Coronal radio-sounding detection of a CME during the 1997 Galileo solar conjunction

Frequency fluctuations of the Galileo S-band radio signal were recorded nearly continuously during the spacecraft’s solar conjunction from December 1996 to February 1997. A strong propagating disturbance, most probably associated with a coronal mass ejection (CME), was detected on 7 February when the radio ray path proximate point was on the west solar limb at about 54 solar radii from the Sun. The CME passage through the line of sight is characterized by a significant increase in the fluctuation intensity of the recorded frequency and by an increase in the plasma speed from about 234 km s⁻¹ up to about 755 km s⁻¹. These velocity estimates are obtained from a correlation analysis of frequency fluctuations recorded simultaneously at two widely-separated ground stations. The density turbulence power spectrum is found to steepen behind the CME front. The Galileo radio-sounding data are compared with SOHO/LASCO observations of the CME in the corona and with WIND spacecraft data near the Earth’s orbit.     

Interplanetary Physics Research in China:2006—2008

This brief report summarized the latest advances of the interplanetary physics research in China during the period of 2006—2007,made independently by Chinese space physicists and through international collaboration.The report covers all aspects of the interplanetary physics,including theoretical studies,numerical simulation and data analysis.     

弹射筒内筒组件钢球收压及检测工艺

本文对航空火箭弹射座椅弹射筒内筒钢球收压技术要求、难点进行了工艺分析;介绍了钢球收压工艺技术难点、检测方法及注意事项等,在工艺技术研究及设计过程中取得了一定的技术积累,具有良好的借鉴、推广应用意义。     

The Role of Magnetic Reconnection in CME Acceleration

Observations carried out from the coronagraphs on board space missions (LASCO/SOHO, Solar Maximum and Skylab) and ground-based facilities (HAO/Mauna Loa Observatory) show that coronal mass ejections (CMEs) can be classified into two classes based on their kinematics evolution. These two classes of CMEs are so-called fast and slow CMEs. The fast CME starts with a high initial speed that remains more or less constant; it is also called the constant-speed CME. On the other hand, the slow CME starts with a low initial speed, but shows a gradual acceleration; it is also called the accelerated and slow CME. Low and Zhang [Astrophys. J. 564, L53–L56, 2002] suggested that these two classes of CMEs could be a result of a difference in the initial topology of the magnetic fields associated with the underlying quiescent prominences. A normal prominence magnetic field topology will lead to a fast CME, while an inverse quiescent prominence results in a slow CME, because of the nature of the magnetic reconnection processes. In a recent study given by Wu et al. [Solar Phys. 225, 157–175, 2004], it was shown that an inverse quiescent prominence magnetic topology also could produce a fast CME. In this study, we perform a numerical MHD simulation for CMEs occurring in both normal and inverse quiescent prominence magnetic topology. This study demonstrates three major physical processes responsible for destabilization of these two types of prominence magnetic field topologies that can launch CMEs. These three initiation processes are identical to those used by Wu et al. [Solar Phys. 225, 157–175, 2004]. The simulations show that both fast and slow CMEs can be initiated from these two different types of magnetic topologies. However, the normal quiescent prominence magnetic topology does show the possibility for launching a reconnection island (or secondary O-line) that might be thought of as a “CME’’.     

高速弹射试验机操稳性能的计算与试飞

本文介绍了为研究高速弹射试验机的操稳性能和在弹射力扰动下飞机的动态响应,把弹射力以瞬态脉冲载荷的形式作用于飞机时所建立的数学模型和采用的计算方法.把计算结果与试飞结果和原型机试飞结果作了比较,计算结果与试飞结果的一致性是令人满意的。这为高速弹射试验机的安全飞行和指导飞行员实施弹射试验提供了可靠的依据。     

一种运载火箭用大功率电动伺服驱动器的散热设计

散热对电子设备的性能有着直接的影响,散热器广泛应用于电子产品的热设计用于改善其散热能力,因此散热器应作为关键部件进行设计。针对航天领域使用的大功率电动伺服驱动器的散热问题,提出了通过热力学理论计算指导散热器结构设计的方法。首先通过理论计算结果确定散热器的结构尺寸,然后通过PRO/E三维建模软件对散热器进行建模并利用ANYSY ICEPAK热仿真软件对所设计的散热器进行热仿真,最后搭建了伺服驱动器的热试验环境。仿真结果和试验数据均验证了该设计方法的正确性。     

气流吹袭时飞行员手臂的受力分析

总结了测量作用在手臂上的气动力的实验结果.。这些实验是用风洞、火箭车和空中弹射进行的。用6名男青年、橡胶假人、1/2人体木模型和1/10人体钢模型,在Ma=0.086～2.04范围内,测量了作用在手臂上的气流解脱力。用这些实验数据,计算出了气流产生的手臂解脱力系数,并推导出这些系数与Ma数之间的关系式,为进一步推导飞行员手臂对气流吹袭的耐力提供了气动力数据。     

高速气流吹袭问题

在高速弹射时,防护气流吹袭对人体产生的损伤目前仍未有令人满意的方法。本文阐述了高速气流吹袭对人体的致伤机理并提供了头及四肢的防护约束方程组。     

两冕流间的对称径向膨胀日冕物质抛射事件

本文讨论了发生在冕流对之间的1980年5月6日日冕物质抛射事件。提出了一种描述事件外环运动的经验模型,把环的观测外形表达为在运动坐标系中的Cassini函数。环的发展过程分为两个阶段:在前一阶段,外环处于冕流对盔状结构之间,事件的发展以角宽度膨胀为主,其对称轴从赤道向北纬方向移动;径向膨胀和上升速度较低,加速效应明显。在后一阶段,外环越过冕流盔状结构所在高度,角膨胀趋于停止;运动接近于等角宽度和纯径向匀速的膨胀和上升运动。当外环向外运动时,其顶部和几何中心的高度均随时间而增加,但其底部高度基本上保持不变。根据上述观测特征,讨论了事件形成的可能机制。