0029                  Table 10048Elemental Abundance Ratios Measured with the0047High Energy Cosmic Ray Experiment on ISEE-300040044Ratio  Value    Uncertainty         Ref.00040042 B/C   0.261    (+0.009,-0.009)      a00040042 C/O   0.976    (+0.034,-0.034)      a0042 N/O   0.251    (+0.006,-0.006)      a00040042 F/Si  0.118    (+0.010,-0.010)      b0042Ne/Si  0.982    (+0.051,-0.051)      b0042Na/Si  0.189    (+0.011,-0.011)      b0042Mg/Si  1.330    (+0.040,-0.040)      b0042Al/Si  0.211    (+0.009,-0.009)      b0042 P/Si  0.037    (+0.003,-0.003)      b0042 S/Si  0.176    (+0.008,-0.008)      b0042Cl/Si  0.036    (+0.003,-0.003)      b0042Ar/Si  0.073    (+0.005,-0.005)      b0042 K/Si  0.064    (+0.005,-0.005)      b0042Ca/Si  0.154    (+0.009,-0.009)      b0042Fe/Si  0.719    (+0.054,-0.054)      b0042Sc/Fe  0.0487   (+0.0044,-0.0037)    c0042Ti/Fe  0.1630   (+0.0084,-0.0077)    c00040042 V/Fe  0.0787   (+0.0053,-0.0047)    c0042Cr/Fe  0.1527   (+0.0074,-0.0067)    c0042Mn/Fe  0.0938   (+0.0056,-0.0050)    c0042Co/Fe  0.0085   (+0.0018,-0.0013)    c0042Co/Fe  0.0085   (+0.0018,-0.0013)    c0042Ni/Fe  0.0482   (+0.0039,-0.0033)    c0042Cu/Fe <0.00083                       c0042Zn/Fe  0.00074  (+0.00072,-0.00022)  c00040014References0067 a "The Isotopic Composition of Cosmic Ray Boron and Nitrogen",0068   K. E.  Krombel and M. E. Wiedenbeck, Ap. J., 328, 940 (1988).0072 b "Composition Measurements from ISEE-3: Fluorine through Calcium",0072   R. A. Leske and M. E. Wiedenbeck, 23rd Internat. Cosmic Ray Conf.0033   (Calgary), submitted 1993.0069 c "The Elemental and Isotopic Composition of Galactic Cosmic-Ray0070   Nuclei from Scandium through Nickel", R. A. Leske, Ap. J., 405,0018   567 (1993).^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^^