在地面观测到的太阳周期中最强的地磁风暴

C. Navia, Marcel N. de Oliveira, C. Augusto
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引用次数: 4

摘要

我们报告了两个不同起源的地磁风暴的地面观测;它们是太阳周期24中最强的地磁风暴之一。第一次是2015年3月17日的圣帕特里克日风暴,起源于日冕物质抛射(cme)对地球大气层的影响,风暴在NOAA地磁尺度中达到G4(严重)级。第二次包括2015年10月7日发生的大型地磁风暴,其起源归因于一个高速流(HSS)在一个正极性日冕洞之前与地球的相互作用。这次风暴达到了G3(强)级别。我们重点介绍了位于巴西海平面(22.53 (cid:1) S, 43.13 (cid:1) W)的New-Tupi μ子望远镜的观测结果。我们将这些观测结果与拉格朗日L1点的ACE和地球静止GOES气象卫星等多点天基观测结果的相关性进行了研究,包括两个全球地磁指数和几个地面探测器。本文报道了这些地磁风暴对地球天气影响的一些考虑。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
The Highest Geomagnetic Storms of the Solar Cycle Observed at Ground Level
We report two ground-level observations, of geomagnetic storms of different origins; they are among the highest geomagnetic storms, in the solar Cycle 24. The first is St. Patrick ’ s Day storm on March 17, 2015, originated by the impact on Earth ’ s atmosphere of coronal mass ejections (CMEs), the storm reaching the condition of G4 (severe) level, in the NOAA geomagnetic scale. The second included the major geomagnetic storm whose origin is attributed to the interaction with the Earth of a High-Speed Stream (HSS) ahead of a positive polarity coronal hole on October 7, 2015. This storm reached the condition G3 (strong) level. We give emphasis to observations detected by the New-Tupi muon tele- scopes, located at sea level in Brazil (22.53 (cid:1) S, 43.13 (cid:1) W). We present a study of these observations in correlation with observations reported by multipoint space-based mea- surements, such as the ACE at Lagrange Point L1 and the geostationary GOES weather satellite, including two global geomagnetic indices and several ground-based detectors. Some considerations on the influence of these geomagnetic storms in the Earth weather are reported.
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