Line intensity enhancements in stellar coronal X-ray spectra due to opacity effects

समान संसाधन

• Enhancement of optically thick to thin line intensities in solar and stellar coronal plasmas through radiative transfer effects: An angularly resolved study
  द्वारा: Kerr, F, और अन्य
  प्रकाशित: (2004)
• X-RAY-LINE WIDTHS AND CORONAL HEATING
  द्वारा: Acton, L, और अन्य
  प्रकाशित: (1981)
• Stellar coronal mass ejections
  द्वारा: Leitzinger M., और अन्य
  प्रकाशित: (2022-01-01)
• X-ray line coincidence photopumping in a solar flare
  द्वारा: Keenan, F, और अन्य
  प्रकाशित: (2017)
• Identification of Fe Emission Lines in Stellar Spectra
  द्वारा: Harper, G, और अन्य
  प्रकाशित: (2001)