共查询到20条相似文献,搜索用时 31 毫秒
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I. Apáthy I. Szemerey P. Bencze K. Kovács V. Afonin V. Bezrukih K. Gringauz N. Shutte 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1981,1(12):101-105
Ion temperature and total ion concentration measured on 25th October 1977 during the flight of the geophysical rocket “Vertical-6” are analyzed. The solar EUV fluxes determined in five wave-length bands with a photoelectron analyzer are also given. The observed anomalous variation of ion temperature between 700 and 900 km and the measured ion concentration can be explained, if the charge exchange reactions H+ ? O+ and diffusion are taken into account. 相似文献
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A. Seiff J.T. Schofield A.J. Kliore F.W. Taylor S.S. Limaye H.E. Revercomb L.A. Sromovsky V.V. Kerzhanovich V.I. Moroz M.Ya. Marov 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1985,5(11):3-58
From a critical comparison and synthesis of data from the four Pioneer Venus Probes, the Pioneer Venus Orbiter, and the Venera 10, 12, and 13 landers, models of the lower and middle atmosphere of Venus are derived. The models are consistent with the data sets within the measurement uncertainties and established variability of the atmosphere. The models represent the observed variations of state properties with latitude, and preserve the observed static stability. The rationale and the approach used to derive the models are discussed, and the remaining uncertainties are estimated. 相似文献
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星座设计与星际链路的建立 总被引:4,自引:1,他引:3
在卫星移动通信系统中 ,若使用 L EO/MEO卫星 ,则其位置相对于地球是时变的 ,卫星之间的相对位置也是时变的。要在星座中建立星际链路(Inter Satellite L inks) ,需要确知卫星的相对位置 ,计算卫星间的方位角和距离。文章在介绍了星座类型和几种星座设计方法的基础上 ,说明了星际链路的空间几何参数关系 ,详细讨论了卫星间的方位角和距离与星座设计的关系 ,并给出了一些有价值的结论。 相似文献
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H.S. Ahluwalia 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1981,1(3):151-154
Data from worldwide network of neutron and muon detectors are used to study 11-year variations of cosmic rays, over four solar activity cycles. We find that the recovery of the cosmic ray intensity follows one of the two distinct modes. During odd cycles recovery is completed in 6 to 8 years, but during even cycles complete recovery occurs in 2 to 3 years. Two model magnetic configurations of the heliosphere are proposed to understand these recovery modes. Implications of these models are also discussed. 相似文献
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行星际起伏向磁层顶的输运 总被引:1,自引:1,他引:0
时间尺度为分钟数量级的太阳风速度和行星际磁场大幅度扰动实际上始终存在于行星际空间的。这些扰动一直传输到紧贴磁层边界面外侧的区域。它们在磁鞘等离子体和磁层顶的相互作用过程中可能起很重要的作用。行星际起伏中的磁场分量在通过地球弓激波时首先经历一次跳跃,然后一部分扰动被带到磁层边界面处。在边界面附近磁场扰动幅度被大大地放大了。弓激波上游的太阳风条件控制了放大因子。本文所作的数值模拟研究结果表明,如果上游有大幅度的扰动,在边界面附近就有大幅度的Alfven起伏的磁场分量。当上游磁场接近垂直于日地联线时,放大因子变得相当大,而且放大因子随上游的等离子体β值和/或Alfven马赫数的增加而增加。上游各向异性对放大因子的影响不大。在磁层边界附近存在大幅度起伏表明这里不存在稳定的片流。 相似文献
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分析总结了计量校准市场的特点和竞争状况。通过实际工作积累的经验,对影响计量校准市场开发的因素进行分析,阐述了应当分析研究计量校准市场的规律和特点,明确市场定位、确定发展方向,才能扬长避短,有效扩大市场占有率,保证计量校准市场开发工作稳定、快速的发展。 相似文献
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M.J. Rycroft I.R. Jones 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1985,5(10):21-27
The paper discusses how profiles of electron and/or ion distributions that are produced by two different computer models can be smoothly coupled together. The first of these models is the empirical International Reference Ionosphere which produces a vertical profile of ionospheric parameters up to an altitude of 1000 km. The second is a physically-based, diffusive equilibrium model of the plasmasphere based upon the theoretical work of Angerami and Thomas /1/, in which plasma is constrained to move parallel to the Earth's magnetic field lines. Some problems associated with this work are considered, as are some initial results. 相似文献
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本文在文献[9]的基础上,通过增加二个时刻的模型计算,给出了更完整的1983年2月3日2B级耀斑脉冲相色球半经验模型,从而进一步描述了脉冲相色球物理过程,并对耀斑动力学参量及能量过程作了初步讨论。 相似文献
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给出了任意速度分布函数条件下复频率的介电函数和色散关系的求解方法. 讨论了16矩近似条件下, 场向热流对电子速度分布函数, 介电函数实部与虚部, 以及离子与电子谐振频率和阻尼率的影响, 并与平衡态时麦克斯韦分布等离子体的计算结果进行了比较. 忽略场向热流效应, 正向电子漂移速度条件下, 上行等离子线探测, 会过高估计场向电流; 负向电子漂移速度条件下, 上行等离子线探测会过低估计场向电流. 对上下行等离子线同时探测情况, 忽略热流效应同样会过高估计场向电流. 相似文献
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Nickolay Ivchenko Jan B?ecki Krzysztof Kossacki Sergey P. Savin 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1997,19(12):1933-1937
