单边膨胀喷管气动和红外辐射特性数值研究

通过计算流体动力学/红外辐射(CFD/IR)数值模拟的方法,研究了单膨胀边倾角、喉道高度、侧壁长度和落压比(NPR)对单边膨胀喷管(SERN)气动性能和红外辐射特性的影响.研究结果表明:轴向推力系数随着单膨胀边倾斜角度增大而急剧减小,推力矢量角随着单膨胀边倾斜角度增大而增大;随着喷管落压比的增大,轴向推力系数先增大后减小,推力矢量角减小;随着喷管侧壁长度的增加,轴向推力系数可略微提高;单膨胀边对尾焰和喷管内壁有显著的遮挡作用,喷管下方的整体红外辐射仅为上方的10%左右;随着喷管落压比的增加,喷管上方的整体红外辐射降低.      

The dynamic chromosphere: Pushing the boundaries of observations and models

The interface between the bright solar surface and the million-degree corona continues to hold the key to many unsolved problems in solar physics. Advances in instrumentation now allow us to observe the dynamic structures of the solar chromosphere down to less than $0_{.}^{″}1$ with cadences of just a few seconds and in multiple polarisation states. Such observational progress has been matched by the ever-increasing sophistication of numerical models, which have become necessary to interpret the complex observations. With an emphasis on the quiet Sun, I will review recent progress in the observation and modelling of the chromosphere. Models have come a long way from 1D static atmospheres, but their predictions still fail to reproduce several key observed features. Nevertheless, they have given us invaluable insight into the physical processes that energise the atmosphere. With more physics being added to models, the gap between predictions and observations is narrowing. With the next generation of solar observatories just around the corner, the big question is: will they close the gap?     

通道曲面的柱面逼近方法及其在叶轮插铣中的应用

为了使叶轮粗加工后的通道表面与其设计曲面尽可能接近,将整体叶轮的定轴插铣理论模型概括为通道曲面的最大内接柱面优化问题。同时,为简化该问题的计算难度,将最大内接柱面的优化问题转化为柱面直母线方向和柱面准线的确定两个步骤。提出了确定内接柱面直母线方向的最小二乘模型与解算方法,在此基础上,将通道曲面沿柱面的直母线方向进行投影,通过相关曲线间的裁剪操作,获得了最大内接柱面的准线。以最大内接柱面的准线作为插铣加工时的边界曲线,以柱面直母线方向作为插铣加工时平头刀的轴线方向,给出了计算刀心位置和安全高度的迭代算法。最后通过数值算例验证了所提方法的正确性。该方法将有助于叶轮粗加工效率的提高,同时为叶轮的精加工预留较均匀的加工余量。     

The role of ultraviolet imaging in studies of resolved and unresolved young stellar populations. M31 and M33

We discuss the relevance of UV data in the detection and characterization of hot massive stars and young stellar populations in galaxies. We show results from recent extensive surveys in M31 and M33 with Hubble Space Telescope (HST) multi-wavelength data including UV filters, which imaged several regions at a linear resolution (projected) of less than half a pc in these galaxies, and from GALEX far-UV and near-UV wide-field, low-resolution imaging of the entire galaxies. Both datasets allow us to study the hierarchical structure of star formation: the youngest stellar groups are the most compact, and are often arranged within broader, sparser structures. The derived recent star-formation rates are rather similar for the two galaxies, when scaled for the respective areas. We show how uncertainties in metallicity and type of selective extinction for the internal reddening may affect the results, and how an appropriate complement of UV filters could reduce such uncertainties, and significantly alleviate some parameter degeneracies.     

