基于扩张状态观测器的高空台进气环境模拟控制技术研究

针对航空发动机高空台推力瞬变等过渡态试验对进气环境模拟控制系统所提出的强抗扰性、强鲁棒性的迫切需求,设计了一种基于扩张状态观测器（ESO）的高空台进气环境模拟主动抗扰控制技术方法。首先分析了现有高空台过渡态环境模拟的技术特点和高品质控制指标难于实现的原因;其次设计线性自抗扰控制器（LADRC）和一体化并行控制器（IPC）;最后通过仿真对高空台进气环境模拟主动抗扰控制方法进行了验证。结果表明,应用基于扩张状态观测器的主动抗扰控制技术能够大幅提高发动机过渡态试验中进气环境模拟的动态响应速度、控制精度和抗扰动能力。     

What are the physical mechanisms of eruptions and CMEs?

CMEs are due to physical phenomena that drive both, eruptions and flares in active regions. Eruptions/CMEs must be driven from initially force-free current-carrying magnetic field. Twisted flux ropes, sigmoids, current lanes and pattern in photospheric current maps show a clear evidence of currents parallel to the magnetic field. Eruptions occur starting from equilibria which have reached some instability threshold. Revisiting several data sets of CME observations we identified different mechanisms leading to this unstable state from a force free field. Boundary motions related to magnetic flux emergence and shearing favor the increase of coronal currents leading to the large flares of November 2003. On the other hand, we demonstrated by numerical simulations that magnetic flux emergence is not a sufficient condition for eruptions. Filament eruptions are interpreted either by a torus instability for an event occurring during the minimum of solar activity either by the diffusion of the magnetic flux reducing the tension of the restraining arcade. We concluded that CME models (tether cutting, break out, loss of equilibrium models) are based on these basic mechanisms for the onset of CMEs.     

Bolometric luminosities and brightness temperatures of BL Lac Objects and FR I radio galaxies

To understand the connection among the subclasses of BL Lac Objects, FR I radio galaxies and Flat spectrum radio quasars (FSRQs), here the correlations of the bolometric luminosities with redshifts and brightness temperatures of these objects are studied. The bolometric luminosities vary linearly with redshifts, but few objects are scattered at high redshift. The bolometric luminosity versus brightness temperature distribution shows a correlation between these two components, except a few scattered objects, mostly RBLs. The bolometric luminosities and brightness temperatures of FR I radio galaxies with low redshift (<0.1) and low spectral index (α_rx < 0.75) are comparable to those of XBLs and those characteristics of FR I radio galaxies, with relatively high redshift (>0.2) and high spectral index, can be comparable with RBLs with low redshift (z < 0.5) and low bolometric luminosity. Those scattered RBLs with high redshifts (z > 0.5) are believed to be in complex environment with companion galaxies, most of these RBLs are still unresolved. The bolometric luminosity and brightness temperature of these scattered RBLs are comparable to those of quasars. The FSRQs are at high redshifts and bolometric luminosities and the brightness temperatures are also high relative to BL Lac Objects. These results support the FRI/BL Lac unification scheme. It suggests that, the FR I radio galaxies may be the parent populations of the BL Lac Objects, but it needs more investigation to confirm the unification of FR I radio galaxies, XBLs and RBLs.     

太阳10.7 cm射电流量中期预报模型研究(Ⅱ)

太阳活动指数中期预报一直是空间环境业务预报的难点之一.本文在自回归方法模型的基础上,利用太阳活动区面积、位置等参数与10.7cm辐射流量之间的定量关系,根据活动区面积衰减规律,建立了一个基于活动区参数及演化规律的改进型太阳活动指数中期预报模型.通过对预报测试实例分析发现,在日面出现较大活动区导致F_(10.7)迅速增长并超过历史数据峰值的情况,在日面活动区消亡导致指数突然出现平静期的情况,新模型的预报准确性相比自回归模型有很大提高,预报的平均相对误差下降约5%～9%.由此可见,新模型在某些特定条件下提高了原有模型的精度.该研究为提高业务型太阳10.7cm射电流量中期预报模型的预报精度奠定了基础.     

