Wu Yi, Wang Yingjian, Wu Xubin. CALIBRATION OF THE OPTICAL QUALITY OF A LARGE TELESCOPE SYSTEMJ. High Power Laser and Partical Beams, 1995, 07(04): 510-514.
Citation:
Wu Yi, Wang Yingjian, Wu Xubin. CALIBRATION OF THE OPTICAL QUALITY OF A LARGE TELESCOPE SYSTEMJ. High Power Laser and Partical Beams, 1995, 07(04): 510-514.
Wu Yi, Wang Yingjian, Wu Xubin. CALIBRATION OF THE OPTICAL QUALITY OF A LARGE TELESCOPE SYSTEMJ. High Power Laser and Partical Beams, 1995, 07(04): 510-514.
Citation:
Wu Yi, Wang Yingjian, Wu Xubin. CALIBRATION OF THE OPTICAL QUALITY OF A LARGE TELESCOPE SYSTEMJ. High Power Laser and Partical Beams, 1995, 07(04): 510-514.
CALIBRATION OF THE OPTICAL QUALITY OF A LARGE TELESCOPE SYSTEM
The optical correlation function is used to determine the correlation time of atmospheric turbulence, within the time the effect of atmospheric turbulence is taken into account by using the optical transfer function,finally,the optical quality of a large telescope system(with aperture of 500mm,focal length of 500m) is calibrated.
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