Towards the next frontier in high precision solar polarimetry: 10^-4
In the last two decades, solar physics has greatly explored the 10^-3 polarimetric sensitivity level (referred to the continuum intensity). This has provided us with a quantitatively accurate picture of the photospheric magnetism for mean longitudinal fields in the range of about 5 Gauss. However, the same 10^-3 detection levels translate into a
Martinez Pillet, V.
Advertised on:
12
2012