高斯反射率镜单谐振光参量振荡器模式分析

采用高斯光束传输矩阵描述光参量谐振腔的行为,通过迭代计算模拟高斯光抽运高斯反射镜单谐振光参量振荡器的振荡过程,分析了谐振腔参数和抽运光口径对腔内输出模式的影响。报道了1 064μm脉冲抽运平 GRM腔单谐振非临界相位匹配KTP光参量振荡器的实验,其结果与理论分析相符。     

自由电子激光器的掠射环形谐振腔

研究一种新型自由电子激光谐振腔结构.采用双曲面-抛物面非球面镜组合的扩束系统,使振荡光束在腔内口径扩大6倍.提高了反射膜层抗激光破坏能力.本文讨论了扩束倍数、非球面参量、谐振腔长度和掠射光斑尺寸等参量对光学系统像差的影响.     

LD端面泵浦Cr~4∶YAG被动调Q激光器输出特性研究

对激光二极管端面泵浦Cr4+∶YAG被动调Q Nd∶YAG激光器输出特性进行了实验研究.实验研究发现,激光器输出功率及脉冲重复频率随谐振腔长度增大而增大.为解释这一实验现象,测量了泵浦光斑在激光晶体内尺寸,同时计算了激光晶体及Cr4+∶YAG晶体内的基模激光光斑半径随谐振腔长度变化.分析结果表明:激光晶体内泵浦光斑尺寸远小于激光晶体内基模光斑半径,腔模间交叠效率较低;当腔长增加时,激光晶体内的基模激光光斑减小,腔模间交叠效率增加,从而导致输出功率及脉冲重复频率随腔长增加而增加;另外,Cr4+∶YAG晶体内光斑半径也随谐振腔长度减小,引起Cr4+∶YAG晶体漂白时间缩短,导致脉冲重复频率随腔长增加而增加.     

光斑矩参量阵列测试法的测量不确定度

为计算和评估光斑矩参量阵列测试法的测量不确定度,以光斑矩参量积分表达式为出发点,推导了零阶近似下光斑矩参量的离散表达式,初步分析了光强分布数据中单元位置及探测光功率的测量不确定度。在此基础上,根据不确定度传递律,推导了阵列测试法下光斑矩参量测量不确定度的一般表达式。进一步得到了数种常用简化条件下的矩参量不确定度表达式,并进行了相应的分析。由此建立了光斑矩参量计算及其不确定度评定的一套完整方法。利用简化公式,对自行研制的激光光斑分析仪和通用的CCD面阵探测器的光斑矩参量测量不确定度进行了分析,给出了计算表达式。     

基于CCD的电玩具中LD和LED光斑尺寸测量

根据高斯光束的传输特性,搭建了一套测量电玩具中LD和LED光束质量和光斑尺寸的测量系统。该系统以CCD作为光斑采集的关键设备,利用自行编写的软件同步控制CCD和数控位移平台,采集LD和LED所发出光束在不同位置的光强分布图样。利用二阶矩计算光束的束宽,并由双曲线拟合得到光束轮廓曲线,计算出光束的M2因子,进而推算出LD和LED光束任一位置的光斑尺寸,实现对电玩具中LD和LED发光光斑尺寸的精确测量。     

泵浦光聚焦特性对高重频1064 nm被动调Q激光器的影响

研究了泵浦光聚焦特性对被动调Q激光器输出激光特性的影响。使用10 W激光二极管(LD)和焦距为4 mm的耦合聚焦镜,在不改变LD和谐振腔结构与间距(15 mm)的情况下,选取5个耦合聚焦镜位置,研究对应泵浦光聚焦特性对输出激光特性的影响,特别是对输出脉冲稳定性的影响。泵浦功率为3.550 W时,相较于其他耦合聚焦镜位置,在耦合聚焦镜距离LD 7.50 mm处,被动调Q激光器实现了更高重复频率(160 kHz)、更高平均输出功率(360 mW)、更高单脉冲能量(2.250 μJ)、更低时域抖动(120 ns)的稳定脉冲输出。实验数据说明,耦合聚焦镜距离LD 7.50 mm处,泵浦光聚焦光斑与谐振腔基模光斑的匹配程度较好。理论计算得出,耦合聚焦镜距离LD 7.50 mm时,谐振腔基模光斑尺寸与泵浦光聚焦光斑束腰尺寸的比值为0.854,该比值对今后开展高重频被动调Q激光器相关研究具有一定的借鉴意义。     

