Journal
SOLAR PHYSICS
Volume 292, Issue 1, Pages -Publisher
SPRINGER
DOI: 10.1007/s11207-016-1035-6
Keywords
Solar activity; Sunspots; Solar observations; Solar cycle
Categories
Funding
- Academy of Finland [272157]
- Junta de Extremadura [GR15137]
- Ministerio de Economia y Competitividad of the Spanish Government [AYA2014-57556-P]
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It has recently been claimed (Zolotova and Ponyavin Solar Phys., 291, 2869, 2016; ZP16 henceforth) that a mid-latitude optical phenomenon, which took place over the city of Astrakhan in July 1670, according to Russian chronicles, were a strong aurora borealis. If this were true, it would imply a very strong or even severe geomagnetic storm during the quietest part of the Maunder minimum. However, as we argue in this article, this conclusion is erroneous and caused by a misinterpretation of the chronicle record. As a result of a thorough analysis of the chronicle text, we show that the described phenomenon occurred during the daylight period of the day (the last morning hour), in the south (towards noon), and its description does not match that of an aurora. The date of the event was also interpreted incorrectly. We conclude that this phenomenon was not a mid-latitude aurora, but an atmospheric phenomenon, the so-called sundog (or parhelion), which is a particular type of solar halo. Accordingly, the claim of a strong mid-latitude aurora during the deep Maunder Minimum is not correct and should be dismissed.
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