Disambiguation of Vector Magnetograms by Stereoscopic Observations from the Solar Orbiter/Polarimetric and Helioseismic Imager (PHI) and the Solar Dynamic Observatory (SDO)/Helioseismic and Magnetic Imager (HMI)
Spectropolarimetric reconstructions of the photospheric vector magnetic field are intrinsically limited by the so-called 180\(^\circ\) ambiguity in the orientation of the transverse component. The successful launch and operation of Solar Orbiter has made the removal of the 180\(^\circ\) ambiguity po...
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Veröffentlicht in: | arXiv.org 2021-12 |
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Sprache: | eng |
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