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RUN SUMMARY - Model 9
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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 = 1.3E+06, B0 = 5.00,  
c  Kred = 0.5, mdot = 0.679, XH(R) = 0.59, XHe(R) = 0.58                
c  XH(0) = 0.53, XHe(0) = 0.41                                          
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Element  Abundance                  Ion Density
          (ppm)         I         II         III        IV
------------------------------------------------------------------------
    H    1.00E+06      0.228     0.0826       0.00       0.00
    He   1.00E+05     0.0156     0.0150   0.000410       0.00
    C        162.   2.22E-08   4.86E-05   1.68E-06       0.00
    N        36.3   6.67E-06   4.61E-06   2.30E-09       0.00
    O        275.   6.45E-05   2.10E-05   9.71E-09       0.00
    Ne       123.   3.87E-06   2.35E-05   1.08E-05   3.12E-10
    Na       2.04   6.35E-10   5.41E-07   9.22E-08   1.94E-12
    Mg       3.16   2.54E-09   7.81E-07   1.99E-07       0.00
    Al     0.0794   1.93E-12   2.41E-08   3.84E-10   2.35E-10
    Si       3.98   5.81E-11   1.23E-06   4.95E-09   3.75E-11
    P       0.219   1.16E-11   6.65E-08   1.50E-09   7.38E-12
    S        8.71   2.27E-10   2.59E-06   1.12E-07   1.03E-11
    Ar       2.82   1.89E-07   4.09E-07   2.79E-07   5.85E-12
    Ca   0.000407   4.28E-15   2.16E-12   1.24E-10   2.84E-14
    Fe       1.26   9.87E-11   3.80E-07   1.17E-08   3.41E-12