一种海洋柔性胶囊波能发电装置研究

海洋波浪能可再生能源的开发是未来发展的趋势,开发设计更为高效的波能转换利用装置是开发利用波浪能的关键。根据脉搏脉动机理,设计发明了一种柔性胶囊发电装置,利用柔性结构的强收缩性,让其随着波峰波谷收缩扩张,进而形成脉动来传输水体,使相连尾端竖管内水位随着脉动骤升骤降来压缩排出和快速吸入空气。进行了一系列探索性实验,着重研究柔性材料厚度、波高、周期、气室孔径对该试验装置的波能转换率的影响,数据表明,柔性硅胶管有很好的聚波作用,气室的设计和建造对波能转换效率有较大的影响。     

Hubble Space Telescope observations of magellanic cloud planetary nebulae: Stellar winds

Narrow-band [OIII] 500.7 nm images and ultraviolet spectrophotometry are obtained for 20 planetary nebulae (PNe) in the Magellanic Clouds using the Hubble Space Telescope (HST). Four objects show P Cygni-like features in the ultraviolet HST data, and/or broad emission complexes near the HeII 468.6 nm and CIV 580.6 nm lines in ground-based spectra. All objects are of excitation class four or lower, and all are compact and dense compared to other objects in the sample. The likelihood of detecting ultraviolet P Cygni-like profiles in future HST spectroscopy of other objects is discussed.     

DA型脉动白矮星G255—2的双站联合观测和初步的星震学分析

介绍中法双方分别于１９９５年和１９９７年对ＤＡ型脉动白矮星Ｇ２５５—２进行的两次高精度的光电测光联合观测．在仔细的数据处理之后进行了多重频率脉动分析,得到了该星的本征脉动模式．同时,结合ＤＡ型脉动白矮星的理论模型进行了初步的星震学分析．     

用地磁脉动日食效应探讨甚低纬Pc3-4地磁脉动源

在3次日食期间,利用甚低纬区和从低纬到甚低纬过渡区地面站进行的地磁脉动观测资料,分析了Pc3-4地磁脉动的南北分量（H）和东西分量（D）在H-D平面内矢端图主轴方向的变化．结果表明,当观测点纬度低于日全食带纬度时,H-D矢端图主轴有90°相移现象;当观测点纬度高于日全食带纬度时,则无这种现象．由此我们推测,甚低纬区和从低纬到甚低纬过渡区Pc3-4地磁脉动可能主要是过滤机制产生的．     

运用谱比法计算福建地区观测台网台站响应

场地动力特性对地震造成的破坏有着重要的影响。因此对场地进行动力特性分析,对于地震的监测预报、地震预警、工程抗震设防、地震勘探等具有十分重要的意义。本文主要结合福建地区现有地震观测台网,利用地脉动记录,采用较为简便的谱比方法（Nakamura方法）对福建地区观测台网中台站响应情况进行计算和分析。     

SMALL项目数字化地磁资料可靠性分析

在对中美合作 SMALL (中国低纬地磁台阵 )项目安装在北京地磁台 (白家疃 )和云南通海地磁台的磁通门磁力仪记录资料与磁变仪模拟记录资料进行了详细的对比分析后 ,得出的结果表明 ,两者的日变形态、日变幅有较好的一致性 ,所选特定事件的变化幅度非常一致 ,说明磁通门磁力仪记录到的变化磁场的资料是真实可靠的。尽管目前磁通门磁力仪的基线值存在温度影响和离散度较大的问题 ,但随温度变化有明显的规律性 ,若能采取改进观测条件和观测方法以及缩短观测时间等措施 ,并对基线值进温度校正 ,磁通门磁力仪完全可以提供长期连续可靠的资料。而其为地震预报 ,空间环境预报 ,为日地物理 ,空间物理和地磁学的研究提供的高精度、高分辨率、连续可靠的数字化变化磁场资料是磁变仪模拟记录无法比拟的。     

prior to surface appearance of sunspot flux tubes and magneto-thermal pulsation of the Sun

We found an evidence that the luminosity of the Sun systematically decreased about 20 days before sunspot surface appearance by analysing time-lag correlation of time derivatives of running mean time profiles of the data of the Active Cavity Radiometer Irradiance Monitor (ACRIM) I experiment on board of Solar Maximum Mission (SMM) and of the data of the daily sunspot number. This indicates that sunspot flux tube cooling and heat transport blocking by the flux tubes start to take place in the interior of the solar convection zone well before the sunspot surface appearance. From this finding and our previous finding that the luminosity of the Sun systematically increased and the blocked heat appeared on the surface about 50 days after the sunspot surface appearance, a new view of sunspot formation and dynamics and a new view of the luminosity modulation emerged. (i) Sunspots of a solar cycle are formed from clusters of flux tubes which can be seen in the running mean time profile of the sunspot number as a peak with duration on the order of 100 to 200 days. (ii) Heat flow is blocked by the cluster of sunspot flux tubes inside the convection zone to decrease the luminosity about 20 days before the surface emergence of the sunspot cluster. (iii) The blocked heat appears on the surface about 50 days after the surface emergence of the cluster of sunspot flux tubes to heat up the surface. This appears as a thermal pulse in the running mean time profile of the ACRIM dat in between the peaks of the sunspot running mean time profile. This process of heating the surface makes the temperature gradient less steep and weakens the buoyancy of sunspot flux tubes below the surface. (vi) The radiative cooling of the surface layer by the excess heat release steepens the temperature gradient so that the buoyancy of the sub-surface magnetic flux tubes becomes stronger to cause the next surge of emergence of a cluster of sunspots and other magnetic activities, which creates a peak in the time profile of the sunspot number. We call this peak a magnetic pulse of the Sun and the coupled process of alternating pulsed appearance of heat and sunspots the magneto-thermal pulsation of the Sun.     

丽江地震台新台址勘选

介绍了丽江地震台新台址勘选过程。使用GL-PS2型一体化地震计进行测点勘选工作,计算分析了2021年12月28日13时至30日12时连续48 h内的地脉动速度均方根值(RMS)和噪声功率谱密度,并对该时段内记录到的天然地震事件进行分析。结果表明,记录到的4次天然地震事件震相清晰易识,拟选台址背景噪声达到Ⅰ类台基噪声水平。综合分析认为,该拟选台址观测环境较好,符合地震台建设要求。     

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