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RUN SUMMARY - Model 1
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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 = 5.00,  
c  Kred = 0.5, mdot = 0.423, XH(R) = 0.48, XHe(R) = 0.60                
c  XH(0) = 0.33, XHe(0) = 0.50                                          
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Element  Abundance                  Ion Density
          (ppm)         I         II         III        IV
------------------------------------------------------------------------
    H    1.00E+06      0.205     0.0915       0.00       0.00
    He   1.00E+05     0.0156     0.0138   0.000211       0.00
    C        457.   6.42E-08   0.000131   4.40E-06       0.00
    N        81.3   1.41E-05   9.98E-06   6.29E-09       0.00
    O        631.   0.000133   5.43E-05   3.00E-08       0.00
    Ne       123.   4.70E-06   2.37E-05   8.05E-06   2.49E-10
    Na       2.04   1.50E-09   5.40E-07   6.26E-08   2.93E-12
    Mg       7.94   3.44E-09   1.98E-06   3.66E-07       0.00
    Al     0.0794   1.90E-12   2.28E-08   4.88E-10   1.75E-10
    Si       10.2   1.66E-10   3.01E-06   5.78E-09   9.33E-11
    P       0.219   1.32E-11   6.29E-08   1.92E-09   6.87E-12
    S        22.4   6.54E-10   6.38E-06   2.56E-07   2.04E-11
    Ar       2.82   1.50E-07   4.22E-07   2.63E-07   6.19E-12
    Ca   0.000407   3.05E-15   2.65E-12   1.18E-10   3.56E-14
    Fe       3.16   1.45E-10   9.01E-07   3.49E-08   1.21E-11