Pre-Main Sequence Stars Seen by ISO

Observations of pre-main sequence objects (T Tauri, Herbig Ae/Be and FU Orionis stars) obtained with the instrumentation on board the Infrared Space Observatory (ISO) are reviewed. All the observations have been mainly carried out by using the two spectrographs SWS and LWS, adopting their low resolution modes and such data have been used both for lines detection and to reconstruct the spectral energy distributions. Line emission and photometric behaviour of pre-main sequence objects have been analyzed in the framework of the current models, discussing the agreement (or disagreement) with them and trying to derive the questions which should be answered by the forthcoming FIR instrumentation. Based on observations with ISO, an ESA project with instruments funded by ESA Member States (especially the PI countries: France, Germany, The Netherlands, and the United Kingdom), and with the participation of ISAS and NASA.     

人造硬壳层扩散作用的研究

主要研究人造硬壳层的扩散作用，运用有限元模拟的方法，在规范规定的基础上确定出了应力扩散角，且得出加肋梁后应力扩散角基本不变的结论。讨论了加肋梁后固化双层地基的硬壳层等效厚度，为工程应用提供参考。     

Extrasolar solar-sail trajectories and dark matter

Hyper-thin, high-speed solar-photon sail space probes exploring the Sun?s Oort comet cloud could also be used to set an upper bound to the concentration of WIMPS (weakly interacting massive particles), one of the suggested (but unconfirmed) forms of dark matter within the vicinity of the solar system. Newton?s Shell Theorem would be applied to determine variations in apparent solar mass as the probe moves further out from the Sun. Application of this technique to the trajectories of Pioneer 10/11 reveals that the upper limit to WIMP concentration within ~60 AU of the Sun is ~0.2 Earth masses, as revealed in studies of the Pioneer Anomaly. If the published accuracy of the Pioneer acceleration measurements can be increased by an order of magnitude, probe trajectory measurements out to ~10,000 AU may confirm or falsify the hypothesis that WIMP mass within the solar vicinity is ~3X star mass. It is shown that a space-manufactured ~40-nm thick beryllium hollow-body solar sail deployed from a ~0.07 AU perihelion is a candidate spacecraft for such a mission. Possible science-team organization strategy for a ~100-year mission to ~10,000 AU is discussed.     

试用暗物质理论解释惯性和惯性力的物理机制(上)

基于对暗物质的多年探讨,我们认为宇宙空间是具有质量、相对均匀、连续稳定和有相当弹性暗物质群体(DMG)的空间.自然、宇宙万物终生处于群体引力制约之中,它们因此也获得了相应的惯性.本文立足于上述的宇宙空间,借助宇宙学原理、马赫原理和爱因斯坦等效原理,提出了物质客体的惯性机制和被称为虚力的惯性力机制 同时本文也解读所有惯...     

临时航线运行效果评估研究

依托2012—2015年福建空管分局进近情况及福州长乐国际机场航班延误情况，由专家及一线管制员为各因素不同延误等级所占比重进行打分，建立延误等级模型，再通过打分情况建立物元评估模型，得出关联隶属度评估机场综合延误程度，以及使用临时航线前后延误程度的变化，最后，得到了福州长乐机场延误影响因素及综合延误程度的定性定量分析结果。     

Optical/infrared observations unveiling the formation,nature and evolution of High-Mass X-ray Binaries

In this review I first describe the nature of the three kinds of High-Mass X-ray Binaries (HMXBs), accreting through: (i) Be circumstellar disc, (ii) supergiant stellar wind, and (iii) Roche lobe filling supergiants.     

Did life exist on Mars? Search for organic and inorganic signatures, one of the goals for “SAM” (sample analysis at Mars)

Observation of Mars shows signs of a past Earth-like climate, and, in that case, there is no objection to the possible development of life, in the underground or at the surface, as in the terrestrial primitive biosphere. Sample analysis at Mars (SAM) is an experiment which may be proposed for atmospheric, ground and underground in situ measurements. One of its goals is to bring direct or indirect information on the possibility for life to have developed on Mars, and to detect traces of past or present biological activity. With this aim, it focuses on the detection of organic molecules: volatile organics are extracted from the sample by simple heating, whereas refractory molecules are made analyzable (i.e. volatile), using derivatization technique or fragmentation by pyrolysis. Gaseous mixtures thus obtained are analyzed by gas chromatography associated to mass spectrometry. Beyond organics, carbonates and other salts are associated to the dense and moist atmosphere necessary to the development of life, and might have formed and accumulated in some places on Mars. They represent another target for SAM. Heating of the samples allows the analysis of structural gases of these minerals (CO₂ from carbonates, etc.), enabling to identify them. We also show, in this paper, that it may be possible to discriminate between abiotic minerals, and minerals (shells, etc.) created by living organisms.     

干式变压器数据采集与测控系统中的数据传输研究

干式变压器的数据采集与监控系统是其安全工作的重要组成部分。本文介绍了该系统中数据传输网络的组成、工作原理及数据传输机制,特别是设计独特的RS-232与RS-485之间的无源电平转换接口模块。     

基于谐波平衡法的含Iwan模型干摩擦振子非线性振动

通过谐波平衡法,研究了由Iwan模型和1个质量块构成的干摩擦振子系统的自由振动和受迫振动问题.对于自由振动,推导了系统卸载和加载过程中各自对应的非线性运动方程;通过谐波平衡法,求得了各方程的1阶谐波解;为了得到方程正确的数值解,提出了确定零速度时刻的策略;数值算例结果表明:谐波平衡法与数值方法得到结果吻合较好,从而验证了谐波平衡法求解此类问题的有效性.对于系统微滑移下的受迫振动,采用谐波平衡法求得了系统的幅频关系.最后,对Iwan模型阻尼特性的研究发现,模型等效黏性阻尼比与其振幅存在非线性关系.      

二自由度扭转干摩擦系统的频域响应计算方法

针对一类作扭转振动的干摩擦系统,基于库仑阻尼模型和谐波平衡思想给出了其频域响应的求解方法,考虑了干摩擦界面上可能出现的周期内全滑移运动及阻滞-滑移运动.首先,建立了扭转干摩擦系统的二自由度集中质量模型,并进行了无量纲化.其次,建立了以谐波平衡思想处理该动力学模型的方法,并给出了系统的接触面作周期内全滑移运动及阻滞-滑移运动的判定条件.最后,对于这两种接触运动状态,分别给出了其摩擦力的处理方法和谐波展开形式,从而建立了扭转干摩擦系统的频域求解方法.以此方法计算了系统在一组不同的正压力下的响应,其结果与数值积分法所得的结果取得了相当的一致.此半解析方法较数值积分方法更能揭示扭转干摩擦系统的工作机理,并可以大幅提高计算时间,其推导和求解过程可用于类似的非线性系统.