The Solar Orbiter Mission and its Polarimetric and Helioseismic Imager (SO/PHI)

Bibcode
2011JPhCS.271a2086G
DOI
10.1088/1742-6596/271/1/012086
Gandorfer, Achim; Solanki, Sami K.; Woch, Joachim; Martínez Pillet, Valentin; Álvarez Herrero, Alberto; Appourchaux, Thierry
Referencia bibliográfica

Journal of Physics: Conference Series, Volume 271, Issue 1, pp. 012086 (2011).

Fecha de publicación:
1
2011
Número de autores
6
Número de autores del IAC
0
Número de citas
13
Número de citas referidas
11
Descripción
We briefly outline the scientific and instrumental aspects of ESA's Solar Orbiter mission. Special emphasis is given to the Polarimetric and Helioseismic Imager, the instrument with the highest relevance for helioseismology applications, which will observe gas motions and the vector magnetic field in the photosphere at high spatial and temporal resolution.
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
Sin árbitro
Física Solar (FS)

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