In this paper,several properties of the compressible Kelvin-Helmholtz unstable waves on the magnetopause including the phase relationship between δB and dp,the polarization of δB,the spatial growth rate and it's local time effects on the geomagnetic pulsations and the response of K-H unstable waves to the variations of IMF are investigated.It is shown that knowing these properties is very helpful in understanding the generations of both MHD weves in the magnetospheric boundary region and low frequency geomagnetic pulsstions.