2014
DOI: 10.1134/s1063773714100065
|View full text |Cite
|
Sign up to set email alerts
|

“Isotopic footprints” of gamma-ray and proton events and anomalous signal in radiocarbon in 775 AD

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1
1
1

Citation Types

0
14
1

Year Published

2015
2015
2022
2022

Publication Types

Select...
4
1

Relationship

0
5

Authors

Journals

citations
Cited by 11 publications
(15 citation statements)
references
References 22 publications
0
14
1
Order By: Relevance
“…The TUNU data set does not even cover AD 774/5, so that it is not clear whether the peak seen in AD 768 is the largest one (data only from 763-770). For the NEEM data set around AD 993/4, they took data for only 13 years, so that the identification of the peak presumably related to the 14 C variation around AD 993/4 is also un- 19 Pavlov et al (2013Pavlov et al ( , 2014) expect a short recombination airglow in 30-40 km height with (4-5) ×10 6 erg cm −2 fluence after a gamma-ray burst, but there is no such evidence: the observations in the Chronicle of Zuqnin for AD 772 and 773 (and maybe also 774) clearly refer to normal aurora curtains with red and yellow color, and a report from the Ulster Chronicle for Ireland for AD 772 September 29 (The hand-clapping on St Michael's Day which called fire from heaven.) also refers to an aurora (fire from heaven), if a celestial event, see Neuhäuser & Neuhäuser (2015a) for discussion (aurorae are usually above 100 km); a gamma-ray burst would also have led to strong ozone layer depletion and weather disturbances (e.g.…”
Section: Discussionmentioning
confidence: 99%
See 4 more Smart Citations
“…The TUNU data set does not even cover AD 774/5, so that it is not clear whether the peak seen in AD 768 is the largest one (data only from 763-770). For the NEEM data set around AD 993/4, they took data for only 13 years, so that the identification of the peak presumably related to the 14 C variation around AD 993/4 is also un- 19 Pavlov et al (2013Pavlov et al ( , 2014) expect a short recombination airglow in 30-40 km height with (4-5) ×10 6 erg cm −2 fluence after a gamma-ray burst, but there is no such evidence: the observations in the Chronicle of Zuqnin for AD 772 and 773 (and maybe also 774) clearly refer to normal aurora curtains with red and yellow color, and a report from the Ulster Chronicle for Ireland for AD 772 September 29 (The hand-clapping on St Michael's Day which called fire from heaven.) also refers to an aurora (fire from heaven), if a celestial event, see Neuhäuser & Neuhäuser (2015a) for discussion (aurorae are usually above 100 km); a gamma-ray burst would also have led to strong ozone layer depletion and weather disturbances (e.g.…”
Section: Discussionmentioning
confidence: 99%
“…also refers to an aurora (fire from heaven), if a celestial event, see Neuhäuser & Neuhäuser (2015a) for discussion (aurorae are usually above 100 km); a gamma-ray burst would also have led to strong ozone layer depletion and weather disturbances (e.g. Pavlov et al 2014), which are not reported (at least for the northern hemisphere). 20 Without the data point for 769.5 in TUNU, which we did not want to assign arbitrarily to either the 769 or the 770 year -if we would include this data point with low 10 Be flux in taking the means, the peak in Fig.…”
Section: Discussionmentioning
confidence: 99%
See 3 more Smart Citations