  We study the neutrino-induced production of nuclides in explosive supernova
nucleosynthesis for progenitor stars with solar metallicity and initial main
sequence masses between 15 M$_\odot$ and 40 M$_\odot$. We improve previous
investigations i) by using a global set of partial differential cross sections
for neutrino-induced charged- and neutral-current reactions on nuclei with
charge numbers $Z < 76 $ and ii) by considering modern supernova neutrino
spectra which have substantially lower average energies compared to those
previously adopted in neutrino nucleosynthesis studies. We confirm the
production of $^7$Li, $^{11}$B, $^{138}$La, and $^{180}$Ta by neutrino
nucleosynthesis, albeit at slightly smaller abundances due to the changed
neutrino spectra. We find that for stars with a mass smaller than 20 M$_\odot$,
$^{19}$F is produced mainly by explosive nucleosynthesis while for higher mass
stars it is produced by the $\nu$ process. We also find that neutrino-induced
reactions, either directly or indirectly by providing an enhanced abundance of
light particles, noticeably contribute to the production of the radioactive
nuclides $^{22}$Na and $^{26}$Al. Both nuclei are prime candidates for
gamma-ray astronomy. Other prime targets, $^{44}$Ti and $^{60}$Fe, however, are
insignificantly produced by neutrino-induced reactions. We also find a large
increase in the production of the long-lived nuclei $^{92}$Nb and $^{98}$Tc due
to charged-current neutrino capture.
