Field formation around negatively biased solar arrays in the LEO-plasma

Heavy emission caused by impacting plasma ions results in a fast discharging effect of the initially large surface potentials on the dielectric solar cells. This eventually counteracts the energization process of the plasma ions to the cover glasses and leaves no significant electric fields. Thus, with an existing thermal plasma, electrons are again able to reach dielectric surfaces. Strong localized electric fields of the order of several 10 kV/cm form near the interconnector-cover glass interface.     

EUV emission from normal galaxies

Using data from the Wide Field Camera EUV all-sky survey, we have established upper limits to the EUV flux from a sample of 30 bright, nearby, non-active spiral galaxies. These galaxies were chosen to be those most likely to be detected in the EUV on the basis of (i) low interstellar absorption within our own galaxy, (ii) brightness in other wavebands, (iii) high star formation activity, and (iv) proximity. The derived EUV upper limits are restrictive, and establish for the first time that the EUV flux escaping from galaxies does not constitute a major component of their bolometric luminosity, and in particular that it cannot be the sink for the energy injected into the interstellar medium by supernova explosions, as had been suggested following the failure to detect this power in the X-ray band.     

A bistatic SAR mission for earth observation based on a small satellite

The authors present a new scientific space mission consisting of a satellite carrying a receiving- only SAR which receives the signal transmitted by the ENVISAT-1 SAR. The integration of ENVISAT-1 SAR and bistatic radar data offers an improved potentiality of surface classification, three-dimensional observation, and the opportunity of advanced scientific experiments in the field of bistatic scattering. The small satellite nominal orbit and the attitude manoeuvres are designed in order to maintain an adequate overlap between the two radar swaths along the whole orbit, taking into account the ENVISAT-1 attitude and pointing. A preliminary satellite design (2-year lifetime) is then performed to evaluate the orbit decay and to determine the appropriate orbit manoeuvres (every 4 days) to control the satellites relative phase. The numerical simulation shows that a spacecraft of about 584kg is able to meet the mission requirements.     

GPS based onboard and onground orbit operations for small satellites

In extension to common applications such as groundtrack displays and antenna steering, the SGP4 orbit model is proposed for operational orbit determination in small satellite missions. SGP4 is an analytical orbit model for Low-Earth orbiting satellites that is widely used for the propagation of NORAD twoline elements. Twoline elements may hence be generated completely independent of NORAD. Their use as exclusive source of orbital information simplifies the operations concept and reduces mission costs through the extensive use of existing low-cost mission support software. Due to small computer resource requirements of 8–10kByte, the SGP4 model may also be applied for onboard orbit computations making use of e.g. a 80186 processor, thus ensuring full compatibility of ground-based and onboard operations. The proposed approach is particularly suited in combination with a space-borne GPS receiver, were the C/A-code navigation solutions are treated as measurements that are adjusted in a least-squares sense using the SGP4 model. As consequence, inherent drawbacks of the pure navigation solutions such as data gaps and scatter as well as limited velocity accuracy are avoided, while the operational navigation activities are kept at a minimum. The feasibility of the concept is illustrated based on real GPS navigation data from the TOPEX/Poseidon and the MIR space station with an inherent data quality of 50–100 m. It is shown that 3 hours of data within a 4 day period are sufficient to keep the position error within 4 km, that is considered sufficient for most applications.     

k-ε-g紊流燃烧模型数值研究

本文对k-ε-g紊流燃烧模型中模型系数C_R,C_(g1),C_(g2)的选定和计算浓度脉动均方值g的不同方法进行数值研究。计算结果表明模型系数值的选定直接与化学反应速率有关,而其中C_R影响最大。g的计算虽然可有不同方法,而其中微分方程求解最佳。并用实验数据来验证计算结果。     

门限自回归模型参数的局部正交设计寻优法

在采用点值图确定门限区间个数的基础上，对门自回归模型中门限值、滞后步长、各门限区间模型阶数，利用正交设计方法寻优，计算工作量锐减，却可得到精度较高的预报模型。     

试论高校职业指导工作的开展与推动

高校职业指导工作是一项复杂的系统工程,这项工作的开展与推动,是贯彻落实党和国家的就业方针、政策的需要,事关毕业生的职业前途与人生目标的实现,对高校教育事业的可持续发展,具有明显的现实意义和重要的战略意义,需要采取切实有效的策略。     

培养学生英语口语交际能力的策略探讨

文章就大学生英语口语交际能力存在的问题进行了分析,探讨如何提高英语口语交际能力的策略。     

弹道导弹中段机动突防研究

针对弹道导弹中段机动突防问题，在瞬时冲量假设下从理论上研究了速度增量大小、方向和机动时刻对零控脱靶量和落点偏差的影响。研究表明：速度增量大小和机动时刻给定时，零控脱靶量随速度增量方向不同存在极小值和极大值，速度增量方向垂直于视线方向时零控脱靶量接近最大，且最大值近似为待飞时间和速度增量大小的乘积；速度增量大小和机动时刻给定时，落点偏差随速度增量方向的不同存在极小值和极大值，极值点对应的速度增量方向可通过解析方法求解，落点偏差极大值与速度增量大小成正比，且机动时刻越晚，落点偏差极大值越小。该研究可为突防方案设计提供理论基础。     

抗辐照PROM 6617在单片机中的具体应用

美国HARRIS公司的程序存储器PROM 6617由于其芯片管脚及功能与EPROM2716完全兼容且又具有耐辐照性能而日渐被航天设计人员所认识和应用。但其内部结构又与2716有所不同,若忽视这一点,只因管脚和功能完全兼容而用2716的典型应用电路设计6617的话,6617肯定无法正常工作。文章详细分析了6617的结构特点及其与2716的区别,并给出了其在80C31单片机中的具体应用电路及其与2716兼容使用的电路。