MEASUREMENTS AND MODEL SIMULATIONS OF SURFACE OZONE VARIATIONS AT DIFFERENT BACKGROUND CONCENTRATIONS OF THE PRECURSORS

Ozone photochemical production and loss in very different environments at Waliguan baselinestation and Lin'an background station were simulated by using the measurement data and photo-chemical box model.The results show that net ozone photochemical production rate is negative,about 0.5 ppb/d,at Waliguan baseline sation,because of very low precursor concentrations.Butat Lin'an background station,the net photochemical ozone production is positive,about 2—3 ppb/h.which is very closed with the measurement at Lin'an.That means ozone production was con-trolled by photochemical reactions at Lin'an background station,because of the higher precursorconcentrations.The net destruction rate,at Waliguan Mt.,is not large,so that future increase inanthropogenic emission of reactive nitrogen will lead to larger production rates of steady-state O_3concentration.     

On determining the noon polar cap boundary from SuperDARN HF radar backscatter characteristics

Previous work has shown that ionospheric HF radar backscatter in the noon sector can be used to locate the footprint of the magnetospheric cusp particle precipitation. This has enabled the radar data to be used as a proxy for the location of the polar cap boundary, and hence measure the flow of plasma across it to derive the reconnection electric field in the ionosphere. This work used only single radar data sets with a field of view limited to 2 h of local time. In this case study using four of the SuperDARN radars, we examine the boundary determined over 6 h of magnetic local time around the noon sector and its relationship to the convection pattern. The variation with longitude of the latitude of the radar scatter with cusp characteristics shows a bay-like feature. It is shown that this feature is shaped by the variation with longitude of the poleward flow component of the ionospheric plasma and may be understood in terms of cusp ion time-of-flight effects. Using this interpretation, we derive the time-of-flight of the cusp ions and find that it is consistent with approximately 1 keV ions injected from a subsolar reconnection site. A method for deriving a more accurate estimate of the location of the open-closed field line boundary from HF radar data is described.     

柯坪6.5级地震的部分前兆异常及预报

1991年2月25日柯坪6.5级地震前,震中附近地区的土层地应力、金属摆倾斜仪等多项前兆观测出现异常变化,说明强震发生前近场灵敏度较低的简陋仪器也能观测到明显的前兆反应。分析、认识这些异常对地震短临预报的决策是有益的。     

“95.8”川西大暴雨成因分析

通过对“９５．８”大暴雨过程的全面技术总结，揭示了多种尺度系统间相互作用对产生大暴雨过程的贡献，并指出了云团的发生及其发展源于北方冷空气和南方低空急流持续影响所形成的两个中间尺度垂直环流。     

滇西普朗斑岩铜矿床中磷灰石的地球化学特征及其地质意义

滇西普朗斑岩铜矿床位于三江特提斯构造带义敦岛弧南端,是晚三叠世甘孜-理塘洋壳俯冲背景下的成矿作用产物。本文选取普朗矿床含矿石英闪长玢岩和石英二长斑岩中蚀变和未蚀变磷灰石进行研究,以探讨其对成岩、成矿作用的指示意义。结果显示,相比于未蚀变磷灰石,蚀变磷灰石的Na、S、Mn、Ca、Y及REE等元素含量均有不同程度的降低。总体而言,普朗矿床中磷灰石均具有高Sr、δEu,低Y的特征,指示了其母岩浆具似埃达克质特点。本次研究表明磷灰石的卤素、Sr和REE可以用来追踪成矿母岩浆成分、氧化状态和结晶演化过程。与三叠纪不成矿的休瓦促岩体相比,普朗矿床成矿岩体的磷灰石具高δEu、低Mn和δCe的特点,且δEu和δCe总体呈负相关趋势,表明普朗矿床成矿岩体氧逸度相对较高。此外,磷灰石中(La/Sm)_N、(La/Yb)_N和(Sm/Yb)_N比值降低可能是岩浆中独居石结晶或含Cl热液出溶的结果。与邻区的春都矿床、白垩纪休瓦促成矿岩体对比研究表明,普朗斑岩成矿岩浆具有高Cl/F特征,可能形成于典型的大洋俯冲环境。     

新型载体与档案保护

随着新材料、新技术逐渐地应用于档案载体,以及计算机技术被应用于档案管理,这些新型载体与档案的保护问题也日益显露出它的重要性和紧迫性,文章阐述对档案库房科学管理以及如何所采取相应的措施进行保护。     

Axisymmetry in protoplanetary nebulae – II. A near-infrared imaging polarimetric survey

