Acta Physica Sinica, Volume. 69, Issue 15, 150701-1(2020)
Fig. 2. Incident energy spectrum of the space radiation environment in the orbit of eXTP.
Fig. 4. Mass model of simplified aluminum spherical shell and SDD.
Fig. 7. Planar density distribution at the position of SDD (left: frontview; right: backview).
Fig. 8. Particle background evolution as a function of the size and the thickness of the aluminum spherical shell.
Fig. 9. Fitting curves of different particle backgrounds as a function of the thickness of the aluminum spherical shell.
Fig. 10. Total particle background evolution as a function of the thickness of the aluminum spherical shell .
Fig. 11. Equivalent aluminum thickness distribution of the whole eXTP at the SDD position.
Fig. 12. Comparison of particle background level obtained with interpolation of planar density distribution and with simulation.
Fig. 13. Structure of the mass model before and after structure modifications (left: before modifications; right: after modifications).
Fig. 14. Equivalent aluminum thickness distribution after the structure modifications.
Fig. 15. Comparison of the particle background levels after the structure modifications, from the interpolation of planar density distribution and the simulation, respectively.
Fig. 16. Variation of the secondary positron composition as a function of the shielding thickness.
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Wen-Li Jiang, Li-Qiang Qi, Da-Wei Han, Ze-Yu Song, Ai-Mei Zhang, Wei Li, Yu-Peng Xu, Yong Chen, Chun-Lei Zhang, Yao-Feng Zhang, Gang Li.
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Received: Apr. 19, 2020
Accepted: --
Published Online: Dec. 30, 2020
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