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R.~Astron.~Soc.} " # "\def \gms{Geophys.~Monogr.~Series} " # "\def \mps{Meteorit.~Planet.~Sci.} " # "\def \Icarus{Icarus} " # "\def \ieee{IEEE~Trans.~Vis.~Comp.~Graphics} " # "\def \igr{International Geology Review} " # "\def \jam{J.~Appl.~Mech} " # "\def \jmps{J.~Mech.~Phys.~Solids} " # "\def \jasa{J.~Acoust.~Soc.~Am.} " # "\def \jcp{J.~Comp.~Phys.} " # "\def \jgr{J.~Geophys.~Res.} " # "\def \jpe{J.~Phys.~Earth} " # "\def \jrssb{J.~R.~Statist.~Soc.~B} " # "\def \mi{Math.~Intelligencer} " # "\def \mwr{Monthly Weather Review} " # "\def \nat{Nature} " # "\def \numa{Num.~Algor.} " # "\def \pjas{Proc.~Jpn.~Acad.~Ser.~} " # "\def \pag{Pure Appl.~Geophys.} " # "\def \pt{Phys.~Today} " # "\def \pepi{Phys.~Earth Planet.~Inter.} " # "\def \prl{Phys.~Rev.~Lett.} " # "\def \ptrsl{Phil.~Trans. 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The interseismic periods $T_{\rm int}(x)$ are defined to be the time when slip rate $V(x,t)$ is less than the long-term slip rate $V_{\rm pl}$.} } @misc{Potencynote, NOTE = {To assign slip potency and magnitudes to the simulated earthquake, a downdip width of 40 km is assumed.} }