Vector Magnetic Fields in Prominences - Part Two Hei d3 Stokes Profiles Analysis for Two Quiescent Prominences
Abstract
The Stokes components of He I D3 emission in two quiescent prominences, using full spectral profile measurements, are analyzed to derive vector magnetic fields. Two independently developed schemes, based on the Hanle effect, are used for interpretation. They involve solutions of the statistical equilibrium equations for the He I D3 multiplet, including the effect of coherency and full level crossing, which predict the magnetic field dependence of the observed polarization. Derived magnetic field vector solutions for each pair of linear polarization Stokes profiles corresponding to an observational point in the prominence are, intrinsically, not uniquely determined, and a set of possible solutions is usually obtained. However, mutual consistency of these solutions with those independently predicted by the form of the circular polarized component, allow, in almost all cases, rejection of all solutions of a set except one symmetrical pair. Of such a pair, a unique solution can be determined with a high confidence level by reference to independent potential field information. Field vectors are found usually to be close to horizontal and normal to the prominence surface, but extreme exceptions are found. Field values range from 6 G to 60 G. The derived vectorfield configurations and their magnitudes are briefly discussed relative to these prominences and to different quiescent prominence models.
- Publication:
-
Solar Physics
- Pub Date:
- April 1985
- DOI:
- 10.1007/BF00149684
- Bibcode:
- 1985SoPh...96..277Q
- Keywords:
-
- D Lines;
- Helium Ions;
- Solar Magnetic Field;
- Solar Prominences;
- Spectrum Analysis;
- Stokes Theorem (Vector Calculus);
- Circular Polarization;
- Emission Spectra;
- Linear Polarization;
- Solar Physics;
- Field Vector;
- Linear Polarization;
- Spectral Profile;
- Magnetic Field Dependence;
- Vector Magnetic Field