Real-Time Controller Based on FPGA and DSP for Solar Ground Layer Adaptive Optics Prototype System at 1-m NVST

Solar ground layer adaptive optics (GLAO), containing a large field of view (FOV) wavefront sensor (WFS) and one deformable mirror (DM), can be used to reduce and stabilize the seeing effectively over a wide FOV. As the brain of the GLAO system, the real-time controller (RTC) computes the commands t...

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Vydáno v:IEEE photonics journal Ročník 9; číslo 2; s. 1 - 11
Hlavní autoři: Kong, Lin, Zhu, Lei, Zhang, Lanqiang, Bao, Hua, Rao, Changhui
Médium: Journal Article
Jazyk:angličtina
Vydáno: IEEE 01.04.2017
Témata:
Adaptive optics
Digital signal processing
digital signal processor (DSP)
Field programmable gate arrays
field programming gate array (FPGA)
ground layer adaptive optics
Imaging
parallel acceleration
Prototypes
Real-time controller
Real-time systems
Telescopes
ISSN:1943-0655, 1943-0647
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Abstract Solar ground layer adaptive optics (GLAO), containing a large field of view (FOV) wavefront sensor (WFS) and one deformable mirror (DM), can be used to reduce and stabilize the seeing effectively over a wide FOV. As the brain of the GLAO system, the real-time controller (RTC) computes the commands to drive the DM according to the average wavefront errors measured by the multi-direction correlating Shack-Hartmann WFS, which is a time-consuming process. A customized RTC based on a high-speed field programming gate array and a multi-core digital signal processor was developed for the solar GLAO prototype system at the 1-m New Vacuum Solar Telescope. Several parallel acceleration techniques are used to reduce the computation time of the RTC. Compared with the previous RTCs, our RTC architecture has nearly no timing jitter. In this paper, the design of the RTC for our solar GLAO prototype will be introduced. The test results of the RTC are also presented. Moreover, the on-sky Sun observational results of the solar GLAO prototype are shown.
AbstractList Solar ground layer adaptive optics (GLAO), containing a large field of view (FOV) wavefront sensor (WFS) and one deformable mirror (DM), can be used to reduce and stabilize the seeing effectively over a wide FOV. As the brain of the GLAO system, the real-time controller (RTC) computes the commands to drive the DM according to the average wavefront errors measured by the multi-direction correlating Shack-Hartmann WFS, which is a time-consuming process. A customized RTC based on a high-speed field programming gate array and a multi-core digital signal processor was developed for the solar GLAO prototype system at the 1-m New Vacuum Solar Telescope. Several parallel acceleration techniques are used to reduce the computation time of the RTC. Compared with the previous RTCs, our RTC architecture has nearly no timing jitter. In this paper, the design of the RTC for our solar GLAO prototype will be introduced. The test results of the RTC are also presented. Moreover, the on-sky Sun observational results of the solar GLAO prototype are shown.
Author Lanqiang Zhang
Hua Bao
Changhui Rao
Lei Zhu
Lin Kong
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SubjectTerms Adaptive optics
Digital signal processing
digital signal processor (DSP)
Field programmable gate arrays
field programming gate array (FPGA)
ground layer adaptive optics
Imaging
parallel acceleration
Prototypes
Real-time controller
Real-time systems
Telescopes
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Title Real-Time Controller Based on FPGA and DSP for Solar Ground Layer Adaptive Optics Prototype System at 1-m NVST
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