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Solar Lower Atmosphere and Magnetism
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Solar Lower Atmosphere and Magnetism

SLAM 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

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