INTEGRATION OF SEISMIC PROFILES WITH OBSERVATIONS FROM THE SITE

Two single-channel, seismic-reflection profiles were obtained across the site by the JOIDES Resolution during Leg 149 (Fig. 1 and Fig. 2). Consequently, these profiles are less distinct than multichannel profiles. Nevertheless, they show a number of reflectors that have been recognized on a regional scale in the vicinity of the Iberia Abyssal Plain and that have been dated by tracing them back to Leg 103 sites west of Galicia Bank (Mauffret and Montadert, 1988) and to Site 398 near Vigo Seamount (Groupe Galice, 1979). JOIDES Resolution Line 3 crosses the site in an east-west direction and one of these reflectors, separating acoustic formations 1A and 1B (Groupe Galice, 1979; Fig. 1), appears to cross the site. This reflector marks a regional unconformity produced by the folding that accompanied the Miocene compressional episode in the Rif-Betic Mountains to the south. The reflector has a rough indistinct surface near the site, which makes it difficult to recognize. The acoustic basement, which is composed of many hyperbolae, is not clearly seen at the base of the sedimentary section either.

Only very limited downhole measurements were obtained at Site 899; downhole velocity logs were obtained from 394 to 455 mbsf. However, the results of two sonobuoy lines shot over the Iberia Abyssal Plain (Whitmarsh, Miles, and Mauffret, 1990) were used to convert from two-way traveltime to depth (Fig. 66 in "Site 897" chapter, "Integration of Seismic Profiles with Observations from the Site" section, this volume). Thus, we did estimate the downhole depths of the formation 1A/1B and basement reflectors seen in the JOIDES Resolution Line 3 seismic-reflection profile; these are summarized in Table 22.

Findings

  1. Reflector R1 (computed to be at 200 mbsf) is difficult to recognize in the vicinity of the site. Normally, it can be discerned from the angular relationship between the tilted and folded underlying, and horizontal onlapping, reflectors (Fig. 1 and Fig. 2). R1 may correlate with the onset at this site of a 3 m.y., late Miocene, hiatus that occurs at about 170 mbsf. This correlation implies a low interval velocity of 1.62 km/s from 0 to 170 mbsf and an improbable higher velocity between 170 mbsf and basement. It seems most likely, therefore, that R1 was picked too late in the seismic section, but the quality of the data does not allow us to make a more objective estimate.
  2. The acoustic basement reflector has been computed to be at 360 mbsf. This reflector is evident in reflection profiles as a broad hyperbola, apparently within the sedimentary column. It correlates with the serpentinite breccia at the top of Unit IV at 370 mbsf. The computed interval velocity from 0 to 370 mbsf is 1.95 km/s.

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