Input Parameters for Models of Energetic Electrons Fluxes at the Geostationary Orbit

The results of cross-correlation analysis between electrons fluxes (with energies of > 0.6MeV, > 2.0 MeV and > 4.0MeV), geomagnetic indices and solar wind parameters are shown in the paper. It is determined that the electron fluxes are controlled not only by the geomagnetic indices, but also by the solar wind parameters, and the solar wind velocity demonstrates the best relation with the electron fluxes. Numerical value of the relation efficiency of external parameters with the highly energetic electrons fluxes shows a periodicity. It is presented here the preliminary results of daily averaged electrons fluxes forecast for a day ahead on the basis of the model of neuron networks.     

考虑传感器倍频干扰的磁轴承自动平衡控制

传感器倍频干扰信号与控制系统相互影响,容易引发磁轴承转子微振动。为了抑制高转速下传感器倍频干扰导致的磁轴承微振动,本文首先建立考虑传感器倍频干扰的磁轴承控制系统模型,分析位移传感器谐波与控制系统微振动的内在机理,然后提出一种基于多频自适应陷波器的磁轴承自动平衡控制方法,消除或抑制轴承的同频或倍频反作用力,使传感器谐波扰动产生的电磁力得到衰减。仿真结果表明,在转速30000(r/min)时,采用该自动平衡控制方法后,与传感器谐波干扰相关的振动力得到一定抑制。     

On the motions of RHESSI flare footpoints

The footpoint motions of flare hard X-ray (HXR) sources are directly related to the reconnection scenario of a solar flare. In this work, we tried to extract the information of footpoint motions for a number of flares observed with RHESSI. We found that the RHESSI flare results of the footpoint motions strongly support the classification proposed from the observations of YOHKOH/HXT. Furthermore, it is found that a flare can consist of two types of footpoint motions. We discussed the connections of the footpoint motions with the two-dimensional reconnection models.     

压气机通道端壁附面层区叶片载荷分布研究

为了探索叶片载荷分布对端壁附面层区流动的影响,设计出3套平面叶栅,叶片载荷分别趋前、居中和靠后。对于低速流动,采用实验和三维Navier-Stkoes方程方法对叶片表面、叶栅出口流场进行了研究。研究表明:叶片载荷靠后叶片(No.3)性能较叶片载荷趋前(No.1)和居中(No.2)叶片差;No.2叶片与No.1叶片比较,出口损失小,但落后角较大,扩压能力较小;在进口端壁附面层一定时,叶片前缘附近的端壁附面层区叶片力亏损变化与叶片力变化呈正相关;端壁面与叶片吸力面之间构成的角区内角涡,没有造成靠近后缘端壁附面层区吸力面静压明显下降。      

Sailing with solar and planetary radiation pressure

Literature on solar sailing has thus far mostly considered solar radiation pressure (SRP) as the only contribution to sail force. However, considering a sail in a planetary mission scenario, a new contribution can be added. Since the planet itself emits radiation, this generates a radial planetary radiation pressure (PRP) that is also exerted on the sail. Hence, this work studies the combined effects of both SRP and PRP on a sail for two case studies, i.e. Earth and Venus. In proximity of the Earth, the effect of PRP can be significant under specific conditions. Around Venus, instead, PRP is by far the dominating contribution. These combined effects have been studied for single- and double-sided reflective coating and including eclipse. Results show potential increase in the net acceleration and a change in the optimal attitude to maximise the acceleration in a given direction. Moreover, an increasing semi-major axis manoeuvre is shown with and without PRP, to quantify the difference on a real-case scenario.     

Global dynamics of high area-to-mass ratios GEO space debris by means of the MEGNO indicator

In this paper we provide an extensive analysis of the global dynamics of high-area-to-mass ratios geosynchronous (GEO) space debris, applying a recent technique developed by Cincotta and Simó [Cincotta, P.M., Simó, C.Simple tools to study global dynamics in non-axisymmetric galactic potentials–I. Astron. Astrophys. (147), 205–228, 2000.], Mean Exponential Growth factor of Nearby Orbits (MEGNO), which provides an efficient tool to investigate both regular and chaotic components of the phase space.     

高超声速钝锥体等离子体流场数值模拟

以小钝锥体为对象建立二维几何模型,利用COMSOL Multiphysics软件对等离子体流场控制方程组进行求解,对高超声速气流流过模型所产生的等离子体流场进行数值模拟.仿真得到了在模型头部激波、尾部膨胀波和尾后激波的共同作用下,考虑烧蚀反应时流场的速度、温度、压强和等离子体电子数密度分布,重点分析了钝锥体模型等离子体包覆层和尾后电子分布的特征和成因.可以为高超声速飞行器的探测和控制提供重要的借鉴和参考.