In-flight performance of SilEye-2 experiment and cosmic ray abundances inside the Mir space station

被引:35
作者
Bidoli, V
Casolino, M [1 ]
De Grandis, E
De Pascale, MP
Furano, G
Morselli, A
Narici, L
Picozza, P
Reali, E
Sparvoli, R
Galper, A
Khodarovich, A
Korotkov, M
Popov, A
Vavilov, N
Mazzenga, G
Ricci, M
Castellini, G
Avdeev, S
Boezio, M
Bonvicini, W
Vacchi, A
Zampa, N
Papini, P
Spillantini, P
Carlson, P
Fuglesang, C
机构
[1] Ist Nazl Fis Nucl, ROMA2, I-00185 Rome, Italy
[2] Univ Roma Tor Vergata, I-00173 Rome, Italy
[3] Moscow Engn Phys Inst, Moscow 115409, Russia
[4] Ist Nazl Fis Nucl, Lab Nazl Frascati, I-00185 Rome, Italy
[5] CNR, Ist Ric Onde Elettromagnet, I-50127 Florence, Italy
[6] Russian Space Corp Energia, Korolev, Moscow Region, Russia
[7] Univ Trieste, I-34127 Trieste, Italy
[8] Ist Nazl Fis Nucl, Sez Trieste, I-34127 Trieste, Italy
[9] Univ Florence, I-50121 Florence, Italy
[10] Ist Nazl Fis Nucl, Sez Firenze, I-50125 Florence, Italy
[11] Royal Inst Technol, S-10044 Stockholm, Sweden
[12] ESA, European Astronaut Ctr, Cologne, Germany
关键词
D O I
10.1088/0954-3899/27/10/307
中图分类号
O57 [原子核物理学、高能物理学];
学科分类号
070202 ;
摘要
Cosmic ray measurements performed with the instrument SilEye-2 on the Mir space station are presented. SilEye-2 is a silicon detector telescope used to study the causes of the light flashes perceived by astronauts. As a stand-alone device, it monitors the short- and long-term radiation composition inside Mir. The cosmic ray detector consists of an array of six active silicon strip detectors which allow nuclear identification of cosmic rays up to iron. The device was operational for more than 1000 h in the years 1998-2000, also measuring several solar particle events. In this work we present the in-flight performance of the instrument and nuclear abundance data from boron to silicon above similar or equal to 150 MeV n(-1) inside Mir.
引用
收藏
页码:2051 / 2064
页数:14
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