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Historical Seismograms - Evidence from the AD 2000 Izu Islands ...

Historical Seismograms - Evidence from the AD 2000 Izu Islands ...

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88 S. Stein, E. A. Okal and D. A. WiensDecember 15, 1947 Event 45IFigure 1. Sample record (top left), first motions (bottom left), and location (right)for <strong>the</strong> 1947 Ms = 6.9 sou<strong>the</strong>rn Pacific earthquake [see Okal (1984) for details]. The firstmotion data (open circles dilatational; closed ones compressional) preclude <strong>the</strong> most likelytectonic setting, as left-lateral strike-slip would be <strong>the</strong> expected mechanism on a nearbytransform fault.Given enough data, and provided instrument responses are known, waveformmodeling can be quite effective. Figure 2 shows P and SH waveforms for a 1944M = 7.2 earthquake near <strong>the</strong> Chagos-Laccadive Ridge in <strong>the</strong> central Indian Ocean(Wiens, 1985). Syn<strong>the</strong>tic body waves, generated for a thrust fault geometry derived<strong>from</strong> first motions and surface waves, match <strong>the</strong> data well and constrain <strong>the</strong> focaldepth to about 12 km for P- and SH-waves at various stations. This modeling alsoshows <strong>the</strong> seismic moment of this event, 1.5 x loz7 dyne-cm is unusually large foran “intraplate” event.Surface wave modeling can also be quite valuable. With abundant modern data,azimuthal coverage is generally adequate to construct an observed radiation pattern<strong>from</strong> equalized spectral amplitudes. This is hard to obtain for historical events. Itis, however, often possible to employ <strong>the</strong> ratio of Love to Rayleigh waves at a smallnumber of stations to provide a valuable constraint, especially if one nodal planeis constrained by first motions. Figure 3 shows an example for <strong>the</strong> 1939 Ms = 7.2earthquake on <strong>the</strong> Ninetyeast Ridge, in <strong>the</strong> central Indian Ocean (Stein and Okal,1978). First motions, mostly taken <strong>from</strong> <strong>the</strong> ISS, are scattered but show two cleargroups which a nodal plane must bisect. Additional constraints come <strong>from</strong> surfacewave ratios at two stations. Figure 3 shows a strainmeter record; after bandpass

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