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An Overview of the Planetary Theory of Solar Activity Variability

S. Mackowski


A summary of current knowledge of solar activity's long-term behaviour on a multi-millennial timescale, as rebuilt using the indirect proxy method, is presented here. The notion of solar activity is addressed, as well as an overview of the particular indices that are used to quantify various elements of changing solar activity, with a focus on sunspot number. Over long periods, only indirect proxies, such as the cosmogenic isotopes 14C and 10Be in natural stratified archives, can be used to derive quantitative information on previous solar activity (e.g., tree rings or ice cores).


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索引于

  • 中国社会科学院
  • 谷歌学术
  • 打开 J 门
  • 中国知网(CNKI)
  • 引用因子
  • 宇宙IF
  • 研究期刊索引目录 (DRJI)
  • 秘密搜索引擎实验室
  • ICMJE

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