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Long-lasting Extreme Magnetic Storm Activities in 1770 Found in Historical Documents

机译:1770年在历史文件中发现的长期极端磁风暴活动

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Dim red aurora at low magnetic latitudes is a visual and recognized manifestation of magnetic storms. The great low-latitude auroral displays seen throughout East Asia on 1770 September 16-18 are considered to manifest one of the greatest storms. Recently found, 111 historical documents in East Asia attest that these low-latitude auroral displays appeared in succession for almost nine nights during 1770 September 10-19 in low magnetic latitude areas (<30°). This suggests that the duration of the great magnetic storm is much longer than usual. Sunspot drawings from 1770 reveal that the sunspot areas were twice as large as those observed in another great storm of 1859, which substantiates these unusual storm activities in 1770. These spots likely ejected several huge, sequential magnetic structures in short duration into interplanetary space, resulting in spectacular worldwide aurorae in mid-September of 1770. These findings provide new insight into the history, duration, and effects of extreme magnetic storms that may be valuable for those who need to mitigate against extreme events.
机译:低磁性纬度的暗红色极光是一种视觉和认可的磁场风暴表现。在9月16日至18日在东亚看到的伟大低纬度极光展示被认为表现出最伟大的风暴之一。最近发现,东亚的111名历史文件证明了这些低纬度的极光展在1770年9月10日至19日在低磁纬度地区(<30°)中的近九个夜晚出现了近九个夜晚。这表明巨大磁风暴的持续时间远远超过平常。从1770年开始的Sunspot图纸显示,太阳黑子区域是在1859年的另一个大风暴中观察到的两倍,这将在1770年证实这些不寻常的风暴活动。这些斑点可能在短时间内喷射了几个巨大的连续的磁性结构,持续到行列间空间,导致了几个在1770年9月9月9月9月中壮观的全球极光。这些调查结果为极端磁风暴的历史,持续时间和影响提供了新的洞察力,这对于需要减轻极端事件的人可能是有价值的。

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