Occurrence of Great Magnetic Storms on 6-8 March 1582
Kentaro Hattori, Hisashi Hayakawa, and Yusuke Ebihara

TL;DR
This study reconstructs a severe magnetic storm on 8 March 1582 using auroral records, revealing its duration, intensity, and possible cause, thus extending knowledge of historical space weather events before the 19th century.
Contribution
It provides the first detailed analysis of a 1582 magnetic storm based on auroral evidence, estimating its severity and duration, and proposing a series of ICMEs as the cause.
Findings
The storm was comparable in intensity to major 20th-century storms.
Auroral oval extended to low latitudes, indicating a severe storm.
The storm lasted at least three days, with auroras observed at mid- and low-latitudes.
Abstract
Although knowing the occurrence frequency of severe space weather events is important for a modern society, it is insufficiently known due to the lack of magnetic or sunspot observations, before the Carrington event in 1859 known as one of the largest events during the last two centuries. Here, we show that a severe magnetic storm occurred on 8 March 1582 based on auroral records in East Asia. The equatorward boundary of auroral visibility reached 28.8{\deg} magnetic latitude. The equatorward boundary of the auroral oval is estimated to be 33.0{\deg} invariant latitude (ILAT), which is comparable to the storms on 25/26 September 1909 (~31.6{\deg} ILAT, minimum Dst of -595 nT), 28/29 August 1859 (~36.5{\deg} ILAT), and 13/14 March 1989 (~40{\deg} ILAT, minimum Dst of -589 nT). Assuming that the equatorward boundary is a proxy for the scale of magnetic storms, we presume that the storm on…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
