The space experiment PAMELA

被引：26

作者：

Boezio, M ^{[1
]}

Bonvicini, V

Mocchiutti, E

Schiavon, P

Vacchi, A

Zampa, G

Zampa, N

Bakaldin, A

Galper, AM

Koldashov, SV

Korotkov, MG

Mikhailov, VV

Voronov, SA

Yurkin, Y

Basili, A

Bencardino, R

Bongiorno, L

Casolino, M

De Pascale, MP

Furano, G

Menicucci, A

Minori, M

Morselli, A

Picozza, P

Sparvoli, R

Wischnewski, R

Adriani, O

Bonechi, L

Bongi, M

Giambi, F

Papini, P

Ricciarini, SB

Spillantini, P

Straulino, S

Taccetti, F

Vannuccini, E

Castellini, G

Carlson, P

Lund, J

Lundquist, J

Orsi, S

Pearce, M

Barbarino, GC

Campana, D

Osteria, G

Rossi, G

Russo, S

Boscherini, M

Menn, W

Simon, M

机构：

[1] Univ Trieste, Ist Nazl Fis Nucl, Trieste, Italy

[2] Univ Trieste, Dept Phys, Trieste, Italy

[3] Moscow Engn & Phys Inst, Moscow, Russia

[4] Univ Roma Tor Vergata, Ist Nazl Fis Nucl, Rome, Italy

[5] Univ Roma Tor Vergata, Dept Phys, Rome, Italy

[6] Univ Florence, Dept Phys, Florence, Italy

[7] Univ Florence, Ist Nazl Fis Nucl, Florence, Italy

[8] Royal Inst Technol, KTH, Stockholm, Sweden

[9] Univ Naples Federico II, Dept Phys, Naples, Italy

[10] Univ Naples Federico II, Ist Nazl Fis Nucl, Naples, Italy

[11] Univ Siegen, D-5900 Siegen, Germany

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

[13] Univ Bari, Dept Phys, Bari, Italy

[14] Univ Bari, Ist Nazl Fis Nucl, Bari, Italy

[15] AF Ioffe Phys Tech Inst, St Petersburg, Russia

[16] PN Lebedev Phys Inst, Moscow 117924, Russia

[17] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA

[18] New Mexico State Univ, Las Cruces, NM 88003 USA

来源：

NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS | 2004年 / 134卷

关键词：

D O I：

10.1016/j.nuclphysbps.2004.08.006

中图分类号：

O412 [相对论、场论]; O572.2 [粒子物理学];

学科分类号：

摘要：

We present in this paper a status report of the space experiment PAMELA. PAMELA is a satellite-borne experiment which primarily aims to measure the antiproton and positron spectra in the cosmic radiation over a large energy range (from 80 MeV up to 190 GeV for antiprotons and from 50 MeV up to 270 GeV for positrons) and to search for antinuclei with a sensitivity of the order of 10(-8) in the antihelium/ helium ratio. In addition, it will measure the light nucleax component of cosmic rays and investigate phenomena connected with Solar and Earth physics. The apparatus will be installed onboard the polar orbiting Resurs DK1 satellite, which will be launched into space by a Soyuz TM2 rocket in 2004 from Baikonur cosmodrome in Kazakhstan, for a 3 year long mission. PAMELA consists of: a time of flight system, a transition radiation detector, a magnetic spectrometer, an anticoincidence detector, an electromagnetic imaging calorimeter, a shower tail catcher scintillator and a neutron detector.

引用

页码：39 / 46

页数：8

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