小型控制力矩陀螺扰动建模及性能指标分析

为实现遥感卫星的高精度指向能力,对遥感卫星星上常用执行机构控制力矩陀螺扰动及性能指标评定进行了研究。首先,充分考虑小型控制力矩陀螺的静动不平衡量以及框架轴的安装误差,根据动量定理和动量矩定理建立了完整的星载小型控制力矩陀螺的动力学模型,并对所建立模型的正确性进行了理论分析和仿真验证;其次,将含有扰动特性的小型控制力矩陀螺应用到星上,建立了整星动力学模型,并选用合适的框架伺服控制系统和转子伺服控制系统,完成整星的姿态稳定控制任务;最后,采用数值仿真的方式分析了陀螺转子静动不平衡因素以及框架角测量误差对星体姿态精度和稳定度带来的影响。结合任务要求,对小型控制力矩陀螺设计提出静动不平衡量等指标要求,以期使其满足星上光学有效载荷的成像要求。     

加力燃烧室NOx排放生成规律试验分析

实现航空发动机大推力通常采用加力燃烧室设计,燃烧室进气温度升高会同步导致排放尾气中NO_x浓度提高.采用典型加力燃烧室主稳定器的V型结构试验件,测试加力燃烧前后(进口600 ℃,出口600~1 200 ℃)燃烧室排放断面的NO_x浓度分布,通过相同流场4种试验工况的NO_x生成浓度组分和氧含量变化分析,验证了加力燃烧室NO_x生成以热力型NO为主的"高温、富氧、贫油"燃烧特性.结果表明加力燃烧室燃烧过程中消耗的氧含量大多贡献于CO₂增量,在800~1 000 ℃燃气排放温度范围内,不完全燃烧产物CO对NO的热力生成有明显抑制作用.     

太阳轨道运动的2400年周期与轨道周期

通过对行星会合指数运动学方程生成的数据进行傅里叶变换, 得到了从年、十年、 百年、千年、万年到十万年时间尺度的周期, 发现这些周期具有后者是前者10n 倍的特殊倍乘关系. 如果将通过傅里叶变换得到的年时间尺度最显 著的周期4.96488a设为单位时间步长代入行星会合指数方程, 则可得到稳定 的2400年周期. 在此基础上由2400年周期振幅的差异性又构成了更长时间尺度的 10万年和40～41万年太阳轨道运动特征周期. 这对于揭示太阳轨道运动与太 阳活动的关系, 以及探讨气候千年尺度和轨道周期变化规律的机制具有重要意义.      

Moment-tensor inversion and decomposition for cracks in thin plates

The knowledge of crack type and dislocation orientation is helpful for the lifetime prediction of thin plates on aircrafts. The moment-tensor inversion utilizes the Acoustic Emission (AE) signals to detect cracks and the source mechanisms can be interpreted by the decomposition of moment tensors. Since the traditional moment-tensor inversion is implemented for the AE sources inside infinite elastic bodies, the inversion needs to be modified for the cracks in thin plates. In this study, the moment tensors of cracks in thin plates are derived and the inversion equation is provided based on the Green's function of second kind. A method of modifying the moment tensors to adapt to the existing decomposition processes and source-type plots is provided. By employing the Finite Element Method (FEM), the wave fields generated by the AE sources are computed. The AE sources continuously changing from pure tensile type (Model I) to shear type (Model II) are achieved in the FE models and the moment tensors are recovered. By the comparison between the reference values and recovered solutions, the source type can be accurately identified in the source-type plot and the applicability of the moment-tensor inversion for cracks in thin plates is confirmed.     

导弹武器系统时间同步网的综合性能评估方法

针对导弹武器系统时间同步网（MWSTSN）现有评估方法不全面、不客观等问题,提出了一种基于权系数优化的导弹武器系统时间同步网的综合性能评估方法。首先,基于时间同步网的工作流程与系统结构,综合分析了影响系统性能的各项指标,建立了导弹武器系统时间同步网性能的评估体系与评估模型。通过构建主、客观指标权重的分配系数最优化模型,利用层次分析法和熵值法对上述指标进行组合赋权,获取具有主、客观特性的组合权重。最后,通过案例验证上述评估过程的有效性,结果表明：该评估体系能够有效反映导弹武器系统时间同步网中各分系统及设备的可用性,并具备可测性和可操作性。     

