比真空更隔热的装置

<正>由于热物体会向周围空间辐射热量,因此人们都认为真空环境更能减少传导。然而美国斯坦福大学的范汕洄(Shanhui Fan)和同事发现真空环境并不能隔热,因为真空中还是有物质的。     

Study of lower emittance dedicated synchrotron radiation mode for the BEPCⅡ

In this paper,a dedicated synchrotron radiation （SR） mode for the BEPCⅡ with an emittance of 85 nm has been designed,including the linear lattice,chromaticity correction and dynamic aperture optimization.The emittance of the new mode is about 60% of the previous mode used for routine operation of the BEPCⅡ .The effect of wigglers on the linear lattice was compensated and the total dynamic aperture including the wigglers’ nonlinear effect was estimated.The preliminary commissioning at the end of 2008 and the formal operation with the new mode confirmed its merits.     

大气模式与气溶胶模型对辐射传输计算的影响

大气模式与气溶胶模型选择是影响定量遥感应用的辐射传输计算的重要因素。人们一般凭感性认识去进行选择,有一定随意性,对其带来的影响程度关注甚少。以太阳辐射计测量为依据,对大气模式与气溶胶模型选择方法作了研究,并利用经辐射定标过的光谱辐射计地面测量对辐射传输计算精度进行了验证。在昆明进行的试验表明,在0.50~0.68μm范围内,选择中纬度冬季大气模式和大陆型气溶胶,经辐射传输计算后得到的光谱辐射亮度与光谱辐射计测量结果一致性很好,差别在3.3%以内;变换大气模式对辐射传输计算产生明显影响,差别达10%左右;选择不同的气溶胶模型对辐射传输计算影响也很大,差别达11%左右。基于辐射计测量的大气模式与气溶胶模型选择避免了主观选择的不可靠性,有益于减少辐射传输计算或卫星遥感大气订正的误差。     

《相对论、宇宙与时空》连载⑧——相对论预言的天体(黑洞)(下)

5 黑洞热力学 人们认为激发态的黑洞具有生命力,而基态的黑洞则是一颗死亡的星,是恒星演化的最后归宿.基态的史瓦西黑洞除去能不断吞食物质外,不会再有任何物理过程.然而,这个认识很快就被推翻了,基态的黑洞,实际上也是一颗充满生命力的活跃的星.我们先看一下黑洞的"无毛定理"和"面积定理"[3-14].     

Ultra-high energy cosmic rays threshold in Randers-Finsler space

Kinematics in Finsler space is used to study the propagation of ultra high energy cosmic rays particles through the cosmic microwave background radiation. We find that the GZK threshold is lifted dramatically in Randers-Finsler space. A tiny deformation of spacetime from Minkowskian to Finslerian allows more ultra-high energy cosmic rays particles to arrive at the earth. It is suggested that the lower bound of particle mass is related with the negative second invariant speed in Randers-Finsler space.     

Hawking Radiation from Plane Symmetric Black Hole Covariant Anomaly

Based on the covariant anomaly cancellation method, which is believed to be more refined than the initial approach of Robinson and Wilczek, we discuss Hawking radiation from the plane symmetric black hole. The result shows that Hawking radiation from the non-spherical symmetric black holes also can be derived from the viewpoint of anomaly.     

A Simple Model for Ignition of Magnetized Target Fusion

A simple model for magnetized target fusion is proposed. Self-consistent equations are made as equivalent circuit is included. Ignition conditions and physical process are analyzed with practical parameters. It is shown that system temperature rises as external work is equal to or greater than the loss of Bremsstrahlung, and ignition of target happens as thermonuclear reaction energy is equal to or greater than the radiation loss from the target.     

电磁激励器屏幕发声系统的数理模型

目前,全面屏手机已经成为一种趋势。为提升全面屏的用户体验效果,业界开发了屏下指纹识别、伸缩式摄像头等技术,对于音频(主要是语音通话),则开发了基于压电陶瓷和电磁激励器的两种屏幕发声方案,其代表产品分别为小米MIX与VIVO NEX。该文针对电磁激励器屏幕发声技术,分别从平板弯曲振动、平板声辐射、电磁激励器阵列驱动等模型出发,推导电磁激励器驱动屏幕振动发声的原理以及简化的力电类比等效线路图;给出仿真与实测频响曲线以及某型号手机语音通话测试数据;最后简要归纳电磁激励器屏幕发声的设计指南以及进一步的研究方向。     

双球聚集粒子辐射特性分析

基于广义Mie理论求解方法(GMM),考虑单元粒子之间的相互作用,计算了不同尺度参数不同间距的双球聚集粒子的衰减因子、散射因子等辐射特性参数,同时分析了双球聚集粒子与不考虑相互作用计算所得的辐射特性差异,分析结果表明:考虑相互作用与不考虑相互作用计算所得的双球聚集粒子的辐射特性存在着一定的差别,这种差别随粒子间距、尺度参数的变化而变化,最大偏差达30%左右.