Jump to content
 







Main menu
   


Navigation  



Main page
Contents
Current events
Random article
About Wikipedia
Contact us
Donate
 




Contribute  



Help
Learn to edit
Community portal
Recent changes
Upload file
 








Search  

































Create account

Log in
 









Create account
 Log in
 




Pages for logged out editors learn more  



Contributions
Talk
 



















Contents

   



(Top)
 


1 Discovery  





2 Time benchmark  





3 See also  





4 References  





5 External links  














Miyake event: Difference between revisions






Беларуская
Deutsch
Español
Euskara
Français
Galego
Italiano
Português
Русский
Українська

 

Edit links
 









Article
Talk
 

















Read
Edit
View history
 








Tools
   


Actions  



Read
Edit
View history
 




General  



What links here
Related changes
Upload file
Special pages
Permanent link
Page information
Cite this page
Get shortened URL
Download QR code
Wikidata item
 




Print/export  



Download as PDF
Printable version
 




Print/export  



















Appearance
   

 





Help
 

From Wikipedia, the free encyclopedia
 


Browse history interactively
 Previous editNext edit 
Content deleted Content added
m removed "the" (outer space)
fix link target
Line 2: Line 2:

A '''Miyake event''' is an observed sharp enhancement of the production of [[Cosmogenic nuclide|cosmogenic isotopes]] by [[cosmic ray]]s. It can be marked by a spike in the concentration of radioactive [[carbon]] [[isotope]] [[Carbon-14|{{chem|14|C}}]] in tree rings, as well as [[Beryllium-10|{{chem|10|Be}}]] and [[Chlorine-36|{{chem|36|Cl}}]] in ice cores, which are all independently dated. At present, five significant events are known (7176 BCE, 5259 BCE, 660 BCE, 774 CE, 993 CE) for which the spike in [[Carbon-14|{{chem|14|C}}]] is quite remarkable, i.e. above 1% rise over a period of 2 years, and four more events (12,350{{nbsp}}BCE,<ref name=Biggest>{{Cite journal |url=https://www.independent.co.uk/news/science/french-university-of-leeds-gap-french-alps-b2426429.html |title=Biggest ever solar storm identified using ancient tree rings |date=9 October 2023 |access-date=9 October 2023 |author=Jane Kirby |journal=Independent}}</ref> 5410 BCE, 1052 CE, 1279 CE) need independent confirmation. It is not known how often Miyake events occur, but from the presently available data it is estimated that such an event would occur once every 400–2400 years.<ref name=Frequency>{{Cite journal |title=Tree-rings reveal two strong solar proton events in 7176 and 5259 BCE |date=7 March 2022 |author=Nicolas Brehm, Marcus Christl, Timothy D. J. Knowles, Emmanuelle Casanova, Richard P. Evershed, Florian Adolphi, Raimund Muscheler, Hans-Arno Synal, Florian Mekhaldi, Chiara I. Paleari, Hanns-Hubert Leuschner, Alex Bayliss, Kurt Nicolussi, Thomas Pichler, Christian Schlüchter, Charlotte L. Pearson, Matthew W. Salzer, Patrick Fonti, Daniel Nievergelt, Rashit Hantemirov, David M. Brown, Ilya Usoskin & Lukas Wacker |journal=Nature Communications|volume=13 |issue=1 |page=1196 |doi=10.1038/s41467-022-28804-9 |pmid=35256613 |pmc=8901681 |bibcode=2022NatCo..13.1196B }}</ref>

