A MONTE CARLO SIMULATION OF SOLAR X-RAY TRANSPORTION IN EARTH'S ATMOSPHERE

Zong Qiu-gang; Ye Zong-hai

doi:10.11728/cjss1994.01.063

Volume 14 Issue 1

Jan. 1994

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Article Navigation > Chinese Journal of Space Science > 1994 > 14(1): 63-69

Zong Qiu-gang, Ye Zong-hai. A MONTE CARLO SIMULATION OF SOLAR X-RAY TRANSPORTION IN EARTH'S ATMOSPHERE[J]. Chinese Journal of Space Science, 1994, 14(1): 63-69. doi: 10.11728/cjss1994.01.063

Citation:

Zong Qiu-gang, Ye Zong-hai. A MONTE CARLO SIMULATION OF SOLAR X-RAY TRANSPORTION IN EARTH'S ATMOSPHERE[J]. Chinese Journal of Space Science, 1994, 14(1): 63-69. doi: 10.11728/cjss1994.01.063

Zong Qiu-gang, Ye Zong-hai. A MONTE CARLO SIMULATION OF SOLAR X-RAY TRANSPORTION IN EARTH'S ATMOSPHERE[J]. Chinese Journal of Space Science, 1994, 14(1): 63-69. doi: 10.11728/cjss1994.01.063

Citation:

Zong Qiu-gang, Ye Zong-hai. A MONTE CARLO SIMULATION OF SOLAR X-RAY TRANSPORTION IN EARTH'S ATMOSPHERE[J]. Chinese Journal of Space Science, 1994, 14(1): 63-69. doi: 10.11728/cjss1994.01.063

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A MONTE CARLO SIMULATION OF SOLAR X-RAY TRANSPORTION IN EARTH'S ATMOSPHERE

doi: 10.11728/cjss1994.01.063 cstr: 32142.14.cjss1994.01.063

Center for Space Science and Applied Research, Academia Sinica, Beijing 100080

Received Date: 1992-09-19
Rev Recd Date: 1900-01-01
Publish Date: 1994-01-24

Abstract

Abstract

The Monte Carlo method is applied to simulate solar X-ray bursts (1-8 Å, 0.5-4 Å) 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. Aexample result of solar X-ray bursts is compared with the value of Riometer absorption observed in antarctic Zhong-Shan station, showing very good correlation.
- Solar X-ray bursts,
- Monte Carlo method,
- Electron production rate,
- Riometer absorption