Transition region line-shifts in the rebound shock spicule model

Spectral emission lines created in the solar chromosphere — corona transition region show net red-shifts. It has been proposed that this may be the result of the return of spicular material. We simulate a spicule numerically using the rebound shock model and find that the resulting hydrodynamic evolution leads to a perceived up-flow in transition region spectral lines even though the average velocity in the line forming region is directed downward. The explanation for this apparent paradox is found in the correlation between density and velocity in the waves generated by the rebound shock spicule.     

跨音速压气机动静叶排相干的三维非定常流动数值分析

采用时空二阶精度ＮＮＤ显式差分格式求解三维Ｅｕｌｅｒ方程，对跨音速压气机级中动静叶排相干形成的非定常流动进行了数值分析。除动静叶排流动的控制方程体系、数值方法外，着重讨论了动静叶排计算域、网格以及边界条件的处理。对某压气机第１级动静叶排相干的非定常流场的计算，给出了叶片表面的马赫数分布、压力波动幅值，以及叶片槽道中瞬态密度等值线等，并分析了结果的合理性。     

二次流动对气冷涡轮叶栅流场的影响

针对典型跨声速高压涡轮叶型平面叶栅吸力面单排孔气膜冷却,采用数值模拟方法,比较分析了加入气膜冷却前后流场变化。结果表明,由于二次流动的影响,加入气膜冷却以后吸力面后部接近下壁面处没有受到冷气保护而直接暴露于主流高温燃气,在实际高压涡轮中将极大的降低叶片寿命。没有气膜冷却情况下,吸力面接近下壁面处边界层仍有可能因受到二次流动的影响发生转捩;加入气膜冷却情况下,气膜孔中心位置下游边界层由于射流和主流的相互作用将转变为湍流边界层,而由于孔间距的影响,只有射流和主流充分掺混以后才能影响到整个叶片的范围。     

IMF connection for energetic protons observed at Ulysses via mid-latitude solar wind rarefaction regions

As Ulysses moved inward and southward from mid-1992 to early 1994 we noticed the occasional occurrence of inter-events, lasting about 10 days and falling between the recurrent events, observed at proton energies of 0.48–97 MeV, associated with Corotating Interaction Regions (CIR). These inter-events were present for several sequences of two or more solar rotations at intensity levels around 1% of those of the neighbouring main events. When we compared the Ulysses events with those measured on IMP-8 at 1 AU we saw that the inter-events appeared at Ulysses after the extended emission (>10 days) of large fluxes of solar protons of the same energy that lasted at least one solar rotation at 1 AU. The inter-events fell completely within the rarefaction regions (dv/dt<0) of the recurrent solar wind streams. The interplanetary magnetic field (IMF) lines in the rarefactions map back to the narrow range of longitudes at the Sun which mark the eastern edge of the source region of the high speed stream. Thus the inter-events are propagating at mid-latitudes to Ulysses along field lines free from stream-stream interactions. They are seen in the 0.39–1.28 MeV/nucleon He, which exhibit a faster decay, but almost never in the 38–53 keV electrons. We show that the inter-events are unlikely to be accelerated by reverse shocks associated with the CIRs and that they are more likely to be accelerated by sequences of solar events and transported along the IMF in the rarefactions of the solar wind streams.     

Temperature Fluctuations,H II Region Abundances,and Primordial Helium

There is evidence for temperature fluctuations in Planetary Nebulae and in some Galactic H II regions. If such fluctuations occur in the low metallicity, extragalactic H II regions used to probe the primordial helium abundance, the derived 4He mass fraction, YP, could be systematically different from the true primordial value. Although this effect could be large, there are no data which allow us to estimate the size of the temperature fluctuations for the extragalactic H II regions. Therefore, we have explored this effect via Monte Carlo simulations of the data in which the abundances derived from a fiducial data set are modified by T chosen from a distribution with 0 T Tmax where Tmax is varied from 500 K to 4000 K.     

纳米粒子表面改性的研究进展

概述了无机纳米粒子表面改性的重要性，重点阐述了不同的表面处理方法及粒子与多种改性剂之间的相互作用机理。指出纳米粒子改性的目的在于降低粒子的表面能，改变粒子的表面极性，提高粒子与基体的亲和力，减少粒子间的团聚，促进纳米粒子在聚合物基体中的分散。     

A novel strategy for fine-grained semantic verification of civil aviation radiotelephony read-backs

During the flight of the aircraft, the pilot must repeat the instruction sent by the controller, and the controller must further confirm these read-backs, in this way to further ensure the safety of air transportation. However, fatigue, tension, negligence and other human factors may prevent the controller from realizing read-back errors in time, which is a huge hidden danger for the safety of civil aviation transportation. This paper proposes a novel strategy to implement fine-grained semantic ...     

Controlling factors of Region 2 field-aligned current and its relationship to the ring current: Model results

One essential component of magnetosphere and ionosphere coupling is the closure of the ring current through Region 2 field-aligned current (FAC). Using the Comprehensive Ring Current Model (CRCM), which includes magnetosphere and ionosphere coupling by solving the kinetic equation of ring current particles and the closure of the electric currents between the two regions, we have investigated the effects of high latitude potential, ionospheric conductivity, plasma sheet density and different magnetic field models on the development of Region 2 field-aligned currents, and the relationship between R2 FACs and the ring current. It is shown that an increase in high latitude potential, ionospheric conductivity or plasma sheet density generally results in an increase in Region 2 FACs’ intensity, but R2 FACs display different local time and latitudinal distributions for changes in each parameter due to the different mechanisms involved. Our simulation results show that the magnetic field configuration of the inner magnetosphere is also an important factor in the development of Region 2 field-aligned current. More numerical experiments and observational results are needed in further our understanding of the complex relationship of the two current systems.     

基于区域划分的LEO卫星星座QoS路由算法

针对LEO卫星网络中由于流量分布不均导致的拥塞问题,以及多种通信业务带来的QoS保障问题,提出了基于区域划分的多业务QoS路由算法(MSR-RP).算法考虑了信关站有限分布造成的漏斗流量问题,一方面通过划分动态区域,减少区域节点数量,降低了算法整体计算复杂度;另一方面,在轻负载区域采用最短路径算法计算路由,重负载区域采...     

Envelope protection for aircraft encountering upset condition based on dynamic envelope enlargement

Upset condition encountered by an aircraft in flight could pose great threat to flight safety, which is of chief importance in civil aviation. The causal factors have the nonlinear and multiple characteristics, and as a result the conventional envelope protection system cannot successfully do with the condition. So dynamic envelope based on differential manifold theory, which can take more coupling factors into account, is proposed as a basis to design a novel envelope protection system. Then the relationship between the dynamic envelope and the control coefficient or pilot command is obtained, and the result shows that the dynamic envelope can be enlarged with the change of control coefficient. Furthermore, quantification of flight security is realized via defining relative distance between flight state and dynamic envelope, which can detect whether there is a risk for an aircraft in flight. Finally, an envelope protection system based on dynamic envelope enlargement is proposed on the basis. NASA’s Generic Transport Model encountering hazard gust wind in climbing phase is taken as an example to verify the system’s feasibility. The result shows that the system can give a better operation encountering upset condition and to a certain extent reduce the number of accidents or incidents.