CFRP超高周疲劳损伤演化过程

碳纤维增强树脂基复合材料（CFRP）在航空航天等领域得到广泛应用，CFRP构件的超高周疲劳问题逐渐凸显出来。本文采用超声三点弯曲疲劳试验系统对CFRP复合材料的损伤演化过程进行研究。结果表明：CFRP复合材料在超高周三点弯曲加载下的S-N曲线呈阶梯状，尤其在10⁸周次后，其疲劳强度明显下降。通过对CFRP复合材料在同一视场不同周次下的损伤过程进行分析，发现该材料在超高周加载下的损伤形貌主要表现为3种特征：纤维束交叉处基体损坏、近纤维束平行段基体空洞、基体贯穿，并随着加载周次的增加，其损伤过程也按照这3种特征依次呈现出来。     

The relationship between inductive electric field and flares

We observationally deduce the inductive electric field in the photosphere for the first time from the horizontal velocities computed by local correlation tracking (LCT) technique and the vector magnetic fields derived from vector magnetograms. We study the relationship between E and powerful flares (X-class) of four active regions (ARs): NOAA 10720, 10486, 9077 and 8100. It is found that the kernels of flares are roughly located near the inversion lines where maxima of E are observed. Our results show that E relates to the accumulation of non-potentiality in the photosphere and the transportation of non-potentiality from the photosphere to the corona.     

用DE求解最小能量借力飞行问题

提出了一种差分演化算法（DE）以求解最小能量借力飞行问题。分析借力飞行的物理过程,用演化算法给出最小能量借力飞行的优化模型。优化算例表明：该算法结果较文献更优。     

Solar Nebula Magnetohydrodynamics

The dynamical state of the solar nebula depends critically upon whether or not the gas is magnetically coupled. The presence of a subthermal field will cause laminar flow to break down into turbulence. Magnetic coupling, in turn, depends upon the ionization fraction of the gas. The inner most region of the nebula (≲0.1 AU) is magnetically well-coupled, as is the outermost region (≳10 AU). The magnetic status of intermediate scales (∼1 AU) is less certain. It is plausible that there is a zone adjacent to the inner disk in which turbulent heating self-consistently maintains the requisite ionization levels. But the region adjacent to the active outer disk is likely to be magnetically ``dead.' Hall currents play a significant role in nebular magnetohydrodynamics. Though still occasionally argued in the literature, there is simply no evidence to support the once standard claim that differential rotation in a Keplerian disk is prone to break down into shear turbulence by nonlinear instabilities. There is abundant evidence—numerical, experimental, and analytic—in support of the stabilizing role of Coriolis forces. Hydrodynamical turbulence is almost certainly not a source of enhanced turbulence in the solar nebula, or in any other astrophysical accretion disk. This revised version was published online in June 2006 with corrections to the Cover Date.     

Standard Solar Composition

We review the current status of our knowledge of the chemical composition of the Sun, essentially derived from the analysis of the solar photospheric spectrum. The comparison of solar and meteoritic abundances confirms that there is a very good agreement between the two sets of abundances. They are used to construct a Standard Abundance Distribution. This revised version was published online in June 2006 with corrections to the Cover Date.     

管制-飞行状态相依网络演化过程

动态、准确的管制系统运行态势预测是航空运输系统各相关单位开展协同决策的关键基础。基于航空器间的冲突情况、管制员对航空器的管控情况以及管制移交情况构建管制-飞行状态相依网络,探究、分析其演化规律,采用相关性分析和主成分分析证明了所选5项指标的合理性。设置自由飞行和固定航线飞行两种仿真场景,通过计算平均节点度、平均点强等拓扑指标的最大李雅普诺夫指数证明各时间序列均具有混沌特性,选择长短期记忆（LSTM）人工神经网络方法对各时间序列的演化规律进行预测,并与其他预测算法进行对比。仿真结果表明LSTM算法能对管制系统的演化过程进行有效的预测,且预测精度高于贝叶斯算法和支持向量机算法;在自由飞行条件下,5项指标的预测误差绝大部分在20%以内,固定航线飞行的预测效果优于自由飞行。     

