液冷模块的热仿真分析

运用基于CFD的热仿真软件Flotherm对液冷模块进行了热仿真分析,分别研究了在不同环境温度,不同冷却液流量以及不同冷却液温度条件下,液冷模块内部温度场的变化规律。仿真分析结果表明,环境温度对液冷模块的温度场影响非常小;液冷模块冷却液流量的增幅与元器件温度的降幅并非正比关系;元器件温度的升幅与冷却液温度的增幅相同。     

Tilts and polarity separation in the sunspot groups and active regions at the ascending and descending phases of the cycle 23

The Solar Feature Catalogues for sunspots and active regions measured with SOHO/MDI instrument and Ca II K3 spectroheliograph of the Paris-Meudon Observatory are analyzed with the automated classification technique for sunspot groups and active region polarities. We report the first classification results for daily variations of tilt angles (normal and trigonometric ones) in sunspot groups (SG) and active (AR) regions in the cycle 23. The average normal tilts are presented for every year at the ascending and descending phases of the cycle 23 which are similar to those deduced by other authors for the cycles 19–22. The normal tilts of both the sunspot groups and active regions are shown to increase in the ascending phase and a decrease in the descending phase. Similar to SG and AR areas, the trigonometric tilts are shown to have the noticeable North–South asymmetry with the Southern hemisphere dominant in the selected ascending and descending periods. The normal tilt variations with latitude follow Joy’s law revealing a periodicity along the meridian of about 10° and reaching the maximum of 14° at the latitude of about 32° corresponding to the top of the ‘royal zone’ where the sunspots appear. The variations of polarity separation with a latitude are in an anti-phase with those of the tilts reaching a maximum at the latitude of 35° and showing a small positive separation for the groups/active regions in a vicinity of the average tilts ±40°. The ratio R of the polarity separation to the trigonometric tilt fits the linear function of a latitude φ as R = −0.0213φ − 0.1245 confirming positive separation for the polarities of active regions with the average tilts, or the dominance of activity in the Southern hemisphere activity, for the selected period of observations.     

A multi-epoch study of the C IV absorption variability in the broad absorption line quasar APM 08279+5255

Broad absorption line (BAL) variability potentially represents a powerful tool to investigate the physical nature and the structure of gas outflows in active galactic nuclei. Most existing BAL variability studies rely on observations taken at a few epochs for samples of tens of BAL QSOs. In this study we present the first “monitoring” of a single object, APM 08279+5255, which has been observed more than 20 times since 2003. All available spectra from the literature have also been analysed, including two high resolution spectra, extending the time interval from 1998 to 2012. A relative stability of the shape of the absorption profile is found. At the same time significant variations of the equivalent width are observed. A correlation of the BAL equivalent width with the QSO luminosity is found for the first time. These results suggest that changes in the ionisation state of the gas are causing opacity changes.     

HORACE: A compact cold atom clock for Galileo

HORACE (HOrloge à Refroidissement d’Atomes en Cellule = clock based on atoms cooled from vapour cell) is a compact cold caesium atom clock developed in SYRTE at Paris Observatory. This clock can operate both on ground and in microgravity environment. Design of HORACE is based on isotropic light cooling, allowing performing the whole clock sequence (cooling, atomic preparation, Ramsey interrogation and detection) at the same place. Compared to more conventional cold atom clocks such as atomic fountains, the use of isotropic light cooling simplifies both the optical part of the setup and the detection sequence, and leads to a drastic size reduction of the physics package. Very good short-term performances have been demonstrated at SYRTE since relative frequency instability of 2.2 × 10⁻¹³ τ^−1/2 has been obtained. Optimization of the long term stability is still under progress and current results show relative frequency instability around 3 × 10⁻¹⁵ in 10⁴ s of integration. With these performances, HORACE appears as a good candidate both for Galileo’s ground segment clock and for onboard Galileo clock.     

飞行器热防护与利用一体化系统实验与模拟

通过设计一种基于主动冷却的点阵桁架结构,在降低飞行器质量的同时,实现有效的热防护效果,并在该结构中加入半导体温差发电装置,将产生的气动热转化为电能,可用于飞行器小型用电设备供电.对该热防护与利用一体化系统进行了实验研究.在不同工况下,温差发电功率远大于主动冷却系统的泵功消耗,可实现主动冷却系统的自驱动.通过添加管内表面...     

采暖空调技术改造对策综合分析

本文对北京一高层建筑采暖空调系统进行了技术改造方案论证，通过对技术先进性及适用性、改造繁简程度、设备寿命以及运行等诸方面的综合技术分析，确定采用新型螺杆冷水机组＋燃气热水锅炉的方案。新的供暖空调系统安全高效运行并提供了高品质人工环境。     

放宽静稳定性在空空导弹总体设计中的应用

将主动控制技术引入空空导弹总体设计中，研究了空空导弹放宽静稳定性设计问题，讨论了放宽静稳定性设计对导弹性能的改善，最后给出了静不稳定弹体的系统稳定性判定条件，并着重讨论了静不稳定弹体的人工稳定问题，研究结果对于新一代先进空空导弹的总体设计工作有一定的参考价值。     

气膜冷却孔几何结构对流量系数的影响

为了研究火焰筒壁面气膜冷却孔几何结构对流量系数的影响规律，设计了几种具有不同几何尺寸和排列结陶的气膜冷却孔实验件。对气膜冷却孔的流量系数进行了实验研究。实验结果表明．在吹风比较小时．随吹风比的增加流量系数大幅度增加．当吹风比较大时，随吹风比的增加流量系数增幅减小。同时．在气膜孔厚径比大于1时，气膜孔的排列形式对流量系数的影响不大，当厚径比小于1时．叉排气膜孔的流量系数要高于顺排气膜孔的流量系数。     

几种液体火箭发动机喷注器的研制

介绍了几种液体火箭发动机喷注喷研制中出现的技术问题及其解决途径。同时,对双组元离心式喷嘴流量偏差作了分析,探讨了控制流量偏差的方法。提出的一种身部内冷却装置,采用斜齿缝隙钎焊整体式结构,在中等推力液体火箭发动机中进行试验得出初步结论。     

冲击粗糙肋壁面流动特性实验研究

对有初始横流的冲击粗糙肋壁面的流场进行了流动特性实验研究 ,通过对大量实验数据的整理、分析以了解多种流动和几何参数对其流动特性的影响规律 ,为优化设计涡轮叶片内部冷却结构提供相应依据