双轴涡喷发动机性能实时模拟简化模型

建立了能够实时模拟双轴涡喷发动机性能的数学模型。该实时模型包括:线性化的压气机特性模型、简化的涡轮特性以及非线性方程组的降维处理。在相同工况及进气条件下, 分别用非实时模型和实时模型对某型双轴加力式涡喷发动机性能进行了模拟, 并与试验结果进行了对比。结果表明, 该模型很好地解决了提高运算速度与保证计算精度之间的矛盾, 并且具有较高的收敛性。      

M stars as targets for terrestrial exoplanet searches and biosignature detection

The changing view of planets orbiting low mass stars, M stars, as potentially hospitable worlds for life and its remote detection was motivated by several factors, including the demonstration of viable atmospheres and oceans on tidally locked planets, normal incidence of dust disks, including debris disks, detection of planets with masses in the 5-20 M() range, and predictions of unusually strong spectral biosignatures. We present a critical discussion of M star properties that are relevant for the long- and short-term thermal, dynamical, geological, and environmental stability of conventional liquid water habitable zone (HZ) M star planets, and the advantages and disadvantages of M stars as targets in searches for terrestrial HZ planets using various detection techniques. Biological viability seems supported by unmatched very long-term stability conferred by tidal locking, small HZ size, an apparent short-fall of gas giant planet perturbers, immunity to large astrosphere compressions, and several other factors, assuming incidence and evolutionary rate of life benefit from lack of variability. Tectonic regulation of climate and dynamo generation of a protective magnetic field, especially for a planet in synchronous rotation, are important unresolved questions that must await improved geodynamic models, though they both probably impose constraints on the planet mass. M star HZ terrestrial planets must survive a number of early trials in order to enjoy their many Gyr of stability. Their formation may be jeopardized by an insufficient initial disk supply of solids, resulting in the formation of objects too small and/or dry for habitability. The small empirical gas giant fraction for M stars reduces the risk of formation suppression or orbit disruption from either migrating or nonmigrating giant planets, but effects of perturbations from lower mass planets in these systems are uncertain. During the first approximately 1 Gyr, atmospheric retention is at peril because of intense and frequent stellar flares and sporadic energetic particle events, and impact erosion, both enhanced, the former dramatically, for M star HZ semimajor axes. Loss of atmosphere by interactions with energetic particles is likely unless the planetary magnetic moment is sufficiently large. For the smallest stellar masses a period of high planetary surface temperature, while the parent star approaches the main sequence, must be endured. The formation and retention of a thick atmosphere and a strong magnetic field as buffers for a sufficiently massive planet emerge as prerequisites for an M star planet to enter a long period of stability with its habitability intact. However, the star will then be subjected to short-term fluctuations with consequences including frequent unpredictable variation in atmospheric chemistry and surficial radiation field. After a review of evidence concerning disks and planets associated with M stars, we evaluate M stars as targets for future HZ planet search programs. Strong advantages of M stars for most approaches to HZ detection are offset by their faintness, leading to severe constraints due to accessible sample size, stellar crowding (transits), or angular size of the HZ (direct imaging). Gravitational lensing is unlikely to detect HZ M star planets because the HZ size decreases with mass faster than the Einstein ring size to which the method is sensitive. M star Earth-twin planets are predicted to exhibit surprisingly strong bands of nitrous oxide, methyl chloride, and methane, and work on signatures for other climate categories is summarized. The rest of the paper is devoted to an examination of evidence and implications of the unusual radiation and particle environments for atmospheric chemistry and surface radiation doses, and is summarized in the Synopsis. We conclude that attempts at remote sensing of biosignatures and nonbiological markers from M star planets are important, not as tests of any quantitative theories or rational arguments, but instead because they offer an inspection of the residues from a Gyr-long biochemistry experiment in the presence of extreme environmental fluctuations. A detection or repeated nondetections could provide a unique opportunity to partially answer a fundamental and recurrent question about the relation between stability and complexity, one that is not addressed by remote detection from a planet orbiting a solar-like star, and can only be studied on Earth using restricted microbial systems in serial evolution experiments or in artificial life simulations. This proposal requires a planet that has retained its atmosphere and a water supply. The discussion given here suggests that observations of M star exoplanets can decide this latter question with only slight modifications to plans already in place for direct imaging terrestrial exoplanet missions.     

辽东湾北岸滨海湿地生态系统的功能及其利用的研究

辽东湾北岸滨海湿地生态系统具有丰富的生物资源,较高的生态价值与环境净化,蓄水防洪等特点和功能。尚存在植被开发利用不合理,污染严重,人口激增,环境被破坏等问题,应大力发展生态农业,利用湿地滞洪蓄水,改善环境,合理开发旅游资源。     

使用液态化学循环的高热效率动力研究(英文)

要使碳氢燃油在常规燃烧循环中高效燃烧,需要非常高的温度,化学循环燃烧可以为大型动力装置提供一个可行的方法。在化学循环燃烧中,使用含氧介质分子来传输两个氧化还原反应之间的氧气,含氧介质在一个反应中被氧化,在另一个与燃油的反应中被减少。从燃烧残余物中分离出含氧介质可以借助于不同的物态,如果介质用钠、钾或锌,这是液态化学循环燃烧的显著优点。液态化学循环燃烧的原理是能量和熵的循环,在考虑用于分离氮和二氧化碳零部件效率、结合水燃气交换、以及用空气作为氧气源的情况下,高的热效率(35Pa下约75%)在理论上可以达到。     

