Exploring the Magnetic Fields of Solar Prominences and Spicules via He I D3 Spectropolarimetry

Bibcode
2011ASPC..437..109R
Ramelli, R.; Trujilo-Bueno, J.; Bianda, M.; Asensio Ramos, A.
Referencia bibliográfica

Solar Polarization 6. Proceedings of a conference held in Maui, Hawaii, USA on May 30 to June 4, 2010. Edited by J. R. Kuhn, D. M. Harrington, H. Lin, S. V. Berdyugina, J. Trujillo-Bueno, S. L. Keil, and T. Rimmele. San Francisco: Astronomical Society of the Pacific, 2011., p.109

Fecha de publicación:
4
2011
Número de autores
4
Número de autores del IAC
0
Número de citas
4
Número de citas referidas
4
Descripción
Over the last few years a large set of spectropolarimetric observations of prominences and spicules in the He I D3 multiplet have been collected at the observatory of the Istituto Ricerche Solari Locarno (IRSOL), using increasingly improved versions of the ZIMPOL polarimeter. The novel HAZEL inversion code of Stokes profiles generated by the joint action of the Hanle and Zeeman effects is being applied to this set of data, in order to infer the strength and geometry of the magnetic field present in these structures. This paper presents a brief overview of the most recent observations and inversions.
Tipo
Sin árbitro

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