基于PCI总线的PC机再入遥测站设计

根据再入遥测的特点 ,提出基于 PCI总线和 Windows平台的 PC机再入遥测站的体系结构 ,重点对其关键技术即多通道高速数据的实时传输与存储技术进行研究     

一种差分键控改进方案的性能分析

为了在保持各种性能不变的情况下,提高DCSK中信息的传输速率,提出了改进的DCSK方案。发送端传输1片的参考信号,接着传送2bit的信息信号,然后在接收端利用两个相关器进行相关解调后,把相关器的输出整流合并,就能恢复所需的信息信号。如果有相同的混沌信号发生器和相同的带宽,以及相同的信噪比,改进的系统能提高信息的传输速率。     

航天器振动试验中的动力吸振现象

振动环境试验是考验航天器中各分机力学品质的重要试验,分机适应力学环境的能力在设计阶段必须充分考虑。目前分机的力学环境条件往往是在考虑了一定的安全系数后,以分机安装处界面的加速度包络曲线给出的。然而一般来说,分机振动试验过程中的边界条件与分机实际工作状态的边界条件是不同的。具体地说就是在振动试验过程中分机通过试验转接托架与振动台面相连,实际工作状态是分机安装在安装件(卫星各舱板)上。由于试验转接托架与安装件的动力学特性不一样,根据多自由度弹簧质量阻尼系统的动力吸振原理,可以推出试验状态分机在固有频率处存在过试验现象。为了减少过试验对分机带来的危害,新的试验方法研究(加速度响应限幅控制、阻抗特性模拟法、限力技术等)已成为国内外航天工作者研究的热点。文章详细阐述了振动试验中动力吸振的机理及过试验产生的缘由。     

雷雨天气下的雷达管制

一、广州区域雷雨天气特点及其影响 广州区域管制中心所管辖的空域处于我国华南地区，雷暴发生的频率纬度比较高的地区高得多。年平均出现雷暴日数为80．5天，年出现雷暴最多日数为115天，最少为57天。雷暴既有由天气系统引起的，也有由对流增热和地形抬升作用造成的。所以，夏季比冬季多，一年之中雷暴多集中出现在4～9月份，以8月份出现最多，为15．3天；12月份出现最少，为0天。另外，雷暴的日变化比较显著，大多出现在下午和傍晚。如：广州，日际雷暴发生的最大频率值（0800～1000UTC）比最小频率值（2300～0200UTC）大约多5倍。     

Identification and status of design improvements to the NASA Shuttle EMU for International Space Station application

To meet the significant increase in EVA demand to support assembly and operations of the International Space Station (ISS), NASA and industry have improved the current Shuttle Extravehicular Mobility Unit (EMU), or "space suit", configuration to meet the unique and specific requirements of an orbital-based system. The current Shuttle EMU was designed to be maintained and serviced on the ground between frequent Shuttle flights. ISS will require the EMUs to meet increased EVAs out of the Shuttle Orbiter and to remain on orbit for up to 180 days without need for regular return to Earth for scheduled maintenance or refurbishment. Ongoing Shuttle EMU improvements have increased reliability, operational life and performance while minimizing ground and on-orbit maintenance cost and expendable inventory. Modifications to both the anthropomorphic mobility elements of the Space Suit Assembly (SSA) as well as to the Primary Life Support System (PLSS) are identified and discussed. This paper also addresses the status of on-going Shuttle EMU improvements and summarizes the approach for increasing interoperability of the U.S. and Russian space suits to be utilized aboard the ISS.     

The Brazilian scientific microsatellite SACI-1

The National Space Research Institute (INPE) is developing the first Brazilian Scientific Microsatellite (SACI-1) based on the vanguard technology and on the experience acquired through projects developed by Brazilian Space Program. The SACI-1 is a 750km polar orbit satellite. The spacecraft will combine spin stabilization with geomagnetic control and has a total mass of 60 kg. The overall dimensions are 640×470×470 mm. The SACI-1 satellite shall be launched together with CBERS (China-Brazil Earth Resource Satellite). Its platform is being designed for multiple mission applications. The Brazilian Academy of Sciences has selected four scientific payloads that characterize the mission. The scientific experiments are: ORCAS (Solar and Anomalous Cosmic Rays Observation in the Magnetosphere), PLASMEX (Study of Plasma Bubbles), FOTSAT (Airglow Photometer), and MAGNEX (Geomagnetic Experiment).     

带充液腔的自旋卫星稳定性问题

本文应用Pfeiffer的思想讨论带轴对称充液腔的卫星系统自旋稳定性。本方法的基本思想为将轴对称腔内的液体旋度平均化,使之与空间位置无关,由此将液体的无限自由度问题离散化为有限自由度问题,从而用线性理论讨论系统的自旋稳定性。用这方法,本文讨论了带充液腔的非轴对称卫星系统、带充液腔的双自旋卫星系统的自旋稳定性,给出了它们的自旋稳定性判据。此外,本文还给出了一些带有不同形状腔体的卫星系统自旋稳定域图,为实际工程设计人员提供理论参考。     

Characteristics and formation of amino acids and hydroxy acids of the Murchison meteorite.

Eight characteristics of the unique suite of amino acids and hydroxy acids found in the Murchison meteorite can be recognized on the basis of detailed molecular and isotopic analyses. The marked structural correspondence between the alpha-amino acids and alpha-hydroxy acids and the high deuterium/hydrogen ratio argue persuasively for their formation by aqueous phase Strecker reactions in the meteorite parent body from presolar, i.e., interstellar, aldehydes, ketones, ammonia, and hydrogen cyanide. The characteristics of the meteoritic suite of amino acids and hydroxy acids are briefly enumerated and discussed with regard to their consonance with this interstellar-parent body formation hypothesis. The hypothesis has interesting implications for the organic composition of both the primitive parent body and the presolar nebula.     

Continuous tracking of cmes using MICA, andLASCO C2 and C3 coronagraphs

In this work we have tracked coronal mass ejections observed with the ground based Mirror Coronagraph for Argentina (MICA) and the Large Angle and Spectroscopic Coronagraph (LASCO) C2 and C3 on board of the Solar and Heliospheric Observatory (SOHO). The MICA telescope is located at El Leoncito (31.8 S, 69.3 W), San Juan (Argentina), since 1997 as part of a bilateral scientific project between Germany and Argentina. SOHO is a project of international cooperation between ESA and NASA. Together these instruments are able to observe the solar corona ranging from 1.05 to 32 solar radii. MICA images the Fe XIV emission line corona and LASCO coronagraphs observe the Thomson scattered white light corona. We have selected events for which there are observations from the three coronagraphs. Using the composite data we were able to obtain height-time diagrams for the corresponding dynamical coronal features traveling outwards in order to determine some of their kinematical properties, i.e., plane of sky velocity and acceleration.     

刚性方程的二阶Gear方法的注记

构造了一个求解刚性方程的二阶差分格式,它是隐式的,并采用简单迭代求解,对于稳定系统,迭代收敛性条件与步长无关,而对不稳定系统,迭代收敛性条件对步长却有所限制,利用这一限制性条件去克服解刚性方程的二阶Gear方法时出现的“危险性”。