双面半色调图像的光谱反射率色彩精确预测模型

为了准确地预测双面半色调图像的光谱反射率,并考虑光在纸张内的散射和油墨在纸基上的扩展渗透,建立了一个统一的双面半色调图像光谱反射率精确色彩预测模型.在油墨是非散射介质,纸张为强散射体以及油墨和纸张具有相同的折射率的条件下,引入Williams-Clapper模型中光在油墨中斜程传播的思想,考虑进入纸基层的光线横向传播和油墨扩展导致的网点扩大效应以及光在纸基和印刷品-空气界面间的多重内反射,利用多重内反射的网状结构分析法和最小二乘曲线拟合方法,确定了各种不同叠印条件下的理论网点面积率和有效网点面积率的函数关系,得出彩色双面图像的光谱反射色彩精确预测模型.新模型的预测值和测量值达到了较好的匹配,同时这也为彩色双面图像的呈色规律分析和印刷品质量检测系统的研制与开发提供了理论依据.     

双面半色调图像的光谱反射率色彩精确预测模型

为了准确地预测双面半色调图像的光谱反射率,并考虑光在纸张内的散射和油墨在纸基上的扩展渗透,建立了一个统一的双面半色调图像光谱反射率精确色彩预测模型.在油墨是非散射介质,纸张为强散射体以及油墨和纸张具有相同的折射率的条件下,引入Williams-Clapper模型中光在油墨中斜程传播的思想,考虑进入纸基层的光线横向传播和油墨扩展导致的网点扩大效应以及光在纸基和印刷品-空气界面间的多重内反射,利用多重内反射的网状结构分析法和最小二乘曲线拟合方法,确定了各种不同叠印条件下的理论网点面积率和有效网点面积率的函数关系,得出彩色双面图像的光谱反射色彩精确预测模型.新模型的预测值和测量值达到了较好的匹配,同时这也为彩色双面图像的呈色规律分析和印刷品质量检测系统的研制与开发提供了理论依据.     

彩色半色调墨点边缘羽化的Clapper-Yule扩展模型

研究了墨点边缘发生羽化现象(非二值理想墨点)对印品光谱反射率的影响,为色彩预测模型的理论研究提供一个新的思路。采用二维高斯函数模拟墨点表面的形态,利用多重积分计算出墨点羽化后的体积,根据体积的恒常性即羽化前后墨点体积相等,推导出含边缘坡度因子σ的网点面积率以及含墨层相对厚度因子的油墨透射率,由此建立了一个Clapper-Yule扩展模型。模型的数值模拟结果表明墨点边缘油墨铺展所导致的网点物理扩大,增加了油墨对光的吸收,从而降低了最终的光谱反射率。采用Clapper-Yule分程模型对颜色进行预测时需考虑墨点边缘羽化所带来的物理网点扩大,该模型适用于彩色半色调印品的颜色预测与控制。     

荧光基半色调彩色图像的Clapper-Yule光学反射率

在假定成像基的吸收光谱与其荧光发射光谱不重合的近似下,采用考虑图像基多重内反射效应的半色调图像反射率预测Clapper-Yule方法研究了荧光基半色调图像的光强反射规律,得出彩色半色调图像反射率新模型.同时考虑了构成半色调图像网点的物理扩大对反射率的影响.     

双面半色调图像的Clapper-Yule色彩预测分程模型

通过印刷品光谱反射比预测半色调图像色彩是印刷质量控制与设备检测研制领域十分关注的课题。在假定油墨是非散射介质以及油墨的折射率与纸张的折射率近似相等的条件下,利用光在油墨与纸张中散射迁移路径长短不同的分程理论和多重内反射的网状结构分析方法,研究了光照射在双面印刷品上的光谱反射规律,建立了双面印刷品的光谱反射色彩预测模型。并在此基础上通过理论分析,论证了新建双面印刷品的Clapper-Yule色彩分程预测模型的合理性。新模型为双面印刷品的呈色规律分析与印刷品在线检测仪的研制提供了理论依据。     

半色调荧光图像的光谱反射与透射模型

荧光油墨半色调印刷品的显色预测规律是彩色成像领域内十分关键的课题。把荧光半色调印刷品反射出来的光分成两个独立的部分,即由最初入射光组成的主光流和由于吸收了主光流而产生的荧光流;并且采用了一个指数矩阵来描述墨层产生的荧光光强,从而得出了荧光半色调图像色彩的光反射规律。考虑到入射光中从一种颜色油墨入射后再由同色油墨出射的概率要比从其它色油墨出射的概率要大的事实,讨论中引入权重因子描述从同色油墨出射部分与从整个表面出射部分比例不同的现象,建立了荧光油墨半色调图像的Clapper-Yule新光谱反射率模型。     

半色调印刷品中光传播过程的蒙特卡罗模拟

基于蒙特卡罗方法思想,结合半色调印刷品网点的结构属性,提出一种研究半色调印刷品呈色性质的模拟方法。考虑光的粒子属性,以程序化语言描述光子在半色调印品中的传播历程,涵盖光子从入射到传播终止的全过程,体现承印物、油墨、网点形状以及面积率变化对光散射行为的影响。对175lpi的不同网点结构模拟结果表明:该算法能合理模拟光与印品相互作用,适用于光子在多种网点结构中的散射模拟。模拟后的光子能量及位置分布均能可视化显示,经统计分析可转化为反射率、光子分布,散射距离等信息,为半色调印品的微观研究及质量控制提供一种新思路。     

