A comparative analysis of solar and geomagnetic activity during different phases of solar cycles 24 and 25

IF 2.1 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS
S. Abila, R. P. Jebin, A. Iren Sobia, M. S. Dhaiya
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引用次数: 0

Abstract

Using hourly data from the OMNIWeb database, we analyze key indices like F10.7 (solar radio flux), Ap, Kp, Dst, and PC (geomagnetic indices) for a few chosen months that represent the solar cycle’s various phases: solar minimum (October 2009), rising phases (August 2010 and December 2022), solar maximum (May 2012), and declining phase (September 2017). Each phase’s unique geomagnetic activity patterns are revealed by our analysis. Only slight disruptions were seen in the solar and geomagnetic activity during the solar minimum. During the rising phase, we saw a steady rise in solar activity, a significant geomagnetic storm in December 2022, and associated improvements in geomagnetic indices. Geomagnetic disruptions were frequent and severe during the solar maximum phase, which was marked by intense and extremely variable solar activity. Moderate geomagnetic activity was detected throughout the falling phase, most likely due to corotating high-speed solar wind streams. This study indicates the statistical analysis of solar parameters like F10.7 index, PC index, AP index, Dst index, KP index.

太阳活动周期24和25不同阶段太阳和地磁活动的比较分析
利用OMNIWeb数据库的每小时数据,我们分析了几个月的关键指标,如F10.7(太阳射电通量)、Ap、Kp、Dst和PC(地磁指数),这些指标代表了太阳周期的各个阶段:太阳极小期(2009年10月)、上升期(2010年8月和2022年12月)、太阳极大期(2012年5月)和下降期(2017年9月)。我们的分析揭示了每个阶段独特的地磁活动模式。在太阳活动极小期,太阳和地磁活动只有轻微的中断。在上升阶段,我们看到太阳活动稳步增加,2022年12月出现了一次显著的地磁风暴,地磁指数也随之改善。在太阳活动极大期,地磁干扰频繁且严重,其特征是太阳活动剧烈且极不稳定。在整个下降阶段检测到适度的地磁活动,很可能是由于高速旋转的太阳风流。本研究对F10.7指数、PC指数、AP指数、Dst指数、KP指数等太阳参数进行统计分析。
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来源期刊
Astrophysics and Space Science
Astrophysics and Space Science 地学天文-天文与天体物理
CiteScore
3.40
自引率
5.30%
发文量
106
审稿时长
2-4 weeks
期刊介绍: Astrophysics and Space Science publishes original contributions and invited reviews covering the entire range of astronomy, astrophysics, astrophysical cosmology, planetary and space science and the astrophysical aspects of astrobiology. This includes both observational and theoretical research, the techniques of astronomical instrumentation and data analysis and astronomical space instrumentation. We particularly welcome papers in the general fields of high-energy astrophysics, astrophysical and astrochemical studies of the interstellar medium including star formation, planetary astrophysics, the formation and evolution of galaxies and the evolution of large scale structure in the Universe. Papers in mathematical physics or in general relativity which do not establish clear astrophysical applications will no longer be considered. The journal also publishes topically selected special issues in research fields of particular scientific interest. These consist of both invited reviews and original research papers. Conference proceedings will not be considered. All papers published in the journal are subject to thorough and strict peer-reviewing. Astrophysics and Space Science features short publication times after acceptance and colour printing free of charge.
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