Thermal reactions in interstellar ice: A step towards molecular complexity in the interstellar medium

Complex organic molecules are widely observed in star-forming regions, although their formation mechanisms are not well understood. Solid-state chemistry is thought to play an important role, but the solid-state reaction network is poorly known. We provide a list of purely thermal reactions involving electronically stable reactants to complement existing grain chemistry networks. The kinetic parameters of the reactions are given when available. These reactions lead to the formation of complex organic molecules, which were not considered previously. Eventually, these complex molecules are either released into the gas phase or incorporated into the organic residue found in meteorites. Thermal reactions are important because they are not limited by the UV flux or the slow diffusion of the radicals, and because they involve both surface and mantle molecules. Thermal reactions represent an important step in the formation of complex organic molecules that constitute the primitive material of comets and asteroids.     

Possibility to detect the cluster emission up to R200 with XMM-Newton data

We present the results of analysis XMM-Newton data of galaxy cluster CL0016+16, which enables us to trace X-ray emission and temperature profile up to the virial radius. We obtained similar results using three different backgrounds. We checked the possibility of detection of cluster emission up to the virial radius with XMM-Newton data with hydrodynamical cosmology simulation from the Adaptive Mesh Refinement technique, code RAMSES by Teyssier [Teyssier, R. Cosmological hydrodynamics with adaptive mesh refinement. A new high resolution code called RAMSES. A&A 385, 337, 2002], convolution with XMM-Newton and the data base of the spectra by Sauvageot et al. [Sauvageot, J.-L., Belsole, E., Pratt, G.W. The late merging phase of a galaxy cluster: XMM EPIC observations of A 3266. A&A, 444, 673, 2005]. For the first time we were able to compute the mass of CL0016 up to R₂₀₀, we found, assuming hydrostatic equilibrium framework, M₂₀₀ = (1.15 ± 0.11) × 10¹⁵M_⊙.     

中介粗集及其在数据挖掘中的应用

粗集理论已成功应用于数据挖掘，如基于粗集方法的属性发现和决策规则的约简等。中介集合论是以中介逻辑为基础，也可以用于数据挖掘。文中将两者相结合，提出了中介粗集的概念。中介粗集是普通粗集的推广，为不完全信息系统的数据挖掘提供了新的工具，不仅可用于一般的信息系统，还适用于数据取空值的信息系统（允许结论取空值）。利用中介粗集进行数据挖掘不但可以得出粗集理论中的约简，还能得到更为简洁的中介约简。文中还给出了     

基于等效板模型的弹翼颤振分析

 基于等效板模型发展了一种适用于导弹翼面的动力学和颤振分析方法。在等效板建模过程中,使用简单多项式定义翼面的几何、结构和位移,利用人工弹簧近似边界条件,通过全局Ritz法得到刚度和质量矩阵的解析表达形式,通过特征值问题的求解得到翼面的固有频率和振型。通过频率和模态的初步比较发现,利用该方法得到的弹翼动力学特性与通过有限元方法得到的结果一致。然后利用这两组模态进行弹翼的颤振分析,通过对比发现,两种方法的颤振分析结果吻合,这也进一步验证了等效板方法在弹翼动力学分析方面的准确性。等效板方法为弹翼初步设计阶段的快速建模提供了一种有效工具。     

GMRT monitoring of Cyg X-1 and Cyg X-3

We present the results of low frequency radio observations of the X-ray binaries, Cygnus X-1 and Cygnus X-3, during different X-ray states. The low frequency observations were made for the first time for these sources at 0.61 and 1.28 GHz using the Giant Meter-wave Radio Telescope (GMRT) between 2003 and 2004. Both Cyg X-1 and Cyg X-3 are highly variable at low radio frequencies. We also compare our data with the observations at 15 GHz conducted by the Ryle telescope. Spectral turnover is seen for both the sources below 2 GHz. The data suggest that the change in the radio flux density in both the sources is correlated to the X-ray hardness ratio and follows a similar behavior pattern.     

