Abstract
In the framework of general linear theory we study the influence of a thin stratification of fields of density and velocity of plane-parallel shear flow on dispersion curves and vertical profiles of modes of free internal gravitational waves. It is shown that an accounting of thin structural singularities can essentially change kinematic characteristics of such waves.
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.