A '''Miyake event''' is an observed sharp enhancement of the production of [[Cosmogenic nuclide|cosmogenic isotopes]] by [[cosmic ray]]s. It can be marked by a spike in the concentration of radioactive [[carbon]] [[isotope]] [[Carbon-14|{{chem|14|C}}]] in tree rings, as well as [[Beryllium-10|{{chem|10|Be}}]] and [[Chlorine-36|{{chem|36|Cl}}]] in ice cores, which are all independently dated. At present, five significant events are known (7176 BCE, 5259 BCE, 660 BCE, 774 CE, 993 CE) for which the spike in [[Carbon-14|{{chem|14|C}}]] is quite remarkable, i.e. above 1% rise over a period of 2 years, and four more events (12,350{{nbsp}}BCE,<ref name=Biggest>{{Cite journal |url=https://www.independent.co.uk/news/science/french-university-of-leeds-gap-french-alps-b2426429.html |title=Biggest ever solar storm identified using ancient tree rings |date=9 October 2023 |access-date=9 October 2023 |author=Jane Kirby |journal=Independent}}</ref> 5410 BCE, 1052 CE, 1279 CE) need independent confirmation. It is not known how often Miyake events occur, but from the presently available data it is estimated that such an event would occur once every 400–2400 years.<ref name=Frequency>{{Cite journal |title=Tree-rings reveal two strong solar proton events in 7176 and 5259 BCE |date=7 March 2022 |author=Nicolas Brehm, Marcus Christl, Timothy D. J. Knowles, Emmanuelle Casanova, Richard P. Evershed, Florian Adolphi, Raimund Muscheler, Hans-Arno Synal, Florian Mekhaldi, Chiara I. Paleari, Hanns-Hubert Leuschner, Alex Bayliss, Kurt Nicolussi, Thomas Pichler, Christian Schlüchter, Charlotte L. Pearson, Matthew W. Salzer, Patrick Fonti, Daniel Nievergelt, Rashit Hantemirov, David M. Brown, Ilya Usoskin & Lukas Wacker |journal=Nature Communications|volume=13 |issue=1 |page=1196 |doi=10.1038/s41467-022-28804-9 |pmid=35256613 |pmc=8901681 |bibcode=2022NatCo..13.1196B }}</ref>



There is strong evidence that Miyake events are caused by extreme [[solar particle event]]s.<ref>{{cite journal | doi=10.1051/0004-6361/201321080 | title=The AD775 cosmic event revisited: the Sun is to blame | date=2013 | last1=Usoskin| first1=I.G. | last2=Kromer| first2=B. | last3=Ludlow| first3=F. | last4=Beer| first4=J. | last5=Friedrich| first5=F. | last6=Kovaltsov | first6=G. | last7=Solanki| first7=S. | last8=Wacker | first8=L. | journal=Astronomy and Astrophysics Letters | volume=552 | page=L3| doi-access=free | arxiv=1302.6897 | bibcode=2013A&A...552L...3U }}</ref><ref name="C22">{{cite journal | doi=10.1007/s41116-022-00033-8 | title=Extreme solar events | date=2022 | last1=Cliver| first1=Edward W. | last2=Schrijver| first2=Carolus | last3=Shibata| first3=Kazunari | last4=Usoskin| first4=Ilya G. | journal=Living Reviews in Solar Physics | volume=19| issue=1 | page=2| doi-access=free | arxiv=2205.09265 | bibcode=2022LRSP...19....2C }}</ref> and they are likely related to [[Solar flare|super-flares]] discovered on solar-like stars.<ref name="C22"/><ref name="M12">{{cite journal | url=https://doi.org/10.1038/nature11063 | doi=10.1038/nature11063| title=Super-flares on solar-type stars | date=2012 | last1=Maehara| first1=Hiroyuki | last2=Shibayama| first2=Tayuka | last3=Notsu| first3=Shota | last4=Notsu | first4=Yuta | last5=Nagao |first5=Takashi | last6=Kusaba | first6=Satoshi |last7=Honda | first7=Satoshi | last8= Nogami | first8=Daisaku | last9=Shibata | first9=Kazunari | journal=Nature | volume=485| issue=7399| page=478| pmid=22622572| bibcode=2012Natur.485..478M}}</ref> Although the Miyake events are based on extreme year-to-year rises of [[Carbon-14|{{chem|14|C}}]] concentration, the duration of the periods over which the [[Carbon-14|{{chem|14|C}}]] levels increase or stay at high levels are longer than one year.<ref>{{cite journal | url=https://doi.org/10.1098/rspa.2022.0497 | doi=10.1098/rspa.2022.0497 | title=Modelling cosmic radiation events in the tree-ring radiocarbon record | date=2022 | last1=Zhang | first1=Qingyuan | last2=Sharma | first2=Utkarsh | last3=Dennis | first3=Jordan A. | last4=Scifo | first4=Andrea | last5=Kuitems | first5=Margot | last6=Büntgen | first6=Ulf | last7=Owens | first7=Mathew J. | last8=Dee | first8=Michael W. | last9=Pope | first9=Benjamin J. S. | journal=Proceedings of the Royal Society A: Mathematical, Physical and Engineering Sciences | volume=478 | issue=2266 | arxiv=2210.13775 | bibcode=2022RSPSA.47820497Z | s2cid=253107601 }}</ref><ref name="M19">{{cite book |last1= Miyake|first1=Fusa |last2=Usoskin |first2=Ilya | last3=Poluianov| first3=Stepan |editor-first1=Fusa |editor-first2=Ilya |editor-first3=Stepan |editor-last1=Miyake |editor-last2=Usoskin |editor-last3=Poluianov |date=2020 |title= Extreme Solar Particle Storms: the hostile Sun | doi= 10.1088/2514-3433/ab404a |location= Bristol UK |publisher= Institute of Physics|isbn=978-0-7503-2232-4 }}</ref> However, a universal cause and origin of all the events is not yet established in the scientific field, and some of these events may be the result of different phenomena coming from outer space (such as a [[Gamma-ray burst]]).<ref name="SA-2023">{{cite web |last1=Kornei |first1=Katherine |title=Mystery of Ancient Space Superstorms Deepens: A fresh analysis of tree-ring data suggests barrages of cosmic radiation that washed over Earth centuries ago may have come from sources besides our sun |url=https://www.scientificamerican.com/article/mystery-of-ancient-space-superstorms-deepens/ |publisher=Scientific American |access-date=3 October 2023 |date=6 March 2023 }}</ref>

