C., De Simone, N., Di Felice, V., Galper, A. M., Gillard, William, Grishantseva, L. A., Jerse, G., Karelin, A. V., Kheimits, M. D., Koldashov, S. V., Koldobskiy, S. A., Krutkov, S.Yu., Kvashnin, A. N., Leonov, A. A., Malakhov, V. V., Malvezzi, V., Marcelli, L., Menn, W., Mikhailov, V. V., Mocchiutti, E., Monaco, A., Mori, N., Nikonov, N. N., Osteria, G., Palma, F., Papini, P., Pearce, Mark, Picozza, P., Pizzolotto, S., Ricci, M., Ricciarini, S., Rozetto, Laura, Runtso, M. F., Sarkar, R., Simon, M., Sparvoli, R., Spilantini, P., Stozhkov, Yu.I., Vacchi, A., Vannuccini, E., Vasilyev, G. I., Voronov, S. A., Wu, Juan, Yurkin, Yu.T., Zampa, G., Zampa, N., Zverev, V. G., Mayorov, A. G., Adriani, O., Barbarino, G., Bazilevskaia, G. A., Belotti, 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, Per, Casolino, M., Castellini, G., Consiglio, L., Danilchenko, I. A., De Pascale, M. P., De Santis, C., De Simone, N., Di Felice, V., Galper, A. M., Gillard, William, Grishantseva, L. A., Jerse, G., Karelin, A. V., Kheimits, M. D., Koldashov, S. V., Koldobskiy, S. A., Krutkov, S.Yu., Kvashnin, A. N., Leonov, A. A., Malakhov, V. V., Malvezzi, V., Marcelli, L., Menn, W., Mikhailov, V. V., Mocchiutti, E., Monaco, A., Mori, N., Nikonov, N. N., Osteria, G., Palma, F., Papini, P., Pearce, Mark, Picozza, P., Pizzolotto, S., Ricci, M., Ricciarini, S., Rozetto, Laura, Runtso, M. F., Sarkar, R., Simon, M., Sparvoli, R., Spilantini, P., Stozhkov, Yu.I., Vacchi, A., Vannuccini, E., Vasilyev, G. I., Voronov, S. A., Wu, Juan, Yurkin, Yu.T., Zampa, G., Zampa, N., and Zverev, V. G.
- Abstract
A method for antiproton selection against a background of electrons, based on a mathematical model of data classification using variations in interparticle interaction in a calorimeter, and a method for excluding events accompanied by scattering in the inner detectors of a tracking system (which result in errors in the measured trajectory's curvature and charge sign) from analysis are discussed in this paper. Antiproton spectra and antiproton/proton flux ratio at energies of 0.06 to 350 GeV with statistics of events surpassing those in [1] are obtained. The results can be used to create models for the generation and distribution of particles in the Galaxy, and for searching and studying the nature of hypothetical dark matter particles., QC 20131125
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- 2013
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8. Solar proton events at the end of the 23rd and start of the 24th solar cycle recorded in the PAMELA experiment
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Bazilevskaya, G. A., Mayorov, A. G., Malakhov, V. V., Mikhailov, V. V., Adriani, O., Barbarino, G. C., Belotti, R., Boezio, M., Bogomolov, E. A., Bonvicini, V., Bongi, M., Bonechi, L., Borisov, S. V., Bottai, S., Bruno, A., Vacci, A., Vanuccini, E., Vasilyev, G. I., Voronov, S. A., Wu, Juan, Galper, A. M., Grishantseva, L. A., Danilchenko, I. A., Gillard, William, Jerse, G., Zampa, G., Zampa, N., Zverev, V. G., Casolino, M., Campana, D., Carbone, R., Karelin, A. V., Carlson, Per, Castellini, G., Cafagna, F., Kvashnin, A. N., Koldashov, S. V., Koldobskiy, S. A., Krutkov, S.Yu., Consiglio, L., Leonov, A. A., Malvezzi, V., Marcelli, L., Menn, W., Mocchiutti, E., Monaco, A., Mori, N., Nikonov, N. N., Osteria, G., Palma, F., Papini, P., Pizzolotto, C., De Pascale, M. P., Picozza, P., Pearce, Mark, Ricci, M., Ricciarini, S. B., Rossetto, Laura, Runtso, M. F., De Santis, C., Sarkar, R., Simon, M., De