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纳米氧化镍微粉的制备及光吸收谱 被引量:33
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作者 汪国忠 张立德 牟季美 《物理化学学报》 SCIE CAS CSCD 北大核心 1997年第5期445-448,共4页
Uniform nanosized NiO particles were prepared by a chedrical coprecipitation usingNiCl2.6H2O as the starting material. The relationship between various annealing telnperaturesand grain size of NiO crystallite was inve... Uniform nanosized NiO particles were prepared by a chedrical coprecipitation usingNiCl2.6H2O as the starting material. The relationship between various annealing telnperaturesand grain size of NiO crystallite was investigated. Optical reflectivity spectra of Nanometer-sizedNiO powders at roonl temperature were studied. The results show that seven optical absorptionbands (P1. P2. P3. P4. P5. P6 and P7) with the peak energies of 3.30, 2.99, 2.78, 2.25,1.92, 1.72 and 1.07eV, respectively, are located on a continuous refiectivity background. P1.P2. P3 and P4 exhibit "blue shift", but P5. P6 and P7 present "red shift"in comparison withthat of single crystal NiO. The continuous reflectivity background increases rapidly with increasingthe annealing temperature from 500℃ to 600℃ to 700℃. The origins of P1 to P7 and thereasons of "blue shift", "red shift" and the increase of the reflectivity background with increasingthe annealing temperature have been analyzed in detail. 展开更多
关键词 共沉淀 光吸收 红移 蓝移 氧化镍 纳米材料
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光谱红移自主导航新方法 被引量:24
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作者 张伟 陈晓 +2 位作者 尤伟 张嵬 方宝东 《上海航天》 2013年第2期32-33,38,共3页
提出了一种基于太阳系天体光谱红移测量的自主导航新方法。以太阳系天体作为光源和信息源,由实时光谱红移测量值获得航天器在惯性坐标系中的飞行速度,实现航天器的自主导航。与现有自主导航方法相比,该法不依赖地面无线电信息,无需引入... 提出了一种基于太阳系天体光谱红移测量的自主导航新方法。以太阳系天体作为光源和信息源,由实时光谱红移测量值获得航天器在惯性坐标系中的飞行速度,实现航天器的自主导航。与现有自主导航方法相比,该法不依赖地面无线电信息,无需引入航天器轨道动力学,具有高度自主、简单易行、无时延等优势,在深空探测领域有广阔的应用前景,并可为近地卫星的自主导航提供参考与借鉴。 展开更多
关键词 深空探测 光谱红移 自主导航
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Two-Dimensional Self-Propelled Fish Motion in Medium: An Integrated Method for Deforming Body Dynamics and Unsteady Fluid Dynamics 被引量:21
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作者 杨焱 吴冠豪 +1 位作者 余永亮 童秉纲 《Chinese Physics Letters》 SCIE CAS CSCD 2008年第2期597-600,共4页
We present (1) the dynamical equations of deforming body and (2) an integrated method for deforming body dynamics and unsteady fluid dynamics, to investigate a modelled freely self-propelled fish. The theoretical ... We present (1) the dynamical equations of deforming body and (2) an integrated method for deforming body dynamics and unsteady fluid dynamics, to investigate a modelled freely self-propelled fish. The theoretical model and practical method is applicable for studies on the general mechanics of animal locomotion such as flying in air and swimming in water, particularly of free self-propulsion. The present results behave more credibly than the previous numerical studies and are close to the experimental results, and the aligned vortices pattern is discovered in cruising swimming. 展开更多
关键词 PULSARS x-ray spectra relativity and gravitation redshift
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纳米银粒子的量子尺寸效应 被引量:9
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作者 季淑莉 司民真 苗润才 《光子学报》 EI CAS CSCD 1999年第1期93-95,共3页
实验上采用吸收光谱发现两种不同粒度的纳米银粒子其吸收峰的位置随粒子尺寸的增加而红移,理论上采用简单的球形势阱模型得到了本征能量与粒子尺寸的解析关系。
关键词 红移 纳米银 尺寸效应 量子效应
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Boundary Slip and Surface Interaction: A Lattice Boltzmann Simulation 被引量:8
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作者 陈艳燕 伊厚会 李华兵 《Chinese Physics Letters》 SCIE CAS CSCD 2008年第1期184-187,共4页
