基于多角度多光谱Stokes参数Q和U测量反演气溶胶偏振相函数

偏振相函数是气溶胶重要的光学参数之一,它对气溶胶复折射指数、粒子尺度和形状都十分敏感。多角度多光谱偏振遥感可以有效获取气溶胶偏振相函数信息。新一代CIMEL太阳-天空偏振辐射计CE318-DP作为高精度地基气溶胶偏振遥感仪器已被引入全球气溶胶自动观测网AERONET(AErosol RObotic NETwork),并作为扩展多波长偏振测量的太阳-天空辐射计观测网SONET(Sun/sky-radiometer Observation NETwork)的主要仪器,已在不同类型气溶胶观测站点积累了多年的偏振数据。但目前偏振反演仅能利用线偏振度或偏振辐亮度。与线偏振度和偏振辐亮度相比,Stokes参数Q和U不仅包含天空光线偏振强度信息还包含偏振方向信息。利用CE318-DP多光谱多角度测量的天空光Stokes参数Q和U反演气溶胶偏振相函数的方法。针对CE318-DP标准主平面偏振观测模式PPP(Polarized Principal Plane)下Stokes参数U对气溶胶特性变化不敏感、信息难以利用的不足,测试了新的平纬圈偏振扫描模式ALMP(ALMucantar Polarization)获取Stokes参数Q和U,并成功应用于偏振相函数的反演。系统分析了340～1 640 nm多光谱通道上典型生物质燃烧型气溶胶和水溶性气溶胶的-P₁₂/P₁₁反演结果并测试了反演方法在晴朗和灰霾不同大气条件下的适用性。无论在主平面还是平纬圈观测几何下,反演结果在可见光和近红外通道上均与真实值具有较好的一致性。进一步讨论了模型中基于气溶胶参数初始值和大气气溶胶参数真实值计算的“大气单次散射/大气散射”的比值近似相等的假设条件在短波通道不能很好地满足是造成紫外波段反演结果偏差较大的原因之一。后续有待进一步提高反演模型在短波通道的适用性,为利用不同光谱通道上-P₁₂/P₁₁的变化特征改进气溶胶微物理参数反演奠定了基础。     

红外波段下湿度对偏振光传输特性的影响

针对红外波段下湿度对偏振光传输特性的影响问题,以自然界中较常见的烟煤粒子作为研究对象,采用蒙特卡洛法仿真研究,不同红外波段下湿度对线偏光和圆偏光传输特性的影响情况及其之间差异特性.结果表明:在短波波段,线偏光与圆偏光的偏振度随湿度的增加都呈现逐渐上升的趋势;在中波波段,随湿度的增加两种偏振光都呈现下降趋势;而在长波波段,湿度对偏振状态几乎没有影响.进一步比较可知,在短波波段,圆偏光具有更好的偏振特性,而在中长波情况下,线偏光的偏振特性更加显著.因此,在应用红外偏振进行探测时,本研究对波段的选取、湿度的控制及偏振态的应用具有重要的指导意义.     

Layer-by-layer three-dimensional chiral photonic crystals

We fabricate and characterize polymeric three-dimensional layer-by-layer chiral photonic crystals. The obtained circular dichroism from polarization stop bands is comparable with that of recently demonstrated circular-spiral photonic crystals. Moreover, telecommunication wavelengths are easily accessible with the layer-by-layer approach; even visible wavelengths are in reach.     

Influence of polarization of laser beam on emission intensity of femtosecond laser-induced breakdown spectroscopy

Laser-induced breakdown spectroscopy(LIBS) is an important technique which is widely used to analyze element composition. In order to improve the sensitivity of LIBS, much effort has been made to enhance the spectral intensity of LIBS by proposing a number of methods. In addition, we find that laser polarization has great influence on the emission intensity of femtosecond LIBS. By comparing the emission intensity of femtosecond LIBS in the circular polarization with that in the linear polarization, the spectral intensity in the case of circular polarization is stronger than that in the case of linear polarization. Moreover, this phenomenon is more obvious as laser energy increases. The polarization plays an important role in LIBS signal intensity. Based on the observation, the enhanced mechanism of the laser polarization for the spectral intensity is discussed in this paper, which will be helpful in spectral analysis and component analysis.     

