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

Παρόμοια τεκμήρια

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