矩形AT切谐振器中耦合模的能陷

沿Z′方向伸长,宽(沿x)厚比(～3)小的矩形AT切谐振器,有很强的能陷,而这个问题在理论上还没有搞清楚。在特定的实验条件下,用干涉法测量与e~(?)成比例的振幅衰减,得出(?)=0.33,然而按照肖克雷(Shockley)等人(1966)的能陷理论,则得到(?)=0.088。测得的衰减常数与观察到的质量因数(一般为500000)是一致的。用闵德林(Mindlin)(1951)的及闵德林和盖奇斯(Gazis)(1961)的片子公式,可以把厚度切变与弯曲和面切变的耦合考虑进去。尽管如此,还是得到了同前面理论值几乎一样的衰减常数。这种谐振器的固有稳定度优于10~(-10)/秒。     

磷石膏基碾压砼

磷石膏作为建筑材料最有效的作用就是用于碾压砼中，磷石膏不会影响砼强度，其干缩补偿作用限制了裂缝的发生。     

Searching for life on Mars: selection of molecular targets for ESA's aurora ExoMars mission

The European Space Agency's ExoMars mission will seek evidence of organic compounds of biological and non-biological origin at the martian surface. One of the instruments in the Pasteur payload may be a Life Marker Chip that utilizes an immunoassay approach to detect specific organic molecules or classes of molecules. Therefore, it is necessary to define and prioritize specific molecular targets for antibody development. Target compounds have been selected to represent meteoritic input, fossil organic matter, extant (living, recently dead) organic matter, and contamination. Once organic molecules are detected on Mars, further information is likely to derive from the detailed distribution of compounds rather than from single molecular identification. This will include concentration gradients beneath the surface and gradients from generic to specific compounds. The choice of biomarkers is informed by terrestrial biology but is wide ranging, and nonterrestrial biology may be evident from unexpected molecular distributions. One of the most important requirements is to sample where irradiation and oxidation are minimized, either by drilling or by using naturally excavated exposures. Analyzing regolith samples will allow for the search of both extant and fossil biomarkers, but sequential extraction would be required to optimize the analysis of each of these in turn.     

采用收缩算法的自适应时空处理：使用真空数据的验证结果

本文叙述了这载雷达所记录的真实杂波数据的处理结果,该雷达采用了一个有由８天线组成的阵列天。处理中采用了构形为梯形收缩阵的时空处,达到了消除杂波和干扰的目的。     

A compliant polymorphing wing for small UAVs

This paper presents the development of a novel compliant polymorphing wing capable of chord and camber morphing for small UAVs. The morphing wing can achieve up to 10% chord extension and ±20° camber changes. The design, modeling, sizing, manufacturing and mechanical testing of the wing are detailed. The polymorphing wing consists of one continuous front spar fixed to the fuselage and a rear spar on each side of the wing. Each rear spar can translate in the chordwise direction(chord morphing) and rotate around itself(camber morphing). A flexible elastomeric latex sheet is used as the skin to cover the wing and maintain its aerodynamic shape whilst allowing morphing. The loads from the skin are transferred to the spars using the compliant cellular ribs that support the flexible skin and facilitate morphing. Pre-tensioning is applied to the skin to minimize wrinkling when subject to aerodynamic and actuation loads. A rack and pinion actuation system,powered by stepper motors, is used for morphing. Aero-structural design, analysis and sizing are conducted. Performance comparison between the polymorphing wing and the baseline wing(non-morphing) shows that chord morphing improves aerodynamic efficiency at low angles of attack while camber morphing improves efficiency at high angles of attack.     

Is the presence of oxygen on an exoplanet a reliable biosignature?

We revisit the validity of the presence of O(2) or O(3) in the atmosphere of a rocky planet as being a biosignature. Up to now, the false positive that has been identified applies to a planet during a hot greenhouse runaway, which is restricted to planets outside the habitable zone (HZ) of the star that are closer to the star. In this paper, we explore a new possibility based on abiotic photogeneration of O(2) at the surface of a planet that could occur inside the HZ. The search for such a process is an active field of laboratory investigation that has resulted from an ongoing interest in finding efficient systems with the capacity to harvest solar energy on Earth. Although such a process is energetically viable, we find it to be a very unlikely explanation for the observation of O(2) or O(3) in the atmosphere of a telluric exoplanet in the HZ. It requires an efficient photocatalyst to be present and abundant under natural planetary conditions, which appears unlikely according to our discussion of known mineral photochemical processes. In contrast, a biological system that synthesizes its constituents from abundant raw materials and energy has the inherent adaptation advantage to become widespread and dominant (Darwinist argument). Thus, O(2) appears to continue to be a good biosignature.     

气固紊流剪切流中颗粒弥散的拉格朗日模拟

本文提出了一种对于气固两相紊流剪切流中圆形固体颗粒弥散的拉格朗日拟计算方法,其中考虑了颗粒间的磁撞对流体相和颗料相的影响,应用该方法对一气固紊流剪切流场进行了模拟计算,并对有、无颗粒间磁撞情况下的模拟计算结果与Lavieville用大涡模拟方法的研究结果进行了比较,并进行了讨论。