Bibcode
Guglielmino, S. L.; Martínez Pillet, V.; Ruiz Cobo, B.; del Toro Iniesta, J. C.; Bellot Rubio, L. R.; Solanki, S. K.; Sunrise/IMaX Team
Referencia bibliográfica
Memorie della Societa Astronomica Italiana, v.84, p.355 (2013)
Fecha de publicación:
0
2013
Número de citas
1
Número de citas referidas
0
Descripción
We present the analysis of a flux emergence event observed with the IMaX
magnetograph flown aboard the SUNRISE balloon. IMaX took a 15' sequence
with cadence of 31 s along the Fe I line at 525.0 nm, acquiring only
Stokes I and V at 12 line positions (L12-2 mode). This sequence shows
the emergence of a flux mantle at mesogranular scale, cospatial with a
large exploding granule. An undesired cross-talk between Stokes U and V
was found in such L12-2 data. We show that the use of a modified version
of the SIR inversion code is able to remove such effect in inferring the
physical quantities of interest.