Abstract <p>We discuss 13 known rapid increases in radiocarbon content in the Earth’s atmosphere and all proposed to date hypotheses of their origin. Comparing the occurrence probability of 4 most powerful events, prescribed likely to the solar superflares, with the Kepler’s mission data it results in a significant discrepancy at least assuming flare energy <i>E</i> ∼ 10<sup>35</sup> erg. The hypothesis of solar superflares (or sequence of flares) cannot likely be the only one accounting for the origin of all measured <sup>14</sup>C signals. For example, some events could be explained by the Solar system encounter with the interstellar inhomogeneities (clouds). For two of them (660 BCE and/or 813 BCE) there is a critical experiment on <sup>3</sup>He content increase in Antarctic ice supporting this suggestion. However, none of the proposed hypotheses can reliably satisfy the experimental data.</p>

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Solar Superflares during the Last 15 ka: Myth or Reality?

  • A. N. Konstantinov,
  • V. M. Ostryakov,
  • A. K. Pavlov,
  • G. I. Vasilyev

摘要

Abstract

We discuss 13 known rapid increases in radiocarbon content in the Earth’s atmosphere and all proposed to date hypotheses of their origin. Comparing the occurrence probability of 4 most powerful events, prescribed likely to the solar superflares, with the Kepler’s mission data it results in a significant discrepancy at least assuming flare energy E ∼ 1035 erg. The hypothesis of solar superflares (or sequence of flares) cannot likely be the only one accounting for the origin of all measured 14C signals. For example, some events could be explained by the Solar system encounter with the interstellar inhomogeneities (clouds). For two of them (660 BCE and/or 813 BCE) there is a critical experiment on 3He content increase in Antarctic ice supporting this suggestion. However, none of the proposed hypotheses can reliably satisfy the experimental data.