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Solar tomography adaptive optics
Deqing Ren; Yongtian Zhu; Xi Zhang; Jiangpei Dou; Gang Zhao
Source PublicationAPPLIED OPTICS
Conventional solar adaptive optics uses one deformable mirror (DM) and one guide star for wave-front sensing, which seriously limits high-resolution imaging over a large field of view (FOV). Recent progress toward multiconjugate adaptive optics indicates that atmosphere turbulence induced wave-front distortion at different altitudes can be reconstructed by using multiple guide stars. To maximize the performance over a large FOV, we propose a solar tomography adaptive optics (TAO) system that uses tomographic wave-front information and uses one DM. We show that by fully taking advantage of the knowledge of three-dimensional wave-front distribution, a classical solar adaptive optics with one DM can provide an extra performance gain for high-resolution imaging over a large FOV in the near infrared. The TAO will allow existing one-deformable-mirror solar adaptive optics to deliver better performance over a large FOV for high-resolution magnetic field investigation, where solar activities occur in a twodimensional field up to 6000, and where the near infrared is superior to the visible in terms of magnetic field sensitivity.
KeywordActive Or Adaptive Optics Imaging Through Turbulent Media
Subject Area自适应光学
Document Type期刊论文
Recommended Citation
GB/T 7714
Deqing Ren,Yongtian Zhu,Xi Zhang,et al. Solar tomography adaptive optics[J]. APPLIED OPTICS,2014,53(8):1683-1693.
APA Deqing Ren,Yongtian Zhu,Xi Zhang,Jiangpei Dou,&Gang Zhao.(2014).Solar tomography adaptive optics.APPLIED OPTICS,53(8),1683-1693.
MLA Deqing Ren,et al."Solar tomography adaptive optics".APPLIED OPTICS 53.8(2014):1683-1693.
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