Monte Carlo Simulation for the Source of Transient Energetic Radiation Generated by Thunderstorm Activity

T. Torii, T. Sugita, M. Kamogawa
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引用次数: 1

Abstract

. Intensive and transient energetic radiations associated with winter thunderstorm activities were detected around the west coast of Sea of Japan. We identified the source location of the transient energetic radiation, lasting for several minutes, through the observations of radiation, atmospheric electric field, and meteorological radar echoes. Our identification indicated that the transient energetic radiation was emitted from a downward hemispherical surface with regardless of lightning discharge, the bottom of which was about 300 m above sea level. This may occurs due to the generation of bremsstrahlung photons caused by electric fields inside the thunderstorm, because the energy of the observed radiation exceeds that of the radiation emitted from natural nuclides. In order to verify this speculation, we calculate the behavior of secondary cosmic ray electrons and photons in intensive electric fields by Monte Carlo technique. The photon flux largely increases just under the thundercloud if we assume that the electric field around the downward hemispherical surface is - 400 kV/m, and the photon energy spectrum shows a large increase in the energy region of several MeV. When the calculated energy spectrum emitted from the thunderstorm is consistent with the observed results, the large electric field around - 400 kV/m is required around the bottom of the thundercloud.
雷暴活动产生的瞬态高能辐射源的蒙特卡罗模拟
。在日本海西海岸附近探测到与冬季雷暴活动有关的强而短暂的高能辐射。通过对辐射、大气电场和气象雷达回波的观测,确定了持续数分钟的瞬态高能辐射源位置。结果表明,瞬态高能辐射是由一个向下的半球表面发射的,而不考虑闪电放电,其底部大约在海拔300 m以上。这可能是由于雷暴内部电场引起轫致辐射光子的产生,因为观测到的辐射能量超过了天然核素发出的辐射能量。为了验证这一推测,我们用蒙特卡罗技术计算了二次宇宙射线电子和光子在强电场中的行为。假设下半球面周围电场为- 400 kV/m时,雷雨云下的光子通量大幅增加,光子能谱在几个MeV的能量区有较大的增加。当计算的雷暴发射能谱与观测结果一致时,雷云底部周围需要- 400 kV/m左右的大电场。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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