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    • Fossati, L.; Kochukhov, O.; Jenkins, James Stewart; Stancliffe, R. J.; Haswell, C. A.; Elmasli, A.; Nickson, E. (2013)
      Aims. Our understanding of magnetic fields in late-type stars is strongly driven by what we know of the solar magnetic field. For this reason, it is crucial to understand how typical the solar dynamo is. To do this we ...