nalike_al97#fe15.dat

• Spontaneous Emission: Fe⁺¹⁵(i) → Fe⁺¹⁵(j) + hv
• Electron Impact Excitation: Fe⁺¹⁵(i) + e → Fe⁺¹⁵(j) + e

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 Date :Tue Oct 22, 1997
 File generated by Alessandro Lanzafame using C2ADAS
 (conversion from CHIANTI 1.01 database) 

 References (from CHIANTI 1.01 data files):

 Energy levels:  
     Theoretical energy levels:  Sampson, D. H., Zhang, H. L.,
     Fontes, C. J., 1990, ADNDT, 44, 209.
    energy levels:  Martin, W. C., Sugar, J., Musgrove, A., and Dalton, G. R., 1995, 
      NIST Database for Atomic Spectroscopy, Version 1.0, NIST Standard Reference Database 61.

 Oscillator strengths: 
    oscillator strengths:  Sampson, D. H., Zhang, H. L., and
    Fontes, C. J., 1990, ADANDT, 44, 209.
    oscillator strengths: hydrogenic values for 4f-5g
    oscillator strengths:  Wiese, W. L., Smith, M. W., and Glennon, B. M.
    Atomic Transition Probabilities, Vol I, Hydrogen through Neon,
    NSRDS-NBS-4

 Collision strengths:
    collision strengths:  Sampson, D. H., Zhang, H. L., and Fontes, C. J.,
    1990, ADANDT, 44, 209.

 Update:
    This ADF04 file contains data for (Na-like) Fe15+ but was incorrectly
    labelled internall and named like it contained (Mg-like) Fe14+.

    The designation inside the file was changed and the filename
    (and location within ADAS) was similarly modified. The old
    filename was mglike_al97#fe14.dat

    Allan Whiteford, 28/07/08

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Contributors

• Alessandro Lanzafame
• CHIANTI
• Hong Zhang
• Douglas Sampson
• Allan Whiteford