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131.
本文运用磁场的最小方差分析法和磁场-电子密度的相关分析法分析了欧洲空间局Giotto飞船对P/Grigg-Skjellerup(简称G-S)彗星弓激波附近磁场和电子能流的部分观测数据.结果表明彗星附近存在大量的频率靠近新生水族离子回旋频率的波动,它们是由彗星新生水族离子环流激发的低频左旋电磁波.波在近似平行于磁场方向传播,斜传播角小于15°.电子数据和磁场数据相关分析表明即使在离彗星很远的地方仍然存在压缩波. 相似文献
132.
133.
A double discontinuity is a rarely observed compound structure composed of a slow shock layer and an adjoining rotational
discontinuity layer in the downstream region. In this paper, we report the observations of a double discontinuity detected
by Wind on May 15, 1997. This double discontinuity is found to be the front boundary of a magnetic cloud boundary layer. We
strictly identify the shock layer and the rotational discontinuity layer by using the high-resolution plasma and magnetic
field data from Wind. The observed jump conditions of the upstream and downstream region of the slow shock layer are in good
agreement with the Rankine – Hugoniot relations. The flow speeds in the shock frame U
n
<V
Acos θ
Bn
on both sides of the slow shock layer. In the upstream region, the slow Mach number M
s1=U
n1/V
s1 is 1.95 (above unity), and in the downstream region, the slow Mach number M
s2=U
n2/V
s2 is 0.31 (below unity). Here V
A and V
s represent the Alfvén speed and the local slow magnetosonic speed, respectively, and θ
Bn
is the angle between the direction of the magnetic field and the shock normal. The magnetic cloud boundary layer observed
by Wind was also detected by Geotail 48 min later when the spacecraft was located outside the bow shock of the magnetosphere.
However, Geotail observations showed that its front boundary was no longer a double discontinuity and the rotational discontinuity
layer disappeared, indicating that this double discontinuity was unstable when propagating from Wind to Geotail. 相似文献
134.
���ϵ�������Ӧ������ǿ����ϵ�о� 总被引:1,自引:0,他引:1
???????????????????????????鹹???????????????????????о?????????????????????GPS?????????????????????????,?????????????????????????????????????????????????????6??????????????????????????????????????????????????????????????????????????????н???????, ??????????????3????????Σ?????? 相似文献
135.
Rossby waves with linear topography in barotropic fluids 总被引:1,自引:0,他引:1
Rossby waves are the most important waves in the atmosphere and ocean, and are parts of a large-scale system in fluid. The theory and observation show that, they satisfy quasi-geostrophic and quasi-static equilibrium approximations. In this paper, solitary Rossby waves induced by linear topography in barotropic fluids with a shear flow are studied. In order to simplify the problem, the topography is taken as a linear function of latitude variable y, then employing a weakly nonlinear method and a perturbation method, a KdV (Korteweg-de Vries) equation describing evolution of the amplitude of solitary Rossby waves induced by linear topography is derived. The results show that the variation of linear topography can induce the solitary Rossby waves in barotropic fluids with a shear flow, and extend the classical geophysical theory of fluid dynamics. 相似文献
136.
Using nine years of solar wind plasma and magnetic field data from the Wind mission, we investigated the characteristics of both magnetic clouds (MCs) and magnetic cloud-like structures (MCLs) during
1995 – 2003. A MCL structure is an event that is identified by an automatic scheme (Lepping, Wu, and Berdichevsky, Ann. Geophys.
23, 2687, 2005) with the same criteria as for a MC, but it is not usually identifiable as a flux rope by using the MC (Burlaga et al., J. Geophys. Res.
86, 6673, 1981) fitting model developed by Lepping, Jones, and Burlaga (Geophys. Res. Lett.
