蓝罗非鱼鳞片表面结构的扫描电镜观察   总被引：5，自引：0，他引：5  

范瑞青  姜明  汝少国  高澜  徐卫 《海洋科学》2000,24(3):48-51

运用扫描电镜技术对蓝罗非鱼侧线上鳞、侧线下鳞和侧经鳞进行了形态结构的观察。研究结果表明,蓝罗非鱼体表睛属栉鳞,外形呈近圆形,分为顶区、基区和侧区三个部分;顶区边缘具细小齿状棘突,区内分布有癌状或棒状突起;基区具有清晰致密的鳞纹和放射状排列的鳞沟,年轮线处鳞纹密集排列;侧区较为平滑,无明显的鳞沟;侧线鳞具有粗壮的侧线管口。  相似文献   

Quantitative particle size,microtextural and outline shape analyses of glacigenic sediment reworked by paraglacial debris flows     

A. M. Curry  P. R. Porter  T. D. L. Irvine‐Fynn  G. Rees  T. B. Sands  J. Puttick 《地球表面变化过程与地形》2009,34(1):48-62

Particle size analysis and scanning electron microscopy have been used with some success to differentiate sediments sampled from varying geomorphological environments. In the paraglacial environment, however, discrimination of paraglacially reworked deposits from in situ glacigenic deposits has proven to be problematic. We consider till sediments that have been reworked by paraglacial debris flows and in situ, unreworked parent material, and apply a series of quantitative techniques in an attempt to discriminate samples from each environment. Initial analysis of particle size suggests some eluviation of fines from the debris‐flow‐reworked deposits but is of insufficient significance to allow reliable differentiation of geomorphological environment. Similarly, although slight differences are identified in terms of quartz grain surface microtextures and quartz grain outline shape, subsequent PCA, cluster and Fourier analyses fail to reliably differentiate quartz grains from each geomorphological environment, owing to high levels of intra‐sample heterogeneity. This lack of apparent difference may arise from a lack of paraglacial process operation of significant magnitude or duration for a characteristic process imprint to emerge at this scale of observation. Accordingly, further assessment of particle‐size and microtextural characteristics of glacial and paraglacial sediments may be most fruitful where sediments have been reworked over long distances. Moreover, differentiating glacial from paraglacial deposits is likely to yield the most reliable results where rigorous statistical analyses are combined with a wide range of sedimentological and geomorphological techniques. Copyright © 2008 John Wiley and Sons, Ltd.  相似文献   

地球基本磁场的成因   总被引：1，自引：1，他引：0       下载免费PDF全文

宋贯一 《地球物理学进展》2009,24(1):89-94

在略高于古藤堡面的压力和温度条件下,地核物质中的原子结构状态发生了质变.如对于外层能级分布是3d64s2的铁原子而言,Fe原子的最外层和极少一部分Fe原子的次外层将受到破坏,使外层电子发生"公有化"现象,残破的原子(处于离子状态)在自引力作用形成的压力作用下,按原子密度的大小产生分异,"内核"多为显示有正电性能的密度较高的残破原子组成,"外核"(包含过渡层)为富含"公有化"电子而显示负电性能的密度相对较低的残破原子组成,这是一个地核物质量子状态变化的静态过程,从地球内部宏观电性结构看来,地球的"内核"和"外核"组成缮了一个静态的巨型似"原子球","外核"显示负电性,"内核"显示正电性,"内核"所带电量与"外核"所带电量相等,但符号相反,在静态的情况下,似"原子球"并不显示磁性.由于地球自转,"外核"上界面赤道上的自转线速度为252.9m/s,"内核"外界面赤道上的自转线速度为88.9 m/s,二者的速度差为164.0 m/s,这种含有由巨大电量的"外核"电子壳层相对"内核"绕固定的轴向(自转轴)转动,自然会形成它的基本磁场.  相似文献   

地球同步轨道高能电子变化   总被引：1，自引：0，他引：1       下载免费PDF全文

张晓芳  符养  严卫  李就 《地球物理学进展》2009,24(6):1951-1957

结合小波分析及交叉小波分析方法,研究了地球同步轨道高能电子动态变化的多时间尺度结构,分析了电子通量在不同周期随着太阳风速、地磁指数D_st变化的具体特点.结果发现：（1）电子通量的长期变化受控于太阳风速,在太阳活动低值年,电子通量值高,具有明显的13.4天,27.4天及187天周期;交叉小波分析表明,电子通量的13.4天及27.4天周期受太阳风速周期变化信号的影响,187天周期变化受D_st指数周期变化信号的影响.（2）电子通量半年变化主要归因于太阳风的驱动作用,在每年的第100天及270左右达到两次峰值,峰值大小不对称,与D_st指数的谷值大小呈反比.（3）由于冕洞形成过程中的太阳风高速流影响,电子通量具有13.4及27.4天的周期,峰值水平受控于太阳风速结构.  相似文献   

