精确动力学模型中的行星引力辅助轨道设计

轨道设计分为初步设计和精确模型迭代两步,初步设计基于等效脉冲模型,用圆锥曲线拼接法确定时间窗口和引力辅助产生的速度脉冲。精确模型中引力辅助看作是一个连续的过程,将简化模型得到的引力辅助双曲线轨道化为行星心目标B平面参数,以地心逃逸速度作为设计变量,通过微分修正的方法进行求解。通过算例对比分析了简化模型和精确模型设计结果之间的关系,结果表明,引力辅助脉冲等效模型精度较好。     

主动重心控制功能仿真建模与应用

减小飞行阻力、节省燃油消耗,是主动重心控制功能的重要收益之一,对功能方案的迭代和优化设计具有重要影响。基于主动重心控制技术原理和方案,耦合飞控系统模型、自动飞控系统模型、燃油系统模型、气动力模型、发动机模型和飞机六自由度（6-DOF）模型,建立某型飞机主动重心控制功能仿真模型。该模型计及燃油消耗引起的重心变化的影响,在指定高度和马赫数下,通过设置不同的目标重心位置,对主动重心控制功能的收益进行评估。结果表明：应用主动重心控制技术能给飞机带来可观的收益,尤其是目标重心越靠后,产生的收益越明显;Ma对功能的收益有影响,相同条件下,Ma越大,收益越大。     

用地球磁场和重力场成功挽救风云一号（B）卫星的控制技术

风云一号气象卫星是我国最早成功发射的太阳同步三轴稳定对地遥感卫星，由于早期的技术和器件原因，星上计算机因空间辐照而失控，造成星上贮气耗尽、卫星高速翻滚。本文详细介绍了了在卫星面临失败的情况下，作者利用地球磁场和重力场与卫星的相互作用，采用星上的磁力矩器和可用的一切手段而设计的一整套抢救这颗卫星的技术方法，并简述了经过75天的艰苦努力，使这颗濒临失败的卫星重新建立三轴稳定的对地定向姿态的历程。     

重力波波包在三维非等温大气和水平风场中非线性传播的数值研究

采用全隐欧拉格式（FICE）对重力波波包在三维非等温大气、均匀和剪切风场中的非线性传播进行了数值模拟，给出了重力波波包三维非线性传播的全过程，分析了重力波的传播特性及背景温度场、风场对重力波传播的影响。结果表明：波包扰动速度振幅的增长比在WKB条件下振幅的增长要慢；波包非线性传播的路径、能量传输速度不同于WKB近似下的结果，非线性效应导致了重力波的传播特性的改变；温度场的非均匀性会改变重力波传播的路径和速度；剪切风场使扰动速度振幅的增加变得缓慢，使垂直波长减小。     

DYNAMO: a Mars upper atmosphere package for investigating solar wind interaction and escape processes, and mapping Martian fields

DYNAMO is a small multi-instrument payload aimed at characterizing current atmospheric escape, which is still poorly constrained, and improving gravity and magnetic field representations, in order to better understand the magnetic, geologic and thermal history of Mars. The internal structure and evolution of Mars is thought to have influenced climate evolution. The collapse of the primitive magnetosphere early in Mars history could have enhanced atmospheric escape and favored transition to the present arid climate. These objectives are achieved by using a low periapsis orbit. DYNAMO has been proposed in response to the AO released in February 2002 for instruments to be flown as a complementary payload onboard the CNES Orbiter to Mars (MO-07), foreseen to be launched in 2007 in the framework of the French PREMIER Mars exploration program. MO-07 orbital phase 2b (with an elliptical orbit of periapsis 170 km), and in a lesser extent 2a, offers an unprecedented opportunity to investigate by in situ probing the chemical and dynamical properties of the deep ionosphere, thermosphere, and the interaction between the atmosphere and the solar wind, and therefore the present atmospheric escape rate. Ultraviolet remote sensing is an essential complement to characterize high, tenuous, layers of the atmosphere. One Martian year of operation, with about 5,000 low passes, should allow DYNAMO to map in great detail the residual magnetic field, together with the gravity field. Additional data on the internal structure will be obtained by mapping the electric conductivity, sinergistically with the NETLANDER magnetic data. Three options have been recommended by the International Science and Technical Review Board (ISTRB), who met on July 1st and 2nd, 2002. One of them is centered on DYNAMO. The final choice, which should be made before the end of 2002, will depend on available funding resources at CNES.     

有限振幅重力波波包在等温可压大气中的非线性传播

采用交替方向隐格式(ADI)建立了二维可压大气全非线性动力学模型，模拟了不同初始振幅的重力波波包的非线性传播，模拟结果表明非线性效应是与波振幅相关的；强非线性效应将严重阻碍波振幅的增长，使波数谱明显变化，同时减小了波包的能量传输速度，在传播过程中，强非线性效应将显著加速平均流，其结果与非线性饱和理论的预测接近。     

DORIS-based point mascons for the long term stability of precise orbit solutions

In recent years non-tidal Time Varying Gravity (TVG) has emerged as the most important contributor in the error budget of Precision Orbit Determination (POD) solutions for altimeter satellites’ orbits. The Gravity Recovery And Climate Experiment (GRACE) mission has provided POD analysts with static and time-varying gravity models that are very accurate over the 2002–2012 time interval, but whose linear rates cannot be safely extrapolated before and after the GRACE lifespan. One such model based on a combination of data from GRACE and Lageos from 2002–2010, is used in the dynamic POD solutions developed for the Geophysical Data Records (GDRs) of the Jason series of altimeter missions and the equivalent products from lower altitude missions such as Envisat, Cryosat-2, and HY-2A. In order to accommodate long-term time-variable gravity variations not included in the background geopotential model, we assess the feasibility of using DORIS data to observe local mass variations using point mascons. In particular, we show that the point-mascon approach can stabilize the geographically correlated orbit errors which are of fundamental interest for the analysis of regional Mean Sea Level trends based on altimeter data, and can therefore provide an interim solution in the event of GRACE data loss. The time series of point-mass solutions for Greenland and Antarctica show good agreement with independent series derived from GRACE data, indicating a mass loss at rate of 210 Gt/year and 110 Gt/year respectively.     

引力模型在导弹制导中的应用

目前国内导弹大部分是以惯性制导为主,一般通过提高惯性器件水平来提高导航精度.而减少引力计算误差,也是提高精度的有效途径.本文定量计算了引力计算误差对导弹精度的影响,提出了一种适用于弹上实时计算的引力高精度快速计算方法及实施流程,为工程应用奠定了基础.     

Recovery of the Earth’s gravity field from formation-flying satellites: Temporal aliasing issues

Temporal and mean gravity field models derived from the twin-satellite, leader–follower mission GRACE have provided a new type of information for Earth sciences. In this contribution, we study the potential of various alternative satellite formations for gravity field determination in the post-GRACE era in a simulation environment. In particular, the effects of spherical harmonic truncation and of temporal aliasing in the processing of gravity products from such future formations are investigated.