1) facula diffusion
光斑扩散
1.
The eye sight principle of the model and control parameters of facula diffusion are expo
在个体轮廓探测环节,运用光斑扩散模型并对它的人眼视觉原理和光斑扩散中各项控制参数进行了深入的阐述和探讨,并在此基础上对它的单点扩散方式进行了改进,解决了此方式在对高屈曲截面纤维进行探测时不能探测到纤维全部轮廓的问题。
2.
In allusion to the traditional contour tracing arithmetic which can only work on binary images and is not able to handle the interlinking phenomena among objects,this paper introduces facula diffusion model based on the principle of human vision,and illustrates its controlling parameters including approximation,closing,length-limiting and hit-rate.
针对传统的轮廓跟踪算法只能应用在二值图像上,无法处理目标间相互溶结的现象,提出基于人眼视觉原理的光斑扩散模型,并从逼近、贴近、径长突变和命中率4个方面阐述了其控制参数。
3.
Based on mechanism of human sight,the facula diffusion method is advanced to detect individual cross-sections in the image and takes out the contours of them.
在人眼视觉机理的基础上,提出光斑扩散方法,用来探测图像中各个纤维截面并得到其轮廓线。
2) used-oil dispersiveness
斑点扩散性
3) diffusion among patches
斑块间扩散
4) hypostasis in diffusion stage
扩散期尸斑
5) laser speckle
激光散斑
1.
Measurement of thermal displacement of welding points for differental metals by laser speckle photography;
激光散斑照相法测量不同金属材料焊接部位的热位移
2.
Measuring heating stress of metal material at the welding points by using one beam laser speckle interferometry;
单光束激光散斑干涉法测量金属材料焊接部的热应变
3.
The measurement of metal material welding flaws by method of laser speckle;
用激光散斑法检测金属材料的焊接缺陷
6) white light speckle
白光散斑
1.
Using the white light speckle and ultrasonic C-scanning method, the internal defects of composite laminate are detected, and a GTF- 182 optical patten digital system is used to analysis white speckle plate that had Fourier thansformed.
用白光散斑法和超声C扫描相结合的方法检测复合材料内部缺陷;并用GTF—182光学图象数字分析系统对白光散斑法所得经付氏变换的图片进行了处理。
2.
The rotating aperture method is used in de focused white light speckle photography, and the experimental result is in agreement with the theoretical analysis.
把转孔法用于离焦白光散斑照相,实验结果同理论分析保持一致。
补充资料:光斑
光斑 faculae 日面上用白光看到的明亮区域,位于太阳光球的上层。其形状不规则,有明亮的纤维状结构。尺度在几千千米到1万千米之间。光斑通常在日面边缘才能清楚看到,多数与黑子相伴,寿命比黑子长。它的数目和总面积与黑子一样有11年的周期变化,和黑子不同的是光斑不仅出现在赤道区也出现在极区。光斑的温度比光球高,深层处的温度比光球约高100度,表面处则比光球约高2000度。与周围光球相比,光斑的亮度约大10%,压力约为光球的10倍。光斑的磁场强度约百分之几特斯拉。 |
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参考词条