一种简易无人机载大气数据计算机的设计

大气数据参数的采集和处理是无人机的关键技术之一。本文针对无人机的具体特点，给出了一种基于C51单片机的简易大气数据计算机的设计方案，并着重对系统的硬件和软件设计进行了分析和研究。实验表明该系统满足无人机的使用要求。     

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.     

Mercury: can any ice exist at subpolar regions?

The heat transfer in a regolith subsurface layer of thickness 20 m has been theoretically simulated for the areas near Mercury's north pole aiming at the clarification of the possible existence of subsurface ice formations of different form. The paper considers different models of the icy regolith structure and composition: pure uniform amorphous ice; a porous dispersive system with ice-filled pores and voids; permafrost. For comparison the heat transfer in dry iceless regolith has been considered as well. It has been shown that the line of maximum distribution of subsurface icy formations depends on the icy regolith model, but for any one in the “hot” regions it does not go below 70°. For the “cool” regions this line has been shown to go from 5° to 10° southward than that for the “hot” ones. The possible thickness of icy regolith near the pole has been estimated for different models assuming an interior heat flow of 15 mW m⁻². It has been shown that the maximum thickness of this layer takes place at the pole and is equal to 10 km for any model.     

Stratospheric polar vortex as a possible reason for temporal variations of solar activity and galactic cosmic ray effects on the lower atmosphere circulation

Possible reasons for the temporal instability of long-term effects of solar activity (SA) and galactic cosmic ray (GCR) variations on the lower atmosphere circulation were studied. It was shown that the detected earlier ∼60-year oscillations of the amplitude and sign of SA/GCR effects on the troposphere pressure at high and middle latitudes (Veretenenko and Ogurtsov, Adv.Space Res., 2012) are closely related to the state of a cyclonic vortex forming in the polar stratosphere. The intensity of the vortex was found to reveal a roughly 60-year periodicity affecting the evolution of the large-scale atmospheric circulation and the character of SA/GCR effects. An intensification of both Arctic anticyclones and mid-latitudinal cyclones associated with an increase of GCR fluxes at minima of the 11-year solar cycles is observed in the epochs of a strong polar vortex. In the epochs of a weak polar vortex SA/GCR effects on the development of baric systems at middle and high latitudes were found to change the sign. The results obtained provide evidence that the mechanism of solar activity and cosmic ray influences on the lower atmosphere circulation involves changes in the evolution of the stratospheric polar vortex.     

上面级发射中高轨道卫星外热流分析

研究发射轨道的外热流是卫星热控制系统设计的基础。针对上面级发射轨道的特点和卫星姿态，推导出上面级滑行段和点火段瞬态及平均外热流计算公式。以北斗三号中轨导航卫星为例，给出了阳光和轨道面夹角随太阳黄经和升交点赤经的变化关系，以及最长阴影时间、滑行段旋转角速度约束条件的分析方法，在此基础上确定了上面级阶段卫星的极端外热流工况并给出了外热流计算结果。     

Two dimensional simulation of amplitude modulated electron plasma waves

Highly modulated waves near electron plasma frequency with both parallel and perpendicular polarization have been observed near diffusion region at dayside and in the tail region. In this paper, two dimensional Particle-In-Cell (PIC) simulation was performed to study the possible generation mechanism of these modulated electron plasma waves. It is shown that weak beam instability could generate the modulated Langmuir wave and the ambient magnetic field plays an important role in the formation of modulation. When the weak beam has loss cone distribution, highly modulated upper hybrid waves are generated and propagate with large angle to the ambient magnetic field. The properties of these modulated waves are discussed and compared with observations.     

导航信号模拟器上位机软件设计与实现

卫星导航信号模拟器可以模拟产生各种动态环境下接收机所接收到的导航卫星信号。为接收机的调试和测试提供仿真信号源。完整的导航信号模拟器由上位机软件、中频信号产生、射频前端电路三个单元组成。文中对信号模拟器的上位机软件单元进行详细的分析,给出软件总体流程图,阐述主要模块的功能及其实现方法,包括人机交互界面、导航电文生成模块、载体运动轨迹计算模块、卫星位置计算模块和等效伪距误差计算模块。通过与商用(?)收机联试,验证了软件设计正确可行。     

伞舱系统在火星环境中的运动特性分析

建立了火星大气环境模型和伞舱系统多体动力学模型,通过仿真分析了火星环境下伞舱系统中进入舱的运动特性,并对其在火星环境和地球环境的运动稳定性进行仿真比较分析,得出的相关结论可为探测器火星登陆技术提供参考。     

基于光纤通道的航空电子网络研究

介绍先进综合化航空电子系统结构及先进综合化航空电子系统对采用光纤统一网络互连的要求;列举光纤通道(FC)互联网络的高可靠性、容错性和确定性等指标,并评估其适于作为新一代航空电子系统互连标准;描述FC在未来航空电子系统应用中复杂的体系结构和多种上层映射协议共用的解决方案;介绍1553上层映射(FC-AE-1553)、虚拟接口结构上层映射(VIA ULP)、音频视频上层映射(FC-AV)等三种FC的上层映射协议适用于未来航空电子系统应用的特点,分析三种上层映射协议在未来航空电子系统中的应用。