烧结温度对Mn-Zn铁氧体吸波性能的影响

研究Mn-Zn铁氧体的烧结温度对其微波吸收性能的影响,选用了5种烧结温度制备铁氧体,并对其作了X-射线衍射相组成分析。实验表明采用1500℃高烧结的铁氧体较其他温度下烧结的吸波性好。     

微波加热实现陶瓷材料同时烧结与连接的研究

利用微波加热方法对ＺＴＡ（Ａｌ２Ｏ３＋２０ｗｔ％ＺｒＯ２）,Ｙ－ＴＺＰ（２．７ｍｏｌ％Ｙ２Ｏ３）进行了同时烧结与连接,并进行了常规加热对比试验。对ＺＴＡ、Ｙ－ＴＺＰ的烧结密度及二者的连接强度进行了评定。利用扫描电镜对微观组织进行了观察。结果表明,利用微波加热可以顺利实现陶瓷材料之间的同时烧结与连接。与常规方法相比,微波加热时致密化过程快,收缩致密化协调性好,组织细小、均匀,连接强度高。     

基于差分吸收光谱技术的烟道SO2浓度的测量

利用差分光谱吸收（DOAS）技术，测量大气中痕量污染气体的浓度，是当前环保行业一项热门技术。对此方法适当改进，可以用来监测工业烟道排出的SO2的浓度和排放量，研究了利用DOAS技术测量烟气的测量方法、数据处理以及减小误差的方法，实现了烟气中SO2的在线实时测量。     

带限位台阶的高阻尼橡胶减振器性能试验分析

航天工程中的有害振动可通过高阻尼橡胶减振器进行控制,但核心耗能单元和其他部件之间的连接容易失效。为了改进高阻尼橡胶减振器中阻尼材料和钢板的连接模式,使两者在较大变形下具有较高的机械连接性能,并且避免采用高温高压整体硫化的生产工艺,提出了一种带限位台阶的装配式高阻尼橡胶减振器。该减振器的阻尼材料和钢板之间采用常温胶黏连接模式,且在阻尼材料和钢板的连接边界面上设置了若干个具有一定高度的阶梯状限位台阶。对限位阶梯总高度分别为3 mm、4 mm、5 mm的3种不同装配式高阻尼橡胶减振器进行了不同加载频率和幅值的性能试验。试验结果表明:新型装配式高阻尼橡胶减振器在大变形下具有较强的耗能能力。带限位台阶的减振器和没有限位台阶的减振器相比,最大储能模量提高了22.3%,损耗因子提高了24.9%,且在较大位移幅值工况下,滞回曲线由原本的椭圆形变成类8字型,在保证较高阻尼力的同时使得滞回曲线所包络的面积增大,最大增幅可达588%。该新型减振器无需高温高压整体硫化,可以显著降低生产成本并提高生产效率,具有显著的性能优势和广泛的应用前景。     

The Ice Survey Opportunity of ISO

The instruments on board the Infrared Space Observatory have for the first time allowed a complete low (PHOT, CVF) to medium resolution (SWS) spectroscopic harvest, from 2.5 to 45 μm, of interstellar dust. Amongst the detected solids present in starless molecular clouds surrounding recently born stellar and still embedded objects or products of the chemistry in some mass loss envelopes, the so-called “ice mantles” are of specific interest. They represent an interface between the very refractory carbonaceous and silicates materials that built the first grains with the rich chemistry taking place in the gas phase. Molecules condense, react on ices, are subjected to UV and cosmic ray irradiation at low temperatures, participating efficiently to the evolution toward more complex molecules, being in constant interaction in an ice layer. They also play an important role in the radiative transfer of molecular clouds and strongly affect the gas phase chemistry. ISO results shed light on many other species than H₂O ice. The detection of these van der Waal's solids is mainly performed in absorption. Each ice feature observed by ISO spectrometer is an important species, with abundance in the 10⁻⁴–10⁻⁷ range with respect to H₂. Such high abundances represent a substantial reservoir of matter that, once released later on, replenishes the gas phase and feeds the ladder of molecular complexity. Medium resolution spectroscopy also offers the opportunity to look at individual line profiles of the ice features, and therefore to progressively reveal the interactions taking place in the mantles. This article will give a view on selected results to avoid to overlap with the numerous reviews the reader is invited to consult (e.g. van Dishoeck, in press; Gibb et al., 2004.). 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.     

