基于南北半球电离层观测站数据的 foF2 与太阳活动指数的关系

IF 0.7 4区 地球科学 Q4 GEOCHEMISTRY & GEOPHYSICS Geomagnetism and Aeronomy Pub Date : 2024-04-26 DOI:10.1134/S0016793223601035
A. D. Danilov, N. A. Berbeneva
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引用次数: 0

摘要

摘要 继续分析 F2 层临界频率对太阳活动指数的依赖关系,这一分析早先是根据 Juliusruh 站的数据开始的。本文分析了北半球六个台站和南半球五个台站的数据。在每种特定情况下(观测站、月份、当地时间),foF2 与太阳活动相关性的确定系数 R2 被用来衡量这种相关性的质量。四种太阳活动代用指标的 R2 在冬季都有明显的昼夜变化,这一结论得到了证实:这一数值在白天最大且变化微弱,但到了夜间则大幅下降。研究发现,F30 代用指标是描述太阳周期中 foF2 行为的最佳太阳代用指标,而太阳黑子数 Rz 则最差。通过比较南北半球观测站同一月份 R2 与 LT 的变化,发现上述 R2 明显的昼夜变化只出现在冬季,夏季则没有。
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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Dependence of foF2 on Solar Activity Indices Based on the Data of Ionospheric Stations of the Northern and Southern Hemispheres

An analysis of the dependence of the F2-layer critical frequency on solar activity indices that has been started earlier based on the Juliusruh station data is continued. The data of six stations in the Northern Hemisphere and five stations in the Southern Hemisphere are analyzed in this paper. The determination coefficient R2 for the foF2 dependence on solar activity in each particular situation (station, month, local time) is taken as a measure of the quality of that dependence. The conclusion that a well-pronounced diurnal variation in R2 is observed in the winter months is confirmed for four solar activity proxies: this value is maximum and changes weakly in the daytime but decreases substantially to the nighttime hours. It is found that the F30 proxy is the best solar proxy to describe the foF2 behavior in the solar cycle, whereas the sunspot number Rz is the worst. Based on a comparison of the changes in R2 with LT in the same months at stations of the Northern and Southern hemispheres, it is shown that the aforementioned well-pronounced diurnal behavior in R2 is observed only in winter and is absent in summer.

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来源期刊
Geomagnetism and Aeronomy
Geomagnetism and Aeronomy Earth and Planetary Sciences-Space and Planetary Science
CiteScore
1.30
自引率
33.30%
发文量
65
审稿时长
4-8 weeks
期刊介绍: Geomagnetism and Aeronomy is a bimonthly periodical that covers the fields of interplanetary space; geoeffective solar events; the magnetosphere; the ionosphere; the upper and middle atmosphere; the action of solar variability and activity on atmospheric parameters and climate; the main magnetic field and its secular variations, excursion, and inversion; and other related topics.
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