95(11), 957, 1990). The average occurrence rate is 9.5 for MCs and 13.6 for MCLs per year for the overall period of interest, and there were
82 MCs and 122 MCLs identified during this period. The characteristics of MCs and MCL structures are as follows: (1) The average
duration, Δt, of MCs is 21.1 h, which is 40% longer than that for MCLs (Δt=15 h); (2) the average
(minimum B
z
found in MC/MCL measured in geocentric solar ecliptic coordinates) is −10.2 nT for MCs and −6 nT for MCLs; (3) the average
Dstmin (minimum Dst caused by MCs/MCLs) is −82 nT for MCs and −37 nT for MCLs; (4) the average solar wind velocity is 453 km s−1 for MCs and 413 km s−1 for MCLs; (5) the average thermal speed is 24.6 km s−1 for MCs and 27.7 km s−1 for MCLs; (6) the average magnetic field intensity is 12.7 nT for MCs and 9.8 nT for MCLs; (7) the average solar wind density
is 9.4 cm−3 for MCs and 6.3 cm−3 for MCLs; and (8) a MC is one of the most important interplanetary structures capable of causing severe geomagnetic storms.
The longer duration, more intense magnetic field and higher solar wind speed of MCs, compared to those properties of the MCLs,
are very likely the major reasons for MCs generally causing more severe geomagnetic storms than MCLs. But the fact that a
MC is an important interplanetary structure with respect to geomagnetic storms is not new (e.g., Zhang and Burlaga, J. Geophys. Res.
93, 2511, 1988; Bothmer, ESA SP-535, 419, 2003). 相似文献
137.
This paper describes studies of the effect of hydrate dissociation on the safety and stability of methane hydrate-bearing sediments. Methane hydrates within the sediments were dissociating under the conditions of a confining pressure of 0.5 MPa, 1 MPa, 2 MPa and a temperature of −5 °C. After 6 h, 24 h, or 48 h, a series of triaxial compression tests on methane hydrate-bearing sediments were performed. The tests of ice-clay and sediments without hydrate dissociation were performed for comparison. Focusing on the mechanical properties of the sediments, the experimental results indicated that the shear strength of the ice-clay mixtures was lower than that of the methane hydrate-bearing sediments. The strength of the sediments was reduced by hydrate dissociation, and the strength tended to decrease further at the lower confining pressures. The secant modulus ES of the sediments dropped by 42.6% in the case of the dissociation time of the hydrate of 48 h at the confining pressure of 1 MPa; however, the decline of the initial yield modulus E0 was only 9.34%. The slower hydrate dissociation rate contributed to reducing the failure strength at a declining pace. Based on the Mohr–Coulomb strength theory, it was concluded that the decrease in strength was mainly affected by the cohesive reduction. Moreover, the mathematical expression of the M–C criterion related to the hydrate dissociation time was proposed. This research could be valuable for the safety and stability of hydrate deposits in a permafrost region. 相似文献
138.
风廓线雷达垂直径向速度应用初探 总被引:2,自引:1,他引:1
利用北京风廓线雷达五波束探测中的垂直波束资料,进行了垂直速度在预报中的应用研究。通过对垂直速度的分级显示,配合地面气象记录,对不同的天气个例进行分析,结果表明:平稳晴空的天气风廓线雷达所测量的垂直速度很小,基本上在±1m·s~(-1)范围内;而有降水时,风廓线雷达所测得边界层的垂直速度基本上都是朝向地面的,不同相态降水粒子的垂直下落速度有明显的差别。分析表明风廓线雷达垂直速度的探测对研究晴空大气的垂直运动、判断降水粒子相态和降水预报有应用价值。 相似文献
139.
随着地理信息系统在三维数字城市建设的广泛应用,更加逼真且信息更丰富的三维立体导航逐渐在导航领域占据主导地位。以A nGeo三维地理信息系统软件为基础,研究了三维导航系统的设计与实现,该系统不仅可以提供基本的信息查询功能,还能完成三维互动式浏览、三维地图导航以及最佳路径选择的功能。 相似文献
140.
Presented in this paper is a mathematical model to calculate the probability of the sediment incipient motion,in which the effects of the fluctuating pressure and the seepage are considered.The instantaneous bed shear velocity and the pressure gradient on the bed downstream of the backward-facing step flow are obtained according to the PIV measurements.It is found that the instantaneous pressure gradient on the bed obeys normal distribution.The probability of the sediment incipient motion on the bed downstream of the backward-facing step flow is given by the mathematical model.The predicted results agree well with the experiment in the region downstream of the reattachment point while a large discrepancy between the theory and experiment is seen in the region near the reattachment point.The possible reasons for this discrepancy are discussed. 相似文献