Ionospheric Ne disturbances before 2007 Pu’er,Yunnan, China,earthquake     

欧阳新艳  张学民  申旭辉  刘静  钱家栋  蔡晋安  赵庶凡 《地震学报(英文版)》2008,21(4):425-437

Selecting three half orbits near the epicenter of Pu’er earthquake, we analyzed the Ne data recorded in their revis-ited orbits during a year before this earthquake, and extracted Ne precursors. The results show that: ① There are significant seasonal variations of ionospheric Ne in night time, which exhibit different shapes respectively in four seasons; ② There are three main shapes of Ne: single-peak, saddle-shaped and even-shaped, all of which may oc-cur in four seasons, but each season with its typical shape relatively; ③ Spatial images of Ne showed high values near the epicenter in 30 days before the earthquake, and there is a good correlation between anomaly and distribu-tion of earthquake in space and time, which reflects that these spatial anomalies were indeed concerned with the earthquake; ④There shows a certain similarity of the Ne curves among revisited orbits, which can provide back-ground information for distinguishing and identification of seismic anomaly.  相似文献   

皱纹盘鲍唾液腺的光镜和电镜研究   总被引：5，自引：1，他引：4  

崔龙波  陆瑶华  刘晨临  唐慧 《海洋学报》2000,22(1):141-144

１引言皱纹盘鲍（Ｈａｌｉｏｔｉｓｄｉ。ｕｓｈａｎｎａｉｌ。）隶属腹足纲、前鳃亚纲、原始腹足目,是我国北方沿海重要的经济贝类．唾液腺作为一种重要的消化腺,几乎存在于所有的腹足类动物．以往对腹足类动物唾液腺的研究,主要集中在肺螺亚纲动物［‘－’］及前鳃亚...  相似文献   

西华山钨矿床晶洞中水晶与黑钨矿流体包裹体显微测温与特征元素测定   总被引：2，自引：0，他引：2  

黄惠兰  常海亮  李芳  谭靖  张春红  周云  杨科  闫芬 《地学前缘》2013,20(2):205-212

摘要：西华山钨矿床晶洞中水晶与黑钨矿以及晶洞外部块状石英与共生黑钨矿中流体包裹体对比研究结果表明,后期应力作用和流体改造是造成共生石英与黑钨矿包裹体均一温度出现重大差异的主要原因。一般来说,在后期应力作用和流体改造下,黑钨矿有较好的稳定性,能较好地保存原生包裹体和较少出现次生包裹体,而与之共生石英中的原生包裹体几乎破坏殆尽,现在所看到的包裹体绝大部分是后来形成的次生包裹体,且很难确切区别原生与次生关系。当后期应力作用和流体改造很微弱时,石英中可保存较多原生包裹体,并且原生与次生关系较易区分。当完全未受应力作用改造时,共生石英(水晶)与黑钨矿中都只有原生包裹体,其Th值和盐度值基本相同或完全一致,且石英(水晶)流体包裹中富含W、Mn、Fe等成矿元素,表明石英与黑钨矿是由同一流体在相同时间和相同条件下沉淀的。鉴于一般金属矿床皆在一定程度上经受了后期应力作用和流体改造,因此在有关流体包裹体研究中应该结合不透明矿物进行全面对比,并且切实加强岩相学研究。  相似文献   

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王成  王解先 《大地测量与地球动力学》2013,33(3):125-128

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刘莹  戴吾蛟  章文毅  陈必焰 《大地测量与地球动力学》2013,33(3):30-33

????GPS??????????????????????????4??1????15??????????????????????????????????2???????????????????????????????????????????????????????￡???????11??UT10:00??13??UT6:00??14??UT6:00-14:00??15??UT14:00-16??00???γ?????Χ???????????????????????????????????????????????4????????????????й??  相似文献   

The intensity ratio I （557.7 nm） / I （427.8 nm） at Zhong- shan Station in Antarctica     

HU Guoyuan  AI Yong  ZHANG Hong 《极地研究(英文版)》2012,(1):9-11

Auroral intensity ratios at Zhongshan Station in Antarctica on 8 April 1999 are studied, along with variations in pene- trated electron energy. Ratios of/（557.7 nm）/I （427.8 nm） during the quiet period were from 5 to 22, and I （630.0 nm） / I （427.8 rim） ranged from 1 to 2.76. These variations were not caused by changes of atomic oxygen concentration, but rather by penetrated electron energy variability, or other mechanisms. Ratios decreased sharply during the auroral substorm, ranging from 1.66--6.5 and 0.071-1, respectively, mainly because of the increase in penetrated electron energy. At the onset of the substorm, the ratios reached their minima. This means that penetrated electron energy was maximized. When the substorm weakened, the penetrated electron energy returned to the pre-substorm level.  相似文献