Inner core wobble and free core nutation of pulsar PSR B1828-11

PSR B1828-11 has long-term, highly periodic and correlated variations in pulse shape and a slow-down rate with period variations of approximately 1000, 500 and 250 days [Stairs, I.H., Lyne, A.G., Shemar, S.L. Evidence for free precession in a pulsar. Nature 406, 484–486, 2000]. There are three potential explanations of pulses time-of-arrival from a pulsar. These are related to the interior of the neutron star, planetary bodies, free precession and nutation. We use the Hamiltonian canonical method of Getino (1995) for analyzing the dynamically symmetric pulsar PSR B1828-11, consisting of a rigid crust, elliptical liquid outer core and solid inner core. Using the theory of differential rotation of a pulsar, we investigate the dependence on Chandler wobble period, inner core wobble, retrograde free core nutation and prograde free inner core nutation from ellipticity of the inner crystal core, outer liquid core and total pulsar.     

CO2气体保护焊的波形模糊逻辑控制的方法

针对CO2气体保护焊恒流特性控制中弧长稳定性差问题,提出了弧长的波形模糊逻辑控制方案,介绍了波形控制系统工作原理和模糊逻辑控制器设计方法,并进行了试验研究.研究结果表明,此波形模糊逻辑控制系统完全实现了弧长恒定控制,得到焊接过程稳定,飞溅小和焊缝成形好等优良的工艺性能.     

Bottom side profiles for two close stations at the southern crest of the EIA: Differences and comparison with IRI-2012 and NeQuick2 for low and high solar activity

Bottom side electron density profiles for two stations at the southern crest of the Equatorial Ionization Anomaly (EIA), São José dos Campos (23.1°S, 314.5°E, dip latitude 19.8°S; Brazil) and Tucumán (26.9°S, 294.6°E, dip latitude 14.0°S; Argentina), located at similar latitude and separated by only 20° in longitude, have been compared during equinoctial, winter and summer months under low (year 2008, minimum of the solar cycle 23/24) and high solar activity (years 2013–2014, maximum of the solar cycle 24) conditions. An analysis of parameters describing the bottom side part of the electron density profile, namely the peak electron density NmF2, the height hmF2 at which it is reached, the thickness parameter B₀ and the shape parameter B₁, is carried out. Further, a comparison of bottom side profiles and F-layer parameters with the corresponding outputs of IRI-2012 and NeQuick2 models is also reported. The variations of NmF2 at both stations reveal the absence of semi-annual anomaly for low solar activity (LSA), evidencing the anomalous activity of the last solar minimum, while those related to hmF2 show an uplift of the ionosphere for high solar activity (HSA). As expected, the EIA is particularly visible at both stations during equinox for HSA, when its strength is at maximum in the South American sector. Despite the similar latitude of the two stations upon the southern crest of the EIA, the anomaly effect is more pronounced at Tucumán than at São José dos Campos. The differences encountered between these very close stations suggest that in this sector relevant longitudinal-dependent variations could occur, with the longitudinal gradient of the Equatorial Electrojet that plays a key role to explain such differences together with the 5.8° separation in dip latitude between the two ionosondes. Furthermore at Tucumán, the daily peak value of NmF2 around 21:00 LT during equinox for HSA is in temporal coincidence with an impulsive enhancement of hmF2, showing a kind of “elastic rebound” under the action of the EIA. IRI-2012 and NeQuick2 bottom side profiles show significant deviations from ionosonde observations. In particular, both models provide a clear underestimation of the EIA strength at both stations, with more pronounced differences for Tucumán. Large discrepancies are obtained for the parameter hmF2 for HSA during daytime at São José dos Campos, where clear underestimations made by both models are observed. The shape parameter B₀ is quite well described by the IRI-2012 model, with very good agreement in particular during equinox for both stations for both LSA and HSA. On the contrary, the two models show poor agreements with ionosonde data concerning the shape parameter B₁.     

