Influence of Fast Global Variations of Solar Magnetic Fields on Space Weather in Cycle 23

It is established that the large-scale and global magnetic fields in the Sun's atmosphere do not change smoothly, and long-lasting periods of gradual variations are superseded by fast structural changes of the global magnetic field. Periods of fast global changes on the Sun are accompanied by anomalous manifestations in the interplanetary space and in the geomagnetic field. There is a regular recurrence of these periods in each cycle of solar activity, and the periods are characterized by enhanced flaring activity that reflects fast changes in magnetic structures. Is demonstrated, that the fast changes have essential influencing on a condition of space weather, as most strong geophysical disturbances are connected to sporadic phenomena on the Sun. An explanation has been offered for the origin of anomalous geomagnetic disturbances that are unidentifiable in traditionally used solar activity indices. Is shown, main physical mechanism that leads to fast variations of the magnetic fields in the Sun's atmosphere is the reconnection process.     

用于低轨卫星精密轨道确定的简化动力学法

全球定位系统(GPS)的测量量可促成一种简化动力学法,用于近地卫星的近厘米级定轨。利用这种方法,不同观测时刻的卫星状态问的转移由正规的动力学模型和由连续GPS载波相位数据以运动学法导出的卫星位置变化来完成。动力学信息和运动学信息间的相对权重可自由变化。协方差分析表明:当观测几何差而动力学模型好时,模型支配着状态转移的计算;动力模型差而观测几何好时,载波相位统治着状态转移的计算;而当运动学和动力学信息间没有明显优劣时,简化动力学联合法可显著提高轨道精度。本文给出简化动力学法中准最佳的择权准则,并研究了求解精度对权的敏感性。     

使用连续流动法测量高氯酸铵表面积

1、引言为了予测复合固体推进剂的弹道性能,必须要知道推进剂中各组份的粒度或表面积。在塑料型推进剂的制造过程中固体粒子会发生机械破碎,尽管如此,仍发现高氯酸铵的初始表面积与推进剂的弹道性能有关。爆炸物研制公司(ERDE)测量高氯酸铵表面积的作法是采用以空气渗透法为基础的菲希尔(Fisher)筛分机。由于塑料型推进剂中使用的高氯酸铵的比表面积范围通常为1000～9000cm~2/cm~3(0.051～0.46m~2/g),因此,菲希尔法完全能满足这一要求。为了生产较高燃速的推进剂,爆炸物研制公司最近研究的推进剂配方中含有更细的高氯酸铵(9000～10000cm~2/cm~3)。在端羧基聚丁二烯和端羟基聚丁二烯两种橡胶型推进剂中,即     

Analysis of a crossed Bragg cell acousto-optical spectrometer for SETI

The search for radio signals from extraterrestrial intelligent beings (SETI) requires the use of large instantaneous bandwidth (500 MHz) and high resolution (20 Hz) spectrometers. Digital systems with a high degree of modularity can be used to provide this capability, and this method has been widely discussed. Another technique for meeting the SETI requirement is to use a crossed Bragg cell spectrometer as described by Psaltis and Casasent. This technique makes use of the Folded Spectrum concept, introduced by Thomas. The Folded Spectrum is a 2-D Fourier Transform of a raster scanned 1-D signal. It is directly related to the long 1-D spectrum of the original signal and is ideally suited for optical signal processing. The folded spectrum technique has received little attention to date, primarily because early systems made use of photographic film which are unsuitable for the real time data analysis and voluminous data requirements of SETI. An analysis of the crossed Bragg cell spectrometer is presented as a method to achieve the spectral processing requirements for SETI. Systematic noise contributions unique to the Bragg cell system will be discussed.     

The SERENDIP piggyback SETI project

The SERENDIP project is an ongoing program of monitoring and processing broadband radio signals acquired by existing radio astronomy observatories. SERENDIP operates in a piggyback mode: it makes use of whatever observing plan (sequence of frequencies, sky coordinates, and polarizations) is under way at its host observatory. Moreover, the SERENDIP data acquisition system, once installed, operates autonomously. This approach makes it possible to obtain large amounts of high quality observing time in a manner that is economical and that does not adversely affect ongoing radio astronomy survey work. The SERENDIP II system has been installed at the NRAO 300-foot telescope at Green Bank, West Virginia, and has operated there for several thousand hours. In this report, we summarize our findings from these observations and describe the present status of the project. Two key elements of SERENDIP are the automated data acquisition system that uses adaptive thresholds and logs only statistically significant peaks in the real-time power spectra, and the subsequent off-line analysis programs that identify and reject a variety of interference signals. Several specific correlations have been identified that offer promise. At present, the development and testing of these interference rejection algorithms is the main thrust of our work.     