The factors affecting slip length in Couette geometry flows are analysed by means of a two-phase mesoscopic lattice Boltzmann model including non-ideal fluid-fluid and fluid-wall interactions. The main factors influen... The factors affecting slip length in Couette geometry flows are analysed by means of a two-phase mesoscopic lattice Boltzmann model including non-ideal fluid-fluid and fluid-wall interactions. The main factors influencing the boundary slip are the strength of interactions between fluid-fluid and fluid-wall particles. Other factors, such as fluid viscosity, bulk pressure may also change the slip length. We find that boundary slip only occurs under a certain density (bulk pressure). If the density is large enough, the slip length will tend to zero. In our simulations, a low density layer near the wall does not need to be postulated a priori but emerges naturally from the underlying non-ideal mesoscopic dynamics. It is the low density layer that induces the boundary slip. The results may be helpful to understand recent experimental observations on the slippage of micro flows. 展开更多
关键词 PULSARS x-ray spectra relativity and gravitation redshift
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电压调制ZnO紫外探测器光响应截止波长的研究 被引量:9
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作者 段雨晗 丛明煜 +1 位作者 蒋大勇 梁庆成 《光学学报》 EI CAS CSCD 北大核心 2020年第20期36-40,共5页
通过射频磁控溅射技术,成功制备了具有金属-半导体-金属(MSM)结构的ZnO紫外光电探测器。研究了外加偏压对探测器响应度和截止波长的影响。随着偏压的增大,器件的响应度逐渐增加并且趋于饱和,探测器的响应截止波长红移了12 nm。这是电场... 通过射频磁控溅射技术,成功制备了具有金属-半导体-金属(MSM)结构的ZnO紫外光电探测器。研究了外加偏压对探测器响应度和截止波长的影响。随着偏压的增大,器件的响应度逐渐增加并且趋于饱和,探测器的响应截止波长红移了12 nm。这是电场引起的耗尽层的展宽以及带隙倾斜造成的。提出了一种利用外加偏压控制探测器截止波长的有效方法,该方法对紫外光电探测器的进一步研究和应用具有重要意义。 展开更多
关键词 探测器 光电探测器 氧化锌 金属-半导体金属结构 响应度 截止波长 红移
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一种基于非线性降维求正常星系红移的新方法 被引量:3
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作者 许馨 吴福朝 +1 位作者 胡占义 罗阿理 《光谱学与光谱分析》 SCIE EI CAS CSCD 北大核心 2006年第1期182-186,共5页
提出了一种确定正常星系红移的有效方法,该方法分为以下3个步骤:(1)利用四阶小波系数作为正常星系的特征表示,它能较好地反映吸收线、跳变点和吸收带的信息;(2)利用非线性降维方法LLE(locallylinearembedding)将特征数据映射到三维空间... 提出了一种确定正常星系红移的有效方法,该方法分为以下3个步骤:(1)利用四阶小波系数作为正常星系的特征表示,它能较好地反映吸收线、跳变点和吸收带的信息;(2)利用非线性降维方法LLE(locallylinearembedding)将特征数据映射到三维空间中一维流形;(3)由一维流形上的红移分布数据,根据最近邻方法得到正常星系的红移值。实验表明,文中所给的方法较文献中通常使用的PCA方法对于红移的确定具有更高的精度。 展开更多
关键词 正常星系 红移 LLE(locally linear embedding) 流形 PCA(principal component analysis)
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A Relationship between Dispersion Measure and Redshift Derived in Terms of New Tired Light 被引量:6
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作者 Lyndon Ashmore 《Journal of High Energy Physics, Gravitation and Cosmology》 2016年第4期512-530,共20页
New data from FRB’s have provided an exciting new window on the cosmos. For the first time we have both Dispersion Measure (DM) from distant sources and their red-shift. This gives us the opportunity to determine the... New data from FRB’s have provided an exciting new window on the cosmos. For the first time we have both Dispersion Measure (DM) from distant sources and their red-shift. This gives us the opportunity to determine the average electron number density in intergalactic space and thus test New Tired Light predictions. Here, in an alternative cosmology, the universe is static and redshifts are produced by an interaction between photons and the electrons in the intergalactic medium. In a paper published in summer 2006 New Tired Light (NTL) predicted an average electron number density of n = 0.5 m<sup>-3</sup>. In 2016 a paper was published reporting that for the first time the DM of a FRB and the redshift of the host galaxy had been found. Using standard physics this confirmed the electron number density as n = 0.5 m<sup>-3</sup>. The prediction NTL made ten years earlier was proved to be correct. Using this measured electron number density enabled a definitive value of