Enhancement of optically thick to thin line intensities in solar and stellar coronal plasmas through radiative transfer effects: An angularly resolved study

Eitemau Tebyg

• Line intensity enhancements in stellar coronal X-ray spectra due to opacity effects
  gan: Rose, S, et al.
  Cyhoeddwyd: (2008)
• An analytic geometry-variant approach to line ratio enhancement above the optically thin limit
  gan: Kerr, F, et al.
  Cyhoeddwyd: (2005)
• Line radiation effects in laboratory and astrophysical plasmas
  gan: Kerr, F, et al.
  Cyhoeddwyd: (2006)
• An Angular Diameter Measurement of β UMa via Stellar Intensity Interferometry with the VERITAS Observatory
  gan: A. Acharyya, et al.
  Cyhoeddwyd: (2024-01-01)
• PLASMA AND MAGNETIC FIELD CHARACTERISTICS OF SOLAR CORONAL MASS EJECTIONS IN RELATION TO GEOMAGNETIC STORM INTENSITY AND VARIABILITY
  gan: Liu, Ying D., et al.
  Cyhoeddwyd: (2015)