zhu ming, zhan jie. Multi-objective star calibration study of total atmospheric transmittance measurement with stellar irradiance[J]. High Power Laser and Particle Beams, 2010, 22.
Citation:
zhu ming, zhan jie. Multi-objective star calibration study of total atmospheric transmittance measurement with stellar irradiance[J]. High Power Laser and Particle Beams, 2010, 22.
zhu ming, zhan jie. Multi-objective star calibration study of total atmospheric transmittance measurement with stellar irradiance[J]. High Power Laser and Particle Beams, 2010, 22.
Citation:
zhu ming, zhan jie. Multi-objective star calibration study of total atmospheric transmittance measurement with stellar irradiance[J]. High Power Laser and Particle Beams, 2010, 22.
Anhui Institute of Optics and Fine Mechanics,Chinese Academy of Sciences,P.O.Box 1125,Hefei 230031,China;
2.
Key Laboratory of Atmospheric Composition and Optical Radiation,Anhui Institute of Optics and Fine Mechanics,Chinese Academy of Sciences,Hefei 230031,China;
3.
Graduate University of Chinese Academy of Sciences,Beijing 100039,China
The Langley-Plot calibration principles and measurement apparatus of total atmospheric transmittance were introduced. The multi-objective star calibration of total atmospheric transmittance measurements with stellar irradiance is presented, and calibration experimentations of the K,A spectral type stars were carried out .The calibration values based on the K, A types of stellar spectra were obtained. Comparison experiments between multi-objective star method and Langley-Plot method were carried out, and the reasonableness and correctness of multi-objective star calibration method have been verified. When take real-time measurement with the same type stellar spectra, the corresponding calibration parameters can be used to carry out the measurements of the atmospheric transmittance.