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The cause of the weak solar cycle 24

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

Research output: Contribution to journal › Article › peer-review

Abstract

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.

Original languageEnglish
Article numberL28
JournalAstrophysical Journal Letters
Volume808
Issue number1
DOIs
StatePublished - 20 Jul 2015
Externally publishedYes

Keywords

  • Sun: activity
  • Sun: magnetic fields

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