Tag Archives: modelling

27. Anomalously Weak Convection on Large Scales in the Sun

Contributed by Shravan Hanasoge. Posted on September 23, 2014

Observed seismic upper bounds on large-scale lateral (horizontal) convective-velocity amplitudes in the solar interior at the depth r/R = 0.96 do not agree with modeling results derived at a similar depth from global convection simulations. The observations of low convective-velocity amplitudes throw into question our understanding of thermal and angular momentum transport in the Sun.

15. Potential field source surface “breathes” over the course of the solar cycle

Contributed by WIlliam Arden. Posted on May 15, 2014

Our results show that raising the source surface height 15-30% during solar minimum (depending on the model used) better reproduces the observed IMF open flux from OMNI. We used two different PFSS models and the MDI/HMI magnetograms as input.