半色调双面图像的色彩预测Clapper-Yule模型

为了准确地预测印刷图像的光谱反射率,在假定油墨是非散射介质以及油墨的折射率与纸张的折射率近似相等的近似下,利用考虑光在纸基内多次内反射的Clapper-Yule理论和描述多重内反射的网状结构分析模型,建立了同色不同加网周期双面墨像的光谱反射色彩预测模型.同时给出了包含纸基的向下体反射和反面纸基-空气构成界面定向反射作用的单面墨像Clapper-Yule色彩预测修正新模型.     

半色调彩色图像的反射率模型

光在纸张与油墨内散射或油墨在纸基内渗透都将影响半色调印刷图像的阶调特性．考虑到油墨在纸面上扩展所形成的墨点非矩形特性、光在纸基内传播的多次散射性和油墨在纸基内的渗透作用，采用纸张与油墨反射率与透射率的迭代修整方法建立了印刷图像的反射率新模型．理论模型中用纸张与油墨的反射率是油墨网点面积率的函数和实验参量砌描述纸张和油墨对反射模型的影响．     

基于光学网点扩大的光谱反射率模型研究

彩色半色调印刷品色彩预测模型是彩色图像复制领域内的关键技术,为建立更加准确的色彩预测模型,本文分析了光子在油墨中的传输,将光子传播类型分成四类并分别进行建模,最后提出了基于马尔可夫链理论的光谱反射率数学模型,并通过实验证明新模型具有更好的色彩预测精度.     

关于"太阳在银河系中所受引力与到银心距离r的关系"的讨论

讨论了银道面内的引力场强分布和太阳在银河系中所受引力与到银心距离r的关系，指出引力场强g并不是与r的平方成反比，这是由于银河系的大小和形状不能忽略造成的．强调了万有引力定律的适用条件．     

On the predictability of the positions of the convergence zones in the ocean

The disagreement between the experimental and calculated positions of the first convergence zone are known from many publications. The most probable cause for such a disagreement, namely, the incorrect specification of the input data for the calculations, is considered. The lack of simultaneity between the hydrological surveys of the region and the acoustic experiments is emphasized. The experimental data obtained by the author in five ocean regions are presented. These data characterize the diurnal variability of the distance from the source to the nearest boundary of the convergence zone. The relations proposed by different researchers for calculating the sound speed from the temperature, salinity, and hydrostatic pressure are analyzed. It is shown that these relations lead to a substantial difference in the estimated depth dependence of the hydrostatic gradient of the sound speed. The position of the first convergence zone is calculated for the propagation conditions determined by vertical temperature and salinity profiles with the subsequent recalculation of these profiles into sound speed profiles by using eight different formulas known from the literature. It is shown that different formulas lead to different values of the distance to the first zone; this difference is substantially greater than that between the calculations and experiment. The necessity of improving the recalculation relations in view of the experimental data on sound propagation in natural oceanic waveguides, including the data on the actual positions of the convergence zones, is emphasized.     

On the calculation of the bremsstrahlung in the region of the plasma frequency

On the basis of the classical theory of radiation produced in incomplete Coulomb interaction, a formula is derived for the coefficient of the bremsstrahlung of fully ionized plasma. In the region of rectilinear approximation a comparison is made with the results of the quantum formula derived from the Born approximation. Furthermore, the influence of dispersion upon the emission coefficient is taken into account; some relations for the region of dispersion are given.     

Dependence of the Intensity of the Spectral Lines and the Composition of the Sample and the Plasma Parameters of the Unipolar Arc

The investigation was made of the dependence of the intensity of Tl, Ga, Mo, Mg, Mn, Sn, Bi, Ni, Zn, Pt and Au spectral lines and the plasma parameters (temperature T, electron concentration n_e, degree of 6 ionnization α) from concentration of lithium additive.     

Extracting the wavefunction of the LSP at the LHC

We consider associated production of squarks and gluinos with the lightest supersymmetric particle (LSP), or states nearly degenerate in mass with it. Though sub-dominant to pair production of color SU(3)-charged superpartners, these processes are directly sensitive to the wavefunction composition of the lightest neutralinos. Exploiting event-shape variables - including some introduced here for the first time - we are able to identify the composition of the LSP by selecting events involving a single high-pT jet recoiling against missing transverse energy. We illustrate the proposed technique on a set of benchmark cases and propose methods for applying these results in more realistic experimental environments.     

Set the controls for the heart of the Sun

In this paper we describe experiments conducted with high-power lasers that are attempting to replicate, for a very short time and in miniature, conditions found in the Sun. Experiments to date have reached conditions in the outer part of the Sun. To reach the Sun's centre requires compression of material to very much greater than solid density and heating to over ten million degrees. To achieve this, a new class of experiments and a new generation of high-power lasers are required.     

On the Question of the Source of the Apokamp

Technical Physics - The object of this work is the apokamp—a new type of plasma jet, which is formed from a bright offshoot emerging at the bending point of a channel of a high-voltage...