神舟飞船生长GaMnSb材料过程及性能分析

利用神舟3号飞船(SZ-3)上的多样品空间晶体炉制备出GaMnSb材料．所设计的石英安瓿使用氧化铝棉毡和特殊设计制造的氮化硼坩锅进行减震，经受住了严峻的力学环境的考验，完成了材料的空间生长实验，达到了空间生长材料的初步要求．对空间生长的GaMnSb晶体进行了X射线能谱分析和X射线衍射分析，发现空间生长的GaMnSb是多晶结构．对未获得GaMnSb单晶的原因进行了分析，发现空间晶体炉温度的波动和提供能量的不足是导致生成GaMnSb多晶结构的主要原因．由于在晶体生长的初始阶段晶体炉提供的能量不足，使GaSb单晶部分未能熔化，从而导致GaMnSb材料的生长在没有籽晶的情况下进行．     

Magnetic storm cessation during sustained northward IMF

Times of sustained strong northward IMF can interrupt the magnetic storm development and lead to lower levels of geomagnetic activity for many hours. During 1997–2000 we have found two events of this kind observed on November 8, 1998 and October 13, 2000. In both cases, the storms started as usual after arrival of ejecta with a southward IMF component from the Sun to the Earth, but ceased after several hours due to the onset of sustained northward IMF leading to the faster recovery process. After the passage of this so-called positive domain, the storm development started again. The heliospheric magnetic field intensity remained enhanced and nearly constant. The solar origins of the geomagnetic storm interruptions have been investigated. Tentatively they may be related to strong nonlinear Alfvйn type solitary waves excited by non-stationary coronal current variations with a characteristic time-scale of about a day.     

高频角振动台中某些特殊问题的研究

以最近研制成功的一种高频角振动台为例，详细阐述了这种台子的执行元件、驱动电路和控制系统的特殊问题和解决方法。提出了可供实用的陀螺测试方法。     

Chromospheric dynamics

This review focuses on dynamics of the solar chromosphere, which serves as a good proxy for understanding processes in stellar chromospheres as well. In the quiet chromosphere it is useful to distinguish between the magnetic network on the boundaries of supergranulation cells, where strong magnetic fields are organized in mainly vertical magnetic flux tubes, and internetwork regions in the cell interior, where magnetic fields are weaker and dynamically less important. Recently, some progress has been made in understanding the physics of the non-magnetic chromosphere. On the other hand, the physical processes that heat the magnetic network have not been fully identified. Is the network heated by wave dissipation and if so, what are their physical characteristics? These and other aspects relating to the dynamics and energy transport mechanisms will be discussed in detail. In addition, some of the outstanding problems in the field such the driving mechanism for spicules and the nature of internetwork magnetic fields will also be highlighted. Furthermore, a critical assessment will be made on the challenges facing theory and the direction for future investigations, particularly in the light of the new space experiments, will be highlighted.     

一种恒跨导轨对轨输入级运算放大器的设计

提出了一种恒跨导轨对轨输入级的结构,从理论上详细分析了这种结构的可行性和优越性,在输入MOS差分对管处于强反型区和弱反型区时,它都能提供几乎不变的跨导,且采用0.6μmCMOS工艺对这种运算放大器进行了模拟仿真,其结果与理论值很相符合。     

Low-latitude geomagnetic response to the interplanetary conditions during very intense magnetic storms

The variations in the horizontal and declination components of the geomagnetic field in response to the interplanetary shocks driven by fast halo coronal mass ejections, fast solar wind streams from the coronal hole regions and the dynamic pressure pulses associated with these events are studied. Close association between the field-aligned current density (j_∥) and the fluctuations in the declination component (ΔD_ABG) at Alibag is found for intense storm conditions. Increase in the dawn-dusk interplanetary electric field (E_y) and ΔD_ABG are generally in phase. However, when the magnetospheric electric field is directed from dusk to dawn direction, a prominent scatter occurs between the two. It is suggested that low-latitude ground magnetic data may serve as a proxy for the interplanetary conditions in the solar wind.     

帕金森大鼠模型的影像特性

利用影像技术对帕金森病（Parkinsondisease，PD）大鼠模型的脑形态与功能信息进行了系统研究。利用磁共振（Magneticresonance imaging。MRI）及磁共振血管成像（Magneticresonanceangiography，MRA）获取PD大鼠脑部形态影像资料，利用质子磁共振波谱（1H—magneticreso—nancespectroscopy，1H—MRS）及CT灌注（CTperfusion，CTP）成像获取波谱及血流变化等功能影像学资料。研究结果表明PD大鼠在形态上影像无特征性异常，在功能影像学纹状体存在局部脑血流降低和波谱变化。     

Preliminary Study on Magnetic Induction Intensity Induced by Plasma During Hypervelocity Impact

An experimental system has been built to produce and measure the magnetic field in the backward ejected matter during hypervelocity impact. The designs of measurement system and coil, the choice of associated equipment, and the system calibration are also described in detail. The measurement of magnetic induction intensity for different given coil positions and azimuth angles are performed with two-stage light-gas gun. On condition that impact velocities are approximately equal and incidence angles are 45°, 60° and 90° respectively, the relationship between average magnetic induction intensity and impact angle at different time spans is obtained. Experimental results show that the average magnetic induction intensity with incidence angle of 90° is larger than those with incidence angles of 45°and 60°.     

The detection of “magnetic element” – Why we need a one-meter Space Solar Telescope

The nature of a magnetic element, the elemental structure of the solar magnetic field, is one of the most important mysteries in solar physics. In this paper, we will discuss the requirements of magnetic element detection, such as spatial resolution and magnetic sensitivity. By these discussions, we conclude that it is almost impossible to detect magnetic element with currently used ground-based telescopes and techniques. The proposed Space Solar Telescope, a one-meter Chinese space project, can match these requirements.     

低噪声放大器输入阻抗匹配网络设计优化方法(英文)

通过分析电路的最佳噪声匹配和最佳功率匹配,研究了根据给定的输入反射系数(S11)计算低噪声放大器(LNA)最佳源阻抗的方法。借助史密斯圆图给出了详细的计算过程,实现了LNA输入匹配网络设计时的最佳噪声和最佳功率之间的折衷匹配。基于Chart0.35-μmCMOS工艺完成了一种cascode结构LNA的核心电路设计,仿真和实验结果与理论分析相吻,表明了理论分析的正确性和方法的可行性。