Speaker
Klaus G. Strassmeier
(Leibniz-Institut fuer Astrophysik Potsdam (AIP))
Description
I will discuss Doppler imaging (DI) and Zeeman-Doppler imaging (ZDI)
techniques to map stellar magnetic fields and differential surface
rotation and possibly meridional flows on cool stars. Emphasis will be
on the techniques and their limitations but I will also highlight
previous results and present some of our more recent DI and ZDI maps.
An outlook is given for observing programs with the next generation of
large telescope and spectrographs.
Primary author
Klaus G. Strassmeier
(Leibniz-Institut fuer Astrophysik Potsdam (AIP))
