---------------------------------------- Type of abstract: Invited Presenter Name: Masaki Tsutsumi Status of first author: non-student ---------------------------------------- Title: Recent Multi-Instrument Mesopause Region Measurements made at Antarctica ---------------------------------------- Authors: Masaki Tsutsumi (1), Takehiko Aso (1), Masaki Ejiri (1), Makoto Taguchi (1), Akio Nomura (2), Takuya D Kawahara (2), and, Tsukasa Kitahara (2) E-mail: tutumi@uap.nipr.ac.jp (1) National Institute of Polar Research (NIPR), Japan (2) Shinshu University, Japan ---------------------------------------- Abstract: Preliminary results of recently started multi-instrument observations of Antarctic MLT region at Syowa st. (69S, 39E) are presented. The instruments are an MF radar (since April 1999), a Sodium temperature lidar (since Feb 2000), an all-sky monochromatic imager (since March 1998), and a Fabry-Perot imager (since March 2001). Two HF radars, which are part of 'SuperDARN', are also co-located. The MF radar, equiped with four receiving antennas unlike conventional three antenna systems, is successfully applied to interferometry observations of night time meteor echoes. Comparison between simultaneously observed meteor and full-correlation-analysis (FCA) winds shows a good agreement below 90km, but suggests that strong meteor echoes may disturb FCA observations above 90km during night when ionospheric return is relatively weak. The sodium lidar has time-height resolution of roughly 6min and 1 km. Day time observation of the lidar is being planed during the next austral summer. The observed wind and temperature fields by the MF radar and the lidar include atmospheric phenomena with various time and height scales. Gravity wave energy in the period band from 20min to 8 hr shows maxima around solstitial periods with a much larger activity in winter. However, the wave energy in summer is strongly polarized in the east-west direction, and their effects on the zonal background wind can be significant. ---------------------------------------- Upper Atmosphere and Ionosphere