There is strong evidence that Miyake events are caused by extreme [[solar particle event]]s.<ref>{{cite journal | doi=10.1051/0004-6361/201321080 | title=The AD775 cosmic event revisited: the Sun is to blame | date=2013 | last1=Usoskin| first1=I.G. | last2=Kromer| first2=B. | last3=Ludlow| first3=F. | last4=Beer| first4=J. | last5=Friedrich| first5=F. | last6=Kovaltsov | first6=G. | last7=Solanki| first7=S. | last8=Wacker | first8=L. | journal=Astronomy and Astrophysics Letters | volume=552 | page=L3| doi-access=free | arxiv=1302.6897 | bibcode=2013A&A...552L...3U }}</ref><ref name="C22">{{cite journal | doi=10.1007/s41116-022-00033-8 | title=Extreme solar events | date=2022 | last1=Cliver| first1=Edward W. | last2=Schrijver| first2=Carolus | last3=Shibata| first3=Kazunari | last4=Usoskin| first4=Ilya G. | journal=Living Reviews in Solar Physics | volume=19| issue=1 | page=2| doi-access=free | arxiv=2205.09265 | bibcode=2022LRSP...19....2C }}</ref> and they are likely related to [[Superflare|super-flares]] discovered on solar-like stars.<ref name="C22"/><ref name="M12">{{cite journal | url=https://doi.org/10.1038/nature11063 | doi=10.1038/nature11063| title=Super-flares on solar-type stars | date=2012 | last1=Maehara| first1=Hiroyuki | last2=Shibayama| first2=Tayuka | last3=Notsu| first3=Shota | last4=Notsu | first4=Yuta | last5=Nagao |first5=Takashi | last6=Kusaba | first6=Satoshi |last7=Honda | first7=Satoshi | last8= Nogami | first8=Daisaku | last9=Shibata | first9=Kazunari | journal=Nature | volume=485| issue=7399| page=478| pmid=22622572| bibcode=2012Natur.485..478M}}</ref> Although the Miyake events are based on extreme year-to-year rises of [[Carbon-14|{{chem|14|C}}]] concentration, the duration of the periods over which the [[Carbon-14|{{chem|14|C}}]] levels increase or stay at high levels are longer than one year.<ref>{{cite journal | url=https://doi.org/10.1098/rspa.2022.0497 | doi=10.1098/rspa.2022.0497 | title=Modelling cosmic radiation events in the tree-ring radiocarbon record | date=2022 | last1=Zhang | first1=Qingyuan | last2=Sharma | first2=Utkarsh | last3=Dennis | first3=Jordan A. | last4=Scifo | first4=Andrea | last5=Kuitems | first5=Margot | last6=Büntgen | first6=Ulf | last7=Owens | first7=Mathew J. | last8=Dee | first8=Michael W. | last9=Pope | first9=Benjamin J. S. | journal=Proceedings of the Royal Society A: Mathematical, Physical and Engineering Sciences | volume=478 | issue=2266 | arxiv=2210.13775 | bibcode=2022RSPSA.47820497Z | s2cid=253107601 }}</ref><ref name="M19">{{cite book |last1= Miyake|first1=Fusa |last2=Usoskin |first2=Ilya | last3=Poluianov| first3=Stepan |editor-first1=Fusa |editor-first2=Ilya |editor-first3=Stepan |editor-last1=Miyake |editor-last2=Usoskin |editor-last3=Poluianov |date=2020 |title= Extreme Solar Particle Storms: the hostile Sun | doi= 10.1088/2514-3433/ab404a |location= Bristol UK |publisher= Institute of Physics|isbn=978-0-7503-2232-4 }}</ref> However, a universal cause and origin of all the events is not yet established in the scientific field, and some of these events may be the result of different phenomena coming from outer space (such as a [[Gamma-ray burst]]).<ref name="SA-2023">{{cite web |last1=Kornei |first1=Katherine |title=Mystery of Ancient Space Superstorms Deepens: A fresh analysis of tree-ring data suggests barrages of cosmic radiation that washed over Earth centuries ago may have come from sources besides our sun |url=https://www.scientificamerican.com/article/mystery-of-ancient-space-superstorms-deepens/ |publisher=Scientific American |access-date=3 October 2023 |date=6 March 2023 }}</ref>



