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111.
SOHO/UVCS data indicate that minor ions in the corona are heated more than hydrogen, and that coronal heating results in T⊥ larger than T‖. Analogous behavior has been known from in situ measurements in solar wind for many years. Here we compare and contrast two
mechanisms which have been proposed to account for the above behavior: ion-cyclotron resonance and gravity damping.
This revised version was published online in June 2006 with corrections to the Cover Date. 相似文献
112.
Michael R. Collier Aaron Roberts Adolfo Viñas 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(10):1704-1709
We describe a new wave mode similar to the acoustic wave in which both density and velocity fluctuate. Unlike the acoustic wave in which the underlying distribution is Maxwellian, this new wave mode occurs when the underlying distribution is a suprathermal κ-function and involves fluctuations in the power law index, κ. This wave mode always propagates faster than the acoustic wave with an equivalent effective temperature and becomes the acoustic wave in the Maxwellian limit as κ → ∞. 相似文献
113.
114.
The review contains the important achievements in dynamics of the galactic disks. Among them there are I. New structures
discovered recently: • giant vortices (including giant anticyclone in the Solar vicinity); • slow bar; • inner oscillating
structure within spiral arms similar that of enveloped soliton; • chaotic streamlines in the velocity field of the gaseous
disk of a real galaxy. II. New collective phenomina discovered recently: • new overreflection instability initiating ‘mini-spiral’
in the innermost central parsec of Galaxy; • large-scale convection caused by nonlinear interaction of density wave with
disk gas; • non-kolmogorovian spectrum of weak turbulence corresponding to the observed one in the • Solar vicinity. III. New
methods worked out recently: • reconstruction of full three-dimensional vector field of gas velocity from the observed line-of-
• sight velocity field; • observational test for verification of the wave-nature of the spiral arms; • observational test
to distinguish two types of vertical motions: warp and z-motions in the • density wave; • derivation of correct system of two-dimensional dynamical equations from the initial three-
• dimensional one.
This revised version was published online in June 2006 with corrections to the Cover Date. 相似文献
115.
116.
K. Andreov L. Pech 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2007,40(12):1871-1880
This paper is devoted to the study of propagation of disturbances caused by interplanetary shocks (IPS) through the Earth’s magnetosphere. Using simultaneous observations of various fast forward shocks by different satellites in the solar wind, magnetosheath and magnetosphere from 1995 till 2002, we traced the interplanetary shocks into the Earth’s magnetosphere, we calculated the velocity of their propagation into the Earth’s magnetosphere and analyzed fronts of the disturbances. From the onset of disturbances at different satellites in the magnetosphere we obtained speed values ranging from 500 to 1300 km/s in the direction along the IP shock normal, that is in a general agreement with results of previous numerical MHD simulations. The paper discusses in detail a sequence of two events on November 9th, 2002. For the two cases we estimated the propagation speed of the IP shock caused disturbance between the dayside and nightside magnetosphere to be 590 km/s and 714–741 km/s, respectively. We partially attributed this increase to higher Alfven speed in the outer magnetosphere due to the compression of the magnetosphere as a consequence of the first event, and partially to the faster and stronger driving interplanetary shock. High-time resolution GOES magnetic field data revealed a complex structure of the compressional wave fronts at the dayside geosynchronous orbit during these events, with initial very steep parts (10 s). We discuss a few possible mechanisms of such steep front formation in the paper. 相似文献
117.
118.
应用钠原子和中性大气分子的质量连续性方程来模拟突发纳层(SSL),垂直风场采用接近实际大气重力波的正弦行波模式,结果较好地反映了SSL的形成过程。SSL的形成时刻在5-15min之间并可持续到30min之后,形成高度大约在90-100km之间,峰宽为0.5-2km之间,这些都与实际观测SSL的特点相符,同时还进一步地研究了当重力波参数(主要指垂直波长和周期)、风速以及常态钠层半宽度发生变化时SSL的变化趋势。 相似文献
119.
A. Guglielmi J. Kangas J. Kultima A. Potapov 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2005,36(12):2413-2416
There are a host of factors influencing the excitation of Pc1 geomagnetic pulsations, which are ULF waves in the frequency range between 0.2 and 5 Hz. We have studied carefully the dependence of the pearl-type Pc1 activity at Sodankylä, Finland (L = 5.1) on the plasma density N in front of the magnetosphere, the bulk velocity V of the solar wind, and the intensity B of the IMF. The result is as follows: high values of N and reduced values of V are favorable to appearance of Pc1, whereas the dependence of Pc1 activity on B is practically absent. We also show that the probability of Pc1 occurrence decreases with the interplanetary electric field, and increases with solar wind impact pressure and with the plasma to magnetic pressure ratio “beta”. 相似文献
120.
复合材料结构中的制造缺陷严重影响航天装备的服役性能,如何实现复合材料缺陷的高精度检测表征与评价对航天装备的安全性设计意义重大。针对树脂基复合材料缺陷的先进表征技术及评价方法进行概述,重点介绍了复合材料成型工艺与典型缺陷类型、常用复合材料缺陷检测与原位表征技术和复合材料缺陷分析评价方法。通过对复合材料缺陷研究现状的梳理,可见计算机断层扫描技术和基于图像的数值计算方法正以其独特的精确度优势在复合材料缺陷的表征与分析领域崭露头角。同时还对先进的复合材料检测与评价技术在航天装备中复合材料结构安全性设计与可靠性分析方面的应用和发展趋势进行了展望。 相似文献