The magnetic field configuration of a solar prominence inferred from spectropolarimetric observations in the He i 10 830 Å triplet
Context. Determining the magnetic field vector in quiescent solar prominences is possible by interpreting the Hanle and Zeeman effects in spectral lines. However, observational measurements are scarce and lack high spatial resolution. Aims: We determine the magnetic field vector configuration along a quiescent solar prominence by interpreting
Orozco Suárez, D. et al.
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2014