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The cause of the weak solar cycle 24

  • CAS - National Astronomical Observatories
  • Max Planck Institute for Solar System Research

科研成果: 期刊稿件 › 文章 › 同行评审

摘要

The ongoing 11 year cycle of solar activity is considerably less vigorous than the three cycles before. It was preceded by a very deep activity minimum with a low polar magnetic flux, the source of the toroidal field responsible for solar magnetic activity in the subsequent cycle. Simulation of the evolution of the solar surface field shows that the weak polar fields and thus the weakness of the present cycle 24 are mainly caused by a number of bigger bipolar regions emerging at low latitudes with a "wrong" (i.e., opposite to the majority for this cycle) orientation of their magnetic polarities in the north-south direction, which impaired the growth of the polar field. These regions had a particularly strong effect since they emerged within ±10° latitude from the solar equator.

源语言英语
期刊论文编号L28
期刊Astrophysical Journal Letters
卷808
期1
DOI
出版状态已出版 - 20 7月 2015
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