Measurement of hydrogen and helium isotopes flux in galactic cosmic rays with the PAMELA experiment

被引：4

作者：

Formato, V. ^{[8
,16
]}

Adriani, O. ^{[1
,2
]}

Barbarino, G. C. ^{[3
,4
]}

Bazilevskaya, G. A. ^{[5
]}

Bellotti, R. ^{[6
,7
]}

Boezio, M. ^{[8
]}

Bogomolov, E. A. ^{[9
]}

Bongi, M. ^{[1
,2
]}

Bonvicini, V. ^{[8
]}

Bottai, S. ^{[2
]}

Bruno, A. ^{[7
]}

Cafagna, F. ^{[7
]}

Campana, D. ^{[4
]}

Carbone, R. ^{[8
]}

Carlson, P. ^{[10
,11
]}

Casolino, M. ^{[12
,13
]}

Castellini, G. ^{[14
]}

De Donato, C. ^{[10
,11
,12
]}

De Pascale, M. P. ^{[12
,15
]}

De Santis, C. ^{[12
,15
]}

De Simone, N. ^{[12
]}

Di Felice, V. ^{[12
]}

Galper, A. M. ^{[17
]}

Karelin, A. V. ^{[17
]}

Koldashov, S. V. ^{[17
]}

Koldobskiy, S. ^{[17
]}

Krutkov, Y. ^{[9
]}

Kvashnin, A. N. ^{[5
]}

Leonov, A. ^{[17
]}

Malakhov, V. ^{[17
]}

Marcelli, L. ^{[15
]}

Martucci, M. ^{[15
,18
]}

Mayorov, A. G. ^{[17
]}

Menn, W. ^{[19
]}

Merge, M. ^{[12
,15
]}

Mikhailov, V. V. ^{[17
]}

Mocchiutti, E. ^{[8
]}

Monaco, A. ^{[7
]}

Mori, N. ^{[2
]}

Munini, R. ^{[8
,16
]}

Osteria, G. ^{[4
]}

Palma, F. ^{[12
,15
]}

Papini, P. ^{[2
]}

Pearce, M. ^{[10
,11
]}

Picozza, P. ^{[12
,15
]}

Pizzolotto, C. ^{[8
,20
,21
]}

Ricci, M. ^{[18
]}

Ricciarini, S. B. ^{[2
]}

Sarkar, R. ^{[8
]}

Simon, M. ^{[19
]}

机构：

[1] Univ Florence, Dept Phys, I-50019 Florence, Italy

[2] Ist Nazl Fis Nucl, Sez Florence, I-50019 Florence, Italy

[3] Univ Naples Federico II, Dept Phys, I-80126 Naples, Italy

[4] Ist Nazl Fis Nucl, Sez Naples, I-80126 Naples, Italy

[5] PN Lebedev Phys Inst, RU-119991 Moscow, Russia

[6] Univ Bari, Dept Phys, I-70126 Bari, Italy

[7] Ist Nazl Fis Nucl, Sez Bari, I-70126 Bari, Italy

[8] Ist Nazl Fis Nucl, Sez Trieste, I-34149 Trieste, Italy

[9] AF Ioffe Phys Tech Inst, RU-194021 St Petersburg, Russia

[10] KTH, Dept Phys, AlbaNova Univ Ctr, SE-10691 Stockholm, Sweden

[11] Oskar Klein Ctr Cosmoparticle Phys, Stockholm, Sweden

[12] Ist Nazl Fis Nucl, Sez Rome Tor Vergata, I-00133 Rome, Italy

[13] RIKEN, Adv Sci Inst, Wako, Saitama, Japan

[14] IFAC, I-50019 Florence, Italy

[15] Univ Roma Tor Vergata, Dept Phys, I-00133 Rome, Italy

[16] Univ Trieste, Dept Phys, I-34147 Trieste, Italy

[17] NRNU MEPhl, RU-115409 Moscow, Russia

[18] Ist Nazl Fis Nucl, Lab Nazl Frascati, I-00044 Frascati, Italy

[19] Univ Siegen, Dept Phys, D-57068 Siegen, Germany

[20] Ist Nazl Fis Nucl, Sez Perugia, I-06123 Perugia, Italy

[21] Agenzia Spaziale Italiana ASI Sci Data Ctr, I-00044 Frascati, Italy

来源：

NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT | 2014年 / 742卷

关键词：

PAMELA; Isotopes; Cosmic ray propagation; LIGHT-NUCLEI; SPECTRA; PROTON; RATIO; FIELD;

D O I：

10.1016/j.nima.2013.11.004

中图分类号：

TH7 [仪器、仪表];

学科分类号：

0804 ; 080401 ; 081102 ;

摘要：

PAMELA is a satellite borne experiment designed to study with great accuracy cosmic rays of galactic, solar, and trapped nature, with particular focus on the antimatter component. The detector consists of a permanent magnet spectrometer core to provide rigidity and charge sign information, a Time-of-Flight system for velocity and charge information, a Silicon-Tungsten calorimeter and a Neutron detector for lepton/hadron identification. The velocity and rigidity information allow the identification of different isotopes for Z = 1 and Z = 2 particles in the energy range 100 MeV/n to 1 GeV/n. In this work we will present the PAMELA results on the H and He isotope fluxes based on the data collected during the 23rd solar minimum from 2006 to 2007. Such fluxes carry relevant information helpful in constraining parameters in galactic cosmic rays propagation models complementary to those obtained from other secondary to primary measurements such as the boron-to-carbon ratio. (C) 2013 Elsevier B.V. All rights reserved.

引用

页码：273 / 275

页数：3

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