the Hubble constant to be made by New Tired Light and the value is 63 km/s per Mpc which compares well with currently accepted values. Importantly, since in NTL the redshift and dispersion are both due to the electrons in IG space, a relationship between DM’s and redshift can be predicted. NTL predicts that DM and LN(1 + z) will be directly proportional and related by the formula DM = mec/2hr<sub>e</sub>(3.086 × 1022) where me, re are the rest mass and classical radius of the electron, c is the speed of light in a vacuum and h is the plank constant. The numerical term is to change units from pccm<sup>-3</sup> to m<sup>-2</sup>. This reduces to DM = 2380LN(1 + z). Using data from five FRB’s this is tested and a linear relation is seen of the form DM = 1830LN(1 + z). The gradient of the plot from the observed data is within 23% of that predicted by NTL. Recently the Tolman Surface Brightness test has been applied to the HUDF and the results support a static universe whilst the possibility of two differing types of SN Ia whose distribution changes wi 展开更多
关键词 redshift Tired Light Hubble Constant Expanding Universe CMB Supernovae Time Dilation
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退火对ZnO:Al薄膜光致发光性能的影响 被引量:7
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作者 徐自强 邓宏 +4 位作者 谢娟 李燕 陈航 祖小涛 薛书文 《强激光与粒子束》 EI CAS CSCD 北大核心 2006年第1期169-172,共4页
采用溶胶-凝胶工艺在石英衬底上制备ZnO:Al(AZO)薄膜,通过不同温度的退火处理,研究了退火对AZO薄膜结构和光致发光特性的影响。XRD图谱表明:所制备的薄膜具有c轴高度择优取向,随着退火温度的升高,(002)峰的强度逐渐增强,同时(002)峰的... 采用溶胶-凝胶工艺在石英衬底上制备ZnO:Al(AZO)薄膜,通过不同温度的退火处理,研究了退火对AZO薄膜结构和光致发光特性的影响。XRD图谱表明:所制备的薄膜具有c轴高度择优取向,随着退火温度的升高,(002)峰的强度逐渐增强,同时(002)峰的半高宽逐渐减小,表明晶粒在不断增大。未退火样品的光致发光(PL)谱由361 nm附近的紫外带边发射峰和500 nm附近的深能级发射峰组成。样品经退火后,以500 nm为中心的绿带发射逐渐减弱,而带边发射强度有所增强,并且逐渐红移到366 nm附近,与吸收边移动的测试结果相吻合。对经过不同时间退火的样品分析表明,AZO薄膜的发光特性与退火时间也有很大关系,时间过短可见波段的发射较强,但时间过长会使晶粒发生团聚,导致紫外发射峰强度减弱。 展开更多
关键词 溶胶-凝胶法 ZNO:AL薄膜 退火处理 光致发光 红移
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活动星系核的演化与宇宙学红移 被引量:8
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作者 尤莉莎 张雄 《天文研究与技术》 CSCD 北大核心 2007年第2期108-112,共5页
通过搜集了457个活动星系核样本,根据活动星系核的演化实质是指宇宙时标上的变化,讨论了红移量与活动星系核演化的关系,最终证明了活动星系核的演化分为两个序列:(1)从类星体到Seyfert星系之间的演化;(2)平谱射电类星体(FSRQ)—BL Lac... 通过搜集了457个活动星系核样本,根据活动星系核的演化实质是指宇宙时标上的变化,讨论了红移量与活动星系核演化的关系,最终证明了活动星系核的演化分为两个序列:(1)从类星体到Seyfert星系之间的演化;(2)平谱射电类星体(FSRQ)—BL Lac天体—射电星系(RG)的演化。 展开更多
关键词 活动星系核 中心黑洞质量 发光度 红移量
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The BTFR and MOND with Redshifts of Graviton Energy
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作者 Firmin J. Oliveira 《Journal of High Energy Physics, Gravitation and Cosmology》 CAS 2024年第4期1903-1917,共15页
This report is about the graviton redshift theory (GRST) which hypothesises the redshift of the energy of gravitons traveling in fields. A new source of energy loss in galaxy dynamics is introduced. Due to the hypothe... This report is about the graviton redshift theory (GRST) which hypothesises the redshift of the energy of gravitons traveling in fields. A new source of energy loss in galaxy dynamics is introduced. Due to the hypothetical interactions of gravitons with the expansion of the universe, which causes an energy loss of the gravitons due to cosmological redshift, the rotation equation for galaxies, which previously had the Newtonian potential energy and the graviton gravitational redshift energy loss, is now updated with the graviton cosmological redshift energy loss. From the galaxy rotation equation, the baryonic Tully-Fisher relation (BTFR) and the modified Newtonian dynamics (MOND) are defined in radial distribution form. Fits to galaxy rotation motion are detailed. A cosmic connection for the BTFR is defined. The result is that galaxy rotation curves are fully accounted for with the GRST rotation equation and the BTFR and MOND theories are incorporated into a unified framework. 展开更多
