物体表面形状对热象仪测温的影响

本文报道利用红外热象仪 AGA780系统测量金属铝、铜和非金属石膏的平板及圆柱表面温度的准确度实验研究的结果。给出了表面形状不影响温度测量的“自由极角”范围,并且对影响测量准确性的其他因素也进行了讨论。     

静压推力轴承各工况下的热油携带及油膜温升特性

针对静压推力轴承运行过程中油膜温度骤升问题,从轴承摩擦副润滑机理出发,阐述斜面式双矩形油垫静压轴承油膜热油携带现象,定义油膜热油携带因子,建立油膜温升数学模型.采用有限体积法,对外载荷工况0～30t及转速工况4～100r/min进行理论计算及ANSYS-FLUENT软件流体仿真分析,得出油膜温度分布及热油携带发生规律,...     

涡轮集气腔出流流量分配和温度特性研究

采用模型实验和数值方法,针对特定的涡轮集气腔结构进行了出流特性研究。首先,在实验室条件下,进行全尺寸基准涡轮集气腔的模型实验研究并验证数值模拟方法;其次,在接近发动机真实气-热参数条件下进行系列的数值模拟,分析进出口压比、腔室高度、出流孔孔径和出流孔轴向位置等对出流孔流量分配和温度分布的影响。研究表明,除了集气腔出流流量分配的不均匀性之外,气流与热壁面之间的对流换热也导致明显的出流温度不均匀性;改变出流孔轴向位置距离、增加集气腔腔室高度是在不影响集气腔通流能力下改善出流均匀性的有效技术措施,当出流孔轴向偏置距离或集气腔腔室高度达到一定值后,其对改善出流流量分配均匀性的作用趋于微弱,但对于改善出流温度分布均匀性依然有较好的作用。     

分布式温度光纤传感器的研制与开发

分布式光纤传感器是一门具有重大价值的新兴技术,从其理论依据入手,全面介绍了该系统软硬件的实现过程,并对实验结果以及一些为了减小误差采用的新措施进行了对比分析.     

匀速升降温激励法温度传感器校准技术研究

为了对温度传感器进行便捷、快速、高效的温度校准,介绍了一种新的温度传感器校准技术,基于该校准技术方法设计了校准炉体,利用数值热分析优化了校准炉体的结构,并分析了校准炉体产生的不确定度分量对校准结果的影响。研究结果满足当前温度传感器校准需求。匀速升降温激励法快速校准技术在测量方法上具有新颖性和创新性,这项技术的成熟和实用普及为温度计量提供全新、高效地校准方法和技术途径。     

全站仪船体分段测量的温度影响研究

根据在相同的环境温度下和不同环境温度下对船体轴系部位同一材料、相同结构的多个目标点进行反复测量,观察全站仪测量数据的变化,分析环境温度变化引起的误差情况,为船舶精度建造工艺研究提供可靠的数据支撑。     

Time series analysis of active galactic nuclei: The case of Arp 102B, 3C 390.3, NGC 5548 and NGC 4051

We used the Z-transformed Discrete Correlation Function (ZDCF) and the Stochastic Process Estimation for AGN Reverberation (SPEAR) methods for the time series analysis of the continuum and the Hα$\alpha$ and Hβ$\beta$ line fluxes of a sample of well known type 1 active galactic nuclei (AGNs): Arp 102B, 3C 390.3, NGC 5548, and NGC 4051, where the first two objects are showing double-peaked emission line profiles. The aim of this work is to compare the time lag measurements from these two methods, and check if there is a connection with other emission line properties. We found that the obtained time lags from Hβ are larger than those derived from the Hα analysis for Arp 102B, 3C 390.3 and NGC 5548. This may indicate that the Hβ   line originates at larger radii in these objects. Moreover, we found that the ZDCF and SPEAR time lags are highly correlated (r∼0.87$r\sim 0.87$), and that the error ranges of both ZDCF and SPEAR time lags are correlated with the FWHM of used emission lines (r∼0.7$r\sim 0.7$). This increases the uncertainty of the black hole mass estimates using the virial theorem for AGNs with broader lines.     

