Global Evolution of Solar Magnetic Fields and Prediction of Activity Cycles

10 Mar 2020 Kitiashvili Irina N.

Prediction of solar activity cycles is challenging because physical processes inside the Sun involve a broad range of multiscale dynamics that no model can reproduce and because the available observations are highly limited and cover mostly surface layers. Helioseismology makes it possible to probe solar dynamics in the convective zone, but variations in differential rotation and meridional circulation are currently available for only two solar activity cycles... (read more)

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Categories


  • SOLAR AND STELLAR ASTROPHYSICS
  • CHAOTIC DYNAMICS
  • DATA ANALYSIS, STATISTICS AND PROBABILITY
  • SPACE PHYSICS