含硝酸酯增塑剂的固体推进剂的脆化研究

本文介绍硝酸酯增塑的聚醚聚氨酯推进剂在低温贮存中,解决失去应变能力(脆化)问题的研究结果。这种高度增塑的推进剂在低温下短期贮存,几乎完全失去了应变能力。研究这种脆化的原因表明,交联密度以及粘合剂配方是起作用的因素。湿度曾被考虑是因素之一,但实验证明并非如此。实验表明增塑剂结晶是脆变的主要原因但不一定与增塑剂的凝固点有关。重新测定某些增塑剂的凝固点是研究工作的一部份。放入增塑剂晶体增加了推进剂脆变速度。单独采用丁三醇三硝酸酯(BTTN)或是混合增塑剂可以解决这个问题。采用混合增塑剂可以得到最好的低温性能。     

机载雷达系统中的空—时自适应处理

本文概述了空—时自适应处理(STAP)在现代雷达系统中，尤其是在强干涉和人为干扰下的机载雷达系统中的应用情况。简要介绍处理方法后，叙述了STAP在导致非平稳信号环境的热杂波和非均匀雷达环境中STAP的应用结果。分析了在这种实际情况下采用STAP处理所存在的局限。结尾部分为使用圆形阵列所得到的一些STAP近期结果。     

Humans to Mars: a feasibility and cost-benefit analysis

Mars is a compelling astrobiological target, and a human mission would provide an opportunity to collect immense amounts of scientific data. Exploration alone, however, cannot justify the increased risk. Instead, three factors drive a human mission: economics, education, and exploration. A human mission has a unique potential to inspire the next generation of young people to enter critically needed science and engineering disciplines. A mission is economically feasible, and the research and development program put in place for a human mission would propel growth in related high-technology industries. The main hurdles are human physiological responses to 1–2 years of radiation and microgravity exposure. However, enabling technologies are sufficiently mature in these areas that they can be developed within a few decade timescale. Hence, the decision of whether or not to undertake a human mission to Mars is a political decision, and thus, educational and economic benefits are the crucial factors.     

Canada and the International Space Station program: overview and status

The twelve months since IAF 2000 have been perhaps the most exciting, challenging and rewarding months for Canada since the beginning of our participation in the International Space Station program in 1984. The highlight was the successful launch, on-orbit check out, and the first operational use of Canadarm2, the Space Station Remote Manipulator System, between April and July 2001. The anomalies encountered and the solutions found to achieve this success are described in the paper. The paper describes, also, the substantial progress that has been made, during the twelve months since IAF 2000, by Canada as it continues to complete work on all flight-elements of its contribution to the International Space Station and as we transition into real-time Space Station operations support and Canadian utilization. Canada's contribution to the International Space Station is the Mobile Servicing System (MSS), the external robotic system that is key to the successful assembly of the Space Station, the maintenance of its external systems, astronaut EVA support, and the servicing of external science payloads. The MSS ground segment that supports MSS operations, training, sustaining engineering, and logistics activities is reaching maturity. The MSS Engineering Support Center and the MSS Sustaining Engineering Facility are providing real-time support for on-orbit operations, and a Canadian Payloads Telescience Operations Center is now in place. Mission Controllers, astronauts and cosmonauts from all Space Station Partners continue to receive training at the Canadian Space Agency. The Remote Multi Purpose Room, one element of the MSS Operations Complex, will be ready to assume backroom support in 2002. Canada has completed work on identifying its Space Station utilization activities for the period 2000 through 2004. Also during the past twelve months the CSA drafted and is proceeding with the approval of a Canadian Space Station Commercialization Policy. Canadian astronauts have now participated in three ISS assembly missions--Julie Payette on STS-96, Marc Garneau on STS-97, and Chris Hadfield on STS-100 in April 2001 during which he performed Canada's first EVA and the successful installation of the Space Station Remote Manipulator System.     

Voluntary head stabilization in space during trunk movements in weightlessness

The ability to voluntarily stabilize the head in space during lateral rhythmic oscillations of the trunk has been investigated during parabolic flights. Five healthy young subjects, who gave informed consent, were examined. The movements were performed with eyes open or eyes closed, either during phases of microgravity or phases of normal gravity. The main result to emerge from this study is that the head may be stabilized in space about the roll axis under microgravity conditions with, as well as without vision, despite the reduction of the vestibular afferent and the muscle proprioceptive inputs. Moreover, the absence of head stabilization about the yaw axis confirms that the degrees of freedom of the neck can be independently controlled, as it was previously shown [1]. These results seem to indicate that voluntary head stabilization does not depend crucially upon static vestibular afferents. Head stabilization in space may be in fact organized on the basis of either dynamic vestibular afferents or a postural body scheme.