In an imaging polarimetry survey of candidate post-AGB stars, scattering envelopes are detected around 20 objects. These envelopes represent the final mass-loss phases at the end of the AGB. In all cases, evidence for axisymmetry in the dust density is seen, suggesting that the presence of an axisymmetric outflow may be a ubiquitous phenomenon of the AGB to post-AGB transition. We use the polarized flux images to classify the objects into detached shell, bipolar and unresolved targets. Modelling based on a simple axisymmetric shell geometry supports the contention that post-AGB objects fall into one of two classes that differ in the amount of dust in the circumstellar environment: the detached shells correspond to stars with an optically thin expanding circumstellar envelope (CSE) whereas the bipolar and unresolved targets have optically thick dust structures, probably in the form of discs, which remain bound to the star, rather than partaking in the expansion of the AGB CSE. It is suggested that this bifurcation in morphology is rooted in the presence or absence of a binary companion, which determines whether or not a disc forms. Because the detached shell objects also appear axisymmetric, an additional mechanism for generating the axisymmetry, such as a magnetically shaped outflow, is needed if they do indeed have single star progenitors.     

四川地区短时强降水事件时空演变特征研究

利用四川地区自动气象站逐小时降水观测资料,分析了2010~2019年5~9月短时强降水事件24h累计降水量、频次和强度的时空分布特征,探讨了短时强降水事件发生的频次、极值分布及其与地形、海拔高度等的关系。结果表明：四川地区平均24h累计降雨量基本在50mm以上,盆地东北部、西南部、南部及阿坝州东部甚至超过100mm,最大值出现在广安,达175mm。四川地区短时强降水事件开始时间的日变化特征表现为“V”型结构的夜间峰值位相,事件持续时段多为傍晚至凌晨,时长可达10h以上,最长甚至可持续22h。在强降水事件极值的日变化上,极大值频次和降水量呈单峰结构,在03时达到最大,其后逐渐减小至15时达到谷值,而后再次增大;降水强度呈弱双峰结构,分别在04时和16时达到谷值,13时和18时达到峰值,其日变化呈“增-减-增-减”的特征。四川短时强降水事件与复杂地形有密切的关系,5~6月事件活跃区在四川盆地中部,7月在盆地西部的龙门山脉一带,8月在雅安、乐山附近,9月在盆地北部且频次明显减少;短时强降水事件的最大小时雨强可达80mm以上,出现在7~8月的盆地西部龙门山一带和南部地区。短时强降水事件随着海拔高度的增加,发生频次和日数逐渐减少,海拔2000m以上地区基本无强降水发生日出现( 峨眉山气象站例外)。     

风电场风资源测量与计算的精度控制

根据多个复杂地形风电场观测操作实践和大量观测数据的计算分析,提出了对观测数据和计算质量精度控制的主要措施,包括:复杂地形测风站布设的5个原则,仪器的合理选型和设置;对由于测风仪固有的系统误差和缺测数据的插补订正可能引起的计算误差进行了定量估算,通过对大量实测数据的对比计算显示:①目前普遍采用的进口风速计的相对偏差在1.6%～5.25%之间,由此可导致轮毂高度附近的年平均风功率密度误差在5%以上,最大达13.8%;②在季风气候区、复杂地形和风的年变率较大的地区,进行缺测数据插补订正时,应选取同季或同一主导风向的数据作为插补订正的基础数据,否则可能导致其平均风功率密度相对误差达20%～50%.     

膨胀蔷薇珊瑚与壮实鹿角珊瑚的胚胎和幼虫发育

造礁石珊瑚的有性繁殖是修复珊瑚礁生态系统的有效途径之一.文章为国内首次报道造礁石珊瑚有性繁殖和幼体发育过程,为利用有性繁殖技术恢复珊瑚礁生态系统提供了发育生物学上的理论基础.海南省三亚市鹿回头海域的大部分珊瑚在2009年3月底至4月中发生有性繁殖行为.2009年4月11日晚采集膨胀蔷薇珊瑚Montipora turgescens和壮实鹿角珊瑚Acropora robusta自然排放的受精卵,研究其胚胎及幼虫发育的过程.通过连续观察和显微拍摄记录了2种珊瑚的受精卵发育过程,结果显示,受精卵经过分裂变为桑葚胚;桑葚胚经过进一步发育变形为虾片状,进而发育成盘状幼体;盘状幼体由四周向内弯曲形成碗状的结构,进而出现原肠胚及纤毛,发育成为椭圆型或圆形的浮浪幼虫;浮浪幼虫发生附着变态,长出触手,发育成珊瑚幼体.通过观察还发现,膨胀蔷薇珊瑚的卵母细胞中本身就含有黄褐色虫黄藻,壮实鹿角珊瑚的卵母细胞中没有虫黄藻,其共生的虫黄藻足在发育过程中从周围环境获得的.