A 3D sunspot model derived from an inversion of spectropolarimetric observations and its implications for the penumbral heating
Aims:I deduced a 3D sunspot model that is in full agreement with spectropolarimetric observations, in order to address the question of a possible penumbral heating process by the repetitive rise of hot flow channels. Methods: I performed inversions of spectropolarimetric data taken simultaneously in infrared (1.5 μm) and visible (630 nm) spectral
Beck, C.
Fecha de publicación:
3
2008