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The evaluation of liquefaction hazard is generally performed in several stages: (1) preliminary<br />
geological/geotechnical site evaluation, (2) quantitative evaluation of liquefaction potential and<br />
its potential consequences, and if necessary, (3) development of mitigation and foundation<br />
remediation programs. The scope of the investigation required is dependent not only on the<br />
nature and complexity of geologic site conditions, but also on the economics of a project and on<br />
the level of risk acceptable for the proposed structure or development.<br />
3.2 PRELIMINARY SITE INVESTIGATION<br />
A preliminary site evaluation involves establishing the topography, stratigraphy, and location of<br />
the ground water table at the project site. These geologic site evaluations must address the<br />
following questions:<br />
1. Are potentially liquefiable soils present?<br />
2. Are they saturated and/or may become saturated at some future date?<br />
3. Are they of sufficient thickness and/or lateral extent as to pose potential risk of damaging<br />
ground deformations?<br />
Sections 3.2.1 through 3.2.3 provide additional guidance regarding the questions to be addressed<br />
in the preliminary evaluation. If this evaluation can clearly demonstrate the absence of a<br />
liquefaction hazard at a project site, then it by itself may be sufficient. If some uncertainty<br />
remains, however, then a more comprehensive geotechnical study should be undertaken. The<br />
reference, “Screening Guide for Rapid Assessment of Liquefaction Hazard at Highway Bridge<br />
Sites” (Youd 1998) provides useful information for preliminary hazard evaluations. In addition,<br />
the reference, “Guidelines for Site-specific Seismic Hazard <strong>Report</strong>s for Essential and Hazardous<br />
Facilities and Major and Special-occupancy Structures in <strong>Oregon</strong>” provides recommendations<br />
for planning the site evaluation (OBGE/OBEELS 1997).<br />
3.2.1 Potentially Liquefiable Soil Types<br />
The quantitative liquefaction evaluation procedures in practice are based on the behavior of<br />
predominantly sandy soils. These methods have been validated with field studies over the last<br />
three decades, and a consensus has emerged regarding their application (Youd and Idriss 1997).<br />
Understanding the liquefaction behavior of silty and gravelly soils has, however, substantially<br />
lagged. Recommendations for these soils have been largely “rules of thumb” tempered by field<br />
observations made after earthquakes. For example, cohesive soils with a fines content greater<br />
than 30%, and whose fines either classify as “clays” based on the Unified Soil Classification<br />
System (USCS), or have a plasticity index (PI) of greater than 30%, are not generally considered<br />
potentially susceptible to soil liquefaction (Seed 1992; Youd and Idriss 1997).<br />
The influence of fine-grained soil on the liquefaction resistance of predominantly sandy soils is a<br />
topic that has received considerable attention over the past decade (Ishihara 1993, 1996;<br />
Prakash and Dakoulas 1994). Laboratory testing of silts has been performed, but to a very<br />
limited scale and with varying results (Chang 1990; Law and Ling 1992; Koester 1994; Singh<br />
1994; Prakash et al. 1998; Guo and Prakash 1999). Recent examination of fine-grained soil<br />
behavior during earthquakes and the results of laboratory tests reveal that uniformly graded loose<br />
sandy soils that contain as much as 25% to 30% non-plastic to low plasticity fines may be highly<br />
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