Correlability of solar wind with seismic events in the Balkan peninsula zone

F. Arnaut, D. Vučković, Ivana Vasiljević, Vesna Cvetkov
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Abstract

The Solar Heliospheric Observatory (SOHO) satellite was launched on the 2nd of December 1995 at L1 Lagrange point (1.5x106 km from Earth) with the purpose of gathering data for helioseismology, remote sensing of the solar atmosphere, and solar wind in situ. The satellite was positioned into orbit in early 1996, with data acquisition expected to commence on January 20th. The correlation between increased values of solar wind parameters and earthquakes in the Balkan peninsula zone between 1996 and 2018 was made possible by data obtained through continuous proton density and proton velocity monitoring. The assessment of the anomalous threshold was based on statistically determined parameters due to the huge fluctuation of solar wind over time and distinct value increases of proton density and speed. Visual representations of proton density and proton speed were created for the time window preceding each earthquake after defining the boundary between normal and anomalous values. According to the chart analysis, increased proton density occurred in 40 of the 50 cases observed, whereas increased proton velocity appeared in 28 of the 50 cases. Using hypergeometrical probability and an unbiased test with randomly generated parameters, the discovered correlation was statistically verified. A retrospective selection bias analysis is also provided in the research paper.
巴尔干半岛地区太阳风与地震事件的相关性
太阳日光层观测卫星(SOHO)于1995年12月2日在L1拉格朗日点(距地球1.5x106公里)发射,目的是收集日震学、太阳大气遥感和太阳风的原位数据。该卫星于1996年初进入轨道,预计将于1月20日开始数据采集。通过连续质子密度和质子速度监测获得的数据,可以获得1996年至2018年巴尔干半岛地区太阳风参数值的增加与地震之间的相关性。异常阈值的评估是基于统计确定的参数,因为太阳风随时间的波动很大,质子密度和速度的值增加明显。在确定了正常和异常值之间的界限后,为每次地震前的时间窗口创建了质子密度和质子速度的可视化表示。根据图表分析,观察到的50例病例中,质子密度增加的病例有40例,而质子速度增加的病例有28例。利用超几何概率和随机生成参数的无偏检验,对发现的相关性进行了统计验证。本文还进行了回顾性选择偏倚分析。
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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