|1||For an animation of a coronal mass ejection (CME) causing a substorm and aurora, see http://sohowww.nascom.nasa.gov/gallery/Movies/recon/reconsm.mpg|
|2||In the following, we assume observations close to the disk center for simplicity, when the vertical and LOS-component are identical. For observations far away from the disk center one has to resolve first the ambiguity and apply coordinate transformations from LOS/transverse to vertical/horizontal fields afterwards.|
|3||Solar Optical Telescope Spectro-Polarimeter|
Living Rev. Solar Phys. 9, (2012), 5
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