最新高性能中速走丝电火花数控线切割机床

<正>秉承苏州三光精心制造的传统,苏州三光科技股份有限公司的产品始终将产品性能、可靠性放在首位。随着高品质产品所带来的市场高认可度,苏州三光的产品走进了越来越多的工厂和车间。同时,市场对高性     

Advanced detectors and instruments for small satellites

This paper presents some approaches to the development of advanced detectors and to miniaturized instrument design which are pursued in the Institute of Space Sensor Technology of DLR (the German Aerospace Research Establishment). The instrument design approach is demonstrated for a low-weight (3 kg) dual camera system with narrow-angle in-track stereo and wide-angle multispectral features. Each camera has its own signal processor and 0,5 G Bit mass memory. The activities for advanced detector development are concentrated on two different kinds of detectors and instrumentations: infrared detector arrays and instruments at wavelengths out to about 240 μm, and superheterodyne receivers in the submillimeter and far-infrared spectral ranges.     

Ma5斜激波串动态特性实验研究

为加深对激波串动态特性的认识,进行了简单管道模型在Ma风洞中的实验研究,探讨了两种不同背压变化条件下斜激波串的流动结构和动态特性。背压的生成和控制通过模型尾部两块斜板的闭合运动实现。为了更好观察实验现象,实验过程中动态压力传感器和高速纹影实行同步采集。研究发现:随着背压升高,激波串逐渐前移,由对称形态发展为非对称形态,并持续整个移动过程。背压增加的速度对激波串前缘的前移速度没有影响。激波串在管道内的前移过程并不是一个恒定运动过程,而是存在有稳定前移和急剧前移两种状态,其特性与管道内流场结构、壁面压强分布、背压大小以及距离管道出口的距离等因素相关。在不同的背压条件下,管道内的斜激波串表现出不同的频谱特征,但在同一工况中,激波串区域内不同位置处壁面压强的频谱特性相似。在Case 1状态中,压强振荡主频为f512Hz在Case 2状态中,振荡主频为f578Hz次级频率约为f260Hz。两次实验的主频均大于Pipon.niau模型理论计算值,而Case 2中频率f和声学振荡频率相近。     

CFD数据交易标准及其软件实现

论述推行统一的CFD数据交换标准的必要性 ;报告在研制通用航空气动力数值模拟系统ANSS2 0 0 0过程中 ,建立内部数据接口文件规范的尝试 ;推荐国际上主流的空气动力学和CFD数据库标准———CGNS ;讨论CGNS在ANSS2 0 0 0中的实现 ;大力呼吁同步使用与国际接轨的CFD数据交换标准。     

EUVITA — An extreme UV imaging telescope array with spectral capability

EUVITA is a set of 8 extreme UV normal incidence imaging telescopes, each of them sensitive in a narrow band (λ/Δλ = 15 to 80), centered at wavelengths between 50 and 175 Å. Each telescope has an effective area of a few cm²; a field of view of 1.2° and a spatial resolution of 10 arcsec.

EUVITA will be flown on the Russian mission SPECTRUM X-G. This satellite will be launched in a highly eccentric orbit with a period of 4 days, allowing long, uninterrupted observations (e.g. 10⁵ seconds). EUVITA's narrow spectral bands allow the measurement of source parameters such as temperature or power law index as well as interstellar absorption, and will resolve groups of strong lines emitted by optically thin hot plasmas.     

Observations of stars with the Hopkins Ultraviolet Telescope

The Hopkins Ultraviolet Telescope (HUT) was flown aboard the space shuttle Columbia as part of the Astro-1 mission during December 1990. During the nine-day flight, HUT carried out 3 Å resolution spectrophotometry of a wide variety of astronomical objects, including a number of stellar targets, in the 912–1860 Å range of the far ultraviolet. A few nearby stars were observed in the 415–912 Å range of the extreme ultraviolet as well. For nearly all of these targets, the spectra obtained by HUT are the first ever obtained in the spectroscopically rich region between Lyman (1216 Å) and the Lyman limit (912 Å). Here, we present highlights of the results obtained by HUT in a variety of areas of stellar astronomy.     

Periodic components in Cyg X-3

Hard X-ray observations of Cyg X-3 in the energy range 20–100 keV were made with a Balloon-borne telescope using two large area proportional counters. The source was seen with a total significance of 20.

A 121 s periodicity was seen during Fourier analysis of the data. The phenomenon can be interpreted as due to transient pulsation since no other peak was seen in our data. Quasi-periodic oscillation in the range 0.06–20 mHz have been observed from Cyg X-3 at lower energies. Interestingly, most of the reported periods are multiple of the present measurements. The observed pulsation at high energies indicate the occasional unstable behaviour of the inner parts of the accretion disk connected with the basic rotation period of the compact object.

The 4.8^h modulation, characteristic of the orbital period of the binary system was seen in the data, with a broad maximum between the phase 0.3 to 0.7.     

SPOT-2 and TOPEX/Poseidon precise orbit determination from DORIS doppler tracking

The French earth observation satellite SPOT-2 has served as a testbed for precise orbit determination from DORIS doppler tracking in anticipation of the TOPEX/Poseidon mission. Using the most up-to-data gravity field model, JGM-2, a radial orbit accuracy of about 2–9 cm was achieved, with an rms of fit of the tracking data of about 0.64 mm/s. Furthermore, it was found that the coordinates of the ground stations can be determined with an accuracy of the order of 2–5 cm after removal of common rotations, and translations.

Using a slightly different model for atmospheric drag, but the same gravity model, precise orbits of TOPEX/Poseidon from DORIS tracking data were determined with a radial orbit accuracy of the order of 4–5 cm, which is far within the 13 cm mission requirement. This conclusion is based on the analysis of 1-day overlap of successive 11-day orbits, and the comparisons with orbits computed from satellite laser tracking (SLR) and from the combination of SLR and DORIS tracking. Results indicate a consistency between the different orbits of 1–4 cm, 4–20 cm, and 6–13 cm in the radial, cross-track, and along-track directions, respectively. The residual rms is about 4–5 cm for SLR data and 0.56 mm/s for DORIS tracking. These numbers are roughly twice as large as the system noise levels, reflecting the fact that there are still some modeling errors left.     

Solar-proton polar-cap intensity structures as a test of magnetic field models

The entry of energetic solar protons to the polar caps offers an interesting way to test models of the geomagnetic field. In this brief report, we present a comparison between SAMPEX observations of solar-particle intensity structure during a polar cap traversal with numerical trajectory calculations using the IGRF + T96 field model.     

认知风格理论对外语教与学的启示

认知风格是学习者习惯性的认知特点,它相对固定。不同学习者往往具有不同的认知特点。在二语习得理论中,认知风格被视为学习者个体内在因素之一。研究认知风格对于教与学都具有重要的意义。