Researchers simulate 1770 magnetic storm using data from historical documentation
Auroras are light shows that typically occur at high latitudes such as the Arctic and Antarctic; however, they can expand toward the equator during severe magnetic storms. Past observations of such unusual auroras can therefore allow researchers to determine the frequency and severity of magnetic storms. The more information that can be gathered about historically intense magnetic storms, the greater the opportunity to mitigate disruption of power grids in a future event.
Historical documents are becoming much more accessible for research as newly discovered records surface from private collections around the world. Researchers at Tokyo's National Institute of Japanese Literature (NIJL) and National Institute for Polar Research (NIPR) examined a detailed painting from a Japanese manuscript Seikai ("Understanding Comets") with associated commentary describing a red aurora occurring over Kyoto on 17 September 1770. They also investigated detailed descriptions of the event from a newly discovered diary of the Higashi-Hakura family of Kyoto.
"The enthusiasm and dedication of amateur astronomers in the past provides us an exciting opportunity," Kiyomi Iwahashi of NIJL says. "The diary was written by a kokugakusha [scholar of ancient Japanese culture], and provides a sophisticated description of the red aurora, including a description of the position of the aurora relative to the Milky Way."
Using astrometric calculations of the elevations of the Milky Way as it would have been viewed from Kyoto on 17 September 1770, the researchers were able to calculate the geometry of the red aurora and check the results against the details from the Seikai painting and the diary. The description of the aurora according to the historical documents allowed the researchers to estimate the strength of the magnetic storm that caused the September 1770 aurora.
So how likely are such magnetic storms? "We are currently within a period of decreasing solar activity, which may spell the end for severe magnetic storms in the near future," Kataoka says. "However, we actually witnessed an extremely fast coronal mass ejection only several days ago [10 September 2017], which might be powerful enough to cause extreme storms. Fortunately, it just missed the Earth."
Regardless of the specific likelihood of another perfect magnetic storm, interdisciplinary historical and scientific collaborations are invaluable in providing important physical details that could help us to understand the greatest magnetic storms in history and prepare for any potential future event.