Collisional excitation of vinylidene (H2CC)

Though H₂CO, H₂CS, H₂CCC, H₂CCCC, H₂CCO have been identified in cool interstellar molecular clouds, identification of H₂CC is still awaited. To analyze its spectrum, collisional rate coefficients are required. We have calculated collisional rate coefficients for rotational transitions between 23 levels of ortho and para H₂CC for kinetic temperatures 10, 20, 30, 40, and 50 K. The scattering problem is analyzed using the computer code MOLSCAT where the colliding partner is He atom. The interaction between H₂CC and He has been calculated with GAUSSIAN 2003. For the interaction potential obtained with GAUSSIAN 2003, MOLSCAT is used to derive the parameters q(L,M,M^′|E)$q(L\text{,}M\text{,}{M}^{\prime }|E)$ as a function of energy E   of the colliding partner. After averaging the parameters q(L,M,M^′|E)$q(L\text{,}M\text{,}{M}^{\prime }|E)$ over a Maxwellian distribution, the parameters Q(L,M,M^′|T)$Q(L\text{,}M\text{,}{M}^{\prime }|T)$ as a function of the kinetic temperature T in the cloud are obtained. Finally, the collisional rate coefficients have been calculated.     

薄膜二次表面镜热控涂层的辐射物性分析

认识热控涂层的热辐射物性对航天器热控制设计具有重要指导作用。文章根据薄膜二次表面镜涂层的吸收与反射过程分析,建立模型方程,结合已有的太阳吸收比、红外发射率等表观数据,采用非线性参数最小二乘法获得了薄膜材料的吸收系数和反射率等辐射物性,并分析了厚度对热控涂层太阳吸收比和红外发射率的影响。研究结果表明,聚酰亚胺薄膜对太阳光的表面反射率为0.571,吸收系数为19.343 mm-1,对红外辐射的表面反射率为0.227,吸收系数为39.615mm-1;F46薄膜对太阳光的表面反射率为0.744,吸收系数为0.757mm-1,对红外辐射的表面反射率为0.111,吸收系数为9.240mm-1。     

红外地球敏感器辐射强度在轨数据分析

为了给在轨卫星红外地球敏感器性能评估提供更多参考依据,通过对某颗长期在轨正常运行卫星所配置的红外地球敏感器辐射强度数据进行统计分析,给出辐射强度短期、中期和长期的变化规律,并分析造成这种变化的内在机理.分析结果表明,辐射强度短期与星下点纬度相关且呈周期变化;中期与季节相关且呈周期变化;长期主要与红外地球敏感器自身特性相关呈逐渐衰减趋势.该结果可以作为在轨红外辐射强度判读的依据.     

航天器进入制导方法综述

航天器制导系统的设计至关重要,直接关乎航天器能否安全返回地球或着陆行星表面指定区域。在给出航天器进入动力学模型的基础上,首先分析了进入制导问题建立及难点,然后综述了航天器进入制导方法的研究现状,分析了各类进入制导方法的优缺点。作为统一或通用方法,介绍了实际应用于中国航天工程再入返回的自适应预测校正制导方法。面向未来发展亟待解决的问题,在线快速规划可行轨迹的重要性凸显,分析了在线轨迹规划方法所需要解决的问题以及今后进入制导方法的发展方向。     

面向飞/发一体化设计的高温尾喷口流场分析

结合飞/发一体化设计理念,以提升红外隐身性能为目的,引入横向掺混技术进行尾喷管构型设计。应用计算流体力学(CFD)数值仿真方法,分别分析了圆形喷管和矩形喷管流场温度分布,并提取矩形喷管中心面,研究喷管带小孔壁板偏折角对尾流冷却效果的影响。研究结果表明:相对于入口热流温度,矩形喷口降温率约为30%,尾气流喷出后偏向两侧流动,高温核心区体积快速衰减;圆形喷口降温率约为10%,尾气流喷出后沿轴向一直保持圆柱形,高温核心区体积衰减缓慢。矩形喷口主动冷却效果明显高于圆形喷口,更有利于实现飞/发一体化的热管理及红外隐身。同时,中面带小孔壁板偏折角的大小与主动冷却效果也存在密切关系。