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RUN SUMMARY - Model 15
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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 = 0.33, Tf = 1.3E+06, B0 = 5.00,  
c  Kred = 0.5, mdot = 0.684, XH(R) = 0.58, XHe(R) = 0.57                
c  XH(0) = 0.51, XHe(0) = 0.40                                          
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Element  Abundance                  Ion Density
          (ppm)         I         II         III        IV
------------------------------------------------------------------------
    H    1.00E+06      0.252     0.0880       0.00       0.00
    He   1.00E+05     0.0176     0.0160   0.000409       0.00
    C        155.   2.47E-08   5.10E-05   1.66E-06       0.00
    N        35.5   7.30E-06   4.77E-06   2.19E-09       0.00
    O        275.   7.12E-05   2.23E-05   9.50E-09       0.00
    Ne       123.   4.53E-06   2.60E-05   1.13E-05   2.97E-10
    Na       2.04   7.43E-10   5.98E-07   9.56E-08   1.84E-12
    Mg       3.24   2.99E-09   8.88E-07   2.11E-07       0.00
    Al     0.0794   2.24E-12   2.64E-08   4.03E-10   2.39E-10
    Si       4.07   6.89E-11   1.38E-06   5.20E-09   3.76E-11
    P       0.219   1.35E-11   7.29E-08   1.55E-09   7.25E-12
    S        8.91   2.72E-10   2.91E-06   1.20E-07   1.03E-11
    Ar       2.82   2.16E-07   4.49E-07   2.94E-07   5.68E-12
    Ca   0.000407   5.23E-15   2.52E-12   1.36E-10   2.86E-14
    Fe       1.29   1.16E-10   4.26E-07   1.26E-08   3.40E-12