Spectro-polarimetric analysis of a short lived solar active region

Bibcode
2019NCimC..42...10V
DOI
10.1393/ncc/i2019-19010-5
Viavattene, G.; Zuccarello, F.; Collados Vera, , M.; Ruiz Cobo, B.
Referencia bibliográfica

Nuovo Cimento C Geophysics Space Physics C

Fecha de publicación:
1
2019
Número de autores
4
Número de autores del IAC
2
Número de citas
0
Número de citas referidas
0
Descripción
The physical processes related to the formation, evolution and disappearance of solar active regions are not completely clear. High-resolution solar spectro-polarimetric data are needed to investigate these processes with unprecedented details. Here we present the analysis of the short-lived NOAA 12549 active region using high-resolution spectro-polarimetric data acquired with the GREGOR solar telescope and the GRIS instrument, inverted using the SIR code.

Proyectos relacionados
Imagen del Proyecto
Magnestismo Solar y Estelar
Los campos magnéticos son uno de los ingredientes fundamentales en la formación de estrellas y su evolución. En el nacimiento de una estrella, los campos magnéticos llegan a frenar su rotación durante el colapso de la nube molecular, y en el fin de la vida de una estrella, el magnetismo puede ser clave en la forma en la que se pierden las capas
Tobías
Felipe García
En ejecución
Tipo
Con árbitro
Física Solar (FS)

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