The optical emission lines of type 1 X-ray bright Active Galactic Nuclei

A strong X-ray emission is one of the defining signatures of nuclear activity in galaxies. According to the Unified Model for Active Galactic Nuclei (AGN), both the X-ray radiation and the prominent broad emission lines, characterizing the optical and UV spectra of Type 1 AGNs, are originated in the innermost regions of the sources, close to the Super Massive Black Holes (SMBH), which power the central engine. Since the emission is concentrated in a very compact region (with typical size r?0.1$r?0.1$ pc) and it is not possible to obtain resolved images of the source, spectroscopic studies of this radiation represent the only valuable key to constrain the physical properties of matter and its structure in the center of active galaxies. Based on previous studies on the physics of the Broad Line Region (BLR) and on the X-ray spectra of broad (FWHM_Hβ ? 2000 km s⁻¹) and narrow line (1000 km s⁻¹ ?FWHM_Hβ ? 2000 km s⁻¹) emitting objects, it has been observed that the kinematic and ionization properties of matter close to the SMBHs are related together, and, in particular, that ionization is higher in narrow line sources. Here we report on the study of the optical and X-ray spectra of a sample of Type 1 AGNs, selected from the Sloan Digital Sky Survey (SDSS) database, within an upper redshift limit of z=0.35$z=0.35$, and detected at X-ray energies. We present analysis of the broad emission line fluxes and profiles, as well as the properties of the X-ray continuum and Fe Kα emission and we use these parameters to assess the consistency of our current AGN understanding.     

A model for the Balmer pseudocontinuum in spectra of type 1 AGNs

Here we present a new method for subtracting the Balmer pseudocontinuum in the UV part of type 1 AGN spectra. We calculate the intensity of the Balmer pseudocontinuum using the prominent Balmer lines in AGN spectra. We apply the model on a sample of 293 type 1 AGNs from SDSS database, and found that our model of Balmer pseudocontinuum + power law continuum very well fits the majority of AGN spectra from the sample, while in ∼$\sim$15% of AGNs, the model fits reasonable the UV continuum, but a discrepancy between the observed and fitted spectra is noted. Some of the possible reasons for the discrepancy may be a different value for the optical depth in these spectra than used in our model or the influence of the intrinsic reddening.     

Response of photosynthetic systems to salinity stress in the desert cyanobacterium Scytonema javanicum

The present study investigated the physiological and biochemical characteristics of Scytonema javanicum, a pioneer species isolated from desert biological crusts, under salinity stress. Pigment analysis showed that salinity decreased chlorophyll a and phycocyanin content, while low salinity increased carotenoid concentration and high salinity decreased carotenoid concentration. Salinity also inhibited CO₂ assimilation rate and photosynthetic oxygen evolution in this cyanobacterium. Chlorophyll a fluorescence transient parameters (φPo, φEo, ψO, RC/ABS, RC/CS, PI_ABS, and PI_CS) were decreased under salt stress, while dVo/dto(Mo), Vj and φDo were increased. The decrease of ETRmax and Yield and the change of chlorophyll a fluorescence transients showed that salt stress had an important influence on photosynthesis. These results indicated that the effects of salinity stress on photosynthesis in S. javanicum may depend on the inhibition of electron transport and the inactivation of the reaction centers, but this inhibition may occur in the electron transport pathway at the PSII donor and acceptor sites.     

Quasi-biennial oscillation signals in outgoing long-wave radiation of the equator

In the present paper, the authors use wavelet transform technique to study time-series of outgoing long-wave radiation (OLR) anomaly at the equator during 1979–2005. The results show that quasi-biennial oscillation (QBO) signals exist in the OLR variation and the QBO cycle has remarkable temporal variability in its amplitude and phase. The periodic length of the QBO fluctuation is about 2.2-year before 1986. After that time, the length mainly changes from about 2.4- to 2.6-year. Analyzing the anomaly data set of 850 MB trade wind index (TWI) at west Pacific during this period, we have found that the obvious time-variations characteristics of the QBO cycle also exist in the TWI change at west Pacific and are in good consistence with that of the OLR change. The quasi-biennial fluctuation of the TWI change can explain that of the OLR change to a large extent.     

中国广州地区电离层闪烁观测结果的初步统计分析

利用在广州站(23o8' N, 113o17' E)建立的GPS电离层闪烁监测系统, 开展了对电离层闪烁的连续观测. 利用这些观测数据, 对广州地区2007年4月至9月及2008年1月至9月电离层闪烁变化特性进行了初步统计分析研究. 分析结果表明, 广州地区闪烁主要发生在太阳活动较低的磁静日期间. 季节变化表现为弱闪烁(0.2相似文献