求解双曲守恒律方程的自适应人工黏性熵稳定格式

采用熵守恒格式求解双曲守恒律方程不满足熵稳定条件.为了达到熵稳定,需要在熵守恒格式的基础上增加黏性机制,使总熵耗散.鉴于自适应人工黏性在不同的计算区域上其黏性大小的变化特点,在熵守恒通量的基础上添加经过修正的自适应人工黏性通量构造出一种新的结构简单的熵稳定格式.根据自适应人工黏性的自适应性,并经过简单调节黏性比例系数C之后,该格式可以在不使用限制器的情况下达到整体的高分辨率,表现出:在间断区域有足够的数值耗散保证稳定;在光滑区域,黏性很小,不会影响格式在此的高精度.最后的几个数值算例以熵稳定ERoe格式和高分辨率熵稳定EYee格式的数值结果作为参照,分析说明这种格式的特性.     

一类模糊时滞系统的鲁棒二次稳定和H∞控制

研究了一类连续不确定模糊时滞系统的鲁棒二次稳定问题。首先给出不确定时滞系统的自治系统稳定的充分条件,在此基础上设计状态反馈控制器,给出全局二次可稳定的充分条件。相比已有的理论成果,更进一步考虑了系统的日。性能指标,使系统在满足二次可稳定的同时也满足H∞性能指标,并将所得的条件转化为线性矩阵不等式以便借助Matlab完成求解。最后的算例验证了方法的可行性。     

基于虚位移原理的宏细观统一本构模型

结合虚位移原理和宏细观统一本构模型的基本理论提出了一种宏细观统一本构模型.该模型将宏观位移表示为宏观应变与细观位移的线性组合,然后应用虚位移原理建立基本方程,采用有限元法进行求解,得到宏观应变增量和应力增量的关系式.通过算例分析对比了模型与FVDAM(finite volume directe average meth...     

GPS derived ionospheric TEC response to geomagnetic storm on 24 August 2005 at Indian low latitude stations

Results pertaining to the response of the low latitude ionosphere to a major geomagnetic storm that occurred on 24 August 2005 are presented. The dual frequency GPS data have been analyzed to retrieve vertical total electron content at two Indian low latitude stations (IGS stations) Hyderabad (Geographic latitude 17°20′N, Geographic longitude 78°30′E, Geomagnetic latitude 8.65°N) and Bangalore (Geographic latitude 12°58′N, Geographic longitude 77°33′E, Geomagnetic latitude 4.58°N). These results show variation of GPS derived total electron content (TEC) due to geomagnetic storm effect, local low latitude electrodynamics response to penetration of high latitude convection electric field and effect of modified fountain effect on GPS–TEC in low latitude zone.     

Some effects in the upper atmosphere during geomagnetic storms

This paper examines the response of the high latitude ionosphere–thermosphere system during two intense geomagnetic storms. For that, data taken by instruments on board Dynamic Explorer 2 taken at heights of the F2-layer are used. These results represent a comparison of simultaneous measurements of storm disturbances in gas composition, electron density and temperature in common local time sectors. Documented are an increase in electron temperature and a decrease in electron density; increases both in electron temperature and electron density; and the correlation between electron density decreases and increases in the ratio N₂/O. It is noticed that the decrease in electron density is sometimes due to an increase in the molecular nitrogen density N₂ and not always is attributed both to the increase in N₂ density and the simultaneous decrease in the atomic oxygen density.     

Variations of the magnetosheath ion flux and geomagnetic activity

The magnetosheath plays a dominant role in the Sun–Earth connection because the magnetosheath field and plasma actually interact with the magnetosphere. The interactions change the magnetospheric magnetic field from its nominal value through a long chain of different processes. The change is usually described by geomagnetic indices and thus it can be expected that these indices would reflect changes in the magnetosheath. The present paper analyzes the relation between geomagnetic activity characterized by changes of the K_p, D_ST and AE indices and ion flux measured in the night-side magnetosheath. The results suggest a weak dependence of the D_ST index on the ion flux in the inner magnetosheath that is connected with a magnetopause displacement. On the other hand, fluctuations of the ion flux in the analyzed frequency range do not correlate with any of the indices.     

