1 INTRODUCTION

2 SELECTING PURE RED CLUMP SAMPLE TO ESTIMATE DISTANCES
2.1 Red Clump calibration and selection
2.2 Distances

3 DATA AND METHODS
3.1 Datasets
3.2 Proper motions
3.3 Kinematic model
3.4 Fourier analysis of velocity fluctuations

4 RESULTS
4.1 GALAXIA all-sky sample: High mass Red Clump stars
4.2 Velocity fluctuations in the mid-plane for observed data
4.3 Off-plane slices and comparison with galaxia

5 DISCUSSION AND CONCLUSIONS