A recently reported sharp spike in [[Carbon-14|{{chem|14|C}}]] that occurred between 12,350 and 12,349{{nbsp}}BCE, may represent the largest known Miyake event. This event was identified during a study conducted by an international team of researchers who measured radiocarbon levels in ancient trees recovered from the eroded banks of the Drouzet River, near [[Gap, Hautes-Alpes|Gap]], France, in the Southern French Alps.<ref>{{cite journal |last1=Alex Wilkins |title=Largest known solar storm struck Earth 14,300 years ago |journal=New Scientist |date=Oct 9, 2023 |volume=260 |issue=3460 |page=9 |doi=10.1016/S0262-4079(23)01892-4 |bibcode=2023NewSc.260Q...9W |url=https://www.newscientist.com/article/2396456-largest-known-solar-storm-struck-earth-14300-years-ago/}}</ref><ref name="royalsocietypublishing.org">{{cite journal|display-authors=etal |last1=Edouard Bard |title=A radiocarbon spike at 14 300 cal yr BP in subfossil trees provides the impulse response function of the global carbon cycle during the Late Glacial |journal=Philosophical Transactions of the Royal Society A |date=Oct 9, 2023 |volume=381 |issue=2261 |doi=10.1098/rsta.2022.0206 |pmid=37807686 |pmc=10586540 |bibcode=2023RSPTA.38120206B }}</ref><ref>{{Cite web |url=https://scitechdaily.com/largest-ever-solar-storm-identified-in-ancient-tree-rings-could-devastate-modern-technology-and-cost-billions/ |title=Largest Ever Solar Storm Identified in Ancient Tree Rings – Could Devastate Modern Technology and Cost Billions |date=9 October 2023 |access-date=9 October 2023}}</ref> According to the initial study the new event is roughly twice the size of the Δ{{chem|14|C}} increase for more recent 774{{nbsp}}CE and 993{{nbsp}}CE events, but the strength of the corresponding solar storm is not yet assessed. However, the newly discovered 12,350 BCE event has not yet been independently confirmed in any other wood from other regions, nor it is reliably supported by a clear corresponding spike in other isotopes <ref name="royalsocietypublishing.org"/> (such as [[Beryllium-10]]) that are usually used in combination for absolute radiometric dating.

