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

被引：0
|
作者：
Ramelli, R. [1 ]
Trujillo Bueno, J. [2 ,3 ,4 ]
Bianda, M. [1 ]
Asensio Ramos, A. [2 ,3 ]
机构：
[1] Ist Ric Solari Locarno, CH-6605 Locarno, Switzerland
[2] Inst Astrofis Canarias, E-38205 Tenerife, Spain
[3] Univ La Laguna, Dept Astrofis, Tenerife, Spain
[4] CSIC, Tenerife, Spain
来源：
SOLAR POLARIZATION 6 | 2011年 / 437卷
基金：
瑞士国家科学基金会;
关键词：
HANLE; POLARIMETRY;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Over the last few years a large set of spectropolarimetric observations of prominences and spicules in the He I D-3 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.
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页码：109 / +
页数：2
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