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11.
刘大云 《南京航空航天大学学报》1988,(3)
本文用Melnikov方法研究高压输电网设计中提出的非线性二阶受迫振动方程的次谐波分枝,分析了系统可能出现次谐解的条件和参数区域,以此为工程应用提供参考。 相似文献
12.
在长距离GPS实时动态定位(RTK)过程中,电离层延迟误差是影响定位精度的主要误差源.目前,由于采用全空间电离层模型精度不够,对长距离RTK定位主要采用双差电离层残差内插方式.本文提出一种新的电离层模型.该模型仅对每个卫星轨迹通过的电离层部分进行建模,可适用于高精度GPS定位.采用香港数据,结果表明,该模型可较好地模拟低纬度电离层变化,并可支持GPS厘米级定位精度. 相似文献
13.
K. Dolag S. Borgani S. Schindler A. Diaferio A. M. Bykov 《Space Science Reviews》2008,134(1-4):229-268
Modern cosmological observations allow us to study in great detail the evolution and history of the large scale structure
hierarchy. The fundamental problem of accurate constraints on the cosmological parameters, within a given cosmological model,
requires precise modelling of the observed structure. In this paper we briefly review the current most effective techniques
of large scale structure simulations, emphasising both their advantages and shortcomings. Starting with basics of the direct
N-body simulations appropriate to modelling cold dark matter evolution, we then discuss the direct-sum technique GRAPE, particle-mesh (PM) and hybrid methods, combining the PM and the tree algorithms. Simulations of baryonic matter in the Universe often use hydrodynamic codes based on both particle
methods that discretise mass, and grid-based methods. We briefly describe Eulerian grid methods, and also some variants of
Lagrangian smoothed particle hydrodynamics (SPH) methods. 相似文献
14.
GRECO与行波求解低散射目标后向RCS 总被引:1,自引:0,他引:1
GRECO(Graphical Electromagnetic Computing)技术是目前分析高频区复杂目标雷达散射截面(RCS)最有效方法之一.对低散射截面目标而言,行波效应往往贡献显著,在行波效应较强的某些区域,行波值甚至超过面元与棱边贡献,本文通过GRECO与行波混合法求解低散射目标后向RCS.利用低散射支架为实例,给出与实验结果符合良好的RCS曲线,具有工程实用价值. 相似文献
15.
VARIABLESTRUCTURECONTROLOFAIRCRAFTFORATMOSPHERICDISTURBANCEZhuXiaoping;ZhouZhou(NanjingUniversityofAeronauticsandAstronautics... 相似文献
16.
Terrestrial technology is now, and increasingly, sensitive to space weather. Most space weather is caused by solar storms
and the resulting changes to the Earth's radiation environment and the magnetosphere. The Sun as the driver of space weather
is under intense observation but remains to be adequately modelled. Recent spacecraft measurements are greatly improving models
of solar activity, the interaction of the solar wind with the magnetosphere, and models of the radiation belts. In-situ data
updates the basic magnetospheric model to provide specific details of high-energy electron flux at satellite orbits. Shock
wave effects at the magnetopause can also be coarsely predicted. However, the specific geomagnetic effects at ground level
depend on the calculation of magnetic and electric fields and further improvements are needed. New work on physical models
is showing promise of raising geomagnetic and ionospheric predictability above the synoptic climatological level.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
17.
18.
Alicia L. Clúa de Gonzalez Walter D. Gonzalez 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2013
In the present paper the local-time variations in the disturbance of the geomagnetic-field horizontal component (H) for eight intense geomagnetic storms that occurred during the descending phase of solar cycle 23 have been analyzed. The study was based on the plot of contour lines of the H-depletion intensity in the plane local time versus universal time (LT–UT maps) with the objective of observing how the morphology and evolution of the ring current is mapped into the surface of the Earth in presence of intense geomagnetic storms. 相似文献
19.
P.P. Batista B.R. ClemeshaD.M. Simonich 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(9):1408-1414
A lidar has been operated in São José dos Campos, Brazil (23.2°S, 45.8°W) since 1972, mainly dedicated to the study of mesospheric sodium at the 589 nm resonant line. The molecular Rayleigh scattering can also be used provided we limit the height to ∼75 km where the sodium scattering begins. Nevertheless, the weak signal obtained only permits the determination of density and temperature profiles by accumulating a large number of shots giving only nocturnal average profiles. Temporal variations in density and temperature on the scale of hours can however, be obtained by performing a superposed epoch analysis for a given time interval and covering a period of several days. In this way we obtained hourly mean profiles grouped by months, seasons and overall, with data acquired from 1993 to 2004. The difference between the hourly temperatures and the nocturnal means shows for some months, with enough data coverage, downward propagating structures that apparently have tidal origin. The seasonal averages show a recurrent feature with high temperatures before and low temperatures after midnight above 50 km. Some similarity is found with the GSWM model, but the observed temperature amplitudes are twice of that for the model. 相似文献
20.
Zhigang Yuan Baiqi Ning Xiaohua Deng 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009,44(9):1013-1018
Based on observations of two ionosondes at Wuhan and Kokubunji, this paper presents effects of TADs on the daytime mid-latitude ionosphere during the intense geomagnetic storm on March 31, 2001. During a positive ionospheric storm, the start of the enhancement of the foF2 (F2 peak plasma frequency) at Wuhan lags that at Kokubunji by 15 min, which corresponds to the time interval of traveling atmospheric disturbances (TADs’) propagation from Kokubunji to Wuhan. Associated with the uplifting of the hmF2 (height of F2 peak) caused by TADs, it is observed by the two ionosondes that the F1 cusp becomes better developed. Therefore, during a geomagnetic storm, TADs originating from the auroral oval may have a strong influence on the shape of the electron density profile in the F1 region ionosphere at middle latitudes. It is highly likely that TADs are responsible for the evolution of the F1 cusp. 相似文献