Implications of meteor observations by the MU radar

We report high resolution meteor echo observations using the Kyoto Universi ty Middle and Upper (MU) Atmosphere 46.5 MHz Radar. When the MU radar was p ointed perpendicular to the geomagnetic field Lines (B), numerous long-live d range spread trail echoes were observed which were largely absent when th e beam was pointed in the vertical and parallel-to-B directions. This shows that this type of trail echo is largely due to scattering structures align ed along B. Additionally, nearly all the head echoes displaying an along-th e-beam velocity component were followed by range spread echoes in the perpe ndicular-to-B pointing geometry. This demonstrates that meteoric field alig ned irregularity is present in essentially all meteors up to the detection limit of the MU radar. Practically all the spectra are limited within a ban dwidth corresponding to a Doppler shift of 320 m/s, suggesting that the two stream instability is absent most of the time. Meteoric field aligned stru ctures can be a potential error source for aeronomical applications if they are not appropriately considered.