水下物体激光圆偏振成象实验及与线偏振成象的比较

采用波长532nm激光作光源,面阵CCD作探测器,利用圆偏振技术进行水下物体成象实验研究,对实验结果进行了分析并与线偏振成象技术进行了比较。结果表明无论是采用圆偏振技术还是线偏振技术都可提高水下物体成象的衬比（度）和成象距离;水体较清时圆偏振成象清晰度远远大于线偏振成象清晰度;当水体较混时,圆偏振成象清晰度大大下降和线偏振成象效果相接近。     

激光偏振编码制导中铌酸锂晶体编码技术研究

针对激光驾束制导系统光束能量调制方式的原理缺陷,讨论了用铌酸锂晶体的电光效应实现空间偏振编码的原理。对铌酸锂晶体的电光效应进行了理论分析,在此基础上设计了基于普科尔效应的空间偏振编码调制器。确定了X轴方向加电场的最佳运用方式,使得经过编码器后的线偏振光具有理想的偏振态梯度分布。对接收数据处理方式进行了讨论,得到了差和比方式对旋转不敏感的结论。在实验室中用可见光进行了近场实验,获得了从最上方近似右旋圆偏振光到中间的线偏振光再到最下方的左旋圆偏振光的偏振态分布。实验曲线表明获得了与理论计算基本一致的结果。     

The present state of the radiopolarization method of stress investigation

In [1] a method was proposed for investigating the mechanical stresses in solids by means of UHF electromagnetic waves; this method has recently been called the radiopolarization method (as distinct from the optical polarization method, in which waves in the optical range are used). An advantage of the new method is that it enables us to detect and investigate stresses in bodies which are opaque to visible light but permeable to ultra-high-frequency radio waves (porcelain, radioceramics, abrasives, ferrites, rubber, etc.). In addition it is comparatively easy to find the numerical values of the principal stresses by this method.Polarization methods reveal the stressed state of a solid as a collection of bands (lines equal in value to the difference between the principal stresses) or as isoclines from which isostats (lines of principal stress) are constructed.The first radiopolariscope described in [1] involved a great amount of work in plotting the bands (isochromes), and the accuracy of the results was not high.     

Circular polarization in scattered light as a possible biomarker

Biological molecules exhibit homochirality and are optically active. Therefore, it is possible that the scattering of light by biological molecules might result in a macroscopic signature in the form of circular polarization. If this is the case, then circular polarization spectroscopy, which may be utilized in remote sensing, can offer a powerful indicator of the presence of a universal biosignature, namely homochirality. Here, we describe laboratory experiments designed to investigate this idea. We focus on photosynthetic microorganisms, and also show results from macroscopic vegetation and control minerals. In the microorganisms, we find unambiguous circular polarization associated with electronic absorption bands of the photosynthetic apparatus. Macroscopic vegetation yields a stronger and more complex signature while the control minerals produce low-levels of circular polarization unrelated to their spectra. We propose a heuristic explanation of our results, which is that the polarization is produced by circular dichroism in the material after the light has undergone its last scattering event. The results are encouraging for the use of circular polarization spectroscopy in remote sensing of a generic biomarker from space or the ground.     

Polarization of atomic transitions in ionized14N after ion beam surface interaction at grazing incidence

The circular polarization of atomic transitions after the interaction of fast nitrogen ions with a solid surface at grazing incidence is investigated at energies for the incident ions from 0.4 up to 15 MeV. Large degrees of circular polarization in the visible part of the spectrum are found so that the application of this technique for producing nuclear spin polarized ions is feasible.     

Circular polarization converters based on bi-layered asymmetrical split ring metamaterials

In this paper, a kind of bi-layered asymmetrical split ring metamaterial was proposed as a circular polarization converter. Simulations and experiments at the microwave regime showed that the proposed structures can achieve the conversions from right-handed circularly polarized electromagnetic waves to left-handed ones and the reversed conversions in the opposite propagating direction. The linear to circular polarization transmission coefficients and the surface currents were investigated to understand the mechanism of the circular polarization conversions. Moreover, we optimized the proposed metamaterials by increasing the distance between the two metal layers. The proposed circular polarization converters have applications in microwave wave plates and metamaterial antennas.     

