玻璃空间电离辐照着色损伤动力学研究
杜继实1,2, 张涛1,2, 赵丽丽1,2, 宋力昕1,2, 胡行方1,2

Study on Dynamic of Space Ionizing Radiation Induced Coloration in Glasses
DU Ji-Shi1,2, ZHANG Tao1,2, ZHAO Li-Li1,2, SONG Li-Xin1,2, HU Xing-Fang1,2
图3 模拟的特征轨道地球磁场捕获质子a地球磁场捕获电子b在K9-HL玻璃中吸收剂量率随深度的变化曲线以及复杂函数拟合、采用SPENVIS中的CREME96模型模拟的一天中最糟糕情况下太阳耀斑质子全方位微分注量率c和最糟糕情况下太阳耀斑质子在K9-HL玻璃中吸收剂量率随作用深度的分布曲线及其复杂函数拟合d. *注: 地球磁场捕获质子是参考文献 [ 4 ] 图5中太阳活动小年数据, 地球磁场捕获电子是参考文献 [ 4 ] 图5中太阳活动大年数据
Fig. 3 Simulated absorbed dose rate distribution curves of trapped proton a, trapped electron b and their complex function fits, worst-day omnidirectional fluence rate of solar flare proton simulated by the model CREME96 of SPENVIS c and its absorbed dose rate distribution curve d. *Note: Fluence rate of trapped proton is the one of solar minimum in Fig. 5 of ref. [ 4 ] , fluence rate of trapped electron is the one of solar maximum in Fig. 5 of ref. [ 4 ]