Abstract
Summary The existence of numerous primary upper mantle travel-time branches contributes significantly to the character of short period body wave spectra observed at intermediate (10°–35°) epicentral distances. The effects can be predicted through the computation of synthetic mantle response functions by the Cagniard-de Hoop algorithm. This method allows definition of the changes in the mantle response as a function of epicentral distance.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
