Based on auroral observations of a multi channels scanning photometer at Zhongshan Station, Antarctica and solar wind parameters data obtained by WIND Satellite at the upstream of the bow shock in 1997 and 1998, the dependence of the high latitude postnoon auroral intensity upon the solar wind parameters are studied quantitatively.

This article will introduce use of the latest photic-energy transfer and luminosity lighting by comparting the traditional lighting embellishment methods with the current mettiods.