一种热电势的简易表达法

当具有不同温度分布的多种导体连接在一个环路中时,按照帕尔贴电势和汤姆逊电势分析环路中的总的热电势是困难的。选择一些导体作为标准电极,就能把总的热电势分成一系列单一导体的独立热电势,用这个方法,分析工作将变得十分简单。     

感应加热中功率延伸电缆结构形式的优选设计

在某些特殊工艺的感应加热中,感应线圈需要通过延伸电缆与电源连接.为了解决延伸电缆带来的功率损耗高的问题,分析了并行实芯导体结构、同轴空心导体结构和多束细漆包线密布结构等3种结构形式的电缆的功率损耗和回路电感储能的情况,并进行了试验测定与分析,结果表明,多束细漆包线密布结构电缆上的功率损耗最小,同轴空心导体结构电缆回路的电感量最小.据此,提出了以同轴空心导体结构为基本结构,内、外导体为多束细漆包线密布而成的延伸电缆结构形式.     

二驱动球形机器人的全方位运动特性分析

介绍一种新型二驱动球形机器人,它使用两个电机作为输入,而球形机器人在平面运动具有三个自由度,所以属于非完整欠驱动系统.内驱动机构通过改变配重重心的位置实现了球形机器人沿任意方向的运动,且球形机器人的位姿影响了球形机器人沿不同方向运动的灵活性.阐述了它的结构特点,利用非完整系统力学理论对球形机器人运动学、动力学进行了初步分析.采用欧拉角和三维转动群知识对球形机器人的全方位运动学特性进行了分析.     

锥形同轴线阻抗渐变对S参数的影响研究CSCD

为了使通用仪器设备的输出阻抗与锥形同轴线的特性阻抗匹配,减少回波反射,设计了锥形同轴线阻抗匹配。分别比较了阻抗指数渐变,三角形渐变和klopfenstein渐变等三种渐变线方式下的阻抗匹配部分的S参数仿真结果,为实现阻抗渐变,分别比较了变内导体曲面和变外导体曲面两种方式,结果表明采用变内导体曲面使得阻抗指数渐变时,具有较好的驻波特性,频率10GHz以下驻波小于1.2,20GHz以下驻波小于2.5。     

磁层顶对磁层磁场的影响

太阳风与地磁场相互作用形成的磁层顶对磁层内磁场有重要影响。本文假定地磁场为偶极子,太阳风为理想导体,在太阳风与磁层的边界上满足磁场法向分量为零的边界条件。采用最小二乘法求得磁层顶电流在磁层内产生的磁场的球谐系数。从计算结果可以看出磁层顶对磁层磁场的影响。结果表明,向阳面的磁场、中性点、极光区的位置与形状与实际观测比较接近;磁尾磁场与实际观测相差较远,原因是没有加上磁尾片电流。文中还给出了太阳风与地磁轴交不同角度时的磁层磁场的计算结果。      

土里生出的球形闪电

谜一样的球形闪电一直是科幻小说的主角，也是众多UFO爱好者重点关注的对象。然而，由于稍纵即逝、神出鬼没，几个世纪以来，球形闪电一直都只有传说而难见真容。科学界甚至认为球形闪电是子虚乌有的现象，直到几十年前才承认它的存在。我们关于球形闪电的认识也大部分局限于一些偶然的、肉眼观测的报告。     

旋转形导体上任意取向线天线辐射场的探讨

对任意旋转平滑形导体上任意取向的线天线所辐射的扬进行探讨。采用了矩量法和傅里叶分析法,给出了导体感应电流谐量表示式,由此可求辐射场。进而以球体上任意取向赫芝振子为例求出辐射场,并与经典法公式计算结果比较,两者一致。     

一种快速测试线缆终端共模阻抗的方法

航空电子设备之间的互联线缆是电磁干扰耦合的重要路径。对线缆耦合进行建模分析时,线缆终端共模阻抗是至关重要的输入参数。而航电系统线缆数量较多,提高线缆终端共模阻抗的测试效率,有利于快速建立线缆耦合模型。为此,提出了一种快速测试线缆终端共模阻抗的方法。首先,根据多导体传输线理论证明,在分析共模电流时可以将多芯线缆等效为一根单导体。进而,将线缆束等效为多导体传输线,并采用矢量网络分析仪和电流探头测量各条线缆2个任选位置处的电压反射系数。然后,基于所建立的多导体传输线模型,构造以终端阻抗为未知数的方程组。最后,采用数值迭代算法求解该方程组,得到各条线缆的终端共模阻抗。与现有方法相比,所提方法提高了测试效率和测试精度。      

