Opto-Electronic Engineering, Volume. 50, Issue 11, 230186-1(2023)
Research on optical field calculation methods in the space gravitational wave telescope
Fig. 1. Schematic diagram of the space gravitational wave detector[4]
Fig. 2. Schematic diagram of the optical structure of the gravitational wave telescope[9]
Fig. 3. Schematic diagram of the algorithm flow of the gravitational wave telescope system model
Fig. 5. Optical path data at the exit pupil of the transmitting telescope at the 0 degree field angle. (a) Calculation results of the optical field simulation model; (b) Calculation results of the simulation software ZEMAX; (c) The difference between (a) and (b)
Fig. 7. Vectorial optical field distributions on the output surface of simulation calculation. (a) Intensity distribution map; (b) X polarization component amplitude distribution map; (c) X polarization component phase distribution map
Fig. 8. The amplitude distributions of the output field change with the waist distance (unit: V/m)
Fig. 9. The phase distributions of the output field change with the waist distance (unit: rad)
Fig. 10. The amplitude distributions of the output field change with the waist radius (unit: V/m)
Fig. 11. The phase distributions of the output field change with the waist radius (unit: rad)
Fig. 12. The changes of Z5 coefficient. (a) Z5 coefficient in the phase distribution changes with the waist distance; (b) Z5 coefficient in the phase distribution changes with the waist radius. (c) Z5 (defocus) term distribution form
Fig. 13. Phase distributions of the output X polarization field. (a) X polarization phase distribution under the ideal reflection; (b) X polarization phase distribution under the aluminum mirror reflection. (c) The difference in X polarization phase distribution between the aluminum mirror reflection case and the ideal reflection case
Fig. 14. Phase distributions of the output Y polarization field. (a) Y polarization phase distribution under the ideal reflection; (b) Y polarization phase distribution under the aluminum mirror reflection; (c) The difference in Y polarization phase distribution between the aluminum mirror reflection case and the ideal reflection case
Fig. 15. Comparison of Z2-Z15 coefficients of the X and Y polarizations phase difference distribution
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Ye Liu, Zheyi Hua, Shaojing Peng, Lan Wu, Dong Liu, Chong Liu. Research on optical field calculation methods in the space gravitational wave telescope[J]. Opto-Electronic Engineering, 2023, 50(11): 230186-1
Category: Article
Received: Jul. 26, 2023
Accepted: Nov. 15, 2023
Published Online: Mar. 26, 2024
The Author Email: Chong Liu (刘崇)