Spectro-polarimetric observations of solar magnetic fields and the SOHO/MDI calibration issue

TL;DR

This study provides a detailed analysis of solar magnetic field measurements using specific spectral lines, highlighting discrepancies with recent data and discussing implications for SOHO/MDI calibration.

Contribution

It offers high-precision measurements of magnetic field ratios in spectral lines and evaluates their implications for calibration issues in SOHO/MDI data.

Findings

Magnetic field ratio R = 1.97 ± 0.02 at disk center

Center-to-limb variation of R from 2.74 to 1.32

Results differ from recent magnetographic observations

Abstract

Comparisons of solar magnetic-field measurements made in different spectral lines are very important, especially in those lines in which observations have a long history or(and) specific diagnostic significance. The spectral lines FeI 523.3 nm and FeI525.0 nm belong to this class. Therefore, this study is devoted to a comprehensive analysis using new high-precision Stokes-meter full-disk observations. The disk-averaged magnetic-field strength ratio R = B(523.3)/B(525.0) equals 1.97 +- 0.02. The center-to-limb variation (CLV) is R = 1.74 - 2.43 mu + 3.43 mu^2, where mu is the cosine of the center-to-limb angle. For the disk center, we find R = 2.74, and for near-limb areas with mu = 0.3, R equals 1.32. There is only a small dependence of R on the spatial resolution. Our results are rather close to those published three decades ago, but differ significantly from recent magnetographic observations. An application of our results to the important SOHO/MDI magnetic data calibration issue is discussed. We conclude that the revision of the SOHO/MDI data, based only on the comparison of magnetic field measurements in the line pair FeI 523.3 nm and FeI 525.0 nm (increasing by a factor of 1.7 or 1.6 on average according to recent publications) is not obvious and new investigations are urgently needed.