Hysteresis effect between geomagnetic activity indices (Ap, Dst) and interplanetary medium

Pub Date : 2023-09-30 DOI:10.12737/stp-93202308
Nadezhda Kurazhkovskaya, Alexander Kurazhkovskii
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Abstract

We have studied the relationship of geomagnetic activity indices (Ap, Dst) on time intervals, equal to solar cycles (∼11 years), with solar activity indicators and heliospheric parameters. It is shown that the plots of the Ap and Dst indices versus solar activity indicators, as well as versus heliospheric parameters, i.e. solar wind and IMF parameters in the ascending and descending phases of solar activity cycles 21–24 do not coincide, which is indicative of the hysteresis phenomenon. The Ap and Dst indices form hysteresis loops with all parameters we analyze during cycles 21–24. The shape and area of the hysteresis loops, as well as the direction of rotation, clockwise or counterclockwise, depend significantly on indicators of solar activity, heliospheric parameters and change from cycle to cycle. We have found a tendency for the extension and area of the hysteresis loops to decrease from cycle 21 to cycle 24. Analysis of the variability in the shape and size of the hysteresis loops formed by the Ap and Dst indices with solar indicators and heliospheric parameters gives reason to believe that the obtained loops reflect the long-term evolution of the solar wind energy flux, which determines global geomagnetic activity and the magnetospheric ring current intensity in the ascending and descending phases of solar activity cycles 21‒24.
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地磁活动指数(Ap、Dst)与行星际介质之间的磁滞效应
我们研究了地磁活动指数(Ap, Dst)在相当于太阳周期(~ 11年)的时间间隔上与太阳活动指标和日球层参数的关系。结果表明,在太阳活动周期21-24的上升和下降阶段,Ap指数和Dst指数与太阳活动指标以及太阳风和IMF参数的曲线并不重合,说明存在滞后现象。Ap和Dst指标在21-24周期内形成具有我们分析的所有参数的滞回回路。磁滞环的形状和面积以及旋转方向(顺时针还是逆时针)在很大程度上取决于太阳活动指标、日球层参数以及周期变化。我们发现,从第21周期到第24周期,磁滞回线的延伸和面积有减小的趋势。分析Ap和Dst指数与太阳指标和日球圈参数形成的磁滞回线形状和大小的变化,可以认为所得到的磁滞回线反映了太阳风能量通量的长期演变,而太阳风能量通量决定了全球地磁活动和太阳活动周期21-24上升和下降阶段的磁层环电流强度。
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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