First Metis Detection of the Helium D3 Line Polarization in a Large Eruptive Prominence

Abstract

Metis on board Solar Orbiter is the space coronagraph developed by an Italian–German–Czech consortium. It is capable of observing solar corona and various coronal structures in the visible-light (VL) and UV (hydrogen Ly α ) channels simultaneously for the first time. Here we present observations of a large eruptive prominence on 2021 April 25–26, in the VL, taken during the mission cruise phase, and demonstrate that apart from the broadband continuum emission, which is due to the Thomson scattering on prominence electrons, we detect a significant radiation in the neutral-helium D _3 line (587.6 nm), which lies within the Metis VL passband. We show how the prominence looks like in Stokes I , Q , and U . We consider two extreme cases of the prominence magnetic field, and we separate the Stokes I and Q signals pertinent to Thomson scattering and to the D _3 line. The degree of linear polarization of the D _3 line (both Q and U ) indicates the presence of the prominence magnetic field; hence Metis can serve as a magnetograph for eruptive prominences located high in the corona.

Keywords

• Solar prominences
• Coronagraphic imaging
• Solar corona
• Solar coronal mass ejections