Evolution of the orbital elements for objects with high area-to-mass ratios in geostationary transfer orbits

A new population of uncatalogued objects in geosynchronous Earth orbits (GEO), with a mean motion of about 1 rev/day and eccentricities up to 0.6, has been identified recently. The first observations of this new type of objects were acquired in the framework of the European Space Agency’s (ESA) search for space debris in GEO and the geostationary transfer orbit (GTO) using the ESA 1-m telescope on Tenerife. Earlier studies have postulated that the perturbations due to the solar radiation pressure can lead to such large eccentricities for GEO objects with a high area-to-mass ratio (A/M). The simulations showed that the eccentricities of GEO objects with large A/M exhibit periodic variations with periods of about one year and amplitudes depending on the value of A/M. The findings of these studies could be confirmed by observations from the ESA 1-m telescope on Tenerife.     

Dynamical evolution of high area-to-mass ratio debris released into GPS orbits

A large set of simulations, including all the relevant perturbations, was carried out to investigate the long-term dynamical evolution of fictitious high area-to-mass ratio (A/M) objects released, with a negligible velocity variation, in each of the six orbital planes used by Global Positioning System (GPS) satellites. As with similar objects discovered in near synchronous trajectories, long lifetime orbits, with mean motions of about 2 revolutions per day, were found possible for debris characterized by extremely high area-to-mass ratios. Often the lifetime exceeds 100 years up to A/M ∼ 45 m²/kg, decreasing rapidly to a few months above such a threshold. However, the details of the evolution, which are conditioned by the complex interplay of solar radiation pressure and geopotential plus luni-solar resonances, depend on the initial conditions. Different behaviors are thus possible. In any case, objects like those discovered in synchronous orbits, with A/M as high as 20–40 m²/kg, could also survive in this orbital regime, with semi-major axes close to the semi-synchronous values, with maximum eccentricities between 0.3 and 0.7, and with significant orbit pole precessions (faster and wider for increasing values of A/M), leading to inclinations between 30° and more than 90°.     

Cosmic ray studies at Moussala – Past,present and future

We review the main activities carried out at Moussala peak (2925 m above sea level, 42°11′N, 23°35′E) station in Bulgaria, connected with cosmic ray investigations during the last five decades. Several important results obtained at the station are reported. The detector design and corresponding methodological studies of the presently operational devices are shown as well, precisely the Cherenkov light telescope, lead free neutron monitor and muon telescope. The scientific potential of the existing complex is discussed.     

卫星大型挠性天线弹性振动抑制的研究

论文从工程实践角度探讨了具有大尺寸（直径几米～几十米）和高精度（０．０５°）的挠性天线指向控制问题。在借鉴和改进有关抑制挠性天线弹性振动研究的基础上，初步设计了星—地回路的挠性天线指向控制方案。最后，通过分析数值仿真结果，给出了提高挠性天线指向精度的主要因素。     

Investigation of natural and artificial stimulation of the ionospheric Alfvén resonator at high latitude

A brief review is provided of recent progress in understanding the ionospheric Alfvén resonator (IAR) at high latitude. Firstly, naturally occurring resonances of the IAR as detected by pulsation magnetometers in the auroral zone at Sodankylä and in the polar cap at Barentsburg are considered. The characteristics of the IAR in the two regions are broadly similar, although the effects of solar illumination are less clear at the higher latitudes. Secondly we review recent attempts to stimulate the IAR through high-power radio frequency experiments both in the auroral zone at Tromsø with the European Incoherent SCATter (EISCAT) heater, and within the polar cap at Longyearbyen with the Space Plasma Exploration by Active Radar (SPEAR) facility. In the auroral zone at, Tromsø the stimulated IAR has been observed by ground-based magnetometers, and through electron acceleration observed on the FAST spacecraft. At SPEAR in the polar cap, the stimulated IAR has been investigated, with ground magnetometers, with the first results indicative of a positive detection.     

基于火箭橇的北斗动态定位精度鉴定方法

介绍了几种现有的以GPS/北斗为主要代表的卫星导航系统的动态定位精度 鉴定方法,分析了这几种方法在模拟实际使用环境、鉴定精度等方面的优缺点,提出了 一种基于火箭橇试验平台的北斗导航定位系统动态定位精度鉴定方法。该方法能够很好 地模拟北斗导航定位系统实际工作环境（速度、加速度、振动和天线角度等）,解决高 动态、高精度北斗导航定位系统动态定位精度鉴定问题,并对该方法的原理和实施方法 作了详细的论述,最后分析了该方法的不确定度及误差,并提出了改进措施。     

锚固站数量及布局对导航星座自主定轨影响分析

针对导航星座自主定轨中的星座整体旋转问题,采用增设少量地面锚固站的方法可有效解决该问题。通过推导星地距离对卫星轨道升交点赤经的偏导数,证明了星地距离对卫星轨道升交点赤经可观。仅考虑在我国大陆范围内布设锚固站的条件下,仿真分析了锚固站数量以及布局对导航星座自主定轨精度的影响。仿真实验结果表明:采用3个以上的锚固站,即可有效控制星座整体旋转,在14d的仿真时段内卫星自主定轨精度保持4m以内;锚固站数量越多,自主定轨精度越高,但随着锚固站数量的增加,自主定轨精度改善程度越来越小;在保持4个锚固站的情形下,采用不同的锚固站布局方案,自主定轨精度并无明显差别。     

如何实现学生从中学物理到大学物理学习的转变

实现学生从中学物理学习到大学物理学习转变的关键是借助高等数学所揭示的数学方法的思想内涵 ,建立起从中学物理的不变到大学物理中变、从宏观到微观、从近似到精确这样一种贯穿于物理学始终的辩证唯物主义物理观。     

某型导弹翼轴花键齿首齿机加工精度研究

就如何保证新一代导弹重要零件翼轴花键齿首齿位置精度达到±１０’的机加工技术作了详细的阐述，着重就花键齿插齿过程中的工装定位、首齿位置精度的提高和测量方法进行了较为认真的研究。实践证明，该种插齿工艺方法能保证翼轴零件首齿位置精度的互换性，在具有类似的首齿位置精度要求的齿轮加工行业中有一定的先进性，并具有借鉴和推广价值。     

高值电阻国际比对的方法研究

介绍了参加亚太实验室认可合作组织(APLAC)开展的高阻1 MΩ;10 MΩ实验间比对的方法,对一种用参考电压测量高阻的方法进行了描述,解决了其中的技术问题,对测量不确定度进行了分析,其结果为测量1MΩ的合成标准不确定度为3.10-6,测量10 MΩ的合成标准不确定度为5.10-6,APLAC公布的比对中期报告证明了该方法的可靠性。