太阳耀斑的x射线辐射对舒曼共振频率的影响

IF 1.8 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS
V.V. Surkov
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引用次数: 0

摘要

本文建立了太阳耀斑x射线辐射对地球电离层和地球电离层波导舒曼共振频率影响的理论模型。考虑入射到地球上的x射线光子的平坦瞬态通量。通过假设光子能量的吸收系数取决于其能量和空气密度,得到了x射线辐射作用下的空气电离率是海拔高度的函数。电子和离子数量密度的变化由一组微分方程来描述,这些方程考虑了粒子的产生和重组的速度,以及电子与中性分子的附着。所有反应常数的高度分布,以及电子和离子的迁移率,用表格数据近似。这些方程的解被用来计算由太阳耀斑产生的x射线引起的电离层电导率的变化。以x6.9级太阳耀斑对电离层的影响为例进行了研究,但模型参数的变化可能会影响模拟结果。电导率的变化影响低频电磁场进入导电电离层的穿透深度,导致舒曼共振频率略有增加。该理论解释了x射线辐射强度与舒曼共振加权平均频率变化之间的关系,这是在许多不同类型的太阳耀斑中观察到的。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
The effect of X-ray radiation from a solar flare on the frequencies of Schumann resonances
In this paper, a theoretical model of the effect of X-ray radiation from a solar flare on the Earth's ionosphere and on the Schumann resonance frequencies in the Earth-ionosphere waveguide has been constructed. A flat transient flux of X-ray photons incident on the Earth is considered. By making the assumption that the absorption coefficient of photon energy depends on their energy and air density, the air ionization rate under the action of X-ray radiation is found as a function of altitude. Changes in the number densities of electrons and ions are described by a set of differential equations, which take into account the rate of production and recombination of particles, as well as the attachment of electrons to neutral molecules. The altitude profiles of all reaction constants, as well as the mobility of electrons and ions, are approximated using tabular data. The solution of these equations is used to calculate changes in ionospheric conductivity caused by X-rays from a solar flare. A case study of X6.9-class solar flare effect on the ionosphere is being studied, although the variability of model parameters could affect the simulation results. The changes in conductivity influence on the penetration depth of the low-frequency electromagnetic field into the conducting ionosphere, which results in a slight increase in the frequencies of the Schumann resonances. The theory explains the relationship between the intensity of X-ray radiation and the change in the weighted average frequency of Schumann resonances, which was observed for a number of solar flares of various classes.
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来源期刊
Journal of Atmospheric and Solar-Terrestrial Physics
Journal of Atmospheric and Solar-Terrestrial Physics 地学-地球化学与地球物理
CiteScore
4.10
自引率
5.30%
发文量
95
审稿时长
6 months
期刊介绍: The Journal of Atmospheric and Solar-Terrestrial Physics (JASTP) is an international journal concerned with the inter-disciplinary science of the Earth''s atmospheric and space environment, especially the highly varied and highly variable physical phenomena that occur in this natural laboratory and the processes that couple them. The journal covers the physical processes operating in the troposphere, stratosphere, mesosphere, thermosphere, ionosphere, magnetosphere, the Sun, interplanetary medium, and heliosphere. Phenomena occurring in other "spheres", solar influences on climate, and supporting laboratory measurements are also considered. The journal deals especially with the coupling between the different regions. Solar flares, coronal mass ejections, and other energetic events on the Sun create interesting and important perturbations in the near-Earth space environment. The physics of such "space weather" is central to the Journal of Atmospheric and Solar-Terrestrial Physics and the journal welcomes papers that lead in the direction of a predictive understanding of the coupled system. Regarding the upper atmosphere, the subjects of aeronomy, geomagnetism and geoelectricity, auroral phenomena, radio wave propagation, and plasma instabilities, are examples within the broad field of solar-terrestrial physics which emphasise the energy exchange between the solar wind, the magnetospheric and ionospheric plasmas, and the neutral gas. In the lower atmosphere, topics covered range from mesoscale to global scale dynamics, to atmospheric electricity, lightning and its effects, and to anthropogenic changes.
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