Extreme Solar Events: Setting up a Paradigm.

Autor: Usoskin, Ilya¹ (AUTHOR) ilya.usoskin@oulu.fi, Miyake, Fusa² (AUTHOR), Baroni, Melanie³ (AUTHOR), Brehm, Nicolas⁴ (AUTHOR), Dalla, Silvia⁵ (AUTHOR), Hayakawa, Hisashi^2,6,7,8 (AUTHOR), Hudson, Hugh^9,10 (AUTHOR), Jull, A. J. Timothy^11,12 (AUTHOR), Knipp, Delores^13,14 (AUTHOR), Koldobskiy, Sergey¹ (AUTHOR), Maehara, Hiroyuki¹⁵ (AUTHOR), Mekhaldi, Florian^16,17 (AUTHOR), Notsu, Yuta^18,19 (AUTHOR), Poluianov, Stepan¹ (AUTHOR), Rozanov, Eugene^20,21 (AUTHOR), Shapiro, Alexander²² (AUTHOR), Spiegl, Tobias²³ (AUTHOR), Sukhodolov, Timofei^20,21 (AUTHOR), Uusitalo, Joonas^24,25 (AUTHOR), Wacker, Lukas⁴ (AUTHOR)

Publikováno v: Space Science Reviews. Dec2023, Vol. 219 Issue 8, p1-114. 114p.

Revisited reference solar proton event of 23-Feb-1956: Assessment of the cosmogenic-isotope method sensitivity to extreme solar events

Autor: Usoskin, Ilya G., Koldobskiy, Sergey A., Kovaltsov, Gennady A., Rozanov, Eugene V., Sukhodolov, Timophei V., Mishev, Alexander L., Mironova, Irina A.

Publikováno v: Journal of Geophysical Research: Space Physics, 125, e2020JA027921 (2020)

Our direct knowledge of solar eruptive events is limited to several decades and does not include extreme events, which can only be studied by the indirect proxy method over millennia, or by a large number of sun-like stars. There is a gap, spanning 1

Externí odkaz: http://arxiv.org/abs/2005.10597

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Investigation of past extreme solar events by radiocarbon analyses

Autor: Fusa Miyake

Publikováno v: Journal of the Atomic Energy Society of Japan. 65:104-107

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::67c2acbc177a589ce1d97ec8738fc3b7
https://doi.org/10.3327/jaesjb.65.2_104

The impact of extreme solar events on the atmosphere

Autor: Thomas Reddmann, Monali Borthakur, Miriam Sinnhuber, Ilya Usoskin, Jan Maik Wissing

Besides the well-known 11 year solar cycle, the Sun occasionally produces strong eruptions on the Sun‘s surface and in the corona. They can first be seen as flare events in electromagnetic spectrum down to X ray wavelengths. Within these strong eru

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::e17fb8ef0050b6bb4ddd32b84b4c54a0
https://doi.org/10.5194/egusphere-egu23-13994