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RUN SUMMARY - Model 4
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Run Description:
c  FUV/EUV/SXR backgrounds - in soft x-rays includes only enough        
c  "additional" emission to account for B band rate                     
c  cosmic abundances assumed in hot gas                                 
c  Mathis, Metzger & Panagia FUV spectrum                               
c  assumed HI column density =  4.00000e+17                             
c  Emission from an evaporative boundary to the Local Cloud             
c  model has: Rcl = 3., Rf = 30., ncl = 0.30, Tf = 1.0E+06, B0 = 2.00,  
c  Kred = 0.5, mdot = 0.313, XH(R) = 0.36, XHe(R) = 0.48                
c  XH(0) = 0.30, XHe(0) = 0.43                                          
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Element  Abundance                  Ion Density
          (ppm)         I         II         III        IV
------------------------------------------------------------------------
    H    1.00E+06      0.235     0.0677       0.00       0.00
    He   1.00E+05     0.0181     0.0120   0.000221       0.00
    C        617.   7.19E-08   0.000182   4.42E-06       0.00
    N        74.1   1.61E-05   6.37E-06   2.30E-09       0.00
    O        631.   0.000151   3.98E-05   1.21E-08       0.00
    Ne       123.   6.24E-06   2.40E-05   7.04E-06   2.08E-10
    Na       2.04   1.48E-09   5.43E-07   7.31E-08   3.45E-12
    Mg       9.12   2.19E-09   2.29E-06   4.72E-07       0.00
    Al     0.0794   1.48E-12   2.33E-08   5.28E-10   2.00E-10
    Si       11.5   1.62E-10   3.48E-06   2.36E-09   9.39E-11
    P       0.219   1.09E-11   6.46E-08   1.72E-09   5.74E-12
    S        25.1   6.04E-10   7.35E-06   2.51E-07   1.79E-11
    Ar       2.82   2.16E-07   4.27E-07   2.11E-07   3.13E-12
    Ca   0.000407   1.35E-15   2.30E-12   1.21E-10   3.34E-14
    Fe       3.55   1.18E-10   1.05E-06   2.65E-08   6.95E-12