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弱压缩真空态的位相特性及光学衰减器中位相扩散的分析<英文>
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作者 张登玉 《郴州师专学报》 1997年第2期40-43,共4页
本文利用Pegg定义的位相,研究了弱压缩真空态的位相特性。分析了光学衰减器中位相演化规律,并将位相几率分布中的扩散与Fokker—Planck得出的结果进行比较。
关键词 位相特性 压缩真空态 光学衰减器 位相扩散
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Determination of isothermal section of Ag-Ti-Zr ternary system at 1 023 K
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作者 周果君 刘华山 +1 位作者 刘立斌 金展鹏 《Journal of Central South University of Technology》 EI 2007年第6期750-752,共3页
The isothermal section of Ag-Ti-Zr ternary system at 1023 K was determined by diffusion triple and electron probe microanalysis. The results indicate that four binary intermetallic phases of AgTi, AgTi2, AgZr and AgZr... The isothermal section of Ag-Ti-Zr ternary system at 1023 K was determined by diffusion triple and electron probe microanalysis. The results indicate that four binary intermetallic phases of AgTi, AgTi2, AgZr and AgZr2 are found in Ag-Ti-Zr ternary system at 1 023 K. AgZr2 and AgTi2 form a continuous solid solution, namely Ag(Ti,Zr)2. Four three-phase regions: AgTi +AgZr + Ag, AgTi +AgZr + Ag (Ti, Zr)2, α-Zr +β(Ti, Zr) + Ag (Ti, Zr) 2 and α-Ti +β(Ti, Zr) + Ag (Ti, Zr)2 exist in the isothermal section. No ternary compound is observed. 展开更多
关键词 Ag-Ti-Zr phase diagram diffusion triple isothermal section
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A phase model for point spread function estimation in ground-based astronomy 被引量:1
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作者 CHAN Raymond Honfu YUAN XiaoMing ZHANG WenXing 《Science China Mathematics》 SCIE 2013年第12期2701-2710,共10页
In ground-based astronomy, images of objects in outer space are acquired via ground-based tele- scopes. However, the imaging system is generally interfered by atmospheric turbulence and hence images so acquired are bl... In ground-based astronomy, images of objects in outer space are acquired via ground-based tele- scopes. However, the imaging system is generally interfered by atmospheric turbulence and hence images so acquired are blurred with unknown point spread function (PSF). To restore the observed images, aberration of the wavefront at the telescope's aperture, i.e., the phase, is utilized to derive the PSF. However, the phase is not readily available. Instead, its gradients can be collected by wavefront sensors. Thus the usual approach is to use regularization methods to reconstruct high-resolution phase gradients and then use them to recover the phase in high accuracy. Here, we develop a model that reconstructs the phase directly. The proposed model uses the tight frame regularization and it can be solved efficiently by the Douglas-Rachford alternating direction method of multipliers whose convergence has been well established. Numerical results illustrate that our new model is efficient and gives more accurate estimation for the PSF. 展开更多
关键词 point spread function astronomical imaging phase model tight frame alternating directionmethod of multipliers
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