基于非线性连续介质损伤力学方法的微动疲劳寿命预测

微动损伤被称为“工业癌症”,为了更加准确预测微动疲劳寿命,本文提出了一种基于多轴非线性连续介质损伤力学(NLCD)模型的微动疲劳寿命预测方法.该方法在Chaboche NLCD模型基础上,引入临界等效塑性应变幅对其进行改进,得到了适用于微动疲劳的NLCD改进模型,对桥式光滑试件和燕尾榫结构模拟件分别进行了微动疲劳寿命预测,与文献试验结果误差分散带在2倍因子之内,且预测裂纹萌生位置与试验吻合良好,验证了本文方法的有效性.     

无刷直流电机高精度换相控制

针对无刷直流电机(BLDCM)换相期间不导通相续流而产生端电压脉冲的问题,依据反电动势(EMF)过零法原理,分析了端电压脉冲产生的原因及对反电动势过零检测精度的影响,提出了一种利用软件算法避开端电压脉冲从而实现无位置传感器BLDCM高精度换相的控制方法。首先,利用条件语句及程序运行时间差避开端电压脉冲；为了在重载情况下提高所设计程序运行时间差的容错率,提出一种减小换相续流时间的方法；最后,搭建了无传感器BLDCM试验平台对上述方法进行试验验证。试验结果证明了所提方法在不同占空比和负载下的有效性和准确性。     

Space weather service activities and initiatives at LAMP (Argentinean Space Weather Laboratory group)

Since more than one decade ago, several institutions started to offer a large variety of Operative Space Weather (SWx) products. This is of major importance because Space Weather events can affect aviation communications, global positioning systems, grid electric power, satellite technologies, and human health in space. The scientific potential on solar-terrestrial physics in Argentina motivated the creation of an interdisciplinary Laboratory of Space Weather in Argentina. The Argentinean Space Weather Laboratory (in Spanish ‘Laboratorio Argentino de Meteorología del esPacio’, LAMP) was initiated in 2016, and it carries out daily monitoring of real-time information (space and ground-based instruments) on Space Weather. The information is synthesized on a weekly bulletin as a summary of the Space Weather conditions, and it is posted on a website (spaceweather.at.fcen.uba.ar). The analyzed information includes own data and of other centers that offer them publicly, and it is also analyzed and discussed later on, during monthly briefings. In particular, one of the regional products that is included in the briefing discussions and it was developed by LAMP in collaboration with INPE-EMBRACE, involves Vertical Total Electron Content (VTEC) maps in the Argentinean region. LAMP set up a Space Weather Laboratory in the Antarctic peninsula, in the Argentine Marambio base, where a Water Cherenkov radiation Detector (WCD) was installed during the Argentinean Antarctic campaign (January-March of 2019). This detector is the southern node of a Latin American Collaboration (LAGO, Latin American Giant Observatory), which is a network of WCDs installed throughout more than 10 Latin American countries.     

基于球堆叠的月壤蓄热器传热特性数值研究

月壤蓄热是月球原位资源利用的一种重要方式，也是解决未来月球基地能源需求的最具潜力的途径之一。针对月壤蓄热过程，建立了基于球形堆叠的月壤蓄热器多孔介质蓄热模型。蓄热器的壳体采用登月舱下降级的燃料罐，流体传热介质采用氦气。通过数值模拟的方法研究了不同流动压降下月壤蓄热球堆叠方式、球直径对蓄热器传热过程的影响规律和机理，并分析了蓄热动态过程。研究结果表明，月壤蓄热球在简单立方体均匀堆叠（SC）和面中心立方体均匀堆叠(FCC)两种方式下，SC堆叠方式的综合蓄热指数比FCC模式可提高302%；同时还发现月壤蓄热球的直径存在最优值，可使得蓄热器在单位泵功下获得最大的蓄热量，并且该最佳值随着流体进出口压差增加而减小。该研究可为未来月壤蓄热器的设计和优化提供理论指导。