Calliope 60Co gamma irradiation facility for space qualification at ENEA-casaccia research centre (Rome)

A. Cemmi, S. Baccaro, I. D. Sarcina
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引用次数: 5

Abstract

Optical and electronic components used on spacecrafts and satellites are exposed to a large variety of environments, often rich in high fluxes of energetic particles, which may cause serious degradation and damaging effects.1–5 The Space experiment radiation environment is characterized by several kind of primary particles. The main sources of Space radiation are galactic cosmic rays, energetic electrons and protons, trapped in the Van Allen Belts, and particles associated to the solar activity (electron, protons and heavy ions). Cosmic rays are charged particles (protons, electrons and heavy ions) whose flux (10-28-103 m-2 sr-1 s-1 GeV-1) and particle energy (from tens to 1014 MeV) vary depending on their solar, galactic and extra galactic origin.6–8 The galactic cosmic rays flux strongly depends on the solar activity: it is low when the solar activity is high because the solar wind does not allow particles to easily enter the solar system. The charged particles of galactic cosmic rays are also influenced by the Earth magnetic field which provides a partial radiation shielding for spacecraft. However, cosmic rays, as well as solar emitted particles, have free access over the polar regions where the magnetic field lines are open to interplanetary Space: the result is that the galactic cosmic ray fluxes are higher at the Poles and lower at the equator.9 The Van Allen belts mainly consist of MeV protons and keV electrons trapped in the Earth magnetic field, with a toroid spatial distribution around the Earth.10 Trapped electrons are positioned in two regions: the former extends to about 2.4 Earth radii and contain electrons with energy lower than 5 MeV while the latter, the outer, goes from about 2.8 to 12 radii and include electrons with energy up to 7 MeV. Finally, the Sun is the source of different kinds of particles such as those produced by the solar wind coming from upper atmosphere of the Sun, and by the solar flares and the coronal mass ejection processes, sporadically occurring.9,11,12
欧洲空间局casaccia研究中心用于空间鉴定的Calliope 60Co伽马辐照设施(罗马)
航天器和卫星上使用的光学和电子部件暴露在各种各样的环境中,这些环境往往富含高通量的高能粒子,可能造成严重退化和破坏性影响。1-5空间实验辐射环境具有几种主要粒子的特征。空间辐射的主要来源是银河宇宙射线、被困在范艾伦带中的高能电子和质子,以及与太阳活动有关的粒子(电子、质子和重离子)。宇宙射线是带电粒子(质子、电子和重离子),其通量(10-28-103 m-2 sr-1 s-1 GeV-1)和粒子能量(从几十兆电子伏到1014兆电子伏)根据其太阳、银河系和银河系外的起源而变化。银河宇宙射线的通量很大程度上取决于太阳活动:当太阳活动高的时候,它是低的,因为太阳风不允许粒子轻易进入太阳系。银河系宇宙射线的带电粒子也受到地球磁场的影响,地球磁场为航天器提供了部分的辐射屏蔽。然而,宇宙射线以及太阳发射的粒子可以自由进入磁力线对行星际空间开放的极地地区:结果是,银河系宇宙射线通量在两极较高,在赤道较低范艾伦带主要由被困在地球磁场中的MeV质子和keV电子组成,在地球周围呈环形空间分布。10被困电子位于两个区域:前者延伸到约2.4个地球半径,包含能量低于5 MeV的电子,后者位于外层,从约2.8到12个半径,包括能量高达7 MeV的电子。最后,太阳是各种粒子的来源,如来自太阳上层大气的太阳风,以及偶尔发生的太阳耀斑和日冕物质抛射过程产生的粒子
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