Bottom side profiles for two close stations at the southern crest of the EIA: Differences and comparison with IRI-2012 and NeQuick2 for low and high solar activity

Bottom side electron density profiles for two stations at the southern crest of the Equatorial Ionization Anomaly (EIA), São José dos Campos (23.1°S, 314.5°E, dip latitude 19.8°S; Brazil) and Tucumán (26.9°S, 294.6°E, dip latitude 14.0°S; Argentina), located at similar latitude and separated by only 20° in longitude, have been compared during equinoctial, winter and summer months under low (year 2008, minimum of the solar cycle 23/24) and high solar activity (years 2013–2014, maximum of the solar cycle 24) conditions. An analysis of parameters describing the bottom side part of the electron density profile, namely the peak electron density NmF2, the height hmF2 at which it is reached, the thickness parameter B₀ and the shape parameter B₁, is carried out. Further, a comparison of bottom side profiles and F-layer parameters with the corresponding outputs of IRI-2012 and NeQuick2 models is also reported. The variations of NmF2 at both stations reveal the absence of semi-annual anomaly for low solar activity (LSA), evidencing the anomalous activity of the last solar minimum, while those related to hmF2 show an uplift of the ionosphere for high solar activity (HSA). As expected, the EIA is particularly visible at both stations during equinox for HSA, when its strength is at maximum in the South American sector. Despite the similar latitude of the two stations upon the southern crest of the EIA, the anomaly effect is more pronounced at Tucumán than at São José dos Campos. The differences encountered between these very close stations suggest that in this sector relevant longitudinal-dependent variations could occur, with the longitudinal gradient of the Equatorial Electrojet that plays a key role to explain such differences together with the 5.8° separation in dip latitude between the two ionosondes. Furthermore at Tucumán, the daily peak value of NmF2 around 21:00 LT during equinox for HSA is in temporal coincidence with an impulsive enhancement of hmF2, showing a kind of “elastic rebound” under the action of the EIA. IRI-2012 and NeQuick2 bottom side profiles show significant deviations from ionosonde observations. In particular, both models provide a clear underestimation of the EIA strength at both stations, with more pronounced differences for Tucumán. Large discrepancies are obtained for the parameter hmF2 for HSA during daytime at São José dos Campos, where clear underestimations made by both models are observed. The shape parameter B₀ is quite well described by the IRI-2012 model, with very good agreement in particular during equinox for both stations for both LSA and HSA. On the contrary, the two models show poor agreements with ionosonde data concerning the shape parameter B₁.     

弹道导弹动态全极化一维像仿真研究

研究了弹道导弹动态全极化一维像的仿真方法,可以为雷达目标检测、识别算法的研究提供基础。对弹道导弹的弹道和运动特性进行了建模,通过对弹头缩比模型静态测量数据进行插值,可以获得任意时刻、任意姿态下弹头的全极化一维距离像;比较了典型宽带雷达体制的信号形式,推导了它们之间的仿真参数转换关系。在计算机上进行了仿真实验,对仿真结果的分析表明本文提出的仿真方法是切实可行的。     

中段弹道目标的温度场与红外辐射特性计算

红外辐射特性是预警系统探测识别弹道中段目标的重要特征之一。通过计算飞行时目标与太阳、地球的相对位置,确定目标的受外辐射照射状态。利用有限容积法计算锥形目标的三维温度场,采用双向反射分布函数（BRDF）计算目标表面对太阳、地球辐射的反射特性,并结合自身红外辐射,得到了不同类型中段目标红外辐射特性变化情况和空间分布情况。最后,分析了外部辐射环境和目标材料特性对目标红外辐射特性的影响,为中段预警探测提供了参考。