空间赛博战研究

赛博作为信息网络时代的产物,正在受到关注和重视。在阐述赛博空间和赛博战新概念的基础上,分析赛博空间和赛博战的特点。介绍了空间赛博战的概念和内涵,重点分析空间赛博战在暴露性、开放性、脆弱性和制约性等方面的特点,并对空间赛博战任务功能进行了分类描述,最后梳理空间赛博战的关键技术。     

Thrust modulation of solid propellant rockets by a fluidic vortex valve with secondary combustion

An analytical model for calculation of the thrust and pressure modulation of a solid propellant rocket by means of a fluidic vortex valve with secondary combustion has been developed. Thrust control by the vortex valve method was found superior to the axial injection of control flow. Addition of oxygen in the injected flow improves the energetic performance of the system as well as the thrust modulation capability. Experiments have been conducted using a mixture of nitrogen and oxygen as the injection gas. The two main parameters investigated in a series of experiments were the oxygen percentage in the injection gas and the ratio between the mass flow rates of the control gas and the solid propellant combustion products. The results show an increase of thrust by a factor of 2 for a 25% addition in mass flow rate by secondary injection at optimal conditions.     

上游转子对下游静子叶片气动力的影响

为研究轴流压气机下游静子叶片非定常气动力的大小和频率的变化规律,采用在静子叶片表面埋设微型动态压力传感器的方法,在低速单级轴流压气机实验器上进行了静子叶片表面压力的测量。测量了不同轴向间距、不同转速下从近堵塞到近失速的宽广流量范围,并对所测得的静子叶片非定常气动力进行了离散傅立叶变换,以分析其频谱特性。实验结果表明：在转子尾迹的影响下,静子叶片表面的波动频率是转子的尾迹频率及其倍频。转子尾迹频率的高频分量对静子叶片吸力面前缘的影响比对其他位置的影响大。叶片表面的非定常压力和气动力随压气机流量、转速和轴向间距的变化而变化。     

The Magnetic Electron Ion Spectrometer (MagEIS) Instruments Aboard the Radiation Belt Storm Probes (RBSP) Spacecraft

This paper describes the Magnetic Electron Ion Spectrometer (MagEIS) instruments aboard the RBSP spacecraft from an instrumentation and engineering point of view. There are four magnetic spectrometers aboard each of the two spacecraft, one low-energy unit (20–240 keV), two medium-energy units (80–1200 keV), and a high-energy unit (800–4800 keV). The high unit also contains a proton telescope (55 keV–20 MeV). The magnetic spectrometers focus electrons within a selected energy pass band upon a focal plane of several silicon detectors where pulse-height analysis is used to determine if the energy of the incident electron is appropriate for the electron momentum selected by the magnet. Thus each event is a two-parameter analysis, an approach leading to a greatly reduced background. The physics of these instruments are described in detail followed by the engineering implementation. The data outputs are described, and examples of the calibration results and early flight data presented.     

利用气动式溜车—管路系统实现散状物料的输送

气动式溜车－管路系统是近年来兴起的一种高效的中,长距,离输送装置,它克服了常规运输系统运费高,噪声大和污染环境的缺点,在工程上有着良好的应用前景。本文对该系统的原理和原理和结构进行了较为细致的分析,并介绍了一个应用实例。     

The 2002 Space Cooperation Protocol between China and Brazil: An excellent example of South–South cooperation

China and Brazil have been cooperating in space since 1986 and, after 15 years of successful joint creative work, the two sides agreed a 2002 Protocol, providing a more concrete framework for further cooperation in space projects. This bilateral agreement was heralded as an authentic bilateral effort amplifying the so-called South–South relationship. A close examination of the Protocol has revealed that the document, while responding to the UN Declaration on International Cooperation, has made a significant contribution and set a good example for space cooperation among developing countries. Placed against the background of ongoing space commercialization, the success of this model can test the viability of existing space commercial rules and help introduce further improvements.     

Scientific Planning and Commanding of the Rosetta Payload

ESA’s Rosetta mission was launched in March 2004 and is on its way to comet 67P/Churyumov-Gerasimenko, where it is scheduled to arrive in summer 2014. It comprises a payload of 12 scientific instruments and a Lander. All instruments are provided by Principal Investigators, which are responsible for their operations. As for most ESA science missions, the ground segment of the mission consists of a Mission Operations Centre (MOC) and a Science Operations Centre (SOC). While the MOC is responsible for all spacecraft-related aspects and the final uplink of all command timelines to the spacecraft, the scientific operations of the instruments and the collection of the data and ingestion into the Planetary Science Archive are coordinated by the SOC. This paper focuses on the tasks of the SOC and in particular on the methodology and constraints to convert the scientific goals of the Rosetta mission to operational timelines.     

High-Resolution, Radar Coherent Linear FM Microwave Source

The microwave CLFM study was directed to generating 14 ?s S-band pulses of 1000 MHz bandwidth and an rms phase error of a few degrees. Over 972 MHz bandwidth, the sampled phase error relative to the reference was 7 degrees rms and 17 degrees peak, with a maximum Fourier component of 4 degrees. The FM pulse train is generated by a gated BWO driven by a stable linearizing waveform. Phase coherency during each pulse is obtained by a sampling technique, where the phase is corrected at intervals of 1/6 ?s, the RF phase having changed an integral number of cycles in each interval. Multiplication of the BWO signal by the sampling pulse train results in band-limited phase error pulses which are applied in a feedback loop. Pulse-to-pulse coherency is obtained by phase lock of the BWO starting frequency to the crystal reference. Feedback leveling holds the output constant to 0.3 dB. The basic MITRE technique was originally demonstrated at 10 MHz in 1964. Range results measured with the X-band model radar using the CLFM generator are given and confirm the phase errors of the CLFM.     

Is the Sun a Sun-Like Star?

Various observable properties of the Sun are compared with those of solar-type stars. It is concluded that the Sun, to a remarkable degree, is “solar-type”. As regards its particular mass and age, and probably its non-binarity, “anthropic” explanations may seem in place. The possible tendency for the Sun, as compared with similar stars, to be somewhat rich in iron relative to other elements needs further exploration. This is also true concerning its presently small micro-variability amplitude. This revised version was published online in June 2006 with corrections to the Cover Date.