A recently reported sharp spike in [[Carbon-14|{{chem|14|C}}]] that occurred between 12,350 and 12,349{{nbsp}}BCE, may represent the largest known Miyake event. This event was identified during a study conducted by an international team of researchers who measured radiocarbon levels in ancient trees recovered from the eroded banks of the Drouzet River, near [[Gap, Hautes-Alpes|Gap]], France, in the Southern French Alps.<ref>{{cite journal |last1=Alex Wilkins |title=Largest known solar storm struck Earth 14,300 years ago |journal=New Scientist |date=Oct 9, 2023 |volume=260 |issue=3460 |page=9 |doi=10.1016/S0262-4079(23)01892-4 |bibcode=2023NewSc.260Q...9W |url=https://www.newscientist.com/article/2396456-largest-known-solar-storm-struck-earth-14300-years-ago/}}</ref><ref name="royalsocietypublishing.org">{{cite journal|display-authors=etal |last1=Edouard Bard |title=A radiocarbon spike at 14 300 cal yr BP in subfossil trees provides the impulse response function of the global carbon cycle during the Late Glacial |journal=Philosophical Transactions of the Royal Society A |date=Oct 9, 2023 |volume=381 |issue=2261 |doi=10.1098/rsta.2022.0206 |pmid=37807686 |pmc=10586540 |bibcode=2023RSPTA.38120206B }}</ref><ref>{{Cite web |url=https://scitechdaily.com/largest-ever-solar-storm-identified-in-ancient-tree-rings-could-devastate-modern-technology-and-cost-billions/ |title=Largest Ever Solar Storm Identified in Ancient Tree Rings – Could Devastate Modern Technology and Cost Billions |date=9 October 2023 |access-date=9 October 2023}}</ref> According to the initial study the new event is roughly twice the size of the Δ{{chem|14|C}} increase for more recent 774{{nbsp}}CE and 993{{nbsp}}CE events, but the strength of the corresponding solar storm is not yet assessed. However, the newly discovered 12,350 BCE event has not yet been independently confirmed in any other wood from other regions, nor it is reliably supported by a clear corresponding spike in other isotopes <ref name="royalsocietypublishing.org"/> (such as [[Beryllium-10]]) that are usually used in combination for absolute radiometric dating.


Revision as of 04:28, 10 May 2024

AMiyake event is an observed sharp enhancement of the production of cosmogenic isotopesbycosmic rays. It can be marked by a spike in the concentration of radioactive carbon isotope 14
C
in tree rings, as well as 10
Be
and 36
Cl
in ice cores, which are all independently dated. At present, five significant events are known (7176 BCE, 5259 BCE, 660 BCE, 774 CE, 993 CE) for which the spike in 14
C
is quite remarkable, i.e. above 1% rise over a period of 2 years, and four more events (12,350 BCE,[1] 5410 BCE, 1052 CE, 1279 CE) need independent confirmation. It is not known how often Miyake events occur, but from the presently available data it is estimated that such an event would occur once every 400–2400 years.[2]

There is strong evidence that Miyake events are caused by extreme solar particle events.[3][4] and they are likely related to super-flares discovered on solar-like stars.[4][5] Although the Miyake events are based on extreme year-to-year rises of 14
C
concentration, the duration of the periods over which the 14
C
levels increase or stay at high levels are longer than one year.[6][7] However, a universal cause and origin of all the events is not yet established in the scientific field, and some of these events may be the result of different phenomena coming from outer space (such as a Gamma-ray burst).[8]

A recently reported sharp spike in 14
C
that occurred between 12,350 and 12,349 BCE, may represent the largest known Miyake event. This event was identified during a study conducted by an international team of researchers who measured radiocarbon levels in ancient trees recovered from the eroded banks of the Drouzet River, near Gap, France, in the Southern French Alps.[9][10][11] According to the initial study the new event is roughly twice the size of the Δ14
C
increase for more recent 774 CE and 993 CE events, but the strength of the corresponding solar storm is not yet assessed. However, the newly discovered 12,350 BCE event has not yet been independently confirmed in any other wood from other regions, nor it is reliably supported by a clear corresponding spike in other isotopes [10] (such as Beryllium-10) that are usually used in combination for absolute radiometric dating.

A Miyake event occurring in modern conditions might have significant impacts on global technological infrastructure such as satellites, telecommunications, and power grids.[7][12][13]

Discovery

The events are named after the Japanese physicist Fusa Miyake who, as a doctoral student, was the first one to identify these radiocarbon spikes and published the results with co-authors in 2012 in the journal Nature.[14] The investigation at that time found a strong 14
C
increase in the annual rings of Japanese cedars for the years 774/775. The event of 775 was independently discovered, using the low-resolution IntCal data.[15] In 2013, Miyake and co-authors published the discovery of another similar radiocarbon spike in the years 993/994.[16] In December 2013, Miyake received her Doctor of Science degree from Nagoya University.[17]

