An Optical Atmospheric Phenomenon Observed in 1670 over the City of Astrakhan Was not a Mid-Latitude Aurora
arXiv:1612.00705 · doi:10.1007/s11207-016-1035-6
Abstract
It has been recently 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, was a strong aurora borealis. If this was 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 direction ("towards noon"), and its description does not match that of an aurora. The date of the event was also incorrectly interpreted. 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 about a strong mid-latitude aurora during the deep Maunder minimum is not correct and should be dismissed.
arXiv commentaccepted to Solar Physics
References in corpus (10)
- Reconstruction of the Sunspot Group Number: the Backbone Method
- The Maunder minimum (1645--1715) was indeed a Grand minimum: A reassessment of multiple datasets
- A Revised Collection of Sunspot Group Numbers
- Solar activity during the Holocene: the Hallstatt cycle and its consequence for grand minima and maxim
- Evidence for distinct modes of solar activity
- Revisited sunspot data: A new scenario for the onset of the Maunder minimum
- Level and length of cyclic solar activity during the Maunder minimum as deduced from the active day statistics
- Sunspots during the Maunder Minimum from Machina Coelestis by Hevelius
- Revised Group Sunspot Number for 1640, 1652, and 1741
- Sunspot Observations during the Maunder Minimum from the Correspondence of John Flamsteed
Cited by in corpus (9)
- Extreme solar events
- Do the Chinese Astronomical Records Dated AD 776 January 12/13 Describe an Auroral Display or a Lunar Halo? A Critical Re-examination
- The Earliest Candidates of Auroral Observations in Assyrian Astrological Reports: Insights on Solar Activity around 660 BCE
- Records of Auroral Candidates and Sunspots in Rikkokushi, Chronicles of Ancient Japan from Early 7th Century to 887
- Candidate Auroral Observations during the Major Solar-Terrestrial Storm in May 1680: Implication for Space Weather Events during the Maunder Minimum
- Intense geomagnetic storm during Maunder minimum possibly by a quiescent filament eruption
- The Celestial Sign in the Anglo-Saxon Chronicle in the 770s: Insights on Contemporary Solar Activity
- Sporadic Aurora near Geomagnetic Equator: In the Philippines, on 27 October 1856
- A possible case of sporadic aurora observed at Rio de Janeiro