Height Variation of the Vector Magnetic Field in Solar Spicules
Proving the magnetic configuration of solar spicules has hitherto been difficult due to the lack of spatial resolution and image stability during off-limb ground-based observations. We report spectropolarimetric observations of spicules taken in the He i 1083 nm spectral region with the Tenerife Infrared Polarimeter II at the German Vacuum Tower
Orozco Suárez, D. et al.
Fecha de publicación:
4
2015