激光捷联惯导车载重力测量试验

惯性导航系统中加速度计测量的比力是载体运动加速度与重力加速度的矢量和,当载体运动加速度能够被有效分离时,满足一定精度水平的惯性导航系统就可以成为动态重力仪。捷联式惯性导航系统体积小、重量轻、系统组成简单,可以在记录下惯性器件原始输出信息之后,通过离线处理过程进行数据处理和精度挖掘。本文通过对某高精度激光捷联惯导进行相应的软硬件更改,获得了兼具导航及重力测量功能的一体式动态重力仪。地面车载试验是验证动态重力仪的测量精度的有效手段之一,本文将一组高速公路重复测线的数据进行了处理和分析,结果表明在平均车速72km/hr的条件下,半波长分辨率2km,自由空间重力异常内符合精度优于1mGal。     

Temporal and spatial variation of equatorial ionization anomaly by using multistation ionosonde data for the 19th solar cycle over the Indian region

The paper deals with the study of temporal and spatial variation of equatorial ionization anomaly (EIA) phenomenon along with its dependence on solar activity and season during the 19th solar cycle by using seven Indian ionosonde stations. Present study is an attempt to carry out the comprehensive study of EIA by using the limited number of ground based instruments. This has been achieved by performing the Gaussian fitting over the latitudinal distribution of F2-region critical frequency (foF2) data. Results reveal that the phenomenon of EIA has a strong dependence on solar activity and seasons. The EIA crest exhibits the feature of latitudinal shifting and expansion with increasing solar activity. It is found out that the effect of solar cycle and seasons on EIA is local time dependent. The observations were also compared with the IRI-2001 model predictions and results reveal that the model values are in general agreement with the observed values with some discrepancies, particularly during the high solar activity period and morning sector. The results have been discussed in the light of relative contribution from transequatorial interhemispheric neutral wind and strength of equatorial fountain process during different local time, season and solar activity levels. Furthermore, an attempt is made to parameterize the location and foF2 of the EIA crest by using the regression analysis. These results can be used to predict the latitudinal position and foF2 of the EIA crest for any given 12-month running average sunspot number (R12).     

Seismo-ionospheric anomalies in total electron content of the GIM and electron density of DEMETER before the 27 February 2010 M8.8 Chile earthquake

In this paper we examine the pre-earthquake ionospheric anomalies by the total electron content (TEC) extracted from GIM (global ionospheric map) and the electron density (Ne) observed by the DEMETER (Detection of Electro-Magnetic Emissions Transmitted from Earthquake Regions) satellite during the 2010 M8.8 Chile earthquake. Temporal variations show the nighttime TEC and Ne simultaneously increase 9–19 days before the earthquake. A cross-comparison of data recorded during the period of 1 February to 3 March in 2006–2010 confirms the above temporal anomalies specifically appear in 2010. The spatial analyses show that the anomalies tend to appear over the epicenter.     

水下重力辅助惯性导航关键技术研究及实现

重力辅助惯性导航已渐成水下导航领域的研究热点,其实现是一项复杂的工程,涉及多项的关键技术.文章首先介绍了重力辅助导航的基本原理;之后详细阐述了在真实海洋环境下,重力辅助导航所需解决的若干关键技术问题,并给出了相应的研究成果;最后总结了我国水下重力辅助导航的发展趋势及研究的若干建议.     

Inversion of satellite gradiometry data using statistically modified integral formulas for local gravity field recovery

The satellite gravity gradiometric data can be used directly to recover the gravity anomaly at sea level using inversion of integral formulas. This approach suffers by the spatial truncation errors of the integrals, but these errors can be reduced by modifying the formulas. It allows us to consider smaller coverage of the satellite data over the region of recovery. In this study, we consider the second-order radial derivative (SORD) of disturbing potential (T_rr) and determine the gravity anomaly with a resolution of 1° × 1° at sea level by inverting the statistically modified version of SORD of extended Stokes’ formula. Also we investigate the effect of the spatial truncation error on the quality of inversion considering noise of T_rr. The numerical investigations show satisfactory results when the area of T_rr coverage is the same with that of the gravity anomaly and the integral formula is modified by the biased least-squares modification. The error of recovery will be about 6 mGal after removing the regularization bias in the presence of 1 mE noise in T_rr measured on the orbit.     

