Identification of Spectral Lines in the 500–1600 A Wavelength Range of Highly Ionized Ne, Na, Mg, Ar, K, Ca, Ti, Cr, Mn, Fe, Co, and Ni Emitted by Flares (T_e≥ 3 x 10⁶K) and Their Potential Use in Plasma Diagnostics

This publication has 50 references indexed in Scilit:

• The solar disk spectrum between 660 and 1175 Å (first order) obtained by SUMER on SOHO
  Astronomy and Astrophysics Supplement Series, 1997
• Transitions in Fluorine-Like Ions
  Atomic Data and Nuclear Data Tables, 1994
• Atomic Data and Spectral Line Intensities for C-like Ca XV
  Atomic Data and Nuclear Data Tables, 1993
• Atomic data and spectral line intensities for Ne-like Fe XVII
  Atomic Data and Nuclear Data Tables, 1992
• Collision strengths and excitation rate coefficients for transitions in Fe XXI
  The Astrophysical Journal Supplement Series, 1991
• Effective collision strengths among fine-structure levels of CA XV: erratum
  The Astrophysical Journal Supplement Series, 1991
• Atomic data and spectral line intensities for the nitrogen isoelectronic sequence (Ar XII through Kr XXX)
  Atomic Data and Nuclear Data Tables, 1989
• A comparison of theoretical and solar-flare intensity ratios for the Fe XIX X-ray lines
  Monthly Notices of the Royal Astronomical Society, 1989
• Discrimination ofn=2?2 UV transitions of he-like ions in a recoil light source
  The European Physical Journal D, 1986
• Theoretical atomic structure and electron scattering data for ions in the nitrogen isoelectronic sequence: MG VI, Si VIII, S x, A XII and Ca XIV
  Monthly Notices of the Royal Astronomical Society, 1980