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Predicting solar cycle 24 with a solar dynamo model.

Arnab Rai Choudhuri1, Piyali Chatterjee, Jie Jiang

  • 1Department of Physics, Indian Institute of Science, Bangalore-560012, India. arnab@physics.iisc.ernet.in

Physical Review Letters
|May 16, 2007
PubMed
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The upcoming solar cycle 24 is predicted to be weaker than the previous one. Our solar dynamo model, using polar magnetic field data, accurately simulated past solar activity, forecasting a 35% reduction in cycle 24's strength.

Area of Science:

  • * Solar physics
  • * Astrophysics
  • * Space weather prediction

Background:

  • * The strength of the solar cycle, specifically solar cycle 24, is a subject of ongoing scientific debate.
  • * Solar cycles are driven by complex internal dynamo mechanisms within the Sun.

Purpose of the Study:

  • * To model past solar cycles using observational data.
  • * To predict the strength of the upcoming solar cycle 24.

Main Methods:

  • * Development and application of a solar dynamo model.
  • * Input of observational data on the Sun's polar magnetic field for cycles 21-23.
  • * Validation of the model against observed sunspot numbers.

Main Results:

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  • * The solar dynamo model successfully reproduced the sunspot numbers for solar cycles 21-23.
  • * The model predicts solar cycle 24 will be approximately 35% weaker than solar cycle 23.
  • Conclusions:

    • * The study provides a quantitative prediction for the strength of solar cycle 24.
    • * The findings suggest a weaker solar maximum for the upcoming cycle, impacting space weather forecasts.