探月回顾

1958年-1976年美国与前苏联一共发射了83个无人月球探测器。 1969年“阿波罗11号”实现了人类登月之梦，在月球探测中取得最辉煌成果。这一年，先后有12名宇航员踏上月球，并向地面带回440kg的月岩样品。     

撞月——再现人造太空奇观

2005年7月,美国航天局在太空导演了一出绚丽壮观、完美无缺的“焰火”大戏:“深度撞击”,探测器极其精确(误差仅1米)地击中了坦普尔-1彗星,成功地在太空进行了首场人工撞击“表演”。时隔一年,美国航天局在近日又公布了一项撞击月球南极的计划,定名为“积极接触月球表面”,目的是希望能成功找到月球存在水的证据。根据计划要求,2009年1月人类将上演撞击星体(月球)的第二场大戏!到时在月球南极表面会有大约1000吨月面尘埃和碎片冲向64千米的高空,在月面上撞出一个直径30米、深4.5米,有1/3个足球场大小的巨型坑,人们在地球上借助望远镜就能观…     

太空中的引力波探测器

欧洲和美国的科学家正致力于建造LISA——空间三角形探测器,用它来倾听黑洞相遇时的喃喃低语。 发射三个绕太阳公转的探测器,并且将它们置于     

Design of a CMOS Adaptive Charge Pump with Dynamic Current Matching

A novel structure for a charge pump circuit is proposed, in which the charge-pump （CP） current can adaptively regulated according to phase-locked loops （PLL） frequency synthesis demand. The current follow technology is used to make perfect current matching characteristics, and the two differential inverters are implanted to increase the speed of charge pump and decrease output spur due to theory of low voltage difference signal. Simulation results, with 1st silicon 0. 25μm 2. 5 V complementary metal-oxide-semiconductor （CMOS） mixed-signal process, show the good current matching characteristics regardless of the charge pump output voltages.     

碘化汞室温X射线探测器的研制

碘化汞室温Ｘ射线探测器的研制李正辉，邹联隆，曹瑞钦，李伟堂（材料科学系）自本世纪７０年代初Ｗｉｌｌｉｎｇ等首先用碘化汞（ＨｇＩ２）晶体制成室温半导体核辐射探测器［１］以来，该晶体在生长和应用等方面都取得了很大的进展［２～４］．由于ＨｇＩ２晶体有效原子...     

土卫七上可能有生命

天学家发现，距离土星第七远的土星卫星——恩克拉多斯上面可能存在生命。早在两年前，“卡西尼号”探测器就发现这颗土卫（土星卫星）上有蒸气喷出。现在又发现，这些喷气中富含氮气。这暗示恩克拉多斯的内核温度达到了，577℃，从而将内核中的氨转化成了氮。在这一温度条件下，同样能制造构筑生命的材料。2008年，“卡西尼号”将飞进恩克拉多斯的喷气中寻找答案。     

浅谈感烟探测器在智能建筑消防系统中的应用

在火灾的最早期,烟雾是其最主要特征,此时几乎没有火焰辐射。感烟探测器就是探测火灾早期产生的烟雾,并且向火灾报警控制器发出报警信号的一种探测装置。它具有发现早,响应快的特点,有利于火灾扑救的特点。因此,在建筑消防工程中,它是应用最为广泛的一种探测装置。按照工作原理的不同,主要分为离子型和光电型。     

西藏高原环境下点式感烟火灾探测器的灵敏度

为研究西藏高原低压低氧环境下烟雾浓度和点式感烟火灾探测器灵敏度的变化,在拉萨和合肥两地标准实验间中,进行国家标准试验火正庚烷火和棉绳阴燃火实验,并对烟雾浓度进行了模拟.研究发现烟雾浓度主要受燃烧质量损失速率的影响,而在拉萨和合肥相同质量损失速率实验产生烟雾浓度近似相等;高原环境对点型散射式光电感烟火灾探测器灵敏度影响较大,对点型离子感烟火灾探测器灵敏度影响不明显.     

Energetic particle radiations measured by particle detector on board CBERS-1 satellite

Using the data measured by energetic particle detector on board CBERS-01 and -02 for the past five years, statistics was made to show the general features of MeV electrons and protons along a solar synchronous orbit at an altitude of 780 km. This height is in the bottom region of the Earth's radiation belts. Detectors are inside the satellite cabinet and such continuous monitoring of particle radiation environment inside a satellite has seldom conducted so far. After a proper and careful treatment, it is indicated that the data inside satellite are well correlated with the radiation environment outside. Be-sides the agreement of the general distribution characteristics of energetic electrons and protons with similar observations from other satellites, attention is particularly paid to the disturbed conditions. Variations of particle fluxes are closely related with solar proton events, in general, electron fluxes of outer belt are well correlated with Dst index after three days' delay while the electron injection occurred almost at the same day during great magnetic storms. It is confirmed that both energetic electrons and protons appear in the Polar Cap region only after the solar proton events.