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Galactic Cosmic Ray Electrons and Positrons over a Decade of Observations in the PAMELA Experiment
by
Marcelli, L
, De Santis, C
, Vacchi, A
, Bogomolov, E. A
, Koldashov, S. V
, Boezio, M
, Malakhov, V. V
, Karelin, A. V
, Bazilevskaya, G. A
, Casolino, M
, Picozza, P
, Vannuccini, E
, Panico, B
, Bellotti, R
, Cafagna, F
, Mayorov, A. G
, Leonov, A. A
, Menn, W
, Merge, M
, Barbarino, G. C
, Mikhailov, V. V
, Zampa, N
, Krutkov, S. Yu
, Zampa, G
, Bongi, M
, Martucci, M
, Vasilyev, G. I
, Di Felice, V
, Koldobskiy, S. A
, Bonvicini, V
, Mocchiutti, E
, Runtso, M. F
, Carlson, P
, Campana, D
, Monaco, A
, Sparvoli, R
, Adriani, O
, Mori, N
, Ricci, M
, Stozhkov, Yu. I
, Voronov, S. A
, Kvashnin, A. A
, Papini, P
, Pearce, M
, Spillantini, P
, Kvashnin, A. N
, Ricciarini, S. B
, Galper, A. M
, Munini, R
, Bruno, A
, Yurkin, Yu. T
, Osteria, G
, Castellini, G
, Simon, M
in
Accuracy
/ Antiparticles
/ Cosmic rays
/ Electrons
/ Experiments
/ Fluxes
/ Galactic cosmic rays
/ Magnetic fields
/ Positrons
/ Propagation
/ Radiation
/ Sensors
2019
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Galactic Cosmic Ray Electrons and Positrons over a Decade of Observations in the PAMELA Experiment
by
Marcelli, L
, De Santis, C
, Vacchi, A
, Bogomolov, E. A
, Koldashov, S. V
, Boezio, M
, Malakhov, V. V
, Karelin, A. V
, Bazilevskaya, G. A
, Casolino, M
, Picozza, P
, Vannuccini, E
, Panico, B
, Bellotti, R
, Cafagna, F
, Mayorov, A. G
, Leonov, A. A
, Menn, W
, Merge, M
, Barbarino, G. C
, Mikhailov, V. V
, Zampa, N
, Krutkov, S. Yu
, Zampa, G
, Bongi, M
, Martucci, M
, Vasilyev, G. I
, Di Felice, V
, Koldobskiy, S. A
, Bonvicini, V
, Mocchiutti, E
, Runtso, M. F
, Carlson, P
, Campana, D
, Monaco, A
, Sparvoli, R
, Adriani, O
, Mori, N
, Ricci, M
, Stozhkov, Yu. I
, Voronov, S. A
, Kvashnin, A. A
, Papini, P
, Pearce, M
, Spillantini, P
, Kvashnin, A. N
, Ricciarini, S. B
, Galper, A. M
, Munini, R
, Bruno, A
, Yurkin, Yu. T
, Osteria, G
, Castellini, G
, Simon, M
in
Accuracy
/ Antiparticles
/ Cosmic rays
/ Electrons
/ Experiments
/ Fluxes
/ Galactic cosmic rays
/ Magnetic fields
/ Positrons
/ Propagation
/ Radiation
/ Sensors
2019
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Galactic Cosmic Ray Electrons and Positrons over a Decade of Observations in the PAMELA Experiment
by
Marcelli, L
, De Santis, C
, Vacchi, A
, Bogomolov, E. A
, Koldashov, S. V
, Boezio, M
, Malakhov, V. V
, Karelin, A. V
, Bazilevskaya, G. A
, Casolino, M
, Picozza, P
, Vannuccini, E
, Panico, B
, Bellotti, R
, Cafagna, F
, Mayorov, A. G
, Leonov, A. A
, Menn, W
, Merge, M
, Barbarino, G. C
, Mikhailov, V. V
, Zampa, N
, Krutkov, S. Yu
, Zampa, G
, Bongi, M
, Martucci, M
, Vasilyev, G. I
, Di Felice, V
, Koldobskiy, S. A
, Bonvicini, V
, Mocchiutti, E
, Runtso, M. F
, Carlson, P
, Campana, D
, Monaco, A
, Sparvoli, R
, Adriani, O
, Mori, N
, Ricci, M
, Stozhkov, Yu. I
, Voronov, S. A
, Kvashnin, A. A
, Papini, P
, Pearce, M
, Spillantini, P
, Kvashnin, A. N
, Ricciarini, S. B
, Galper, A. M
, Munini, R
, Bruno, A
, Yurkin, Yu. T
, Osteria, G
, Castellini, G
, Simon, M
in
Accuracy
/ Antiparticles
/ Cosmic rays
/ Electrons
/ Experiments
/ Fluxes
/ Galactic cosmic rays
/ Magnetic fields
/ Positrons
/ Propagation
/ Radiation
/ Sensors
2019
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Galactic Cosmic Ray Electrons and Positrons over a Decade of Observations in the PAMELA Experiment
Journal Article
Galactic Cosmic Ray Electrons and Positrons over a Decade of Observations in the PAMELA Experiment
2019
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Overview
AbstractThe PAMELA magnetic spectrometer was launched onboard the Resurs-DK1 satellite into a near-polar Earth orbit with an altitude of 350–600 km, in order to study fluxes of cosmic ray particles and antiparticles in the wide energy range of ~80 MeV to hundreds of GeV. The results from observations of electron and positron fluxes in 2006–2016 are presented.
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