关键词 GRAVITONS Gravitational redshift Cosmological redshift Graviton Coupling Coefficients Spiral Galaxies
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A High-Energy Good-Beam-Quality Krypton-Lamp-Pumped Nd:YAG Solid-State Laser with One Pump Cavity 被引量:5
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作者 刘学胜 王智勇 +1 位作者 鄢歆 曹银花 《Chinese Physics Letters》 SCIE CAS CSCD 2008年第2期521-523,共3页
We investigate a high-energy good-beam-quality krypton-lamp-pumped pulsed Nd: YA G solid-state laser with one pump cavity. The symmetrical resonator laser is developed and is rated at 80 J with beam parameter product... We investigate a high-energy good-beam-quality krypton-lamp-pumped pulsed Nd: YA G solid-state laser with one pump cavity. The symmetrical resonator laser is developed and is rated at 80 J with beam parameter product 12mm mrad. The total system electro-optics efficiency of the lamp-pumped YAG laser is as high as 3.3% and the stability of output energy is ±2% with pulse width tunable between 0.1 ms and 10ms. The experimental results are consistent with the theoretical analysis and simulation. 展开更多
关键词 PULSARS x-ray spectra relativity and gravitation redshift
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Efficient Laser-Diode End-Pumped Passively Q-Switched Mode-Locked Yb:LYSO Laser Based on SESAM 被引量:5
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作者 徐世祥 李文雪 +2 位作者 郝强 翟惠 曾和平 《Chinese Physics Letters》 SCIE CAS CSCD 2008年第2期548-551,共4页
We report an efficient Q-switched laser action based on a semiconductor saturable absorber mirrors (SESAMs) as passively Q-switched laser starter and a Yb:LYSO alloyed crystal as gain material pumped directly by 97... We report an efficient Q-switched laser action based on a semiconductor saturable absorber mirrors (SESAMs) as passively Q-switched laser starter and a Yb:LYSO alloyed crystal as gain material pumped directly by 974nm InGaAs laser diodes. The output pulse duration is measured to be about 7μs, while the average power and the repetition rate of the pulse chain are about 0.92 W and 6.2 kHz, respectively, under 12.5 W absorbed pumping power. The Q-switched mode-locked pulse train is also observed in this setup. The laser performance shows that Yb:LYSO is a promising laser gain medium for laser-diode pumped compact solid-state lasers. 展开更多
关键词 PULSARS x-ray spectra relativity and gravitation redshift
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Cosmological Redshift Caused by Head-On Collisions with CMB Photons, Not by Expansion of Space
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作者 Gurcharn S. Sandhu Ishaan S. Dhindsa 《Journal of High Energy Physics, Gravitation and Cosmology》 CAS 2024年第4期1675-1698,共24页
The Big Bang model was first proposed in 1931 by Georges Lemaitre. Lemaitre and Hubble discovered a linear correlation between distances to galaxies and their redshifts. The correlation between redshifts and distances... The Big Bang model was first proposed in 1931 by Georges Lemaitre. Lemaitre and Hubble discovered a linear correlation between distances to galaxies and their redshifts. The correlation between redshifts and distances arises in all expanding models of universe as the cosmological redshift is commonly attributed to stretching of wavelengths of photons propagating through the expanding space. Fritz Zwicky suggested that the cosmological redshift could be caused by the interaction of propagating light photons with certain inherent features of the cosmos to lose a fraction of their energy. However, Zwicky did not provide any physical mechanism to support his tired light hypothesis. In this paper, we have developed