by Qev » Wed Aug 30, 2006 3:16 pm
As I understand it, the orientation of the local magnetic field on the surface of the Sun changes how electrons there behave. Due to these differences, when these electrons emit light, areas with differing magnetic fields will show differences in the separation of spectral lines (Zeeman splitting) as well as differing degrees of polarization. Using a spectrograph and a polarizing filter, you can then determine the strength and orientation of the magnetic field in a given spot.
As I understand it, the orientation of the local magnetic field on the surface of the Sun changes how electrons there behave. Due to these differences, when these electrons emit light, areas with differing magnetic fields will show differences in the separation of spectral lines (Zeeman splitting) as well as differing degrees of polarization. Using a spectrograph and a polarizing filter, you can then determine the strength and orientation of the magnetic field in a given spot.