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Measurement conditions in the space experiment MONICA

机译:空间实验MONICA中的测量条件

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The present contribution is dedicated to the investigation of the background conditions for cosmic ray ion ionization state measurements in MONICA experiment [1]. The future experiment MONICA is aimed to study the cosmic ray ion fluxes from H till Ni in energy range 10-300 MeV/n by multilayer semiconductor telescope-spectrometer installed onboard satellite. The satellite orbit parameters (circular, altitude is about 600 km, polar) were chosen for the realization of the unique method for the measurement of the charge state of the ions with energies>10 MeV/n by using the Earth magnetic field as a separator of ion charge. The analysis of the background particle fluxes is presented taking into account the recent data of the satellite experiments and known AE-8, AP-8 models and elaborated the recommendations to improve the background conditions for the MONICA experiment.
机译:目前的贡献致力于调查Monica实验中的宇宙射线离子电离状态测量的背景条件[1]。未来的实验MONICA旨在通过安装在卫星上安装的多层半导体望远镜光谱仪在10-300 mev / n中的H TLOT NI的宇宙射线离子通量。选择卫星轨道参数(圆形,高度约600公里,极性),以实现通过使用地球磁场作为分离器测量电荷的电荷状态> 10mev / n的独特方法离子电荷。考虑到卫星实验和已知AE-8,AP-8模型的最近数据,并阐述了背景粒子通量的分析,并详细阐述了改进MONICA实验的背景条件的建议。

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