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Abstracts—LWSFT

TITLE

PIINSTITUTE

Study of Global-Scale Surface Flows and Migration of Polar Crown Filaments of the Sun in Past 10 Solar Cycles in Comparison with Helioseismology Results in 2 Recent Cycles

Haimin WangNew Jersey Institute of Technology

Linking Active Regions and Solar Cycles to Understand How Variable Flows in the Solar Interior Affect Surface Magnetic Field Evolution

Philip ScherrerHEPL

Active Region Dynamics and the Variability of Meridional and Zonal Flows

Douglas BraunNorthWest Research Associates, Inc. 
Simulating active longitudes by coupling magnetograms with a nonlinear MHD tachocline model: a data assimilation approachMausumi DikpatiUniversity Corporation for Atmospheric Research

Processes Shaping the Solar Meridional Circulation

Nicholas FeatherstoneUniversity of Colorado

Do Flows in the Upper Solar Convection Zone Drive Global-Scale Magnetic Fields?

Rudolf KommNational Solar Observatory

Improving Long Term Forecasts of Solar Variability with the Advective Flux Transport Model

Lisa UptonSpace Systems Research Corporation
   
   
   

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The National Center for Atmospheric Research is sponsored by the National Science Foundation. Any opinions, findings and conclusions or recommendations expressed in this publication are those of the author(s) and do not necessarily reflect the views of the National Science Foundation.

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