Simone, N., Sparvoli, R., Spillantini, P., Stozhkov, Yu.I., Di Felice, V., Kheymits, M. D., Yurkin, Yu.T., Bazilevskaya, G. A., Mayorov, A. G., Malakhov, V. V., Mikhailov, V. V., Adriani, O., Barbarino, G. C., Belotti, R., Boezio, M., Bogomolov, E. A., Bonvicini, V., Bongi, M., Bonechi, L., Borisov, S. V., Bottai, S., Bruno, A., Vacci, A., Vanuccini, E., Vasilyev, G. I., Voronov, S. A., Wu, Juan, Galper, A. M., Grishantseva, L. A., Danilchenko, I. A., Gillard, William, Jerse, G., Zampa, G., Zampa, N., Zverev, V. G., Casolino, M., Campana, D., Carbone, R., Karelin, A. V., Carlson, Per, Castellini, G., Cafagna, F., Kvashnin, A. N., Koldashov, S. V., Koldobskiy, S. A., Krutkov, S.Yu., Consiglio, L., Leonov, A. A., Malvezzi, V., Marcelli, L., Menn, W., Mocchiutti, E., Monaco, A., Mori, N., Nikonov, N. N., Osteria, G., Palma, F., Papini, P., Pizzolotto, C., De Pascale, M. P., Picozza, P., Pearce, Mark, Ricci, M., Ricciarini, S. B., Rossetto, Laura, Runtso, M. F., De Santis, C., Sarkar, R., Simon, M., De Simone, N., Sparvoli, R., Spillantini, P., Stozhkov, Yu.I., Di Felice, V., Kheymits, M. D., and Yurkin, Yu.T.
- Abstract
The PAMELA magnetic spectrometer was launched into a near-Earth orbit on board the Resurs-DK1 satellite in June 2006; in December 2006, it recorded the last strong solar high-energy particle event of the 23rd solar cycle. A deficit was thereafter observed in solar energetic particle events because of the lengthy solar activity minimum and the weak evolution of the next (24th) solar cycle. As a result, only a few solar events involving protons with energies of more than 100 MeV were recorded between 2010 and 1012. This work presents the preliminary results from measurements of charged particle fluxes in these events, recorded by the Pamela spectrometer., QC 20131125
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- 2013
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9. Two years of flight of the Pamela experiment : Results and perspectives
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Casolino, M., De Simone, N., Bongue, D., De Pascale, M. P., Felice, V. D., Marcelli, L., Minori, M., Picozza, P., Sparvoli, R., Castellini, G., Adriani, O., Bonechi, L., Bongi, M., Bottai, S., Papini, P., Ricciarini, S., Spillantini, P., Taddei, E., Vannuccini, E., Barbarino, G., Campana, D., Carbone, R., De Rosa, G., Osteria, G., Boezio, M., Bonvicini, V., Mocchiutti, E., Vacchi, A., Zampa, G., Zampa, N., Bruno, A., Cafagna, F. S., Ricci, M., Hofverberg, Petter, Pearce, Mark, Carlson, Per, Bogomolov, E., Krutkov, S.Yu., Nikonov, N. N., Menn, W., Simon, M., Galper, A. M., Grishantseva, L., Koldashov, S., Leonov, A., Mikhailov, V. V., Voronov, S. A., Yurkin, Y. T., Zverev, V. G., Bazilevskaya, G. A., Kvashnin, A. N., Maksumov, O., Stozhkov, Y., Casolino, M., De Simone, N., Bongue, D., De Pascale, M. P., Felice, V. D., Marcelli, L., Minori, M., Picozza, P., Sparvoli, R., Castellini, G., Adriani, O., Bonechi, L., Bongi, M., Bottai, S., Papini, P., Ricciarini, S., Spillantini, P., Taddei, E., Vannuccini, E., Barbarino, G., Campana, D., Carbone, R., De Rosa, G., Osteria, G., Boezio, M., Bonvicini, V., Mocchiutti, E., Vacchi, A., Zampa, G., Zampa, N., Bruno, A., Cafagna, F. S., Ricci, M., Hofverberg, Petter, Pearce, Mark, Carlson, Per, Bogomolov, E., Krutkov, S.Yu., Nikonov, N. N., Menn, W., Simon, M., Galper, A. M., Grishantseva, L., Koldashov, S., Leonov, A., Mikhailov, V. V., Voronov, S. A., Yurkin, Y. T., Zverev, V. G., Bazilevskaya, G. A., Kvashnin, A. N., Maksumov, O., and Stozhkov, Y.