Time benchmark

After a Miyake event is well-studied and confirmed, it can serve as a reference time benchmark, a "year-stamp", enabling more precise dating of historical events. Six diverse historical occurrences, from archaeological sites to natural disasters, have thus been dated to a specific year, using Miyake events as benchmarks and counting tree rings.[18] For example, wooden houses in the Viking site at L'Anse aux MeadowsinNewfoundland were dated by finding the 993 CE Miyake event and then counting tree rings, which showed that the wood is from a tree felled in 1021 CE.[19]

See also

References

  1. ^ Jane Kirby (9 October 2023). "Biggest ever solar storm identified using ancient tree rings". Independent. Retrieved 9 October 2023.
  • ^ Nicolas Brehm, Marcus Christl, Timothy D. J. Knowles, Emmanuelle Casanova, Richard P. Evershed, Florian Adolphi, Raimund Muscheler, Hans-Arno Synal, Florian Mekhaldi, Chiara I. Paleari, Hanns-Hubert Leuschner, Alex Bayliss, Kurt Nicolussi, Thomas Pichler, Christian Schlüchter, Charlotte L. Pearson, Matthew W. Salzer, Patrick Fonti, Daniel Nievergelt, Rashit Hantemirov, David M. Brown, Ilya Usoskin & Lukas Wacker (7 March 2022). "Tree-rings reveal two strong solar proton events in 7176 and 5259 BCE". Nature Communications. 13 (1): 1196. Bibcode:2022NatCo..13.1196B. doi:10.1038/s41467-022-28804-9. PMC 8901681. PMID 35256613.{{cite journal}}: CS1 maint: multiple names: authors list (link)
  • ^ Usoskin, I.G.; Kromer, B.; Ludlow, F.; Beer, J.; Friedrich, F.; Kovaltsov, G.; Solanki, S.; Wacker, L. (2013). "The AD775 cosmic event revisited: the Sun is to blame". Astronomy and Astrophysics Letters. 552: L3. arXiv:1302.6897. Bibcode:2013A&A...552L...3U. doi:10.1051/0004-6361/201321080.
  • ^ a b Cliver, Edward W.; Schrijver, Carolus; Shibata, Kazunari; Usoskin, Ilya G. (2022). "Extreme solar events". Living Reviews in Solar Physics. 19 (1): 2. arXiv:2205.09265. Bibcode:2022LRSP...19....2C. doi:10.1007/s41116-022-00033-8.
  • ^ Maehara, Hiroyuki; Shibayama, Tayuka; Notsu, Shota; Notsu, Yuta; Nagao, Takashi; Kusaba, Satoshi; Honda, Satoshi; Nogami, Daisaku; Shibata, Kazunari (2012). "Super-flares on solar-type stars". Nature. 485 (7399): 478. Bibcode:2012Natur.485..478M. doi:10.1038/nature11063. PMID 22622572.
  • ^ Zhang, Qingyuan; Sharma, Utkarsh; Dennis, Jordan A.; Scifo, Andrea; Kuitems, Margot; Büntgen, Ulf; Owens, Mathew J.; Dee, Michael W.; Pope, Benjamin J. S. (2022). "Modelling cosmic radiation events in the tree-ring radiocarbon record". Proceedings of the Royal Society A: Mathematical, Physical and Engineering Sciences. 478 (2266). arXiv:2210.13775. Bibcode:2022RSPSA.47820497Z. doi:10.1098/rspa.2022.0497. S2CID 253107601.
  • ^ a b Miyake, Fusa; Usoskin, Ilya; Poluianov, Stepan (2020). Miyake, Fusa; Usoskin, Ilya; Poluianov, Stepan (eds.). Extreme Solar Particle Storms: the hostile Sun. Bristol UK: Institute of Physics. doi:10.1088/2514-3433/ab404a. ISBN 978-0-7503-2232-4.
  • ^ Kornei, Katherine (6 March 2023). "Mystery of Ancient Space Superstorms Deepens: A fresh analysis of tree-ring data suggests barrages of cosmic radiation that washed over Earth centuries ago may have come from sources besides our sun". Scientific American. Retrieved 3 October 2023.
  • ^ Alex Wilkins (Oct 9, 2023). "Largest known solar storm struck Earth 14,300 years ago". New Scientist. 260 (3460): 9. Bibcode:2023NewSc.260Q...9W. doi:10.1016/S0262-4079(23)01892-4.
