“…) and appear to propagate westwards following the motion of the Sun (e.g., Chapman and Lindzen, 1970). Remote sensing investigations of the MLT region using ground-based radar (e.g., Avery et al, 1989;Vincent et al, 1989;Franke and Thorsen, 1993;Thayaparan, 1997) and spaceborne optical sensors on the Upper Atmospheric Research Satellite (UARS) (e.g., Hays et al, 1994;Burrage et al, 1995;Shepherd et al, 1995;McLandress et al, 1996;Geller et al, 1997) have provided a wealth of data on the local time and global scale effects of solar tides on the wind field. Together with recent model developments such as the Global Scale Wave Model (GSWM) Hagan, 1996), these studies have revealed a complex, yet understandable, mean global variation Copy right c The Society of Geomagnetism and Earth, Planetary and Space Sciences (SGEPSS); The Seismological Society of Japan; The Volcanological Society of Japan; The Geodetic Society of Japan; The Japanese Society for Planetary Sciences.…”