- Abstract
PAMELA is a satellite borne experiment designed to study with great accuracy cosmic rays of galactic, solar, and trapped nature in a wide energy range (protons: 80 MeV-700 GeV, electrons 50 MeV-400 GeV). Main objective is the study of the antimatter component: antiprotons (80 MeV-190 GeV), positrons (50 MeV-270 GeV) and search for antinuclei with a precision of the order of 10~8). The experiment, housed on board the Russian Resurs-DKl satellite, was launched on June, 15th 2006 in a 350 x 600 km orbit with an inclination of 70 degrees. In this work we describe the scientific objectives and the performance of PAMELA in its first two years of operation. Data on protons of trapped, secondary and galactic nature - as well as measurements of the December 13th 2006 Solar Particle Event - are also provided., QC 20141007
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- 2009
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10. Secondary electron and positron fluxes in the near-Earth space observed in the ARINA and PAMELA experiments
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Adriani, O., Bazilevskaya, G. A., Barbarino, G. C., Bellotti, T. R., Bzheumikhova, M. A., Bogomolov, E. A., Boezio, V. M., Bonvicini, V., Bongi, M., Bonechi, L., Bottai, S., Bruno, A., Vacchi, A., Vannuccini, E., Vasiliev, G. V., Voronov, S. A., Galper, A. M., Grishantseva, L. A., Zampa, G., Zampa, N., Zverev, V. G., Casolino, M., Campana, T. D., Carlson, Per, Castellini, G., Cafagna, F., Kvashnin, A. N., Koldashov, S. V., Krutkov, S.Yu., Leonov, A. A., Malakhov, V. V., Malvezzi, V., Marcelli, L., Menn, W., Mikhailov, V. V., Mocchiutti, E., Orsi, Silvio, Osteria, G., Papini, P., De Pascale, M. P., Picozza, T. P., Pearce, Mark, De Rosa, G., Ricci, M., Ricciarini, S. B., Simon, M., De Simone, N., Sparvoli, R., Spillantini, P., Stozhkov, Yu.I., Taddei, E., Felice, V., Fedele, D., Hofverberg, Petter, Yurkin, Yu.T., Adriani, O., Bazilevskaya, G. A., Barbarino, G. C., Bellotti, T. R., Bzheumikhova, M. A., Bogomolov, E. A., Boezio, V. M., Bonvicini, V., Bongi, M., Bonechi, L., Bottai, S., Bruno, A., Vacchi, A., Vannuccini, E., Vasiliev, G. V., Voronov, S. A., Galper, A. M., Grishantseva, L. A., Zampa, G., Zampa, N., Zverev, V. G., Casolino, M., Campana, T. D., Carlson, Per, Castellini, G., Cafagna, F., Kvashnin, A. N., Koldashov, S. V., Krutkov, S.Yu., Leonov, A. A., Malakhov, V. V., Malvezzi, V., Marcelli, L., Menn, W., Mikhailov, V. V., Mocchiutti, E., Orsi, Silvio, Osteria, G., Papini, P., De Pascale, M. P., Picozza, T. P., Pearce, Mark, De Rosa, G., Ricci, M., Ricciarini, S. B., Simon, M., De Simone, N., Sparvoli, R., Spillantini, P., Stozhkov, Yu.I., Taddei, E., Felice, V., Fedele, D., Hofverberg, Petter, and Yurkin, Yu.T.