耐碱棉纸中含铁量的测定方法

用Ｎ２ＯＣ２Ｈ２原子吸收法来测定某型导弹热电池耐碱棉纸中的铁含量。并对测定条件和干扰困素进行了综合考虑。该测定方法具有很好的灵敏度，很好的精确度、干扰少、选择性和重现性好等优点。相对标准偏差ＲＳＤ＜１．０％（ｎ＝１０）。标准加入回收率均在９８％～１０２％（ｎ＝３）范围内。完全适用于耐碱棉纸中的含铁量的控制和样品系统分析。在实际应用中取得了很好的效果。     

微波测量中电缆线变化的校正方法

根据三天线法的原理,提出了用三电缆线法来校正信号传输中由于电缆线的移动、弯曲或老化引起的电缆线传输特性的变化.该方法将三条电缆线两两组合成三对,进行三次连续的测量,从而得出电缆线的传输特性和校正因子,对测得的信号进行校正.该方法对传输信号而非反射信号的测量,克服了电缆线损耗引起的对交换反射计的使用限制.     

民用飞机机身段适坠性数值仿真分析

在飞机紧急迫降过程中,首先要保证碰撞后乘客在客舱区域有足够的逃生空间,其次基于结构强度和撞击持续时间,要确保传递给乘客的加速度和冲击载荷必须降低到人体损伤容限以下。对飞机机身部分结构进行了有限元建模,模拟了其从4.27 m的高度开始坠落,产生9.14 m/s的垂直冲击速度,整个分析过程使用ABAQUS/Explicit计算完成。对机身碰撞后的整体变形展开研究,如机身选定位置的加速度时间历程以及关键结构部件的能量吸收历程,最后确定机身隔框对冲击过程中的能量吸收起着最重要的作用,其次为蒙皮和客舱地板梁。在机身结构的右侧(本文的方向为飞行员视角,与读者看到的方向左右相反)有货舱门和门框,由于机身结构的不对称性,造成左右两侧的速度和加速度不一致。     

Black hole accretion and X-ray spectra of QSOS

Changes in Eddington accretion ratios are thought to result in X-ray spectral index changes in Galactic binary black hole systems. Objects with higher Eddington ratios have softer X-ray spectra. Can we apply this result to much more massive black hole systems such as QSOs? If so, X-ray observations will give us valuable insight into the physics of QSOs. Among QSOs, X-ray spectral index is part of a large set of correlated optical and UV observational properties, especially optical Fe II and [O III] strengths in the Hβ region. To investigate whether this set of correlations is related to Eddington ratio, we use as probes, BALQSOs that have been suggested to be youthful super-accretors. We conducted infrared spectroscopy of the Hβ rest wavelength region for a sample of BALQSOs and compared line measurements with those for high and low redshift non-BAL QSOs. Hβ line widths and bolometric luminosity are used to calculate QSO black hole masses and Eddington ratios. Our results support the hypothesis that optical Fe II and [O III] line strengths are Eddington ratio indicators in QSO central engines. A possible explanation is that strong Fe II and weak [O III] indicate abundant cold gas that could fuel near Eddington accretion.     

六端口反射计测量复介电常数的改进方法

提出了六端口反射计测量介质材料复介电常数的一种改进方法,新的算法使测量面与参考面分离,消除了传统测量方法中测量面与参考面无法完全重合引入的误差.给出超越方程的简单准确的数值解法,得到了相对介电常数多值间隔与测量频率和样品长度的关系.实际测量结果表明本文方法的有效性和实用性.