Relativistic beaming effect for blazars

In this paper, we revisit the relationship between the spectral index and the core-dominance parameter using a larger sample of 157 blazars (23 BL Lacertae objects and 134 flat spectrum radio quasars), compiled from the available literature. From the relevant data, we find the spectral index associated with the core-dominance parameter, for which a relativistic beaming effect is responsible. In addition, we make a comparison of the properties between BL Lacertae objects and flat spectrum radio quasars.     

Circular-polarization-dependent study of the microwave photoconductivity in a two-dimensional electron system

The polarization dependence of the low field microwave photoconductivity and absorption of a two-dimensional electron system has been investigated in a quasioptical setup in which linear and any circular polarization can be produced in situ. The microwave induced resistance oscillations and the zero resistance regions are notably immune to the sense of circular polarization. This observation is discrepant with a number of proposed theories. Deviations between different polarizations occur only near the cyclotron resonance where an unprecedented large resistance response is observed.     

Detecting axionlike particles with gamma ray telescopes

We propose that axionlike particles (ALPs) with a two-photon vertex, consistent with all astrophysical and laboratory bounds, may lead to a detectable signature in the spectra of high-energy gamma-ray sources. This occurs as a result of gamma rays being converted into ALPs in the magnetic fields of efficient astrophysical accelerators according to the "Hillas criterion", such as jets of active galactic nuclei or hot spots of radio galaxies. The discovery of such an effect is possible by GLAST in the 1-100 GeV range and by ground-based gamma-ray telescopes in the TeV range.     

Circular-polarization-dependent study of the microwave-induced magneto-resistance oscillations in the 2D electron system

We have investigated the influence of the polarization of the incident radiation on the recently discovered microwave-induced resistance oscillations in state-of-the-art highest purity 2D electron systems. A quasi-optical setup allows us to tune in situ between different circular as well as linear polarization states. We find that the microwave-induced zero resistance and the resistance oscillations are notably immune to changes in the polarization. This observation is discrepant with a number of proposed theories. Deviations for different polarizations only occur for a bolometric contribution to the resistance associated with the resonant heating at the cyclotron resonance itself.     

Circular-polarization-dependent study of the microwave-induced magneto-resistance oscillations in the 2D electron system

We have investigated the influence of the polarization of the incident radiation on the recently discovered microwave-induced resistance oscillations in state-of-the-art highest purity 2D electron systems. A quasi-optical setup allows us to tune in situ between different circular as well as linear polarization states. We find that the microwave-induced zero resistance and the resistance oscillations are notably immune to changes in the polarization. This observation is discrepant with a number of proposed theories. Deviations for different polarizations only occur for a bolometric contribution to the resistance associated with the resonant heating at the cyclotron resonance itself.     

GAMMA-RAY AND X-RAY EMISSION FROM GAMMA-RAY-LOUD BLAZARS

We present a strong correlation of the gamma-ray (above 100 MeV) mean spectral indices α_γ and X-ray (1 keV) mean spectral indices α_X for 34 gamma-ray-loud blazars (16 BL Lac objects and 18 flat spectrum radio quasars). A strong correlation is also found between the gamma-ray flux densities F_γ and X-ray flux densities F_X in the low state for 47 blazars (17 BL Lac and 30 flat spectrum radio quasars). Possible correlation on the gamma-ray emission mechanism is discussed. We suggest that the main gamma-ray radiation mechanism is probably the synchrotron process. The gamma-ray emission may be somewhat different from that of BL Lac objects and flat spectrum radio quasars.     