- Abstract
Secondary electron and positron fluxes in the energy range from 3 MeV to 7 GeV were measured with the ARINA and PAMELA spectrometers onboard the Resurs-DK satellite launched on June 15, 2006 into an elliptical orbit with an inclination of 70.4° and an altitude of 350-600 km. It is shown that positrons dominate over electrons by a factor of up to 4-5 in the geomagnetic equator region (L < 1.2 and B > 0.25)., QC 20141006
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- 2009
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11. Positrons and electrons in primary cosmic rays as measured in the PAMELA experiment
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Adriani, O., Bazilevskaya, G. A., Barbarino, G. C., Bellotti, R., Boezio, M., Bogomolov, E. A., Bonechi, L., Bongi, M., Bonvicini, V., Borisov, S. V., Bottai, S., Bruno, A., Cafagna, F., Campana, D., Carlson, P., Casolino, M., Castellini, G., Pascale, M. P., Rosa, G., Fedele, D., Felice, V., Galper, A. M., Grishantseva, L. A., Hofverberg, Petter, Leonov, A. A., Koldashov, S. V., Krutkov, S.Yu., Kvashnin, A. N., Malvezzi, V., Marcelli, L., Menn, W., Mikhailov, V. V., Minori, M., Mocchiutti, E., Orsi, Silvio, Osteria, G., Papini, P., Pearce, Mark, Picozza, P., Ricci, M., Ricciarini, S. B., Simon, M., Simone, N., Sparvoli, R., Spillantini, P., Stozhkov, Yu.I., Taddei, E., Vacchi, A., Vannuccini, E., Vasil'ev, G. V., Voronov, S. A., Yurkin, Yu.T., Zampa, G., Zampa, N., Zverev, V. G., Adriani, O., Bazilevskaya, G. A., Barbarino, G. C., Bellotti, R., Boezio, M., Bogomolov, E. A., Bonechi, L., Bongi, M., Bonvicini, V., Borisov, S. V., Bottai, S., Bruno, A., Cafagna, F., Campana, D., Carlson, P., Casolino, M., Castellini, G., Pascale, M. P., Rosa, G., Fedele, D., Felice, V., Galper, A. M., Grishantseva, L. A., Hofverberg, Petter, Leonov, A. A., Koldashov, S. V., Krutkov, S.Yu., Kvashnin, A. N., Malvezzi, V., Marcelli, L., Menn, W., Mikhailov, V. V., Minori, M., Mocchiutti, E., Orsi, Silvio, Osteria, G., Papini, P., Pearce, Mark, Picozza, P., Ricci, M., Ricciarini, S. B., Simon, M., Simone, N., Sparvoli, R., Spillantini, P., Stozhkov, Yu.I., Taddei, E., Vacchi, A., Vannuccini, E., Vasil'ev, G. V., Voronov, S. A., Yurkin, Yu.T., Zampa, G., Zampa, N., and Zverev, V. G.
