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

Slični predmeti

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