Seismic structure of the upper oceanic crust revealed by in situ Q logs

In situ seismic attenuation is computed through 2.1 km of the upper oceanic crust in the vicinity of ODP Hole 504B. The results strongly tie crustal properties to seismic measurables and observed geological structures: we find that the attenuation can be used to define seismic layer boundaries and is closely related to the intensity of vertical heterogeneity. The in situ attenuation Q(-1) consists of both intrinsic and scattering contributions, but is dominated by the scattering attenuation unless porosities are near zero, when it approaches typical estimates from seismic refraction studies. The attenuation is analytically modeled by multiple backscattering from heterogeneities observed in a sonic Vp log and is found to decrease step-wise in relatively homogeneous layers from Q = 25 to Q > 300 between the top of seismic laver 2A and a sharp discontinuity at 1.3 km depth. These changes correspond with heterogeneities at 1.0-1.3 m and at 5.6-10.0 m wavelengths that we interpret to be associated with fracturing and structure of pillow basalts and lava flows in seismic layers 2A and 2B. Although seismic velocity studies suggest that the layer 2/3 boundary also occurs at about 1.3 km, the large variation in Q (140 to 460) below this depth indicates that a seismically homogeneous and uniform layer 3 has not been reached in Hole 504B. We derive an empirical relationship between attenuation and porosity Q(-1) = Q(0)(-1) e(beta phi), where Q(0)(-1) = 0.004 and beta = 25, that may be applicable at other oceanic crust locations and useful for constraining seismic inversion models.