Journal
ASTRONOMY & ASTROPHYSICS
Volume 582, Issue -, Pages -Publisher
EDP SCIENCES S A
DOI: 10.1051/0004-6361/201526827
Keywords
atomic data; line: identification; atomic processes; radiation mechanisms: thermal
Categories
Funding
- NASA [NNX15AF25G, NNX11AC20G]
- NSF [AGS-1159353]
- STFC via the University of Strathclyde [PP/E001254/1, ST/J000892/1]
- SPACE Project under the Seventh Framework Programme of the European Commission [313188]
- NASA [NNX15AF25G, 804055] Funding Source: Federal RePORTER
- Science and Technology Facilities Council [ST/J00054X/1, ST/L000636/1, ST/J001570/1, PP/E001254/1, PP/E004857/2, ST/J000892/1] Funding Source: researchfish
- STFC [ST/J001570/1, PP/E004857/2, ST/J00054X/1, ST/L000636/1, PP/E001254/1, ST/J000892/1] Funding Source: UKRI
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We present version 8 of the CHIANTI database. This version includes a large amount of new data and ions, which represent a significant improvement in the soft X-ray, extreme UV (EUV) and UV spectral regions, which several space missions currently cover. New data for neutrals and low charge states are also added. The data are assessed, but to improve the modelling of low-temperature plasma the effective collision strengths for most of the new datasets are not spline-fitted as previously, but are retained as calculated. This required a change of the format of the CHIANTI electron excitation files. The format of the energy files has also been changed. Excitation rates between all the levels are retained for most of the new datasets, so the data can in principle be used to model high-density plasma. In addition, the method for computing the differential emission measure used in the CHIANTI software has been changed.
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