Characteristics of field line resonance type geomagnetic pulsations and variations of plasmaspheric plasma density distribution

The period of field line resonance (FLR) type geomagnetic pulsations depends on the length of the field line and on the plasma density in the inner magnetosphere (plasmasphere), where field lines are closed. Here as FLR period, the period belonging to the maximum occurrence frequency of the occurrence frequency spectrum (equivalent resonance curve) of pulsations has been considered. The resonance system may be replaced by an equivalent resonant circuit. The plasma density would correspond to the ohmic load. The plasma in the plasmasphere originates from the ionosphere, thus FLR period, occurrence frequency are also affected by the maximum electron density in the ionosphere. The FLR period has shown an enhancement with increasing F region electron density, while the occurrence frequency indicated diminishing trend (possible damping effect). Thus, the increased plasma density may be the cause of the decreased occurrence of FLR type pulsations in the winter months of solar activity maximum years (winter anomaly).     

航天器机械臂柔性力控辅助装配方法

文章从装配的实际需求出发,提出一种航天器机械臂柔性力控辅助装配方法:通过在机械臂末端法兰与负载之间安装的六维力传感器感知作用力与力矩信息,人手直接作用于机械臂末端的负载,系统通过负载的重力补偿算法获得人手作用的力与力矩信息,而后以力/力矩信息作为输入来控制机械臂进行移动或转动,使负载柔性跟随人手运动。文章给出了装配方法的详细设计方案与相关算法,并进行了初步试验验证。试验表明,该装配方法可以有效提高在航天器狭小空间内进行大重量工件安装的效率,且安全可靠。     

Pioneer 10 Doppler data analysis: Disentangling periodic and secular anomalies

This paper reports the results of an analysis of the Doppler tracking data of Pioneer probes which did show an anomalous behaviour. A software has been developed for the sake of performing a data analysis as independent as possible from that of Anderson et al. [Anderson, J., Laing, P.A., Lau, E.L., Liu, A.S., Nieto, M.M., Turyshev, S.G. Study of the anomalous acceleration of Pioneer 10 and 11. Phys. Rev. D 65, 082004, 2002], using the same data set. A first output of this new analysis is a confirmation of the existence of a secular anomaly with an amplitude about 0.8 nm s⁻² compatible with that reported by Anderson et al. A second output is the study of periodic variations of the anomaly, which we characterize as functions of the azimuthal angle φ$\phi$ defined by the directions Sun–Earth Antenna and Sun-Pioneer. An improved fit is obtained with periodic variations written as the sum of a secular acceleration and two sinusoids of the angles φ$\phi$ and 2φ$2\phi$. The tests which have been performed for assessing the robustness of these results are presented.     

微型飞机降低重心位置对稳定性的影响

由于微型飞机有最大尺寸的限制,通常平尾/升降舵距离机翼和全机重心很近,造成气动效率和纵向静稳定性都比较低。研究了不使用平尾/升降舵、而是通过降低微型飞机重心位置来获得纵向静稳定性的思路。分析了重心低置情况下的纵向力矩平衡关系,推导了相应的纵向静稳定性的计算公式,并构造了计算模型和试飞样机进行实例分析。结果表明,通过降低重心位置可以有效地增大微型飞机的纵向静稳定性,并可以在没有平尾的情况下实现纵向力矩平衡和获得静稳定性。其静稳定性裕度可以通过重心与气动中心的纵向距离来调节。     

The nighttime anomalies using Global IGS VTEC Maps

In this paper we show the VTEC variations at night, considering their geomagnetic, seasonal and solar activity dependences. The variations are analyzed in two time periods 10 p.m. (pre-midnight) and 2 a.m. (post-midnight); and for two different solar conditions; one during high solar activity (2000) and the other during low solar activity (2008). Spatial and temporal ionosphere variability is investigated from Global IGS VTEC maps applying Principal Component Analysis (PCA).