一种可主动控制工作温度的低温回路热管

低温回路热管是一种应用前景广阔的航天器热控设备。为了利用低温回路热管实现航天器低温部件的主动控温,进行了低温回路热管传热性能试验,并对试验中发现的低温回路热管控温性能进行了理论分析,进而对现有低温回路热管的结构进行了改进。改进后的低温回路热管能够在全功率范围内保持系统温差（主蒸发器与冷凝器温差）恒定,并能通过调节储液器上的加热功率,实现一定温度范围内的主动温度控制,使低温回路热管具有了毛细泵回路的控温功能。     

小天体主动附着制导与控制技术研究进展

结合目前已实施的小天体附着探测任务,对小天体探测器主动附着涉及的制导与控制技术进行了系统性的回顾。首先,针对小天体附着任务风险高、不确定性强的特点,明确了主动附着的内涵,并分析了现有附着探测技术在自主性和安全性上面临的挑战,阐述了提高探测器主动附着能力的重要性。在此基础上,归纳梳理了与主动附着相关的制导与控制技术最新研究进展。最后,结合未来小天体探测任务需求,总结了今后具有进一步研究价值的几个问题。     

Galaxy evolution in groups. USGC U268 and USGC U376 in the Leo cloud

With the aim of investigating galaxy evolution in nearby galaxy groups, we analyzed the spectral energy distribution of 24 galaxies, members of two groups in the Leo cloud, USGC U268 and USGC U376. We estimated the ages and stellar masses of the galaxies by fitting their total apparent magnitudes from far-ultraviolet to near-infrared with population synthesis models. The comparison of the results for a subsample of galaxies with smooth particle hydrodynamic (SPH) simulations with chemo-photometric implementation, shows that in most cases the estimated stellar masses obtained with the two different approaches are in good agreement. The kinematical and dynamical analysis indicates that USGC U268 is in a pre-virial collapse phase while USGC U376 is likely in a more evolved phase towards virialization.     

A study of acoustic halos in active region NOAA 11330 using multi-height SDO observations

We analyze data from the Helioseismic Magnetic Imager (HMI) and the Atmospheric Imaging Assembly (AIA) instruments on board the Solar Dynamics Observatory (SDO) to characterize the spatio-temporal acoustic power distribution in active regions as a function of the height in the solar atmosphere. For this, we use Doppler velocity and continuum intensity observed using the magnetically sensitive line at 6173?Å as well as intensity at 1600?Å and 1700?Å. We focus on the power enhancements seen around AR 11330 as a function of wave frequency, magnetic field strength, field inclination and observation height. We find that acoustic halos occur above the acoustic cutoff frequency and extends up to 10?mHz in HMI Doppler and AIA 1700?Å observations. Halos are also found to be strong functions of magnetic field and their inclination angle. We further calculate and examine the spatially averaged relative phases and cross-coherence spectra and find different wave characteristics at different heights.     

星载降水测量雷达有源定标技术研究*

针对降水测量雷达的定标需求,提出基于四个有源雷达定标器的多站有源定标方法,给出定标器布设方式,并设计有源定标时序。分析定标过程中的误差源及其对定标精度的影响,仿真验证表明,四站有源定标的波束匹配偏差定标精度优于0.01°,系统定标精度优于1dB。方法在满足高精度定标的同时,能够实现在降水观测模式下对雷达性能的评估,降低天地定标试验的复杂度。     

一种高超声速试飞器助推段主动弹性抑制方法

针对高超声速试飞器助推段由于其高静不稳定特性所引起的低频弹性模态与刚体高带宽控制之间动态耦合问题，具有低频模态和大静不稳定度等特征，引入主动弹性抑制技术，即在传统控制器的设计基础上引入弹性振动能量在线辨识技术相结合的改进自适应增广控制技术(Adaptive augmenting control, AAC)，动态改变开环系统控制增益，以降低弹性模态对舵机的影响，同时增加刚体控制系统的稳定性。仿真结果验证了该方法能够有效减小由干扰激励出的弹性模态所引起的附加舵机摆角，抑制伺服弹性耦合作用。该方法对高超声速试飞器助推段的控制具有重要的理论意义和工程应用价值。