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RUN SUMMARY - Model 3
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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 =  9.00000e+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 = 0.432, XH(R) = 0.60, XHe(R) = 0.55                
c  XH(0) = 0.53, XHe(0) = 0.36                                          
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Element  Abundance                  Ion Density
          (ppm)         I         II         III        IV
------------------------------------------------------------------------
    H    1.00E+06      0.233     0.0800       0.00       0.00
    He   1.00E+05     0.0171     0.0139   0.000248       0.00
    C        166.   2.28E-08   5.05E-05   1.43E-06       0.00
    N        34.7   6.75E-06   4.11E-06   1.59E-09       0.00
    O        275.   6.57E-05   2.04E-05   7.19E-09       0.00
    Ne       123.   5.12E-06   2.49E-05   8.46E-06   1.86E-10
    Na       2.04   7.41E-10   5.70E-07   6.77E-08   2.05E-12
    Mg       3.09   2.36E-09   7.99E-07   1.65E-07       0.00
    Al     0.0794   1.85E-12   2.42E-08   3.71E-10   2.38E-10
    Si       4.07   5.77E-11   1.27E-06   4.31E-09   3.39E-11
    P       0.219   1.14E-11   6.72E-08   1.28E-09   6.17E-12
    S        8.91   2.30E-10   2.69E-06   9.68E-08   7.10E-12
    Ar       2.82   2.07E-07   4.25E-07   2.50E-07   3.92E-12
    Ca   0.000407   3.88E-15   2.14E-12   1.25E-10   2.10E-14
    Fe       1.26   8.86E-11   3.83E-07   1.12E-08   2.62E-12