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461.
L. Dam M. Derrien 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2002,29(12):373-2073
This paper presents the scientific objectives of the Solar Physics and Interferometry Mission (SPI), describes succinctly the model payload and summarizes mission's issues. Novel instrumentation (interferometry) and clever mission design (small platform on low orbit with high telemetry and dedicated smaller platform on hexapod for permanently Sun-centered instruments) allow both spectral imaging and Helioseismology at very high spatial and temporal resolutions. Although not retained by ESA, this mission could become reality through NASA MIDEX and/or CNES PROTEUS opportunities as soon as 2007–2008. 相似文献
462.
K. Arai J. Sakakibara 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2006,37(12):2202-II
A method for estimation of sea surface temperature, ocean wind speed and water vapor with microwave radiometer data based on simulated annealing is proposed. The proposed method shows about 60% improvement of sea surface temperature estimation accuracy in comparison to the existing method using Newton’s iterative algorithm. 相似文献
463.
应用数值计算的方法模拟了细长体截面绕流结构的演变过程.指出随着细长体背涡的发展,导致截面流场的拓扑结构发生变化,会出现一种临界流动状态.并用微分方程的定性理论分析了此时流场中出现的一种高阶奇点.这种高阶奇点的指数为-3/2,它是结构不稳定的,稍有扰动就会产生分叉,使流场的拓扑结构发生变化.得出了定常对称背涡流态下细长体的空间绕流结构图. 相似文献
464.
A. Aran B. Sanahuja D. Lario 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2005,36(12):2333-2338
We present a preliminary version of a potential tool for real time proton flux prediction which provides proton flux profiles and cumulative fluence profiles at 0.5 and 2 MeV of solar energetic particle events, from their onset up to the arrival of the interplanetary shock at the spacecraft position (located at 1 or 0.4 AU). Based on the proton transportation model by Lario et al. [Lario, D., Sanahuja, B., Heras, A.M. Energetic particle events: efficiency of interplanetary shocks as 50 keV E < 100 MeV proton accelerators. Astrophys. J. 509, 415–434, 1998] and the magnetohydrodynamic shock propagation model of Wu et al. [Wu, S.T., Dryer, M., Han, S.M. Non-planar MHD model for solar flare-generated disturbances in the Heliospheric equatorial plane. Sol. Phys. 84, 395–418, 1983], we have generated a database containing “synthetic” profiles of the proton fluxes and cumulative fluences of 384 solar energetic particle events. We are currently validating the applicability of this code for space weather forecasting by comparing the resulting “synthetic” flux profiles with those of several real events. 相似文献
465.
P.L Pritchett 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1997,19(12):1807-1816
Recent developments regarding collisionless reconnection in current sheets with a finite normal magnetic field component (Bz) are reviewed. In 2-D x, z configurations the ion tearing mode is stabilized by the electron compressibility. When the y dependence is included, cross-field current instabilities can be excited. Of these, the drift kink mode appears to be particularly important. 3-D electromagnetic particle simulations indicate that this mode can act as the precursor to the growth of tearing modes and subsequent reconnection. 相似文献
466.
467.
低轨航天器致空间等离子体尾流 总被引:1,自引:0,他引:1
建立起一个低轨道航天器引起的等离子体尾的二维计算机模式,结果表明:(1)尾流的宽度随表面负电位值的增加而变窄。(2)随离子马赫数增加尾流位垒变宽;(3)对正电位表面情况尾流近区有电子聚集,并且离子的放空更远。 相似文献
468.
Some comparisons of orbit determination and parameter estimation based on LAGEOS 1 and LAGEOS 2 data
H. Montag 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1995,16(12):149-154
The modelling accuracy of the LAGEOS 1 orbit was continously improved since its launch in 1976. In spite of these experiences the modelling accuracy of LAGEOS 2 is still about 20 per cent worse. Considering e. g. only the influence of different gravity field models it has been shown that the orbital fits for arc lengths of one month is generally about 25 mm for LAGEOS 1 and more than 30 mm for LAGEOS 2. This is mainly due to the fact that LAGEOS 2 has not yet been used for the determination of most gravity field models. The influences of different model parameters on the estimation of station coordinates, Earth rotation parameters, the geogravitational coefficient, the radiation pressure coefficient, and the empirical acceleration has been studied. The differences and peculiarities of both satellites are discussed. Although the analysis of LAGEOS 2 data still does not reach the high level of LAGEOS 1 combination solutions using both satellites allow new insights, higher accuracies, and a higher time resolution for the parameters and phenomena investigated. 相似文献
469.
共轴式小型直升机操纵系统动态特性分析研究 总被引:1,自引:0,他引:1
对某共轴式小型遥控直升机纵向系统建立了工程实用的数学模型,分析研究了该系 统动态特性和参数变化对其动特性的影响.通过与试验、试飞比较,证明该模型是正确的、 可信的、其精度符合工程要求. 相似文献
470.
在“CCIR”534-1号报告(以下简称“CCIR”)中,提供了全球性E,出现概率的分布,见图1 相似文献