电邮这篇文章 Cosmogenic isotopes in the lunar soil: solar activity and nearby Supernova outbreak
- 作者: Vasilyev G.I.1, Konstantinov A.N.2, Ostryakov V.M.2, Pavlov A.K.1, Frolov D.A.1
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隶属关系:
- Ioffe Physical-Technical Institute of the Russian Academy of Sciences
- Peter the Great Saint Petersburg Polytechnic University
- 期: 卷 88, 编号 2 (2024)
- 页面: 307-310
- 栏目: Physics of Cosmic Rays
- URL: https://journals.rcsi.science/0367-6765/article/view/266132
- DOI: https://doi.org/10.31857/S0367676524020244
- EDN: https://elibrary.ru/RQNQHM
- ID: 266132
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The lunar soil is an integral detector of cosmic rays (CRs) of different origin (Solar and Galactic). Analysis of the deep profiles of cosmogenic isotopes (14C, 41Ca, 36Cl, 10Be, 26Al, 53Mn) allows us to restore the intensity of CR on time scales of 3–4 half-lives of the corresponding isotope. To coordinate data on 10Be, it is required (in addition to the average flux of CRs) the presence of an additional source of accelerated particles with hard spectrum. Such a source can be, for example, an outbreak of a nearby SN 2–3 million years ago.
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作者简介
G. Vasilyev
Ioffe Physical-Technical Institute of the Russian Academy of Sciences
编辑信件的主要联系方式.
Email: gennadyivas@gmail.com
俄罗斯联邦, Saint Petersburg
A. Konstantinov
Peter the Great Saint Petersburg Polytechnic University
Email: gennadyivas@gmail.com
俄罗斯联邦, Saint Petersburg
V. Ostryakov
Peter the Great Saint Petersburg Polytechnic University
Email: gennadyivas@gmail.com
俄罗斯联邦, Saint Petersburg
A. Pavlov
Ioffe Physical-Technical Institute of the Russian Academy of Sciences
Email: gennadyivas@gmail.com
俄罗斯联邦, Saint Petersburg
D. Frolov
Ioffe Physical-Technical Institute of the Russian Academy of Sciences
Email: gennadyivas@gmail.com
俄罗斯联邦, Saint Petersburg
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