the mechanism of producing cosmological redshift through head-on collision between light and CMB photons. The process of repeated energy loss of visual photons through n head-on collisions with CMB photons, constitutes a primary mechanism for producing the Cosmological redshift z. While this process results in steady reduction in the energy of visual photons, it also results in continuous increase in the number of photons in the CMB. After a head-on collision with a CMB photon, the incoming light photon, with reduced energy, keeps moving on its original path without any deflection or scattering in any way. After propagation through very large distances in the intergalactic space, all light photons will tend to lose bulk of their energy and fall into the invisible region of the spectrum. Thus, this mechanism of producing cosmological redshift through gradual energy depletion, also explains the Olbers’s paradox. 展开更多
关键词 redshift CMBR Big Bang COSMOLOGY Elastic Collisions Tired Light
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Data from Twenty-Three FRB’s Confirm the Universe Is Static and Not Expanding
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作者 Lyndon Errol Ashmore 《Journal of High Energy Physics, Gravitation and Cosmology》 CAS 2024年第3期1152-1177,共26页
Fast Radio Bursts from far away galaxies have travelled through the IGM and provide a tool to study its composition. Presently there are 23 FRB’s whose host galaxies have been identified and the redshift found. This ... Fast Radio Bursts from far away galaxies have travelled through the IGM and provide a tool to study its composition. Presently there are 23 FRB’s whose host galaxies have been identified and the redshift found. This gives us the opportunity to test Dispersion Measure versus redshift predictions made by two models. The Macquart relation for an expanding Universe and the New Tired Light relationship in a static universe. In New Tired Light, redshifts are produced when a photon is absorbed and re-emitted by the electrons in the IGM which recoil on both occasions. Some of the energy of the photon has been transferred to the kinetic energy of the recoiling electron. The photon has less energy, a lower frequency and a longer wavelength. It has been redshifted. Since dispersion is due to an interaction between radio signals and these same electrons one would expect a direct relationship between DM and redshift in the New Tired light model. The relation is DM=(mec/2hre)ln(1+z)and contains no adjustable parameters—just a combination of universal constants related to the electron and photon. Notice that the relation is independent of the electron number density ne since a change in ne affects both the DM and redshift equally. A graph of DM versus ln(1 + z) will be a straight line of gradient (mec/2hre)and, using SI units, substituting for the constants gives 7.318 × 1025 m−2. Using the data from the 23 well localized FRB’s, with the weighting of the DM’s for expansion removed (so that the data corresponds to a static universe), a graph of DM versus ln(1 + z) has a gradient of 6.7 × 1025 m−2—9% below the predicted (mec/2hre). The Macquart relation involves highly processed data and adjustable parameters to allow for “dark energy” and “dark matter” (neither of which has yet been found) and can be reduced to DM = 850z (in units of pc∙cm−3). Using the data from this set of localized FRB’s gives a trendline with gradient 1.10 × 103 pc∙cm−3—almost 30% higher than that predicted in an expandin 展开更多
关键词 redshift Dispersion Measure Fast Radio Bursts FRB’s Tired Light Static Universe IGM
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Does the Redshift Distribution of Swift Long GRBs Trace the Star-Formation Rate?
