Discussion on the complete-form vorticity equation and slantwise vorticity development          下载免费PDF全文

王秀明  周小刚  陶祖钰  刘华 《Acta Meteorologica Sinica》2016,30(1):67-75

The complete form of the vertical vorticity tendency equation (the complete-form vorticity equation) is derived from the Ertel potential vorticity equation to contain thermodynamic factors. In this study, a new complete-form vorticity equation, which has the same form as the original complete-form vorticity equation, is deduced from the absolute vorticity vector equation combined with the continuity equation and the expression of three-dimensional (3D) entropy gradient. By comparing the complete-form vorticity equation with the classical vertical vorticity equation, it is found that regardless of whether or not the isentropic surface is tilting, the two vorticity equations are in essence the same. The “baroclinic term” of the complete-form vorticity equation is exactly equal to the solenoidal term of the classical one, and there is a significant amount of cancellation between the two baroclinic items (the “slantwise term” and the horizontal vorticity change term) in the complete-form vorticity equation. In operational weather analysis, the tilt of the isentropic surface can be diagnosed according to the density of the isotherm on the upper-level isobaric map. For synoptic-scale motion, the vertical vorticity produced by the tilt of the isentropic surface is due to the contribution of atmospheric baroclinicity, which is measured by the solenoid. The 3D solenoid is parallel to the isentropic surface, so the more tilted the isentropic surface, the bigger the projection of the 3D solenoid in the vertical direction. The baroclinic contribution can be interpreted based on the PV thinking theory, but the relationship between the vorticity field and the potential vorticity field is not immediate.  相似文献   

分块DPCM与5/3整数小波变换结合的天文图像无损压缩     

朱贵富  邓辉  王锋  季凯帆 《天文研究与技术》2011,8(1)

针对海量的天文图像数据与有限的存储空间和带宽资源之间矛盾日益突出这一问题,提出一种无损压缩方法,首先将超大天文图像分块,再使用差分脉冲编码调制和5/3整数小波变换,最后使用霍夫曼算法编码。对该方法的原理和具体实现做了详细的分析与介绍,通过实验验证该方法比天文中常用的tar、PKZip、WinZip、WinRar软件在压缩比上分别提高了30%、29%、26%、2%,压缩速度远大于WinZip和WinRar;且该算法实现简单,适合硬件实现和利于并行处理。  相似文献   

Dependence of the holmberg effect on separations between paired galaxies     

Xin-Fa Deng  Yong Xin  Jiang Peng  Ping Wu 《Astrophysics》2010,53(3):342-350

To investigate the dependence of the Holmberg effect of paired galaxies on three-dimensional separations, we have constructed four subsamples characterized by three-dimensional separations s ≤ 50 kpc, 50 kpc < s ≤ 100 kpc , 100kpc < s ≤150kpc , and 150 kpc < s ≤ 200 kpc , respectively. In this study, linear correlation coefficients and surplus standard deviations of color indices, luminosity, and size between two components of paired galaxies are calculated. It is found that there is a weak tendency for correlation coefficients of color indices to increase with decreasing three-dimensional separations, but such a tendency does not exist for ones of luminosity and size. We also note that there is no tendency for surplus standard deviations to decrease with decreasing three-dimensional separations. This suggests that it is still very difficult to clearly affirm the dependence of the Holmberg Effect of paired galaxies on three-dimensional separations.  相似文献   

Secular period decreasing of detached chromospherically active binaries     

Chang Qing Luo  Xiao Bin Zhang  Li Cai Deng  Yang Ping Luo  Zhi Quan Luo  Shu Zheng Yang 《Astrophysics and Space Science》2010,327(1):9-17

The long-term orbital period changes of a large sample of detached chromospherically active binaries (CABs) were studied. Eleven such systems were found to be undergoing secular period decreases with the rates of ?6.3×10^?9 to ?1.1×10^?6 days per year. The period decreasing rates are found to vary depending on the orbital period. The longer the orbital period is, the more rapidly the period decreases. Following Stepien (Mon. Not. R. Astron. Soc. 274:1019, 1995), the period decreasing rate predicted by angular momentum loss (AML) caused by magnetic wind is computed for each system. A comparison between the observed and calculated period decreasing rates shows that the former values are obviously larger than the latter by 1–3 orders of magnitude. It suggests that the magnetic wind is not likely the determinant mechanism driving the AML in these systems. Finally, the orbital angular momentum (AM) and the rate of AML, $\dot{J}$ , are computed for each system. It shows that the AM have a similar change with the orbital period like dP/dt does, but $\log\dot{J}/J$ presents no strict changing with the kinematical ages.  相似文献   

