一种复杂表面的平行光辐射传递系数计算方法

提出了复杂表面之间平行光辐射传递系数的一种新型计算方法,克服了蒙特卡洛法在计算平行光辐射系数时存在运算量较大、计算精度难以保证等缺点,并且从计算精度及耗时性两方面对新方法进行了比较分析,计算结果表明新方法在计算精度及耗时性上都要优于蒙特卡洛法。     

晨昏时段大气辐射对成像有效信噪比的影响

从成像有效信噪比的角度出发,利用MODTRAN辐射传输软件,分析计算了晨昏时段大气辐射的分布特点及其对成像的潜在影响。结果表明选择近红外成像谱段,可有效抑制大气背景辐射,实现晨昏时段一定观测倾角下的目标探测能力。     

进气总温畸变在压气机中的数值模拟

为了研究进气总温畸变在压气机中的传递特性,建立了压缩系统的几何模型,通过求解非稳态三维欧拉控制方程,计算了气流参数在压气机各截面的分布,获得了一种计算进气总温畸变的方法。以某三级压气机为例,对模型的有效性进行了验证。在进口存在周向总温畸变的情况下,计算得到了总压、静压、总温、静温和流量系数在各截面上的分布规律,得出了该三级压气机对总温畸变的响应。     

圆转矩形喷管射流掺混特性试验

采用热线风速仪对圆转矩形收敛喷管的射流流场与掺混特性进行了试验研究,测量了喷口下游不同截面上,射流宽、窄对称面上的速度、雷诺剪应力、湍流强度的分布规律.发现沿径向,雷诺剪应力先增大后减小,最大值出现在射流与外流的交界面附近,湍流强度则逐渐减小;在轴向上,雷诺剪应力在近喷口区存在小幅波动,而后逐渐减小,湍流度则先略有增大而后变化逐渐减慢.射流特性在宽对称面与窄对称面上的分布规律相同.      

Determination of Angular Distribution Models for Indian desert scene: Comparison with other desert models

In this paper, the shortwave and longwave anisotropy for clear sky Indian desert scene has been estimated using long-term surface data, radiative transfer calculations and Helmholtz reciprocity for missing values. This study is important in the perspective of the low inclination satellites like Megha–Tropiques (MT) mission, carrying Scanner for Radiation Budget (ScaRaB) payload, which will provide broadband radiative fluxes at the top of the atmosphere (TOA). Due to low inclination angle, the angular models for clear sky land scenes for the MT-ScaRaB orbits will be dominated by desert points.The Angular Distribution Models (ADMs) determined in this study were compared with existing desert models. It is observed that for longwave radiation, the largest disagreement is observed for higher values of viewing zenith angle, especially for the summer season, where the difference in flux can reach up to 13 W/m². For the shortwave radiation, higher values of both solar zenith angle and viewing zenith angle cause largest incongruity in the computed albedo from the different models, suggesting the need of caution in interpretation of the flux computations from these bins. In fact at the higher solar zenith angle bin, the disparity in albedo can go up to 6.4%.     

D300mm×3420mm圆管内旋转流流场的LDV实验测量

利用激光多普勒测速仪(LDV)对直径D 300mm×3420mm圆管内的旋转流场进行了实验测量,重点测量切向速度与轴向速度的分布以及湍流强度分布.测量结果表明圆管内的旋转流是Rankine涡结构形态,旋转流强度沿轴向存在着明显的衰减特性,且最大切向速度的径向位置沿轴向逐渐向内移动,即由上游的刚性涡逐渐向下游的准自由涡和刚性涡组合过渡;轴向速度的分布存在着很大的不均匀性,在r=0.5R区域存在一个轴向速度的低速区,甚至出现上行,但在轴向位置z>10R后轴向速度全部向下,并向均匀分布发展;圆管内的切向湍流强度比轴向湍流强度大一倍,两者的湍流强度在准自由涡区径向分布比较平均,中心刚性涡区域的湍流强度比较高,而且随轴向位置的变化衰减不明显.     

内燃机声强测试的有效性研究

有普通内燃机试验间内用声强法对发动机噪声进行测量,重点依据ＩＳＯ９６１４－Ｉ国际标准对测试数据的有效性和精度进行较深入的分析和校核,结果表明其方法可行,数据有效。通过测量分析,估算了发动机辐射的声功率及声能分布,进行了内燃机声源识别,获得了该型发动机噪声的有关特征和规律。此项研究为在普遍试验间进行内燃机噪声测量分析提供了经验。     

一种微波关联成像的新方法

将强度关联量子成像理论引入到雷达成像技术中,提出了一种全新的微波关联成像方法。向目标发射多个幅度、相位可控的单元信号,同时记录各个信号的状态并结合距离信息制作＂成像底版＂,通过对回波信号和＂成像底版＂的关联结果进行数理统计后可实现雷达高分辨成像。     

Solar EUV flux variation and flare brightenings

On 2010 February 8, the Extreme ultraviolet (EUV) flux variation in 195 Å and flare brightening has been examined in different sizes of active regions by using SOHO/EIT, MDI and Hα$\alpha$ observational data. These three active regions represent a large active region with a sunspot group, a moderate active region without a sunspot and a small region with weak plage in Hα$\alpha$ band respectively. Our study shows that the main full disk EUV flux comes from active regions, especially from large active regions. The sudden increases of EUV flux are corresponding to the EUV flare brightenings. For the large active region, the local EUV 195 Å flux peaks are well correlated to that of the GOES X-ray flux. The EUV 195 Å flux peaking time of M-class flares delay GOES X-ray flux a few minutes. For the moderate active region, the local EUV 195 Å flux is not well correlated to GOES X-ray flux. The EUV 195 Å flare brightenings in the moderate active region appeared in the duration of sudden increase of its own local EUV flux. For the small active region, the local EUV 195  Å flux varied almost independently of the GOES X-ray flux. Our study suggests that for an active region its local EUV 195 Å flux is more closely correlated to the EUV flare brightening than the full disk GOES X-ray flux.     

Development of a regional rain retrieval algorithm for exclusive mesoscale convective systems over peninsular India

The present study emphasize the development of a region specific rain retrieval algorithm by taking into accounts the cloud features. Brightness temperatures (T_bs) from various TRMM Microwave Imager (TMI) channels are calibrated with near surface rain intensity as observed from the TRMM – Precipitation Radar. It shows that T_b–R relations during exclusive-Mesoscale Convective System (MCS) events have greater dynamical range compared to combined events of non-MCS and MCS. Increased dynamical range of T_b–R relations for exclusive-MCS events have led to the development of an Artificial Neural Network (ANN) based regional algorithm for rain intensity estimation. By using the exclusive MCSs algorithm, reasonably good improvement in the accuracy of rain intensity estimation is observed. A case study of a comparison of rain intensity estimation by the exclusive-MCS regional algorithm and the global TRMM 2A12 rain product with a Doppler Weather Radar shows significant improvement in rain intensity estimation by the developed regional algorithm.