  Existing experimental data for the breakup of 8B at energies from 30 to 1000
MeV/nucleon on light through heavy targets are analyzed in detail in terms of
an extended Glauber model. The predictions of the model are in excellent
agreement with independent reaction data (reaction cross sections and parallel
momentum distributions for core like fragments). Final state interactions have
been included in the Coulomb dissociation component. We extract asymptotic
normalization coefficients (ANC) from which the strophysical factor S17(0) for
the key reaction for solar neutrino production, 7Be(p,gamma)8B, can be
evaluated. Glauber model calculations using different effective interactions
give consistent, though slightly different results. The differences give a
measure of the precision one can expect from the method. The unweighted average
of all ANCs extracted leads to S17(0)=18.7+/-1.9 eVb. The results of this new
analysis are compared with the earlier one. They are consistent with the values
from most direct measurements and other indirect methods.
