Do the Chinese Astronomical Records Dated AD 776 January 12/13 Describe an Auroral Display or a Lunar Halo? A Critical Re-examination
arXiv:1903.06806 · doi:10.1007/s11207-019-1425-7
Abstract
The enhancement of carbon-14 in tree rings around AD 774/775 has generated wide interest in solar activity at that time. The historical auroral records have been examined critically. Of particular interest was the "white vapour" observed in China on AD 776 January 12/13. Both Usoskin et al. (2013, Astron. Astrophys. 55, L3; U13) and Stephenson (2015, Adv. Sp. Res. 55, 1537; S15) interpreted this record as an auroral display. Subsequently, Neuhäuser and Neuhäuser (2015, Astron. Nachr. 336, 225; NN15) proposed five "criteria" for the likeliness of aurorae and on this basis rejected an auroral interpretation. Instead, they interpreted it as a lunar halo, and suggested there were no auroral records as a proxy of solar activity in the interval AD 774-785. We consider if their "lunar halo hypothesis" and their auroral criteria could be of use in future researches on historical auroral candidates. We first show a counter-example for the lunar halo hypothesis from a parallel record on 1882 November 17, which was seen as a whitish colour, in the southerly direction, and near the Moon. We then consider NN15's criteria on colour, direction, and sky brightness and investigate other counter-examples from early-modern auroral observations. We also consider the extension of the white vapour in AD 776 according to the distribution of Chinese asterisms, and show that its large extension was inconsistent with the lunar halo hypothesis. Conversely, the streaks of white vapour penetrating the eight Chinese asterisms can be reproduced if we consider auroral-ray structures at altitudes between 97 km and 170 km, along geomagnetic field lines between the L-shells L=1.55 and 1.64. Our investigations show that we should consider candidate auroral records in historical documents not on the basis of the newly suggested a priori criteria by NN15 but on all the available observational evidence.
arXiv comment28 pages, 6 figures, accepted for publication in Solar Physics on 5 February 2019
References in corpus (19)
- The AD775 cosmic event revisited: the Sun is to blame
- Starspot activity and superflares on solar-type stars
- Long-Lasting Extreme Magnetic Storm Activities in 1770 Found in Historical Documents
- Low-Latitude Aurorae during the Extreme Space Weather Events in 1859
- The Great Space Weather Event during February 1872 Recorded in East Asia
- Solar activity around AD 775 from aurorae and radiocarbon
- Records of sunspot and aurora during CE 960-1279 in the Chinese chronicle of the Song dynasty
- East Asian Observations of Low Latitude Aurora during the Carrington Magnetic Storm
- Records of Sunspots and Aurora Candidates in the Chinese Official Histories of the Yuán and Míng Dynasties during 1261-1644
- The earliest drawings of datable auroras and a two-tail comet from the Syriac Chronicle of Zūqnīn
- Historical Auroras in the 990s: Evidence for Great Magnetic Storms
- A Great Space Weather Event in February 1730
- An Optical Atmospheric Phenomenon Observed in 1670 over the City of Astrakhan Was not a Mid-Latitude Aurora
- Records of sunspot and aurora activity during 581-959 CE in Chinese official histories in the periods of Suí, Táng, and the Five Dynasties and Ten Kingdoms
- Unusual rainbows as auroral candidates: another point of view
- Records of Auroral Candidates and Sunspots in Rikkokushi, Chronicles of Ancient Japan from Early 7th Century to 887
- A review of East Asian reports of aurorae and comets circa AD 775
- "Unusual Rainbow and White Rainbow" A new auroral candidate in oriental historical sources
- The Celestial Sign in the Anglo-Saxon Chronicle in the 770s: Insights on Contemporary Solar Activity
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- Provenance of the Cross Sign of 806 in the Anglo-Saxon Chronicle: A possible Lunar Halo over Continental Europe?
- Intense geomagnetic storm during Maunder minimum possibly by a quiescent filament eruption
- Candidate Auroral Observations during the Major Solar-Terrestrial Storm in May 1680: Implication for Space Weather Events during the Maunder Minimum
- The Celestial Sign in the Anglo-Saxon Chronicle in the 770s: Insights on Contemporary Solar Activity
- A possible case of sporadic aurora observed at Rio de Janeiro
- "The sun was darkened for seventeen days (AD 797)". An interdisciplinary exploration of celestial phenomena between Byzantium, Charlemagne, and a volcanic eruption