- Abstract
The PAMELA experiment is being carried out on board the Russian satellite Resurs DK1 placed in the near-earth near-polar orbit on June 15, 2006. The apparatus comprising a silicon-strip magnetic spectrometer and an electromagnetic calorimeter allows measurement of electron and positron fluxes in cosmic rays in a wide energy interval from ∼100 MeV to hundreds of GeV. The high-energy electron and positron separation technique is discussed and the data on positron-to-electron ratio in primary cosmic rays up to E ≃ 10 GeV from the 2006 - 2007 measurements are reported in this work., QC 20141007
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- 2009
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12. Sub-cutoff electrons and positrons in the near Earth space
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Grishantseva, L. A., Adriani, O., Barbarino, G., 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., Carlson, Per, Casolino, M., Castellini, G., De Pascale, M. P., Di Felice, V., Galper, A. M., Hofverberg, Petter, Leonov, A. A., Koldashov, S. V., Krutkov, S.Yu., Kvashnin, A. N., Malakhov, V. V., Malvezzi, V., Marcelli, L., Menn, W., Mikhailov, V. V., Mocchiutti, E., Osteria, G., Papini, P., Pearce, Mark, Picozza, P., Ricci, M., Ricciarini, S., Simon, M., De Simone, N., Sparvoli, R., Spillantini, P., Stozhkov, Yu.I., Vacchi, A., Vannuccini, E., Vasiliev, G. V., Voronov, S. A., Yurkin, Yu.T., Zampa, G., Zampa, N., Zverev, V. G., Grishantseva, L. A., Adriani, O., Barbarino, G., 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., Carlson, Per, Casolino, M., Castellini, G., De Pascale, M. P., Di Felice, V., Galper, A. M., Hofverberg, Petter, Leonov, A. A., Koldashov, S. V., Krutkov, S.Yu., Kvashnin, A. N., Malakhov, V. V., Malvezzi, V., Marcelli, L., Menn, W., Mikhailov, V. V., Mocchiutti, E., Osteria, G., Papini, P., Pearce, Mark, Picozza, P., Ricci, M., Ricciarini, S., Simon, M., De Simone, N., Sparvoli, R., Spillantini, P., Stozhkov, Yu.I., Vacchi, A., Vannuccini, E., Vasiliev, G. V., Voronov, S. A., Yurkin, Yu.T., Zampa, G., Zampa, N., and Zverev, V. G.
- Abstract
Precise spectra of electron and positron fluxes in energy range from 80 MeV to several GeV below the geomagnetic cutoff rigidity were obtained using data of the PAMELA spectrometer. It was launched on June 15th 2006 onboard the Resurs-DK satellite on an elliptical orbit (the inclination is 70°, the altitude is 350-610 km). The work presents measurements of secondary lepton fluxes produced in interactions of cosmic ray protons with the atmosphere in the near Earth space (out of the South Atlantic Anomaly). Latitudinal dependences are discussed. These results are particularly interesting for more accurate definition of electron/positron flux model in the Earth magnetosphere., QC 20150421
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- 2009
13. Launch of the space experiment PAMELA
- Author
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Casolino, M., primary, Picozza, P., additional, Altamura, F., additional, Basili, A., additional, De Simone, N., additional, Di Felice, V., additional, De Pascale, M.P., additional, Marcelli, L., additional, Minori, M., additional, Nagni, M., additional, Sparvoli, R., additional, Galper, A.M., additional, Mikhailov, V.V., additional, Runtso, M.F., additional, Voronov, S.A., additional, Yurkin, Y.T., additional, Zverev, V.G., additional, Castellini, G., additional, Adriani, O., additional, Bonechi, L., additional, Bongi, M., additional, Taddei, E., additional, Vannuccini, E., additional, Fedele, D., additional, Papini, P., additional, Ricciarini, S.B., additional, Spillantini, P., additional, Ambriola, M., additional, Cafagna, F., additional, De Marzo, C., additional, Barbarino, G.C., additional, Campana, D., additional, De Rosa, G., additional, Osteria, G., additional, Russo, S., additional, Bazilevskaja, G.A., additional, Kvashnin, A.N., additional, Maksumov, O., additional, Misin, S., additional, Stozhkov, Yu.I., additional, Bogomolov, E.A., additional, Krutkov, S.Yu., additional, Nikonov, N.N., additional, Bonvicini, V., additional, Boezio, M., additional, Lundquist, J., additional, Mocchiutti, E., additional, Vacchi, A., additional, Zampa, G., additional, Zampa, N., additional, Bongiorno, L., additional, Ricci, M., additional, Carlson, P., additional, Hofverberg, P., additional, Lund, J., additional, Orsi, S., additional, Pearce, M., additional, Menn, W., additional, and Simon, M., additional
- Published
- 2008
- Full Text
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