Magnetic Maps of Prominences from Full Stokes Analysis of the He I D3 Line

By R. Casini, A. Ariste, Steven Tomczyk, B. Lites. 2003

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Physics of Solar Prominences: II—Magnetic Structure and Dynamics (2010, background): “Casini et al. (2003) published the first map of the vector field in a prominence.”
QUIESCENT PROMINENCE DYNAMICS OBSERVED WITH THE HINODE SOLAR OPTICAL TELESCOPE. I. TURBULENT UPFLOW PLUMES (2010, background): “Later multispectral measurements confirm the earlier findings but find field strengths in the 20–80 G range (López Ariste & Casini 2003; Casini et al. 2003).”
Emergence of a Helical Flux Rope under an Active Region Prominence (2008, methodology): “This value is consistent with active-region prominences according to previous measurements of magnetic fields (e.g., Tandberg-Hanssen and Malville 1974; Wiehr and Stellmacher 1991; Casini et al. 2003; Okamoto et al. 2007), and this flux rope is strong enough to support prominences.”
Advanced Forward Modeling and Inversion of Stokes Profiles Resulting from the Joint Action of the Hanle and Zeeman Effects (2008, methodology): “…interpreting spectropolarimetric observations of solar plasma structures in the He I D3 multiplet (e.g., Landi Degl’Innocenti 1982; Bommier et al. 1994; Casini et al. 2003; López Ariste & Casini 2005) and in the He I 10830 Å triplet (e.g., Trujillo Bueno et al. 2002b, 2005; Merenda et al. 2006).”