Abstract
The motion of vortex sheets in three-dimensional inviscid and incompressible Richtmyer–Meshkov and Rayleigh–Taylor instabilities (RMI and RTI) with axial symmetry is investigated analytically and numerically. A comparison is made with the homogeneous case where density stratification does not exist, and possible solutions are discussed for RMI and RTI. When density stratification exists, it is shown that azimuthal motion (deformation) of the vortex sheet occurs without a swirl flow. This azimuthal motion is different from the rotational motion by the swirl. We present the numerical results for the interfacial motion in RMI and RTI with axial symmetry obtain by the vortex blob method, and discuss the differences from the motion of a vortex sheet in a homogeneous fluid.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Disclaimer: 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.