Concerning the Existence of a ``Turbulent'' Magnetic Field in the Quiet Sun
We report on the a5F-y5Fo multiplet of Ti I and its interest for the study of ``turbulent'' magnetic fields in the quiet solar photosphere. In particular, we argue that the sizable scattering polarization signal of the 4536 Å line (whose lower and upper levels have Landé factors equal to zero), relative to the rest of the lines in the multiplet
Manso Sainz, Rafael et al.
Fecha de publicación:
10
2004