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    • Modeling Solar Cycles 15 to 21 Using a Flux Transport Dynamo 

      Işık, Emre; Jiang, J.; Cameron, R. H.; Schmitt, D. (Edp Sciences S A, 17, Ave Du Hoggar, Pa Courtaboeuf, Bp 112, F-91944 Les Ulis Cedex A, France, 2013-05)
      Context. The Sun's polar fields and open flux around the time of activity minima have been considered to be strongly correlated with the strength of the subsequent maximum of solar activity. Aims. We aim to investigate ...
    • Surface Flux Evolution Constraints For Flux Transport Dynamos 

      Işık, Emre; Cameron, R. H.; Schmitt, D.; Jiang, J. (Edp Sciences S A, 17, Ave Du Hoggar, Pa Courtaboeuf, Bp 112, F-91944 Les Ulis Cedex A, France, 2012-06)
      The surface flux transport (SFT) model of solar magnetic fields involves empirically well-constrained velocity and magnetic fields. The basic evolution of the Sun's large-scale surface magnetic field is well described by ...