{"title":"The effect of X-ray radiation from a solar flare on the frequencies of Schumann resonances","authors":"V.V. Surkov","doi":"10.1016/j.jastp.2025.106537","DOIUrl":null,"url":null,"abstract":"<div><div>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.</div></div>","PeriodicalId":15096,"journal":{"name":"Journal of Atmospheric and Solar-Terrestrial Physics","volume":"271 ","pages":"Article 106537"},"PeriodicalIF":1.8000,"publicationDate":"2025-05-05","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Atmospheric and Solar-Terrestrial Physics","FirstCategoryId":"89","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S136468262500121X","RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"GEOCHEMISTRY & GEOPHYSICS","Score":null,"Total":0}
引用次数: 0
Abstract
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.
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.