We use cookies to distinguish you from other users and to provide you with a better experience on our websites. Close this message to accept cookies or find out how to manage your cookie settings.
To save content items to your account,
please confirm that you agree to abide by our usage policies.
If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account.
Find out more about saving content to .
To save content items to your Kindle, first ensure no-reply@cambridge.org
is added to your Approved Personal Document E-mail List under your Personal Document Settings
on the Manage Your Content and Devices page of your Amazon account. Then enter the ‘name’ part
of your Kindle email address below.
Find out more about saving to your Kindle.
Note you can select to save to either the @free.kindle.com or @kindle.com variations.
‘@free.kindle.com’ emails are free but can only be saved to your device when it is connected to wi-fi.
‘@kindle.com’ emails can be delivered even when you are not connected to wi-fi, but note that service fees apply.
In von Karmam-type random media, when the center wavenumber is higher than the corner wavenumber of the PSDF and the phase shift across the correlation length is not small enough, the conventional Born approximation is not applicable. To overcome this difficulty, Chapter 7 presents an ongoing study of a hybrid MC simulation using the spectrum division method for scalar/vector wavelet propagation. Taking the center wavenumber as a reference, we divide the PSDF into two parts, then we serially use the Born wide-angle scattering for the high-wavenumber spectral component and the Eikonal narrow-angle ray bending and travel distance fluctuation for the low-wavenumber spectral component. For the elastic case, the synthesized three-component RMS velocity amplitude time traces are compared with the ensemble average of the FD simulation results in realized random elastic media.
Chapter 5 presents the realization of random media for a given power spectral density function for FD simulation of scalar wavelet propagation. We verify the MC simulation results with the ensemble average of the FD simulation results in realized random media for a given power spectral density function.
Chapter 6 studies vector wave scattering in random elastic media. The Born approximation leads to PP, PS, SP, and SS scattering coefficients, from each of which we construct the corresponding PRNG of scattering angles. Using these in MC simulations, we synthesize three-component RMS velocity amplitude time traces for the radiation from a point shear dislocation (PSD) source. The simulation results are compared with the ensemble average of FD simulation results in random elastic media for a given power spectral density function.
Recommend this
Email your librarian or administrator to recommend adding this to your organisation's collection.