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作者 Ali M. Hasan Walid J. Azzam 《International Journal of Astronomy and Astrophysics》 2024年第1期20-44,共25页
Gamma-ray bursts (GRBs) are extremely powerful explosions that have been traditionally classified into two categories: long bursts (LGRBs) with an observed duration T<sub>90 </sub>> 2 s, and short burst... Gamma-ray bursts (GRBs) are extremely powerful explosions that have been traditionally classified into two categories: long bursts (LGRBs) with an observed duration T<sub>90 </sub>> 2 s, and short bursts (SGRBs) with an observed duration T<sub>90</sub> T<sub>90</sub> is the time interval during which 90% of the fluence is detected. LGRBs are believed to emanate from the core-collapse of massive stars, while SGRBs are believed to result from the merging of two compact objects, like two neutron stars. Because LGRBs are produced by the violent death of massive stars, we expect that their redshift distribution should trace the star-formation rate (SFR). The purpose of our study is to investigate the extent to which the redshift distribution of LGRBs follows and reflects the SFR. We use a sample of 370 LGRBs taken from the Swift catalog, and we investigate different models for the LGRB redshift distribution. We also carry out Monte Carlo simulations to check the consistency of our results. Our results indicate that the SFR can describe the LGRB redshift distribution well for high redshift bursts, but it needs an evolution term to fit the distribution well at low redshift. 展开更多
关键词 Gamma-Ray Bursts redshift Distribution Star-Formation Rate
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Dynamic Spacetime: Key to the Mysteries of Dark Matter and Dark Energy
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作者 Tianxi Zhang 《Journal of Modern Physics》 2024年第4期416-434,共19页
Physics is a branch of science to study matter and its motion in space and time. Development of physics usually upgrades human perspective and understanding of the space and time. Einstein successfully developed speci... Physics is a branch of science to study matter and its motion in space and time. Development of physics usually upgrades human perspective and understanding of the space and time. Einstein successfully developed special and general theories of relativity and creatively promoted our perspective of spacetime from Newton’s absolute space and time to his relative spacetime. Based on redshift and distance measurements of galaxies and distant type Ia supernovae, cosmologists have suggested that our universe is expanding at an ever-increasing rate driven by a mysterious dark energy. Recently, the author has proposed that spacetime is dynamic. Spacetime is said to be absolute if it is independent of matter and motion, relative if it is affected by matter and motion, and dynamic if it mutually interacts with matter and motion. In dynamic spacetime, not only do matter and motion distort spacetime, but they are also affected by the distorted spacetime. Spacetime to be dynamic is a consequence of a deep insight to Mach’s principle, which tells us that the inertia of an object results from the gravitational interaction by the rest of the universe. Reaction of dynamic spacetime on a traveling light causes light redshift. Reaction of dynamic spacetime on a fast moving neutrino slows down the neutrino. The derived redshift-distance relation perfectly explained the measurements of distant type Ia supernovae and gamma ray bursts (GRBs) and also naturally obtained Hubble’s law as an approximate relation at small redshift. This explanation of cosmological redshift as the opposition of dynamic spacetime does not mandate the universe to be expanding and accelerating, so that it does not need the universe to be initiated from a Big Bang and driven out mainly by a mysterious dark energy. Extremely slowed down neutrinos in dynamic spacetime, when they are gravitationally trapped around clusters, galaxies, and any celestial objects, would play the role of dark matter in explaining the velocity-radius relations of galaxy’s or clust 展开更多
