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In [19], it was shown that using separate CA models for strong RSS values improves the positioning accuracy.
These findings are quite important for the assumption of source models for strong motion predictions from such huge interplate earthquakes.
We construct characterized source models for strong ground-motion prediction using the procedure of HERP (2008b) and Irikura and Miyake (2010).
Areas of anomalous GF amplitude are important for the asperity/SMGA setting of source models for strong motion predictions for megathrust earthquakes.
We use the two methodologies to construct characterized source models for strong ground-motion simulations of the 1891 Nobi earthquake, which was a multi-segment rupture event occurring in the Nobi active-fault system.
Geese are models for strong family values.
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Building similar $L$-like models for stronger large cardinals, such as strong, or Woodin, is much harder.
The branch of set theory known as inner model theory is devoted to the construction of such "L-like" models for stronger and stronger large cardinal axioms.
He paid tribute to his mother as his role model for strong female leads and said Hollywood is slowly changing.
Irikura and Miyake (2001) have proposed a characterized source model for strong ground-motion prediction.
Kuriyama and Iwata (2011) examined the construction methodology of a source model for strong ground motion prediction of a scenario earthquake for the Nobi earthquake.
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Justyna Jupowicz-Kozak
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