用内文丘里管流量计测量酸气流量

介绍了新型差压装置--内文丘里管的结构、测量原理、技术性能;根据差压式流量计的测量原理,建立了计算酸气流量的数学模型,并将内文丘里管流量计成功地应用于酸气流量的测量.     

一种双斜切双压缩面气道性能的数值模拟

采用LU－SGS隐式推进方法及ROE的通量差分分裂格式，结合带非线性限量因子的MUSCL插值方法编写了雷诺平均的三维N－S方程的数值求解程序，并供助该流场计算程序研究了一种双斜切双压缩面进气道在未经流场控制情况下的流动结构和气动性能（M＝1.9,H=11Km）。计算结果表明：所编制的流场计算程序能够准确快速地求解三维粘性流场，并对流场间断具有较高的分辨率；所研究的进气道即使在未经流场控制的情况下也具有较高的总压恢复系数，这体现了双斜切双压缩面进气道总压恢复系数高的优点，但由于流场中存在分离流动，应采取抽吸附面层等流场控制措施。     

The scientific payload of the space-based Solar and Heliospheric Observatory (SOHO)

The space-based Solar and Heliospheric Observatory (SOHO) is a joint venture of ESA and NASA within the frame of the Solar Terrestrial Science Programme (STSP), the first Cornerstone of ESA's long-term programme Space Science — Horizon 2000. The principal scientific objectives of the SOHO mission are: a) a better understanding of the structure and dynamics of the solar interior using techniques of helioseismology, and b) a better insight into the physical processes that form and heat the Sun's corona, maintain it and give rise to its acceleration into the solar wind. To achieve these goals, SOHO carries a payload consisting of 12 sets of complementary instruments which are briefly described here.     

Dynamic behavior and topology of 3D magnetic fields

We investigate numerically the dynamical evolution of a boundary driven, topologically complex low plasma. The initial state is a simple, but topologically nontrivial 3D magnetic field, and the evolution is driven by forced motions on two opposite boundaries of the computational domain. A large X-type reconnection event with a supersonic one-sided jet occurs as part of a process that brakes down the large scale topology of the initial field. An energetically steady state is reached, with a double arcade overall topology, in which the driving causes continuous creation of small scale thin current sheets at various locations in the arcade structures.     

嵌入式大气数据传感系统压力传感器设计研究

嵌入式大气数据传感(FADS)系统较之传统的大气数据系统有很大的优势,它依靠飞行器前端的压力传感器间接得到飞行大气数据.在本文中,首先简要介绍了FADS系统的压力模型;然后通过分析压力传感器几何外形设计对系统性能的影响,建立了压力传感器的动力学模型,并提出了FADS系统中的压力传感器的设计准则;最后给出了仿真结果.     

毫秒级资料处理的新方法：1991年5月16日2.84GHz太阳资料分析

本文对1991年5月16日事件的资料进行了数据处理,不仅证明毫秒级资料可以通过平均平滑还原为秒级,还表明经1990年修改后的2.84GHz接收机输出的不同时间常数资料内部是自洽的。同时对太阳毫秒级资料作带通滤波将不同时间尺度的快速起伏分离出来。虽然在1991年5月16日的太阳资料中仅能发现亚秒级的起伏,但这种新的资料处理办法对今后的太阳射电快速起伏资料研究与证认是有帮助的。     

One-up on L1: Can X-rays provide longer advanced warning of solar wind flux enhancements than upstream monitors?

Observations of strong solar wind proton flux correlations with ROSAT X-ray rates along with high spectral resolution Chandra observations of X-rays from the dark Moon show that soft X-ray emission mirrors the behavior of the solar wind. In this paper, based on an analysis of an X-ray event observed by XMM-Newton resulting from charge exchange of high charge state solar wind ions and contemporaneous neutral solar wind data, we argue that X-ray observations may be able to provide reliable advance warning, perhaps by as much as half a day, of dramatic increases in solar wind flux at Earth. Like neutral atom imaging, this provides the capability to monitor the solar wind remotely rather than in situ.     

A space radiation shielding model of the Martian radiation environment experiment (MARIE)

The 2001 Mars Odyssey spacecraft was launched towards Mars on April 7, 2001. Onboard the spacecraft is the Martian radiation environment experiment (MARIE), which is designed to measure the background radiation environment due to galactic cosmic rays (GCR) and solar protons in the 20–500 MeV/n energy range. We present an approach for developing a space radiation-shielding model of the spacecraft that includes the MARIE instrument in the current mapping phase orientation. A discussion is presented describing the development and methodology used to construct the shielding model. For a given GCR model environment, using the current MARIE shielding model and the high-energy particle transport codes, dose rate values are compared with MARIE measurements during the early mapping phase in Mars orbit. The results show good agreement between the model calculations and the MARIE measurements as presented for the March 2002 dataset.     

Progress on Solar Physics Research in China

The progress on Chinese Space Solar Telescope (SST) in 2002-2004 is introduced. The documentations on plans and outlines based on the standards of Chinese aerospace industry for SST mission has been fulfilled. The key technical problems of SST satellite platform and payloads are tackled during pre-study stage of the mission. The laboratory assembly and calibration of the main optical telescope of 1.2 m spherical mirror and 1 m plain mirror have been carried out with the accuracy of λ/40 and λ/30, respectively. The prototype at 17.1 nm for extreme ultraviolet telescope is under development and manufacture with a diameter of 13 cm. Its primary and secondary mirrors have a manufacturing error of 5 nm with a roughness degree of less than 0.5 nm and a multiplayer reflection factor of better than 20%. The on-board scientific data processing unit has been developed. Prototypes for other payloads such as H. and white light telescope, wide band spectroscopy in high energy and solar and interplanetary radio spectrometer have been developed accordingly.     

SAR天线功率方向图误差补偿的新方法

首先提出了一种经济而有效的仅改变激励相位的新方法来补偿ＳＡＲ天线功率方向图误差；其次讨论了ＳＡＲ天线在温度载荷作用下的特定的“缓慢变化”的系统变形；然后给出了一些算例以验证方法的有效性；最后给出了一些重要结论。