Fig. 1. Seeing distribution of Subaru telescope in the whole year^[3]

Fig. 2. Measurement results of slope of different mirror reflection distance R measured by autocollimation method ^[4]

Fig. 3. Measuring system of pentaprism scanning plane^[5]

Fig. 4. Curvature/slope wavefront sensor^[7-8]

Fig. 5. Using Hartmann-Shack wavefront sensor to measure fence seeing^[9]

Fig. 6. [in Chinese]

Fig. 6. Curvature wavefront sensor

Fig. 7. Holographic wavefront sensor ^[17]

Fig. 8. Performance of holographic wavefront sensor in adaptive system under different modes^[21]

Fig. 9. Calibration curves under input mode Z(3,3)^[23]

Fig. 10. Four different schlieren imaging system^[34]

Fig. 11. Images under different cutting scales of source grid^[34]

Fig. 12. Holographic double exposure system ^[1]

Fig. 13. Flow field with different pulse intervals ^[1]

Fig. 14. Holographic particle velocimetry^[35]

Fig. 15. CFD mode^[42]

Fig. 16. Temperature distribution on air and coupling surface at different wind speeds U^[42]

Fig. 17. Mirror seeing under different wind speeds and temperature differences ^[42]