Investigating and comparing the IRIS spectral lines Mgii, Si iv, and Cii for flare precursor diagnostics

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作者：
Zbinden, Jonas [1 ,2 ]
Kleint, Lucia [1 ,2 ]
Panos, Brandon [1 ,2 ]
机构：
[1] Astronomical Institute of the University of Bern, Sidlerstrasse 5, Bern,3012, Switzerland
[2] University of Geneva, 7, Route de Drize, Carouge,1227, Switzerland
来源：
Astronomy and Astrophysics | 2024年 / 689卷
关键词：
This work was supported by a SNSF PRIMA grant. We are grateful to LMSAL for allowing us to download the IRIS database. IRIS is a NASA small explorer mission developed and operated by LMSAL with mission operations executed at NASA Ames Research Center and major contributions to downlink communications funded by ESA and the Norwegian Space Centre. This research has made use of NASA's Astrophysics Data System Bibliographic Services. Some of our calculations were performed on UBELIX (http://www. id.unibe.ch/hpc); the HPC cluster at the University of Bern.We are also very thankful for the insightful discussions with Dr. Philip Judge about line formation of Mgii h&k;
D O I：
10.1051/0004-6361/202347824
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