非等强度多道冲击波作用下空泡溃灭机制分析

航空航天、生物医学等领域均存在冲击波与空泡作用问题,冲击波尤其是多道冲击波作用下空泡溃灭包含着复杂的多相瞬变行为与物理现象。基于自主搭建的可压缩多相流并行数值平台,对液体中单一/多道冲击波与空泡的作用过程进行了数值模拟。通过对冲击波作用下空泡内波系性质,以及多道冲击波与空泡作用后的系列反射波系在液体中的相互作用过程进行详细解析,分析了不同冲击波作用下空泡的形变演化过程,探究了空泡的溃灭机制与特性。研究发现,相较于单一冲击波的作用,多道冲击波作用下空泡内部及周围液体流场中的波系结构更为复杂,然而无论是单一冲击波或是多道冲击波工况,其最终诱发的空泡溃灭形态均十分相似。而且,当空泡发生溃灭前所受到多道冲击波的总强度与单一冲击波强度相等时,空泡的溃灭波强度也十分相近,为多道冲击波与空泡作用效果的定量化评估提供了理论基础和依据。     

基于Kriging代理模型的约束差分进化算法

广泛应用的高精度分析模型使得飞行器设计优化的计算成本不断增加,为了缩短优化耗时,基于代理模型的进化算法（SAEAs）近年来得到了广泛关注。针对现有SAEAs处理约束优化问题优化效率低下的缺陷,提出了一种基于Kriging代理模型的约束差分进化算法（KRG-CDE）,结合约束改善概率与最优适应度定制了一种改进的可行准则,从而提高新增样本点的潜在可行性与最优性,并根据种群改善情况,平衡算法全局探索与局部搜索性能。标准测试算例对比研究结果表明,相比于基于全局与局部代理模型的差分进化算法、（μ+λ）-约束差分进化算法,KRG-CDE算法在优化效率、全局收敛性及鲁棒性等方面具有显著优势。最后,运用KRG-CDE算法求解全电推卫星多学科设计优化问题,验证了该算法的工程实用性。     

SETI in the light of cosmic convergent evolution

Theodosius Dobzhansky, one of the founding fathers of the modern evolutionary synthesis, once famously stated that “nothing makes sense in biology except in the light of evolution”. Here it will be argued that nothing in astrobiology makes sense except in the light of “Cosmic Convergent Evolution” (CCE). This view of life contends that natural selection is a universal force of nature that leads to the emergence of similarly adapted life forms in analogous planetary biospheres. Although SETI historically preceded the rise of astrobiology that we have witnessed in the recent decade, one of its main tenets from the beginning was the convergence of life on a cosmic scale toward intelligent behavior and subsequent communication via technological means. The question of cultural convergence in terms of symbolic exchange, language and scientific capabilities between advanced interstellar civilizations has been the subject of ongoing debate. However, at the core of the search for extraterrestrial intelligence lies in essence a biological problem since even post-biological extraterrestrial intelligences must have had an origin based on self-replicating biopolymers. Thus, SETI assumes a propensity of the Universe towards biogenesis in accordance with CCE, a new evolutionary concept which posits the multiple emergence of life across the Cosmos. Consequently, we have to wonder about the biophilic properties the Universe apparently exhibits, as well as to try to find an encompassing theory that is able to explain this “fine-tuning” in naturalistic terms. The aims of this paper are as follows: 1) to emphasize the importance of convergent evolution in astrobiology and ongoing SETI research; 2) to introduce novel and biology-centered cosmological ideas such as the “Selfish Biocosm Hypothesis” and the “Evo Devo Universe” as valuable arguments in theorizing about the origin and nature of extraterrestrial intelligence and 3) to synthesize these findings within an emerging post-biological paradigm on which future SETI efforts may be founded.     

The ultraviolet view of the Magellanic Clouds from GALEX: A first look at the LMC source catalog

The Galaxy Evolution Exporer (GALEX) has performed unprecedented imaging surveys of the Magellanic Clouds (MC) and their surrounding areas including the Magellanic Bridge (MB) in near-UV (NUV, 1771-2831 Å) and far-UV (FUV, 1344-1786 Å) bands at 5^″$5^{″}$ resolution. Substantially more area was covered in the NUV than FUV, particularly in the bright central regions, because of the GALEX FUV detector failure. The 5σ$\sigma$ depth of the NUV imaging varies between 20.8 and 22.7 (ABmag). Such imaging provides the first sensitive view of the entire content of hot stars in the Magellanic System, revealing the presence of young populations even in sites with extremely low star-formation rate surface density like the MB, owing to high sensitivity of the UV data to hot stars and the dark sky at these wavelengths.