利用孤立导体建立等离子体探测载荷参考电位方法

研究讨论了一种利用孤立导体在空间等离子体环境中建立探测器参考电位的技术.将一个金属导体与航天器进行电隔离,利用电路将孤立导体电位引入探测器电源模块,为探测器建立参考电位.该技术可安全方便地应用于卫星等航天器,使探测器的地电位与空间等离子体电位基本一致,避免航天器本体电位对探测器的影响.该技术将应用于中国空间站等离子体原位探测器,通过测试验证了该技术方法可以建立-210～+210V的参考电位,满足空间站等离子体原位探测器-200～+200V的参考电位技术需求.      

Monitoring of environmental UV radiation by biological dosimeters.

As a consequence of the stratospheric ozone layer depletion biological systems can be damaged due to increased UV-B radiation. The aim of biological dosimetry is to establish a quantitative basis for the risk assessment of the biosphere. DNA is the most important target molecule of biological systems having special sensitivity against short wavelength components of the environmental radiation. Biological dosimeters are usually simple organisms, or components of them, modeling the cellular DNA. Phage T7 and polycrystalline uracil biological dosimeters have been developed and used in our laboratory for monitoring the environmental radiation in different radiation conditions (from the polar to equatorial regions). Comparisons with Robertson-Berger (RB) meter data, as well as with model calculation data weighted by the corresponding spectral sensitivities of the dosimeters are presented. Suggestion is given how to determine the trend of the increase in the biological risk due to ozone depletion.     

Improved environment radiation models

The two components of the space radiation environment, galactic cosmic rays and solar energetic particles, are of special importance for the planning of space missions and designing space vehicles for flights in the inner heliosphere. There is a constant need for developing and updating the models for calculating the fluxes of these particles for purposes of forecasting radiation conditions anticipated for future flights, including missions to the Moon and Mars.     

商用器件的空间应用需求、现状及发展前景

随着微电子技术的飞速发展及空间任务对高性能需求的日益增强,现有的宇航级抗辐射器件和技术已经远远不能满足目前空间飞行器高性能系统的需求,使得高性能商用器件Commercial-Off-The-Shelf(COTS)在空间的应用成为可能．本文就空间任务对商用器件的需求进行了综述,阐述了空间飞行器使用商用器件存在的问题及面临的风险,介绍了国内外空间任务中商用器件应用的现状,以及我国在这一领域的差距,并对商用器件在空间应用中的发展前景进行了展望．     

Radiation protection problems for the space station and approaches to their mitigation.

With the advent of a permanent manned space station the longstanding problems of radiation protection in manned spaceflight have acquired an immediacy. This paper endeavors to emphasize the gaps of our knowledge which must be closed for effective radiation protection. The information that is required includes the accurate determination of the exposure inside the space station to the various components of tile ionizing radiation, the evaluation of the biological importance of the different radiation qualities and the depth dose distribution of the less penetrating component. There is also the possibility of an interaction with weightlessness. It is necessary to establish adequate radiation protection standards and a system of dosimetric surveillance. There is a need for studies of possible methods of hardening selective shielding of the space station. Spaceflight experiments, which might contribute to the solution of some of these problems are discussed.     

Estimates of HZE particle contributions to SPE radiation exposures on interplanetary missions.

Estimates of radiation doses resulting from possible HZE (high energy heavy ion) components of solar particle events (SPEs) are presented for crews of manned interplanetary missions. The calculations assume a model spectrum obtained by folding measured solar flare HZE particle abundances with the measured energy spectra of SPE alpha particles. These hypothetical spectra are then transported through aluminum spacecraft shielding. The results, presented as estimates of absorbed dose and dose equivalent, indicate that HZE components by themselves are not a major concern for crew protection but should be included in any overall risk assessment. The predictions are found to be sensitive to the assumed spectral hardness parameters.     

Advanced biostack: experiment 1 ES 027 on Spacelab-1.

The radiobiological properties of the heavy ions of cosmic radiation were investigated on Spacelab 1 by use of biostacks, monolayers of biological test organisms sandwiched between thin foils of different types of nuclear track detectors. Biostacks were exposed to cosmic radiation at several locations with different shielding environments in the module and on the pallet. Evaluations of the physical and biological components of the experiment to date indicate that in general they survived the spaceflight in good condition. Dosimetric data are presented for the different shielding environments.     

