Take without loss of generality, putand write the incident field as the imaginary part of . The kinematic boundary condition on isFor a flat boundary the reflected wave is . Expanding the boundary condition in a Taylor expansion about creates the topographic sidebands of an internal gravity wave. With upward-radiating vertical wavenumber , their complex amplitudes through second order areThus the general compact result isFor the convenient nondegenerate case , all displayed sideband wavenumbers are positive. Defining , the same answer is the explicitly real formulaValidity requires a linear incident wave, an inviscid uniformly stratified bulk, an outgoing-radiation condition, strict separation from critical slopes, and small boundary excursions for every retained mode, in particular and . A vanishing is a degenerate zero-horizontal-wavenumber case and must be treated by taking the corresponding zero-amplitude limit rather than dividing by .
Articles by others on the same topic
There are currently no matching articles.