在强地磁活动期间热层大气成份和密度的变化

选用了１９７４－０７－０６,１９８２－０３－０２和１９８２－０９－０６三次强地磁活动时的Ａｐ值,由ＡＥ－Ｃ和ＤＥ－Ｂ卫星所测得的热层成份数据,进行统计分析,结果表明;在强地磁活动期间,热层大气密度涨落变化十分清晰、涨幅随高度增高而增大,高度６００ｋｍ附近涨幅可直达４倍,热层大气成份中Ｎ２的数密度涨幅最大,而原子氧的丰度在强地磁活动期间明显地下降。     

带电卫星地磁摄动力及其寿命问题的讨论

文章给出了带电卫星受到地磁摄动力的一般表达式,并就带电对卫星寿命的影响问题进行了定性讨论.     

1998年9月24日地磁暴前宇宙线各向异性特性分析

分析了日本Nagoya 宇宙线闪烁体望远镜30°, 49°, 64° 倾角的东、西、南、北方向探测数据的变化特点, 运用小波分析方法定性地探讨了磁暴前后宇宙线南北、东西各向异性的变化特征. 研究发现, 当发 生大地磁暴时, 地面宇宙线强度的各向异性特征将发生非常大的变化, 这种变化一般在磁暴发生前10~20 h就开始出现. 当描述这种各向异性特征的各向异性指数的小波系数变化达到一定阈值时, 就可能有大地磁暴发生.      

Solar particle dynamics during magnetic storms of July 23–27, 2004

It is a case study of a chain of three magnetic storms with a special attention to the particle dynamics based on CORONAS-F and SERVIS-1 low altitude satellite measurements. Solar proton penetration inside the polar cap and inner magnetosphere and dynamics at different phases of the magnetic storms was studied. We found, that solar protons were captured to the inner radiation belt at the recovery phase of the first and the second magnetic storms and additionally accelerated during the last one. No evidence of sudden commencement (SC) particle injection was found. Enhanced solar proton belt intensity with small pitch angles decreased slowly during satellite orbits for 30 days until the next magnetic storm. Then in 20–30 h we registered strong precipitation of these protons followed by the trapped proton flux dropout. Intensity decrease was more pronounced at lower altitudes and higher particle energies.     

Ionospheric oscillations caused by geomagnetic Pi2 pulsations and their observations by multipoint continuous Doppler sounding; first results

In 2004, we started operating a continuous Doppler sounding system to investigate ionospheric signatures of infrasonic, short period acoustic gravity waves and geomagnetic pulsations. Since January 2007, four stable 3.59 MHz transmitters have been in operation in the western part of the Czech Republic. Multipoint measurements enable us to investigate horizontal propagation of waves and disturbances in the ionosphere and to estimate horizontal distances over which these waves (disturbances) are correlated.     

新Omega涡识别法在液体火箭发动机涡轮氧泵中的应用

离心泵中流动不稳定现象与流场中旋涡的形成及演化过程密切相关。为解决传统涡识别法在高速离心泵流场涡结构捕捉方面的缺陷,引入新Omega涡识别法,对液体火箭发动机涡轮氧泵流场中的涡结构进行了分析。确定了新Omega涡识别法在高速离心泵流场涡结构捕捉方面的优势,利用该方法对涡轮氧泵中离心轮与扩压器之间的动静干涉机理进行了阐释。结果表明:对于高速离心泵,传统Q准则以及λ2准则涡识别法错误地将壁面强剪切层识别为旋涡,而新Omega涡识别方法能够有效滤除流场中非旋转涡量部分,较好地捕捉流场中涡结构,可作为高速离心泵流场涡结构识别的首选方法。通过离心轮与扩压器动静干涉区域旋涡演化过程分析可知,涡轮氧泵离心轮与扩压器之间的动静干涉效应主要源自于扩压器叶片压力面上的周期性涡脱落现象。     

CHANGES OF THE THERMOSPHERE DENSITY IN THE SUNSHINE AND SHADE AREA OBSERVED BY "SZ-2" ATMOSPHERIC DENSITY DETECTOR

In this paper, thermosphere density data of "SZ-2" Atmospheric Density Detec tor From February to April 2001 are used to study the changes of the thermo sphere density in the sunshine and shaded area during solar and geomagnetic activity. The results show that in the sunshine area, the peak value of atmo spheric density changes as F10.7 varies; during geomagnetic activity, the peak value of atmospheric density in the shaded area increases as Ap increases, and start off with higher latitude, therefore move to lower latitude.     

神舟4号大气成分探测的新结果

神舟4号(SZ-4)大气成分探测器搭载在SZ-4留轨舱上于2002年12月30日发射入轨，在在轨运行的前3个多月中，正值地球南半球处于夏半球季节，并发生了多次中低强度的地磁扰动事件，SZ-4大气成分探测器测得了轨道舱运行高度上(330-362km附近)大气成分的响应变化和异常现象新结果．探测数据表明，中低强度的地磁扰动事件也能引起热层大气中主要成分O和N2的数密度值增高的响应变化．同样在进入地磁扰动峰期后较高纬度处出现了N2的异常增变和O的异常降变以及大气密度异常扰动的现象，但此期间所出现异常现象的地域与SZ-3和SZ-2大气成分探测器探测结果相反，它仅位于南半球较高纬度地区．     

Polar ionosphere and geomagnetic response for the flux transfer events: A case study

On April 15th 2003, Cluster crossed the dayside magnetopause boundary and observed a series flux transfer events (FTEs) during the interval from 0630 to 0730 UT. During this period, the interplanetary magnetic field (IMF) showed a negative z component and a positive y component. Simultaneous corresponding transient plasma flows were identified in the near-conjugate polar ionosphere by the CUTLASS Finland HF radar, and the geomagnetic field disturbances were observed by the IMAGE ground-based magnetometers. By combing these data and applying the Cooling model, we show that the transient plasma flows and the geomagnetic field disturbances are closely related to the dayside FTEs.