Computation of radiation environment during ground level enhancements 65, 69 and 70 at equatorial region and flight altitudes

The radiation environment in the troposphere of the Earth is governed by cosmic rays of galactic and solar origin. During major solar energetic particles events the radiation environment changes dramatically. As a results the risk of biological effects due to exposure to ionizing radiation of aircrew increases. Here we present a numerical model for computation of absorbed dose in air due to cosmic rays of galactic and solar origin. It is applied for computation of radiation environment at flight altitude in the equatorial region during several major ground level enhancements, namely GLE65 on 28 October 2003, GLE69 on 20 January 2005 and GLE70 on 13 December 2006. The model is based on a full Monte Carlo simulation of cosmic ray induced atmospheric cascade. The cascade simulation is carried out with CORSIKA 6.990 code with corresponding hadron generators FLUKA 2011 and QGSJET II. The contribution of different cascade components, namely electromagnetic, hadron and muon is explicitly obtained. The spectra of arriving solar energetic particles are calculated from ground level measurements with neutron monitors and satellite data from GOES. The obtained results are discussed.     

Radiation measurements inside a human phantom aboard the International Space Station using Liulin-5 charged particle telescope

Liulin-5 is a particle telescope developed for the investigation of the radiation environment within the Russian spherical tissue-equivalent phantom on the International Space Station (ISS). Liulin-5 experiment is conducted aboard the Russian segment of ISS since 28 June 2007 as an adherent part of the international project MATROSHKA-R. The main objective of Liulin-5 experiment is to study the depth-dose distribution of the different components of the orbital radiation field in a human phantom. Additional objectives are mapping of the radiation environment in the phantom and its variations with time and orbital parameters (such as solar cycle, solar flare events, inclination and altitude). Liulin-5 is an active instrument, capable to provide real-time radiation data for the particle flux and dose rates, energy deposition and LET spectra. Data are recorded automatically on memory cards, periodically transported to ground by returning vehicles. In this report we present some first results from data analysis including energy deposition spectra, absorbed dose, dose rate and flux distribution measured simultaneously at 3 different depths of phantom’s radial channel and linear energy transfer (LET) spectrum. Data discussed are for the period July 2007–April 2008.     

Stability of nucleic acid under the effect of UV radiation.

Nucleic acids (combined with protein molecules) are essential constituents of the living systems playing an important role in the early evolution of life as well. A specific feature of these molecules has been found and directly confirmed recently: under the influence of short-wavelength UV radiation bipyrimidine photoproducts (cyclobutane dimers and 6-4 bipyrimidines) are induced and the reversion of them can be provoked by the same photons. However, reversion is preferred by the shorter wavelengths. With increasing ratio of the longer wavelength components of the radiation (using artificial UV sources and solar light on the Earth's surface) the impact of the reversible photoproducts in the harmful biological effect decreases and other photoproducts are dominant. Assuming the photoinduced reactions (dimerisation and reversion) are statistical events, during the irradiation the chance for a number of nucleoprotein molecules to survive the radiation damage can be reality. The theoretical and experimental basis of these assumptions will be discussed in the case of bacteriophage T7 nucleoprotein.     

Possible effects of protracted exposure on the additivity of risks from space radiations.

Conventional radiation risk assessments are presently based on the additivity assumption. This assumption states that risks from individual components of a complex radiation field involving many different types of radiation can be added to yield the total risk of the complex radiation field. If the assumption is not correct, the summations and integrations performed to obtain the presently quoted risk estimates are not appropriate. This problem is particularly important in the area of space radiation risk evaluation because of the many different types of high- and low-LET radiation present in the galactic cosmic ray environment. For both low- and high-LET radiations at low enough dose rates, the present convention is that the addivity assumption holds. Mathematically, the total risk, Rtot is assumed to be Rtot = summation (i) Ri where the summation runs over the different types of radiation present. If the total dose (or fluence) from each component is such that the interaction between biological lesions caused by separate single track traversals is negligible within a given cell, it is presently considered to be reasonable to accept the additivity assumption. However, when the exposure is protracted over many cell doubling times (as will be the case for extended missions to the moon or Mars), the possibility exists that radiation effects that depend on multiple cellular events over a long time period, such as is probably the case in radiation-induced carcinogenesis, may not be additive in the above sense and the exposure interval may have to be included in the evaluation procedure. It is shown, however, that "inverse" dose-rate effects are not expected from intermediate LET radiations arising from the galactic cosmic ray environment due to the "sensitive-window-in-the-cell-cycle" hypothesis.