Solar Lower Atmosphere and Magnetism

Imaging and spectroscopy of the Sun in the near UV, visible and near IR:

High-resolution solar imaging using phase diversity image reconstruction techniques
High-precision spectro-polarimetry (Zeeman polarimetry and Hanle diagnostics of scattering polarization)

Facilities used for the observations include the new Swedish 1-m Solar Telescope (NSST), the German Vacuum Tower Telescope (VTT), the GREGOR telescope and the THEMIS telescope.

Solar Lower Atmosphere and Magnetism Group Homepage

A. Lagg
29-03-2011