NUCLEAR TECHNIQUES, Volume. 47, Issue 11, 110501(2024)
Monte Carlo simulation of delayed γ-rays ionizing the atmosphere based on debris motion model
Fig. 1. The simulated shape of debris at different time (a) H=40 km, Q=100 kt, (b) H=80 km, Q=4 Mt
Fig. 2. Diagram of the delayed γ-ray source from the spheroidicity debris (a) and inverted pear-shaped debris (b)
Fig. 3. Geometry model of the transport of delayed γ-rays from single layer debris in the atmosphere
Fig. 4. Varistions of γ-fluence and energy fluence of delayed γ-rays with height
Fig. 5. Electron production rate caused by the debris in different layer after 5 min of the explosion with the equivalent of 4 Mt at the height of 80 km (a) 1st layer debris, (b) 4th layer debris, (c) 7th layer debris, (d) 10th layer debris
Fig. 6. Electron production rate caused by delayed γ-rays after 5 min (a) and 20 min (b) of the explosion with the equivalent of 4 Mt at the height of 80 km
Fig. 7. Electron production rate caused by delayed γ-rays after 5 min (a) and 20 min (b) of the explosion with the equivalent of 4 Mt at the height of 40 km
Fig. 8. Electron production rate caused by delayed γ-rays after 5 min (a) and 20 min (b) of the explosion with the equivalent of 100 kt at the height of 80 km
Fig. 9. Electron production rate caused by delayed γ-rays after 5 min (a) and 20 min (b) of the explosion with the equivalent of 100 kt at the height of 40 km
Fig. 10. Electron density caused by delayed γ-rays after 5 min (a) and 20 min (b) of the explosion with the equivalent of 4 Mt at the height of 80 km
|
Get Citation
Copy Citation Text
Li LIU, Shengli NIU, Yinghong ZUO, Jinhui ZHU, Jun ZHUO, Xiazhi LI. Monte Carlo simulation of delayed γ-rays ionizing the atmosphere based on debris motion model[J]. NUCLEAR TECHNIQUES, 2024, 47(11): 110501
Category: NUCLEAR PHYSICS, INTERDISCIPLINARY RESEARCH
Received: May. 10, 2024
Accepted: --
Published Online: Jan. 2, 2025
The Author Email: LIU Li (liuli@nint.ac.cn)