Satellite observations near the magnetopause and within the magnetosheath revealed the existence of some structures characterised by specific magnetic field and plasma signatures. They have been called “Flux Transfer Events”. One of the models of FTEs is a reconnected fluxtube, extending from the inner magnetosphere into the magnetosheath. ELF-ULF waves are often observed in together with other FTE's signatures. Wideband emissions are associated with the boundaries of FTEs with characteristic maxima at lower hybrid and ion-cyclotron frequencies. They provide a tool for better timing of the events. These emissions might also be related to the reconnection process. Observations of FTE's by Prognoz-8 satellite are presented in our paper. Wave signatures of the FTEs are described. Various mechanisms of generation of the emissions by instabilities depending on local plasma conditions are discussed along with non-local aspects of such waves. Numerical solutions of the dispersion equation for the typical conditions in FTEs are presented. Possible relation of these waves to the reconnection process are discussed. 相似文献
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G.W. Prölss M. Roemer 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1985,5(7):193-202
The magnitude, dissipation mechanism, and spatial distribution of the solar wind - magnetospheric energy source are discussed briefly. Using N2 measurements of the ESRO 4 satellite, the temperature increase in the polar thermosphere associated with this energy source are investigated. Part of the locally dissipated energy is transported toward lower latitudes. Possible modes of energy transfer are reviewed, and local time variations are documented. Some suggestions are made with respect to future empirical models of the thermosphere. 相似文献
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J. Dorschner 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1981,1(8):75-84
The distribution of interstellar dust within 500 pc from the sun obtained from recent investigations is described. Statistical properties of dust clouds in the neighbourhood of the sun and individual data of two near clouds in high galactic latitudes are discussed. The present knowledge of the chemical composition of the interstellar dust grains is outlined. Possible relations between solar system solids and interstellar solids are indicated. 相似文献
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近地航天器测控设备分配策略 总被引:1,自引:0,他引:1
对多个近地航天器同时在轨运行时,如何分配地面有限的测控设备以完成各航天器的测控任务提出了一种分配策略,并编写了相应的软件进行试算,取得了满意的结果。 相似文献
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U.W. Langner M.S. Potgieter 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2005,35(12):2084-2090
The effects of changing the position of the solar wind termination shock and the position of the heliopause, and therefore the extent of the heliosheath, on the modulation of cosmic ray protons are illustrated. An improved numerical model with diffusive termination shock acceleration, a heliosheath and drifts is used. The modulation is computed in the equatorial plane and at 35 heliolatitude using recently derived diffusion coefficients applicable to a number of cosmic ray species during both magnetic polarity cycles of the Sun. It was found that qualitatively the modulation results for the different heliopause positions are similar although they differ quantitatively, e.g., clearly different radial gradients are predicted for the regions beyond the termination shock compared to inside the shock. The difference between the modulation for the two solar polarity cycles are less significant at a heliolatitude of 35° than in the equatorial plane. We found that moving the termination shock from 90 to 100 AU, with the heliopause fixed at 120 AU, caused only quantitative differences so that the exact position of the TS in the outer heliosphere seems not crucially important to global modulation. Moving the heliopause outwards, to represent the modulation in the tail region of the heliosphere, causes overall decreases in the cosmic ray intensities but not linearly as a function of energy, e.g., at 1 GeV the effect is insignificant. We conclude from this modelling that the modulation of protons in the heliospheric nose and tail regions are qualitatively similar although, clear quantitative and interesting differences occur. 相似文献
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为了实现守时系统与授时系统的高准确度时间同步,通过搬运钟法对微波时间传输系统的可测量时延部分进行准确测量,应用测量结果对微波时间传输系统进行校准,将GPS共视比对结果与微波时间传输系统的单、双向比对结果进行分析研究,并用BIPM(BUREAU INTERNATIONAL DES POIDS ET MESURES)给出的结果进行验证,得出两种不同时间同步方法的同步误差和两种不同方法产生误差的主要原因,给出了两种不同方法在时间统一系统中的的最佳应用模式。 相似文献