Abstract

We present test results on the simultaneous inversion of the Stokes profiles of the He I lines at 587.6 nm (D₃) and 1083.0 nm in prominences (90° scattering). We created data sets of synthetic Stokes profiles for the case of quiescent prominences (B
Show moreWe present test results on the simultaneous inversion of the Stokes profiles of the He I lines at 587.6 nm (D₃) and 1083.0 nm in prominences (90° scattering). We created data sets of synthetic Stokes profiles for the case of quiescent prominences (B < 200 G), assuming a conservative value of 10⁻³ of the peak intensity for the polarimetric sensitivity of the simulated observations. In this work, we focus on the error analysis for the inference of the magnetic field vector, under the usual assumption that the prominence can be assimilated to a slab of finite optical thickness with uniform magnetic and thermodynamic properties. We find that the simultaneous inversion of the two lines significantly reduces the errors on the inference of the magnetic field vector, with respect to the case of single-line inversion. These results provide a solid justification for current and future instrumental efforts with multi-line capabilities for the observations of solar prominences and filaments. Show less