We analysed short-period seismograms from about 250 very local events recor
ded by a network of high dynamic range short-period seismic stations deploy
ed on Mt Vesuvius to estimate the site-corrected short-period seismic atten
uation. We calculated Q(C)(-1), the inverse of the quality factor for coda
waves, for short lapse times (12 s), and Q(P)(-1) and Q(S)(-1), the inverse
of the direct body wave quality factors for P and S waves following shallo
w rah paths. We used the single scattering assumption to fit the amplitude
envelopes of the coda at different frequency bands, obtaining a Q(C)(-1) sl
owly varying with frequency, similar to values measured for other volcanoes
at the same lapse time. Site-corrected Q(P)(-1) and Q(S)(-1) were estimate
d using the frequency decay method for both P and S waves in two frequency
bands, 1-6 Hz and 15-24 Hz. Results show that Q(P)(-1) is 0.028 in bot freq
uency bands, and Q(S)(-1) is 0.015 and 0.017 at low and high frequencies re
spectively, almost independent of the frequency, and that the value of Q(P)
(-1) is about twice that of Q(S)(-1), as measured worldwide. A check was ma
de by measuring the broadening of the first P-wave pulse with station-sourc
e distance, finding Q(P)(-1) = 0.024. Using the independent estimates of Q(
C)(-1) and Q(S)(-1), we separated the intrinsic from the scattering quality
factor at Mt Vesuvius, obtaining a high scattering and a low intrinsic Q(-
1), as already observed for other volcanoes. This result confirms the hypot
hesis of the predominant role of the scattering phenomena with respect to t
he intrinsic dissipation in the seismogram formation for volcanic earthquak
es.