Feasibility of planet detection in two-planet solar system with rotationally-shearing interferometer

被引：2
|
作者：
Bravo-Medina, B. [1 ,2 ]
Strojnik, M. [2 ]
Kranjc, T. [1 ,2 ]
机构：
[1] Univ Guadalajara, Guadalajara, Jalisco, Mexico
[2] Opt Res Ctr, AP 1-948, Leon 37000, Gto, Mexico
来源：
INFRARED REMOTE SENSING AND INSTRUMENTATION XXVII | 2019年 / 11128卷
关键词：
simulation; rotational shearing interferometry; simulated solar systems; wavefront; interference; DOVE PRISM;
D O I：
10.1117/12.2538817
中图分类号：
V [航空、航天];
学科分类号：
08 ; 0825 ;
摘要：
We simulate the interference patterns of solar systems, incorporating an Estrella and two Tierras, as detected by a rotational shearing interferometer, to compare with laboratory setup. Three rays are propagated to represent each wavefront in the interferometer, using the exact ray tracing technique. Then, the phase, with which light beams are incident into the detection plane is used to calculate the orientation of the incident wavefront. Finally, all the incident wavefronts are summed together to obtain the resulting interference pattern.
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页数：12
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