HELIO: The Heliophysics Integrated Observatory

Heliophysics is a new research field that explores the Sun–Solar System Connection; it requires the joint exploitation of solar, heliospheric, magnetospheric and ionospheric observations.     

SEP events and multi-spacecraft observations: Constraints on theory

Fifteen solar energetic particle (SEP) events have been analyzed using proton flux data recorded by the Helios 1, Helios 2, and IMP 8 spacecraft in the energy range ∼4–40 MeV during 1974–1982. For each of the events at least two of the spacecraft have their nominal magnetic footpoint within 20° in heliocentric longitude from each other. The SEP events are sub-grouped as a function of their heliocentric longitudinal separation and heliocentric radial distance from the SEP associated solar flare and several case studies are presented in this paper. Main results concerning their usage in estimating the SEP radial dependence are given. Moreover, we investigate the behavior of the third not connected spacecraft in order to study the dependence of the proton flux as a function of flare location. It is found that the contribution of the longitudinal gradient in determining variations in the SEP proton flux is particularly relevant for spacecraft having their magnetic connection footpoint separated from the flare between 30° and 50°.     

Ionospheric heating due to solar flares as measured by SROSS-C2 satellite

The data on thermal fluctuations of the topside ionosphere have been measured by Retarding Potential Analyser (RPA) payload aboard the SROSS-C2 satellite over the Indian region for half of the solar cycle (1995–2000). The data on solar flare has been obtained from National Geophysical Data Center (NGDC) Boulder, Colorado (USA) and other solar indices (solar radio flux and sunspot number) were download from NGDC website. The ionospheric electron and ion temperatures show a consistent enhancement during the solar flares. The enhancement in the electron temperature is 28–92% and for ion temperature it is 18–39% compared to the normal day’s average temperature. The enhancement of ionospheric temperatures due to solar flares is correlated with the variation of sunspot and solar radio flux (F10.7cm). All the events studied in the present paper fall in the category of subflare with almost same intensity. The ionospheric electron and ion temperatures enhancement have been compared with the IRI model values.     

基于对应直线的飞行器接近角估计

提出了一种新的基于对应直线估计飞行器接近角的方法,对线性方法作归一化变换以提高算法的鲁棒性。用至少4组对应直线计算两图像间的单应矩阵。用序列图像间的单应矩阵估计接近角,无需着陆目标已知。模拟实验验证了算法的可行性。     

单站无源定位中角度变化率的测量方法研究

讨论了单站无源定位中角度变化率测量的问题.首先简要介绍了差分法、最小二乘拟合法和卡尔曼滤波法的测量原理,其次为了解决滤波模型非线性的影响,提出了一种并行分段处理的卡尔曼滤波方法,最后从数字滤波的角度,通过设计相应的低通滤波器对估计获得的角度变化率数据流进行处理,进一步提高了角度变化率的测量精度.仿真实验对比分析了所述几...     

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.     

带控制律CTS试验的实现

FL24风洞在国内首次进行了带控制律的CTS试验,这是改进捕获轨迹试验方式的一次探索。文中对国内外研究现状、试验技术原理、实现过程进行了阐述。试验结果表明在加控制律的CTS试验中导弹的滚转角和偏航角输出趋稳,呈有控状态。     

大迎角体涡,翼涡干扰的Euler方程数值模拟

本文用Ｅｕｌｅｒ方程的简化区算法计算翼－身组合体绕流。当大迎角时，计算能自动捕捉到大后掠前缘的分离涡，机射的分离涡由强加Ｋｕｔｔａ条件生成，形成体涡与翼涡的相互干拢。本文对加长前机身的ＡＧＡＲＤ－Ｂ翼－射组合体模型，给出机射有分离和无分离时，横流截面的速度矢量分布、法向力和压力中心，分析体涡的影响。     

论"中部崛起"的七大关系

从地理学的空间视角对新时期中部崛起的重大理论进行初步探讨，在研究中部地区经济与社会发展情况的基础上，重点探讨了中部六省发展过程中应当注意的七大关系：内生性发展与外生性发展、工业化与城市化、比较优势与竞争优势、乡村城市化与异地城市化、城市用地扩张与农村耕地保护、行政区经济与经济区经济、经济增长与建设和谐社会，最后提出了中部地区应注重“内力”培养，因地制宜地推动城市化进程，大力发展经济区经济，以及对社会问题保持高度敏感等政策建议。     

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.