Corpus ID: 226289613

CHIANTI -- an atomic database for emission lines -- Paper XVI: Version 10, further extensions

@article{Zanna2020CHIANTIA,
  title={CHIANTI -- an atomic database for emission lines -- Paper XVI: Version 10, further extensions},
  author={G. D. Zanna and K. Dere and P. R. Young and E. Landi},
  journal={arXiv: Atomic Physics},
  year={2020}
}
  • G. D. Zanna, K. Dere, +1 author E. Landi
  • Published 2020
  • Physics
  • arXiv: Atomic Physics
  • We present version 10 of the CHIANTI package. In this release, we provide updated atomic models for several helium-like ions and for all the ions of the beryllium, carbon and magnesium isoelectronic sequences that are abundant in astrophysical plasmas. We include rates from large-scale atomic structure and scattering calculations that are in many cases a significant improvement over the previous version, especially for the Be-like sequence, which has useful line diagnostics to measure the… CONTINUE READING
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    Fe VII emission lines in the wavelength range 193-197 \AA.
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