Magnetic polarity reversals

Image sequence showing the polarity reversal of the surface magnetic field in the course of a magnetic cycle developing in a magnetohydrodynamical numerical simulation of solar convection. The color scale codes the radial magnetic field, red-yellow for positive magnetic polarity and blue-green for negative, peaking here at +/- 0.04 Tesla. Even though the surface magnetic field is spatiotemporally very intermittent, a well-defined axisymmetric component is present, amounting to a magnetic dipole well aligned with the rotation axis. In this specific simulation the full magnetic cycle lasts about 78 years, corresponding to a pseudo-activity cycle of duration 39 years.


Click here for a higher resolution version.

For more information:

   Image added 31 janvier 2012 par

Tous droits réservés / Copyrighted by
Université de Montréal