基于半导体泵浦倍频绿光激光器的探究性实验设计

为探究在谐振腔中倍频晶体位置对绿光激光器输出功率的影响，利用半导体泵浦固体激光实验仪设计了腔内和腔外倍频绿光的探究性实验。分析了绿光倍频效率与基频光束的功率密度及光斑半径之间的关系，分别测量了磷酸钛氧钾(KTP)倍频晶体位于谐振腔內部和外部不同位置时，532 nm倍频绿光的输出功率。其中在腔外倍频实验中，分别设计了腔外不加透镜时KTP晶体位于腔外不同位置，以及加上透镜时KTP晶体位于聚焦位置两种实验方案。同时，在实验中引导学生利用谐振腔理论和高斯光束传输理论等激光原理计算1 064 nm基频光在腔内外不同位置的光斑半径，分析了KTP晶体在不同位置时532 nm倍频光输出功率出现差别的原因，以及利用透镜聚焦提高激光功率密度以达到提高倍频效率的方法。     

激光陀螺谐振腔横模特征的测量与分析

为了判定被测激光的模式特征,基于激光的频率特性,提出了一种测量激光陀螺谐振腔横模特征的方法.利用F-P扫描干涉仪,可以实时在线测量激光模式分布特性,该方法以已知F-P扫描干涉仪的频率间隔和扫频速度为比例尺,将难以测量的横模频率间隔转化为易于测量的时间间隔,通过测量从扫描干涉仪给出的谱图,计算出不同横模的频率间隔与纵模间隔的比例系数,并与该陀螺的理论比例系数进行比较,从而实现对激光陀螺谐振腔横模特征的精确判定.通过对某型环形激光谐振腔的测量实验,得到了该陀螺模式特征随着工作电流大小变化的规律:随着放电电流的增加,激光陀螺腔内所振荡的横模由单一的基模逐渐转变为基模和高阶模的混合模,并准确地判定出该谐振腔横模特征,其测量结果与理论结果误差小于2%.利用该方法横模频率间隔测量准确度可达1 MHz,重复性可达0.4 MHz.     

平面谐振腔参数对腔内模式椭圆率影响的机理研究

腔内模式椭圆偏振态和磁场是激光陀螺产生磁致误差的两个必要条件,减小腔内模式椭圆率是降低激光陀螺磁灵敏度的重要途径。基于琼斯矩阵的谐振腔理论,提出了建立自洽方程的位置原则;提出了自洽方程求解中起振模式的选取方法;形成了准确、完善的腔内模式椭圆率计算公式。采用数值分析法,分析了平面腔激光陀螺反射镜参数及光路非共面误差对腔内本征模式偏振态的影响机理;提出了两种通过配置反射镜反射相移减小腔内模式椭圆率的新方法。     

LD端面泵浦Cr4:YAG被动调Q激光器输出特性研究

对激光二极管端面泵浦Cr⁴⁺:YAG被动调QNd:YAG激光器输出特性进行了实验研究.实验研究发现,激光器输出功率及脉冲重复频率随谐振腔长度增大而增大.为解释这一实验现象,测量了泵浦光斑在激光晶体内尺寸,同时计算了激光晶体及Cr⁴⁺:YAG晶体内的基模激光光斑半径随谐振腔长度变化.分析结果表明:激光晶体内泵浦光斑尺寸远小于激光晶体内基模光斑半径,腔模间交叠效率较低;当腔长增加时,激光晶体内的基模激光光斑减小,腔模间交叠效率增加,从而导致输出功率及脉冲重复频率随腔长增加而增加;另外,Cr⁴⁺:YAG晶体内光斑半径也随谐振腔长度减小,引起Cr⁴⁺:YAG晶体漂白时间缩短,导致脉冲重复频率随腔长增加而增加.     

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...