Virtual Laboratory Astrophysics and the STARK-B database VAMDC node: a resource for electron and ion impact widths and shifts of isolated lines

Synopsis Stark broadening theories and calculations can now be considered as mature. The fast computers allow to calculate a great number of atomic data needed for accurate spectroscopic diagnostics and modeling, such as for stellar atmospheres and envelopes, laboratory and technological plasmas, an...

Full description

Saved in:
Bibliographic Details
Published in:Journal of physics. Conference series 2020-01, Vol.1412 (13), p.132052
Main Authors: Sahal-Bréchot, S, Dimitrijević, M S, Moreau, N
Format: Article
Language:English
Subjects:
Astronomical models
Astrophysics
Atmospheric models
Atomic properties
Ion impact
Laboratories
Physics
Plasmas (physics)
Sciences of the Universe
Stellar atmospheres
Virtual environments
Citations: Items that this one cites
Items that cite this one
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
Description
Summary:Synopsis Stark broadening theories and calculations can now be considered as mature. The fast computers allow to calculate a great number of atomic data needed for accurate spectroscopic diagnostics and modeling, such as for stellar atmospheres and envelopes, laboratory and technological plasmas, and laser equipments. Thus the access to these data via an on line database is essential. The STARK-B database is intended to meet this need. It contains calculated widths and shifts of isolated atomic lines due to electron and ion impacts. It is still under development and will be presented at the Conference.
ISSN:1742-6588
1742-6596
1742-6596
1742-6588
DOI:10.1088/1742-6596/1412/13/132052