SWG2: Observing and Quantifying Solar Magnetism
Advance our understanding of solar magnetism, by engaging with the scientific community to further the study of fundamental plasma processes (kinetic, magnetic, radiative) and advance the development of polarized radiation transfer models and new diagnostic tools.
- Design, execution, and interpretation of solar magnetism observations
- Science definition and development of spectro-polarimetric instrumentation
- Development and maintenance of spectro-polarimetric data pipelines
The magnetism of the solar atmosphere drives and shapes all phenomena of space weather(SW)