关键词 SPACETIME Cosmology redshift NEUTRINO GRAVITATION Dark Matter Dark Energy
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Predicting Dark Energy Survey Results within the Haug-Tatum Cosmology Model
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作者 Eugene Terry Tatum Espen Gaarder Haug 《Journal of Modern Physics》 2024年第12期2220-2227,共8页
Given the pending completion and publication of the final Dark Energy Survey (DESI) results, this letter presents the corresponding predictions of the Haug-Tatum cosmology (HTC) model. In particular, we show in tabula... Given the pending completion and publication of the final Dark Energy Survey (DESI) results, this letter presents the corresponding predictions of the Haug-Tatum cosmology (HTC) model. In particular, we show in tabular and graphic form the “dark energy decay” curve which the HTC model predicts for cosmological redshifts covering the range of 0 - 2.0 z. Furthermore, we present the HTC model distance-vs-redshift curve in comparison to the three very different curves (for luminosity distance, angular diameter distance, and co-moving distance) calculated within the Lambda-CDM model. Whether the expansion of our universe is actually undergoing slight acceleration or the finely-tuned cosmic coasting at constant velocity of Rh = ct models, including HTC, will hopefully soon be answered by the many pending observational studies. 展开更多
关键词 Haug-Tatum Cosmology Dark Energy Lambda-CDM Cosmology Cosmological redshift Hubble Parameter Upsilon Constant DESI Rh = ct Cosmology
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Hybrid Deconvolution of Adaptive Optics Retinal Images from Wavefront Sensing 被引量:4
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作者 田雨 饶长辉 +6 位作者 饶学军 王成 余翔 刘倩 薛丽霞 凌宁 姜文汉 《Chinese Physics Letters》 SCIE CAS CSCD 2008年第1期105-107,共3页
Adaptive optics can be used to compensate for the wave aberration of the human eyes to achieve high-resolution imaging in real time. However the correction & partial due to the limitation of hardware. We propose a ki... Adaptive optics can be used to compensate for the wave aberration of the human eyes to achieve high-resolution imaging in real time. However the correction & partial due to the limitation of hardware. We propose a kind of hybrid image post-processing method, which uses the blind deconvolution combined with the residual data in wavefront sensor to restore the partially adaptive optics corrected retinal image. This method is applied in the image restoration of the vivid human retinal images. The results show that it is effective to improve the retinal image quality. 展开更多
关键词 PULSARS x-ray spectra relativity and gravitation redshift
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Eye-Safe Raman Laser at 1.5μm Based on BaWO4 Crystal 被引量:4
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作者 王正平 胡大伟 +4 位作者 方新 张怀金 许心光 王继扬 邵宗书 《Chinese Physics Letters》 SCIE CAS CSCD 2008年第1期122-124,共3页
Using an external couple cavity and a pump beam compression system, efficient 1.5 μm eye-safe Raman laser is obtained based on BaWO4 crystal. The largest output energy is 8.5mJ, corresponding to an electric-optical c... Using an external couple cavity and a pump beam compression system, efficient 1.5 μm eye-safe Raman laser is obtained based on BaWO4 crystal. The largest output energy is 8.5mJ, corresponding to an electric-optical conversion efficiency of 47%. 展开更多
关键词 PULSARS x-ray spectra relativity and gravitation redshift
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