第22太阳周地磁活动峰值和时间的预计

本文讨论了从第13—22太阳周太阳和地磁周的特征.运用自激励门限自回归时间序列模型和最大熵谱原理自回归数学方法来模拟和预报地磁aa指数年均值峰值和时间.峰值时间是1993年秋天或1994年春天.地磁aa指数年均值峰值是26—29.第22地磁周是一个中等活动的周.     

含中介轴承内圈局部缺陷的双转子系统的组合共振特性

针对航空发动机双转子系统建立简化的动力学模型,在考虑中介轴承非线性Hertz接触力和径向游隙等非线性因素的情况下,将中介轴承内圈局部缺陷模拟成倒置的等腰梯形凹槽,利用4阶Runge-Kutta法进行数值计算,得到系统的分岔图,并着重分析分岔区域的组合共振特性,结果表明：相较于无故障系统,该系统在分岔图上出现三个新的分岔区域,前两个分岔区域是由内圈故障特征频率与高低压转子的转频形成的组合频率诱发的组合共振引起的,第三个是由内圈故障特征频率诱发共振引起的,在分岔区域内,系统运动的周期性的变化规律表现为从近似单周期运动到概周期运动再到近似单周期运动。     

Ionospheric F-region response to geomagnetic disturbances

The F2-region reaction to geomagnetic storms usually called as an ionospheric storm is a rather complicated event. It consists of so called positive and negative phases, which have very complicated spatial and temporal behavior. The main morphological features of ionospheric storms and the main processes governing their behavior were understood at the end of the 1900s and described in a series of review papers. During the recent decade there were many publications dedicated to the problem of ionospheric storms. In this paper a concept of ionospheric storm morphology and physics formulated at the end of the 1990s is briefly summarized and the most interesting results obtained in the 2000s are described. It is shown that the main features of the studies of the previous decade were: the use of GPS TEC data for analyzing the ionospheric storm morphology, attraction of sophisticated theoretical models for studying the processes governing ionospheric behavior in disturbed conditions, and accent to analysis of ionospheric behavior during prominent events (very strong and great geomagnetic storms). Also a special attention was paid to the pre-storm enhancements in foF2 and TEC.     

Modeling solar proton access to geostationary spacecraft with geomagnetic cutoffs

Solar energetic particle (SEP) cutoffs at geosynchronous orbit are sensitive to moderate geomagnetic activity and undergo daily variations due to the day–night asymmetry of the magnetosphere. At geosynchronous orbit, cutoff rigidity also has a large directional dependence, with the highest cutoff rigidity corresponding to ions arriving from magnetic east and lowest cutoff rigidity corresponding to ions incident from the west. Consequently, during geomagnetically quiet periods, the SEP flux observed by an eastward facing particle detector is significantly lower than observed by a westward facing particle detector. During geomagnetically disturbed periods the cutoff is suppressed allowing SEPs access well inside of geosynchronous, so that the east–west SEP flux ratio approaches unity. Variations in the east–west SEP flux ratio observed by GOES Energetic Particle Sensors (EPS) have recently been reported by Rodriguez et al. (2010). In NOAA’s operational processing of EPS count rates into differential fluxes, the differential flux is treated as isotropic and flat over the energy width of the channel. To compare modeled SEP flux with GOES EPS observations, the anisotropy of the flux over the EPS energy range and field of view must be taken into account. A technique for making direct comparisons between GOES EPS observations and SEP flux modeled using numerically computed geomagnetic cutoffs is presented. Initial results from a comparison between modeled and observed flux during the 6–11 December 2006 SEP event are also presented. The modeled cutoffs reproduce the observed flux variations well but are in general too high.