  • ^ a b Edouard Bard; et al. (Oct 9, 2023). "A radiocarbon spike at 14 300 cal yr BP in subfossil trees provides the impulse response function of the global carbon cycle during the Late Glacial". Philosophical Transactions of the Royal Society A. 381 (2261). Bibcode:2023RSPTA.38120206B. doi:10.1098/rsta.2022.0206. PMC 10586540. PMID 37807686.
  • ^ "Largest Ever Solar Storm Identified in Ancient Tree Rings – Could Devastate Modern Technology and Cost Billions". 9 October 2023. Retrieved 9 October 2023.
  • ^ Brehm, Nicolas; Christl, Marcus; Knowles, Timothy D. J.; Casanova, Emmanuelle; Evershed, Richard P.; Adolphi, Florian; Muscheler, Raimund; Synal, Hans-Arno; Mekhaldi, Florian; Paleari, Chiara I.; Leuschner, Hanns-Hubert; Bayliss, Alex; Nicolussi, Kurt; Pichler, Thomas; Schlüchter, Christian; Pearson, Charlotte L.; Salzer, Matthew W.; Fonti, Patrick; Nievergelt, Daniel; Hantemirov, Rashit; Brown, David M.; Usoskin, Ilya; Wacker, Lukas (2022). "Tree-rings reveal two strong solar proton events in 7176 and 5259 BCE". Nature Communications. 13 (1): 1196. Bibcode:2022NatCo..13.1196B. doi:10.1038/s41467-022-28804-9. PMC 8901681. PMID 35256613.
  • ^ "Radiocarbon (14C)". www.isee.nagoya-u.ac.jp. 17 November 2021. Retrieved 2023-03-06.
  • ^ Miyake, F.; Nagaya, K.; Masuda, K.; Nakamura, T. (2012). "A signature of cosmic-ray increase in AD 774–775 from tree rings in Japan". Nature. 486 (7402): 240–242. Bibcode:2012Natur.486..240M. doi:10.1038/nature11123. PMID 22699615.
  • ^ Usoskin, Ilya; Kovaltsov, Gennady (2012). "Occurrence of Extreme Solar Particle Events: Assessment from Historical Proxy Data". Astrophysical Journal. 757 (1): 92. arXiv:1207.5932. Bibcode:2012ApJ...757...92U. doi:10.1088/0004-637X/757/1/92.
  • ^ Miyake, Fusa; Masuda, Kimiaki; Nakamura, Toshio (2013). "Another rapid event in the carbon-14 content of tree rings". Nature Communications. 4: 1748. Bibcode:2013NatCo...4.1748M. doi:10.1038/ncomms2783. PMID 23612289. S2CID 256624509.
  • ^ "Faculty Profiles: MIYAKE Fusa". Nagoya University. Retrieved 17 October 2023. Degree: 博士(理学)( 2013.12 名古屋大学 )
  • ^ Price, Michael (13 April 2023). "Marking time: Radiocarbon timestamps left in ancient tree rings by cosmic ray bombardments can date historical events with unprecedented precision". Science. A previous version "Marking time: Cosmic ray storms can pin precise dates on history from ancient Egypt to the Vikings" appeared in Science, Vol 380, Issue 6641.
  • ^ Kuitems, Margot; et al. (20 October 2021). "Evidence for European presence in the Americas in AD 1021" (PDF). Nature. 601 (7893): 388–391. doi:10.1038/s41586-021-03972-8. PMC 8770119. PMID 34671168. S2CID 239051036. Archived (PDF) from the original on 2022-10-09.
  • External links


    Retrieved from "https://en.wikipedia.org/w/index.php?title=Miyake_event&oldid=1223139318"

    Categories: 
    Geomagnetic storms
    Astrophysics
    Geophysics
    Stratigraphy
    Dating methods
    Hidden categories: 
    CS1 maint: multiple names: authors list
    Articles with short description
    Short description is different from Wikidata
     



    This page was last edited on 10 May 2024, at 04:28 (UTC).

    This version of the page has been revised. Besides normal editing, the reason for revision may have been that this version contains factual inaccuracies, vandalism, or material not compatible with the Creative Commons Attribution-ShareAlike License.



    Privacy policy

    About Wikipedia

    Disclaimers

    Contact Wikipedia

    Code of Conduct

    Developers

    Statistics

    Cookie statement

    Mobile view



    Wikimedia Foundation
    Powered by MediaWiki