首页 正文

Advances in space research : the official journal of the Committee on Space Research (COSPAR). 1996;17(2):19-30. doi: 10.1016/0273-1177(95)00508-c Q22.82024

Galactic cosmic ray flux simulation and prediction

银河宇宙射线通量的模拟与预测 翻译改进

R A Nymmik  1, M I Panasyuk, A A Suslov

作者单位 +展开

作者单位

  • 1 Skobeltsyn Institute of Nuclear Physics, Moscow State University, Russia.
  • DOI: 10.1016/0273-1177(95)00508-c PMID: 11540366

    摘要 Ai翻译

    A dynamic galactic cosmic ray model is proposed to quantitatively describe the z=1-28 ions and electrons of E=10-10(5) MeV/nucleon and their particle flux variations around the Earth's orbit and beyond the Earth's magnetosphere due to diverse large-scale variations of solar activity factors. The variations of large-scale heliospheric magnetic fields and the galactic cosmic ray flux variation time delays relative to solar activity variations are simulated. The lag characteristics and sunspot number predictions having been determined in detail, the model can be used to predict galactic cosmic ray flux levels.

    Keywords:galactic cosmic rays; flux simulation

    Copyright © Advances in space research : the official journal of the Committee on Space Research (COSPAR). 中文内容为AI机器翻译,仅供参考!

    相关内容

    期刊名:Advances in space research

    缩写:ADV SPACE RES

    ISSN:0273-1177

    e-ISSN:1879-1948

    IF/分区:2.8/Q2

    文章目录 更多期刊信息

    全文链接
    引文链接
    复制
    已复制!
    推荐内容
    Galactic cosmic ray flux simulation and prediction