Centrifugal acceleration of plasma in pulsar magnetosphere

We present a relativistic model for the centrifugal acceleration of plasma bunches and the coherent radio emission in pulsar magnetosphere. We find that rotation broadens the width of leading component compared to the width of trailing component. We explain this difference in the component widths using the nested cone emission geometry. We estimate the effect of pulsar spin on the Stokes parameters, and find that the inclination between the rotation and magnetic axes can introduce an asymmetry in the circular polarization of the conal components. We analyse the single pulse polarization data of PSR B032954 at 606 MHz, and find that in its conal components, one sense of circular polarization dominates in the leading component while the other sense dominates in the trailing component. Our simulation shows that changing the sign of the impact parameter changes the sense of circular polarization as well as the swing of polarization angle Article presented at the International Conference on the Frontiers of Plasma Physics and Technology, 9–14 December 2002, Bangalore, India.     

沙尘气溶胶粒子群的散射和偏振特性

根据Mie散射理论,以对数正态分布函数描述沙尘气溶胶粒子群的粒径尺度分布,计算了沙尘气溶胶粒子群在0.2～40μm波段间对太阳短波辐射和地球大气长波辐射的单次散射反照率、散射相矩阵函数,揭示了不同相对湿度时,沙尘粒子群对入射辐射的散射和偏振的特征。结果表明,沙尘粒子群的单次散射反照率随着入射波长的增加有较大起伏,不同相对湿度条件下,变化趋势基本一致;在可见光、近红外波段单次散射反照率随湿度增加而变大,湿度95%时非常接近于1;大于10μm的热红外波段单次散射反照率随相对湿度增加而减小,具有较强的吸收辐射能力。散射辐射强度受湿度影响较小,随散射角的增加呈现先减小后增大的趋势,且增大的趋势随着波长的增加而减弱;不同波段上,线偏振和圆偏振随散射角和相对湿度变化存在差异;在前向和后向仅对入射辐射为圆偏振辐射产生圆偏振散射;散射光的偏振特性及其湿度差异主要表现在后向散射区,多以拱形形式体现。拱顶峰值散射角位置存在差异,且峰值散射角随相对湿度的降低向后向漂移。     

Manifestation of anisotropic collisional generation of higher polarization moments in polarization of quadrupole emission

Direct observability of polarization moments of a higher order—octupole orientation of atomic angular momenta (κ=3) and their hexadecapole alignment (κ=4)—from polarization of quadrupole radiation is discussed. The case when atoms are excited through dipole absorption of light producing orientation or alignment of angular momenta with κ=1 or 2 and higher polarization moments are induced by collisions with a beam of particles is considered. It is shown that differences in the laws of transformation of polarization moments of various ranks κ in rotations of coordinate axes allow us to select the pure contribution of the higher polarization moment under study from the signal of polarization of quadrupole emission by excluding the contribution of orientation or alignment with κ=1 or 2. Optimum systems of coordinate axes for the observation of octupole orientation from circular polarization of light and for the observation of hexadecapole alignment from linear polarization of light, in which the pure contribution of the higher polarization moment under study to polarization of quadrupole emission reaches its maximum, are calculated.     

The study of the weibel electromagnetic instability growth rate in the presence of the body stress

Body stress flow can be expected in the fast ignition imploding of the inertial fusion process that strongly damps small‐scale velocity structures. The Weibel instability is one of the plasma instabilities that require anisotropy in the distribution function. The body stress effect was neglected in the calculation of the Weibel instability growth rate. In this article, the propagation condition of impinging waves and the growing modes of the Weibel instability on the plasma density gradient of the fuel fusion with the body stress flow are investigated. Calculations show that the minimum value of the body stress rate threshold in the linear polarization is about 2.96 times greater than that of the circular polarization. Increasing 10 times of the density gradient and decreasing 2 times of the wavelength in the linear polarization and the circular polarization, respectively, lead to about 1.78 × 10⁶ times increment and 0.019 times decrement in the maximum of the Weibel instability growth rate. Also, the Weibel instability growth rate maximum in the circular polarization is about 10⁷ times greater than that of the linear polarization. The body stress flow and the density gradient tend to stabilize the Weibel instability in the circular polarization and act as a destabilizing source in the linear polarization. Therefore, by increasing steps of the density gradient plasma near the relativistic electron beam‐emitting region, in the circular polarization, the Weibel instability occurs at a higher stress flow.