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The CHIANTI atomic database
Young, P. R.; Mason, H. E.; Del Zanna, G. +2 more
The freely available CHIANTI atomic database was first released in 1996 and has had a huge impact on the analysis and modeling of emissions from astrophysical plasmas. It contains data and software for modeling optically thin atom and positive ion emission from low density (≲1013 cm-3) plasmas from x-ray to infrared wavelengt…
TOPICAL REVIEW The solar UV-x-ray spectrum from 1.5 to 2000 Å
Doschek, G. A.; Feldman, U.
This review illustrates the potential of UV-x-ray spectroscopy for determining the physical conditions in the solar chromosphere, transition region and corona, and how spectroscopy can be used as a tool to understand the physical mechanisms governing the atmosphere. It also illustrates the potential for understanding transient events such as solar…