日冕物质抛射的观测性质

综述日冕物质抛射的观测和持性，简短的前言之后，给出ＣＭＥ的发现经过及统计特性，着重介绍ＣＭＥ与其他种类太阳活动的相关。然后介绍ＣＭＥ的一般特性，包括可能与ＣＭＥ相关的一些物理过程的观测特性。初步结论是：ＣＭＥ是一种演变中的磁结构现象。     

Solar radiative output and its variability: evidence and mechanisms

Electromagnetic radiation from the Sun is Earths primary energy source. Space-based radiometric measurements in the past two decades have begun to establish the nature, magnitude and origins of its variability. An 11-year cycle with peak-to-peak amplitude of order 0.1 % is now well established in recent total solar irradiance observations, as are larger variations of order 0.2 % associated with the Suns 27-day rotation period. The ultraviolet, visible and infrared spectral regions all participate in these variations, with larger changes at shorter wavelengths. Linkages of solar radiative output variations with solar magnetism are clearly identified. Active regions alter the local radiance, and their wavelength-dependent contrasts relative to the quiet Sun control the relative spectrum of irradiance variability. Solar radiative output also responds to sub-surface convection and to eruptive events on the Sun. On the shortest time scales, total irradiance exhibits five minute fluctuations of amplitude %, and can increase to as much as 0.015 % during the very largest solar flares. Unknown is whether multi-decadal changes in solar activity produce longer-term irradiance variations larger than observed thus far in the contemporary epoch. Empirical associations with solar activity proxies suggest reduced total solar irradiance during the anomalously low activity in the seventeenth century Maunder Minimum relative to the present. Uncertainties in understanding the physical relationships between direct magnetic modulation of solar radiative output and heliospheric modulation of cosmogenic proxies preclude definitive historical irradiance estimates, as yet.Received: 26 August 2004, Published online: 16 November 2004 Correspondence to: Claus Fröhlich     

边坡虹吸排水管内空气积累原因及应对措施

坡体地下水位上升是诱发滑坡的重要因素,实时排出地下水是防治边坡地质灾害的有效手段。虹吸排水具有免动力和流动过程由液位变化自动控制的物理特性,可满足实时排出坡体地下水的需要,但虹吸管中空气积累会导致虹吸过程中断,制约了边坡虹吸排水技术的推广应用。溶解于水的空气因虹吸管内压力降低而释出是形成气泡的物理基础。实验结果表明,虹吸进水口水面以上垂直高度3.5 m以上就会出现大量气泡,经过虹吸顶点后,气泡发生强烈的兼并形成大气泡。当虹吸管的进出水口的水头差较大时,气泡间的水弹容易推动气泡从出水口排出。当虹吸管直径大于5 mm时,缓慢的虹吸流动,会发生管内气泡的积累,最终破坏虹吸过程;虹吸管的直径小于4 mm时,可以形成基本稳定的弹状流。因此,为保持边坡虹吸过程长期有效,经常性降雨并且坡体地下水丰富的地区可选用直径为5 mm的虹吸管,非经常性降雨的地区应选择小于等于4 mm的虹吸管。     

小口径加筋砼灌注桩应用初探

在小口径加筋砼灌注桩试桩基础上结合工程实例对小口径加筋砼灌注桩的设计、施工和检测进行了初步探讨     

浅谈超声波透射法在灌注桩检测中的应用

目前国内外对于钻孔灌注桩水下混凝土质量检测的方法很多,如低应变反射波法、高应变动测法、单桩竖向静载抗压试验、钻芯法、超声波透射法等,每种检测方法都有它的适用范围和局限性。超声波透射法与其他检测法相比,该方法检测精度高,结果直观可靠,适合大直径桩、超长桩的基桩检测,故在钻孔灌注桩的完整性检测中,得到了广泛的运用,尤其在桥梁灌注桩中,超长、大直径桩几乎都采用了超声波透射法检测。本文对某工地大直径桩进行了超声波透射法检测,通过波形与照片对比,更好地验证了超声波透射法测试超长、大直径取得的效果。     

太阳射电爆发中Spike辐射的准周期振荡

本文介绍了在1981年5月16日微波大爆发中毫秒级时间轮廓Spike辐射中发生的准周期振荡现象。这种准周期振荡可能与日面活动区磁杯中的阿尔芬波运动有关,由此我们可以得到爆发源区一些基本物理条件。最后对于准周期振荡现象对Spike辐射的作用和影响作了简单的讨论。     

微波爆发区的日冕磁场研究

回顾了日冕磁的研究历史,介绍了我们首镒提出的日冕磁场的微波诊断方法及其应用的带来的启迪,提出进一步开展日冕磁场及其相关研究的建议。