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太阳X射线暴在地球大气中传输的Monte Carlo模拟
A MONTE CARLO SIMULATION OF SOLAR X-RAY TRANSPORTION IN EARTH’S ATMOSPHERE
【摘要】 应用MonteCarlo方法对太阳X射线暴(1—8A及0.5—4A)与地球大气相互作用过程进行跟踪模拟,得到了X射线暴在电离层D层产生的电子产生率,并计算了由此产生的宇宙噪声吸收值.结果与作者在南极观测得到的X射线暴期间宇宙噪声吸收值符合较好
【Abstract】 The Monte Carlo method is applied to simulate solar X-ray bursts (1-8 A, 0.5-4 A) transportation in earth’s atmosphere. And the electron production rate due to solar X-ray bursts penetrating in ionospheric D-layer is calculated. From that, we can get the value of cosmic noise absorption. A example result of solar X-ray bursts is compared with the value of Riometer absorption observed in antarctic Zhong-Shan station, showing very good correlation.
【关键词】 太阳X射线暴;
MonteCarlo方法;
Riometer吸收;
电子产生率;
【Key words】 Solar X-ray bursts; Monte Carlo method; Electron production rate; Riometer absorption;
【Key words】 Solar X-ray bursts; Monte Carlo method; Electron production rate; Riometer absorption;
- 【文献出处】 空间科学学报 ,CHINESE JOURNAL OF SPACE SCIENCE , 编辑部邮箱 ,1994年01期
- 【分类号】P183.4
- 【下载频次】59