Article
Open Access
Modeling of Highly-Excited Atomic Level Populations in Astrophysical Plasmas
-
Dmitrijs Docenko
Published/Copyright:
February 18, 2017
Received: 2013-9-3
Accepted: 2013-9-17
Published Online: 2017-2-18
Published in Print: 2013-12-1
© 2013 Dmitrijs Docenko, published by De Gruyter Open
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- Physical Alternative to the Dark Energy Paradigm
- Preparation of the VIRAC Radio Telescope RT-32 for e-VLBI Observations
- First Results of the VLBI Experiment on Radar Location of the Asteroid 2012 DA14
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Keywords for this article
atomic data;
recombination lines;
supernova remnants: individual: Cassiopeia A
Creative Commons
BY-NC-ND 3.0
Articles in the same Issue
- A New Empirical Metallicity Calibration for Vilnius Photometry
- Optical Spectroscopy of a post-AGB star HD 187885
- Physical Alternative to the Dark Energy Paradigm
- Preparation of the VIRAC Radio Telescope RT-32 for e-VLBI Observations
- First Results of the VLBI Experiment on Radar Location of the Asteroid 2012 DA14
- Compressive Sensing: Analysis of Signals in Radio Astronomy
- Modeling of Highly-Excited Atomic Level Populations in Astrophysical Plasmas