激光合成金属间化合物基复合材料研究进展

对激光合成颗粒增强金属间化合物基复合材料进行了研究,包括Ni3Al/WC、NiAl/TiC、Ti3Al/TiC和MoSi2/SiC,用扫描电镜、能谱仪和X射线衍射仪对材料成分和组织特征进行了分析,提出并讨论了影响激光合成金属间化合物基复合材料的关键问题.激光合成具有多种强韧化方法协同、提高金属间化合物强度和塑性的特点,有利于金属间化合物性能的综合改善.     

涡轮叶栅前缘上游端壁气膜冷却的传热实验研究

对前缘上游有单排和双排孔冷却的涡轮导向叶栅端壁进行了详细的传热实验,在吹风比1,2,3下获得了当地气膜冷却效率和换热系数,结合流场测量结果分析了端壁冷却和换热规律。结果表明端壁气膜冷却在很大程度上受二次流的影响,冷却效果主要由吹风比决定,低吹风比喷射时,压力面附近的一个三角形区域没有冷气的覆盖,中、高吹风比喷射可以大幅度提高平均冷却效率并使冷气很均匀的覆盖在端壁上,双排孔喷射比单排孔喷射平均效率提高1倍左右。结果还表明尽管冷气喷射使端壁换热系数随吹风比的增大而显著增大,气膜冷却还是能有效的降低端壁的热负荷,其中以中吹风比双排孔喷射的效果最为显著。      

旋转失速状态下叶片激振频率的研究

研究了各不同几何状态下（平均半径处叶片安装角从３２．９°－４７．９°，叶栅稠度从０．５８３－１．１６５）的旋转失速流场及叶片受迫振动的激振频率。在失速压力信号为非正弦信号及周向叶片并非完全轴对称的假设下，建立了旋转失速状态下叶片激振频率的预测公式，预测结果与实验结果较好的吻合表明，本文所提出的预测公式是可靠的，满足工程精度要求。     

用作热防护材料的PAN基碳纤维织物

粘胶基碳纤维织物已广泛用作烧蚀和绝热复合材料。由于行情和利润不断下降,用连续粘胶纤维制得的碳纤维制品最终可能不易买到或限制供应。因此,围绕获得相应的PAN基碳布、测定其性能并制作布带缠绕酚醛树脂复合材料开展了研究。市场上买得到的PAN基碳布具有强度高和质量均匀等特性,但绝热性和化学纯度较差。特殊的PAN基碳布是在较低的(低于1350℃)热处理温度下获得的,并且应用于20°布带缠绕酚醛复合材料中。对这种复合材料的烧蚀、热物理、机械和化学性能的测定表明,所研制的复合材料可以代替粘胶基碳布/酚醛,但纤维与基体之间的粘结和纤维的纯度尚需进一步改善。     

中层大气钠层的流星蒸发模式

本文计算了地球中层大气的钠层模式。在此模式中,流星蒸发是形成钠层的源而尘埃的吸附足汇。本文考虑和比较了有关钠层形成机制的已往工作中所出现过的所有光化学反应,选出了四十个合理而重要的化学反应作为本模式的化学基础。模式也考虑进了高度变化的涡流扩散和带电粒子受地磁场作用的向下飘移等机制。本文对各化学反应和模式中各个因素的重要性作了比较和评价。本文计算结果表明,在各高度上中层大气中的钠及其化合物的相对浓度主要取决于化学反应过程本身,与源、汇及各层间扩散机制等关系不大。虽然在钠层模式计算中必须考虑到十种钠成分,但105公里以上主要成分足钠离子(Na+)。80公里以下主要成分是氢氧化钠(NaOH)。80公里到105公里间主要成分是中性钠原子(Na)。所有成分的总浓度主要地取决于源和汇随高度的分布。大气背景及电离常数的变化可以引起钠层相当显著的季变化和周日变化。理论计算结果与历年来的观测结果作比较后可以看到两者大体上符合得相当好。      

~(201)Hg~+离子贮存式频率标准

本文讨论利用在潘宁离子收集器中贮存~201Hg~+离子实现微波频率(和时间)标准以及光频标性能的潜力与存在的问题。有许多讨论一般都适用于离子贮存式频标。激光致冷、光抽运、以及微波或光时钟跃迁的光检测,可利用在194.2nm6P~2P_(1/2)←6~2S_(1/2)跃迁的窄带幅射,而有选择地将基态超精细能级与适当的微波幅射加以混频来完成。特别适用于采用潘宁(冷阴极)离子收集器的一阶独立场微波时钟跃迁是在1.534T 磁场的25.9GHz(F,M_F)=(2,1)←→(1,1)超精细跃迁。在563nm(毫微米)的双量子无多普勒5d~96S~(22)D_(5/2)←→5d~(10)6S~2S_(1/2)迁可能是光频标所要选用的。两种频标的绝对准确度具有达到好于1×10~(-15)而频率稳定度低于10~(-16)的潜力。