壁稳电弧等离子体温度和辐射标准设备的研制

研制了氩壁稳电弧等离子体装置,其最大功率25kW,电流0～140A,4小时内电流的稳定性0.005%,纹波系数0.1%。在可靠的状态诊断实验基础上测试了主要性能。当压力为0.1～0.5MPa、电流不小于20A 时,电弧轴心区等离子体是LTE(局部热力学平衡)的。60A 电流下4小时内 ArI430.0nm 谱线辐射的稳定性±1.0%,1个月内的再现性±1.8%,温度可调范围10000～16000K,不确定度0.4%。同时测定了某些特定谱线斯塔克宽度与电子密度的实验关系。结果表明,性能完全达到了建立10000～15000K温度和近紫外高强度及真空紫外辐射标准的要求。     

电弧加热器变参数运行技术研究

电弧加热器通过调节空气流量和电弧电流实现变参数运行,可以更接近实际地模拟飞行器再人轨道。笔者论述了电弧加热器变参数运行的技术原理、试验设备改造、测试探针研制及原理性试验等。研究结果表明：供电、供气、控制等系统经过适当改造,电弧加热器可以实现变参数运行。     

铝锂合金氩弧焊与激光焊研究

研究了Ａｌ－Ｌｉ－Ｍｇ－Ｃｕ－Ｚｒ系国产铝锂合金的焊接性。研究表明，用净化的氩气保护并带拖罩的氩弧焊接铝锂合金，焊接接头及其热影响区表面仅有轻微的氧化色。金相分析表明，焊接接头结合良好，且有相当的机械性能。电子探针微区域分析表明，焊缝与热影响区及母材成分除锂未能分析，其余成分变化甚微，厚度３．５０ｍｍ试样均焊透。用ＹＡＧ激光焊，氩气保护，单面焊能焊透≤０．７０ｍｍ厚的铝锂合金板，而双面焊能焊≤１．５０ｍｍ厚的板，焊件的接头及其热影响区保持原金属光泽，焊缝窄。微区域成分分析表明，焊缝、热影响区与母材几乎无变化。     

电弧熔丝增材制造复合填充路径规划算法

合理的路径规划可以提高电弧熔丝增材制造成形零件的表面质量和强度。针对电弧熔丝增材制造的特点,将多种增材制造路径规划算法相结合,提出了一种复合路径规划算法,实现了单空洞截面的填充,并进一步讨论了其他类型截面的路径规划方法。在填充截面过程中,内外表面采用轮廓偏置路径填充,保证了零件的表面质量;零件内部采用改进的扫描线算法进行填充,减少了空行程,提高了成形效率。实验验证了本文算法填充复杂截面轮廓的可行性。     

燃油冷却面板传热特性试验与计算分析研究

采用热电偶测温、气壁红外测温及燃油样品裂解度测量等多种手段,在DJ-21电弧加热器上进行了燃油冷却面板传热特性试验.进行了共计19次燃油冷却面板传热特性试验,试验高状态对应平均热流为1.6MW/m2,低状态对应平均热流为1.1MW/m2;用于冷却的燃油质量流率为1.84~5.8g/s.为了反映冷却面板热流密度分布,以喷管三维流动计算结果作为输入条件,将计算得到的热流密度与试验测量的冷壁热流密度比较,用以确定流场计算方案、流场切取方案和热流密度计算方案.发展了冷却面板稳态准三维热分析程序,将等效热流对应的冷壁对流换热系数和燃气总温作为高温燃气侧的边界条件.使用热分析程序完成了相应的计算.通过试验与计算数据对比研究,表明热分析计算的可信性.试验验证了冷却面板的设计与加上是可行的.     

发动机滑油消耗率监控的精益管理

应用精益管理的方法,利用大数据管理技术,分析和改进发动机滑油消耗率的监控方式。     

基于MPS4021的20W LED驱动电源设计

采用原边反馈方案设计出一款20W LED驱动电源,通过变压器初次级隔离省去了副边反馈电路,提高了驱动电源的安全性和可靠性,并节约了BOM成本。所设计的驱动电源实现了在全电压范围内输出电流精度达±5%、功率因数大于0.9、效率大于85%,使用寿命大于3万小时,电磁干扰符合EN55015限制要求,并且具备有过流保护和过压保护功能,对设计大功率LED驱动电源具有一定的参考价值。