Changes in the solar wind’s isotope component, due to interaction between solar flare particles and the photosphere

G. I. Vasilyev; V. M. Ostryakov; A. K. Pavlov; M. E. Chakchurina

doi:10.3103/S1062873817020435

Changes in the solar wind’s isotope component, due to interaction between solar flare particles and the photosphere

作者: Vasilyev G.I.¹, Ostryakov V.M.², Pavlov A.K.¹^,2, Chakchurina M.E.²
隶属关系:
1. Ioffe Institute
2. St. Petersburg State Polytechnic University
期: 卷 81, 编号 2 (2017)
页面: 143-145
栏目: Proceedings of the 34th All-Russian Conference on Cosmic Rays
URL: https://journals.rcsi.science/1062-8738/article/view/184952
DOI: https://doi.org/10.3103/S1062873817020435
ID: 184952

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详细

Possible mechanisms responsible for changes in the solar wind’s isotope component caused by interaction between solar flare protons and helium isotopes with photospheric nuclei are considered. Depth profiles of the rates of ⁶Li, ⁷Li, ⁷Be, ¹⁴C production in the solar atmosphere are simulated using the GEANT4 software package. It is concluded that anomalous isotopic compositions of the solar wind relative to the average values can form during the coronal mass ejections.