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Landslides in the Sydney Basin - Geoscience Australia

Landslides in the Sydney Basin - Geoscience Australia

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Seismic Hazard <strong>in</strong> <strong>Sydney</strong>Proceed<strong>in</strong>gs of <strong>the</strong> one day workshopFigure 7 Magnitude versus length data used to correct for <strong>the</strong> overestimation of rupturelength. Open circles are for reverse, oblique-reverse, and rare strike-slip faults <strong>in</strong> regions oflow slip rate from <strong>the</strong> world-wide database of Stirl<strong>in</strong>g et al. (2002). Solid diamonds are fromNew Zealand seismological data for earthquakes <strong>in</strong> regions of low-to-moderate slip rate.Next we provide a basis to calculate a distribution of possible characteristic magnitudes and rupturelengths associated with <strong>the</strong> SED’s calculated for a fault. We br<strong>in</strong>g more knowledge to bear on <strong>the</strong>problem by impos<strong>in</strong>g constra<strong>in</strong>ts on allowable rupture lengths and widths. Fault scal<strong>in</strong>g relations arerequired for determ<strong>in</strong><strong>in</strong>g magnitude and rupture length given SED. We have discussed <strong>the</strong> choice ofsuitable scal<strong>in</strong>g relations for <strong>the</strong> <strong>Sydney</strong> Bas<strong>in</strong> <strong>in</strong> <strong>the</strong> previous section. The relations fordisplacement-length are given by Equations 8 and 11, while those for displacement-magnitude aregiven by Equations 7 and 10.Rupture lengths derived us<strong>in</strong>g Equations 8 and 11 have also been used to constra<strong>in</strong> allowable SEDvalues <strong>in</strong> that earthquake rupture lengths are likely to be limited by <strong>the</strong> maximum fault length for <strong>the</strong>dip-slip fault zones (see section “New fault data <strong>in</strong> <strong>the</strong> <strong>Sydney</strong> Bas<strong>in</strong>”). In general <strong>the</strong>se zones aretruncated by more dom<strong>in</strong>ant NW-SE oriented strike-slip faults. There is some possibility that anenergetic rupture could jump across to a neighbour<strong>in</strong>g zone, a classic example of this be<strong>in</strong>g <strong>the</strong> 1992Landers, California, earthquake (e.g. Johnson et al., 1994). To allow for such an eventuality weallow <strong>the</strong> maximum rupture length to be equal to <strong>the</strong> seismogenic thickness (18 km), i.e. to have anaspect ratio of 1:1, <strong>in</strong> 50% of cases. For <strong>the</strong> rema<strong>in</strong><strong>in</strong>g cases, <strong>the</strong> maximum rupture length is limitedto 10 km — <strong>the</strong> largest dip-slip fault zone length <strong>in</strong> <strong>the</strong> south <strong>Sydney</strong> Bas<strong>in</strong> (see section “New faultdata <strong>in</strong> <strong>the</strong> <strong>Sydney</strong> Bas<strong>in</strong>”). When <strong>the</strong> rupture length calculated for a given SED value exceeds <strong>the</strong>allowable length as def<strong>in</strong>ed above, that particular branch of <strong>the</strong> probability calculations has beendiscarded.Similarly, SED’s associated with very short rupture lengths are also excluded. This is because veryshort ruptures will also have small widths (given that we are assum<strong>in</strong>g 1:1 aspect ratios, suitable fordip-slip faults) and will thus not be capable of generat<strong>in</strong>g surface ruptures. Coalfield data show adecrease <strong>in</strong> total fault offsets towards <strong>the</strong> surface over depths of ~2 km, imply<strong>in</strong>g that surfaceruptures are driven from depths greater than this. Seismicity is also sparse <strong>in</strong> <strong>the</strong> top 2 km, so with<strong>in</strong>this depth range moderate to large earthquakes are very unlikely to nucleate. A m<strong>in</strong>imum allowablewidth (and length) of 2 km has thus been used to exclude small SED values.

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