Constraining the magnetic vector in the quiet solar photosphere and the impact of instrumental degradation
Constraining the magnetic vector in the quiet solar photosphere and the impact of instrumental degradation
Context. With the advent of next generation high resolution telescopes, our understanding of how the magnetic field is organized in the internetwork (IN) photosphere is likely to advance significantly. Aims. We aim to evaluate the extent to which we can retrieve accurate information about the magnetic vector in the IN …