Spectral line shapes in astrophysics and related topics /

Spectral line shapes in astrophysics and related topics / / Milan S. Dimitrijevi, Luka, Popovi,.

Spectral lines, widths, and shapes are powerful tools for emitting/absorbing gas diagnostics in different astrophysical objects (from the solar system to the most distant objects in the universe--quasars). On the other hand, experimental and theoretical investigations of laboratory plasma have been...

Full description

Saved in:
Bibliographic Details
VerfasserIn:
Dimitrijevi, Milan S.,
Luka,
Popovi,
TeilnehmendeR:
Luka,
Popovi,
Place / Publishing House:[Place of publication not identified] : : MDPI - Multidisciplinary Digital Publishing Institute,, [2020]
©2020
Year of Publication:2020
Language:English
Physical Description:1 online resource (268 pages)
Tags: Add Tag
No Tags, Be the first to tag this record!
Table of Contents:
  • About the Special Issue Editors
  • Preface to "Spectral Line Shapes in Astrophysics and Related Topics"
  • Collaboration between Paris and Belgrade Observatories in Scientific Researches on Spectral Line Shapes
  • Stark Broadening from Impact Theory to Simulations
  • Quantum and Semiclassical Stark Widths for Ar VII Spectral Lines
  • Semiclassical Stark Broadening Parameters of Ar VII Spectral Lines
  • Stark Widths of Ar II Spectral Lines in the Atmospheres of Subdwarf B Stars
  • Stark Broadening of Se IV, Sn IV, Sb IV and Te IV Spectral Lines
  • Stark Widths of Na IV Spectral Lines
  • Regularities and Systematic Trends on Zr IV Stark Widths
  • Stark-Zeeman Line Shape Modeling for Magnetic White Dwarf and Tokamak Edge Plasmas: Common Challenges
  • A New Analysis of Stark and Zeeman Effects on Hydrogen Lines in Magnetized DA White Dwarfs
  • Line Shape Modeling for the Diagnostic of the Electron Density in a Corona Discharge
  • Contribution of Lienard-Wiechert Potential to the Electron Broadening of Spectral Lines in Plasmas
  • Using the Pairs of Lines Broadened by Collisions with Neutral and Charged Particles for Gas Temperature Determination of Argon Non-Thermal Plasmas at Atmospheric Pressure
  • Effect of Turbulence on Line Shapes in Astrophysical and Fusion Plasmas
  • Doppler Broadening of Spectral Line Shapes in Relativistic Plasmas
  • Active Galactic Nuclei Search
  • Models of Emission-Line Profiles and Spectral Energy Distributions to Characterize the Multi-Frequency Properties of Active Galactic Nuclei
  • Quasar Black Hole Mass Estimates from High-Ionization Lines: Breaking a Taboo?
  • Photometric and Polarimetric Interpretation of Blazar AO 0235+164 Behaviour
  • Symmetric Atom-Atom and Ion-Atom Processes in Stellar Atmospheres
  • Nonlinear Spectroscopy of Alkali Atoms in Cold Medium of Astrophysical Relevance
  • Radiative and Collisional Molecular Data and Virtual Laboratory Astrophysics
  • Rosetta Mission: Electron Scattering Cross Sections-Data Needs and Coverage in BEAMDB Database
  • The Screening Characteristics of the Dense Astrophysical Plasmas: The Three-Component Systems
  • The Application of the Cut-Off Coulomb Model Potential for the Calculation of Bound-Bound State Transitions
  • Detailed Investigation of the Electric Discharge Plasma between Copper Electrodes Immersed into Water.

Similar Items