Numerical Modeling of the 1964 Alaska Tsunami Web project by Elena Suleimani, PHYS-645 |
the model and grids
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We calculate the extent of inundation caused by tsunami
waves using numerical modeling of tsunami wave runup. The model is based
on the vertically integrated nonlinear shallow water equations of motion
and continuity with friction and Coriolis force (Murty, 1984). We apply
a space-staggered grid, which requires either sea level or velocity as
a boundary condition. The first order scheme is applied in time and the
second order scheme is applied in space. Integration is performed along
the north–south and west–east directions separately as described
by Kowalik and Murty (1993).
The region shown in the above figure has a number of embedded grids. The first grid of 24-second resolution covers the lower part of Cook Inlet and waters around Kodiak Island. The two 8-second grids cover Kachemak Bay and waters adjacent to Resurrection Bay. There are several 3-second resolution grids covering communities of Homer, Seldovia and Seward. Finally, there are 1-second resolution grids where runup calculations are performed. In these grids, the combined bathymetric and topographic data allow for application of the moving boundary condition as well as calculating the runup heights and extent of the inundation.
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