厦门国家级珍稀海洋物种自然保护区文昌鱼(Branchiostoma belcheri)种群健康评价     

黄良敏  黎中宝  吝涛  李元跃  陈融斌  王家樵  陈强  李军 《海洋与湖沼》2013,44(1):103-110

利用2009-2010年四个季度月用底栖生物抓斗式采样器捕获的文昌鱼样品,从其资源分布、年龄结构、生物学和生态学特征等方面对厦门国家级珍稀海洋物种自然保护区文昌鱼的种群健康状况进行评价研究.结果表明:(1)文昌鱼种群资源分布衰减趋势明显,只在黄厝—前埔海区、小嶝岛—角屿海区和南线—十八线海区3个核心区还有分布,但资源密度低,分布范围狭小,而在鳄鱼屿实验区未能发现.(2)文昌鱼体重与体长之间关系:W=6.6895×10-4L3.1818;体长与体质量生长方程分别为:厶=65.63[1-e-0.68(t+032)],Wt=404.62[1-e-0.68(t+032)]3.1818;夏季、冬季航次的优势体长组分别为25-35mm和35-45mm,优势体重组分别为25-50mg和50-100mg;秋季低龄鱼较多,而冬季高龄鱼比例较高.(3)采用ELEFAN Ⅰ技术分析了厦门文昌鱼的Von Bertalanffy生长参数K、L∞、总死亡系数Z、自然死亡系数M和开发率E,发现其生长参数K值较大,自然死亡系数较高,开发率较大(0.69).综之,厦门自然保护区内的文昌鱼种群健康状况整体不佳,应注意资源保护,加强保护文昌鱼栖息地的底质和水质以及防止过度捕捞以实现其资源可持续利用.  相似文献   

Spatial distribution and species composition of PAHs in surface sediments from the Bohai Sea   总被引：1，自引：0，他引：1  

Liu WX  Chen JL  Lin XM  Tao S 《Marine pollution bulletin》2007,54(1):113-116

  相似文献   

银根-额济纳旗及邻区石炭-二叠系的沉积特征及石油地质意义   总被引：1，自引：0，他引：1  

赵省民  陈登超  邓坚 《地质学报》2010,84(8):1183-1194

长期以来,由于埋藏深、地质复杂及自然条件恶劣等原因,银根-额济纳旗及邻区石炭系-二叠系的油气勘查程度低,相关研究成果少.鉴于此,本文充分利用研究区的周缘露头,借助近30条剖面的详细调查,分析了本区石炭系-二叠系的沉积特征.研究表明,本区石炭系-二叠系包括了泥岩、砂岩、砂砾岩、碳酸盐岩和火山岩(或火山碎屑岩)等,海相生物丰富.暗色泥岩是石炭系-二叠系的主体,是潜在的烃源岩和盖层;火山岩(或火山碎屑岩)发育,碳酸盐岩多呈透镜状且硅化普遍,砂砾岩相对较少,三者构成石炭系-二叠系重要储层.岩石组成及展布特征表明,石炭纪-二叠纪期间,本区张裂频繁,火山作用强烈,远离陆源区,水体深而宁静,利于生烃物质发育.期间,区内主要发育了浅海相、广海海岸相、碳酸盐台地相、辫状三角洲相、扇三角洲相和火山喷发相等沉积类型.其中,浅海相和局限海岸相主要形成了烃源岩和盖层,其他沉积则形成了储层,为区内石炭系-二叠系造就了良好的油气地质条件.  相似文献   

临南油田街2断块沙三上亚段Ⅴ砂岩组沉积微相研究     

郭涛  张卫海  袁巍 《西安地质学院学报》2010,(4):363-367

基于区域地质背景资料,综合运用岩芯观察、岩相和测井相分析等手段,对临南油田街2断块沙三上亚段Ⅴ砂岩组沉积微相的沉积相标志、类型以及展布特征进行了系统研究。结果表明：临南油田街2断块沙三上亚段Ⅴ砂岩组为一套湖泊三角洲沉积体系,亚相类型为三角洲前缘亚相;沙三上亚段Ⅴ砂岩组主要沉积微相可细分为水下分流河道、水下分流河道间湾、河口坝、远砂坝和前缘席状砂等5种微相,并建立了沉积微相识别模式;沉积特征和沉积微相的平面展布呈现在近东西向剖面上砂体连续性较好,可见河口坝与前缘席状砂的交替出现,而在近西南—北东向剖面上,砂体横向上一般由水下分流河道过渡到河口坝或前缘席状砂。总之,临南油田街2断块沙三上亚段Ⅴ砂岩组是研究区三角洲形成的高峰期,水下分流河道、河口坝、前缘席状砂为主要的储集砂体。  相似文献   

云南大坪金矿区煌斑岩的地球化学特征及成因探讨   总被引：3，自引：0，他引：3  

王治华  郭晓东  葛良胜  陈祥  徐涛  范俊杰 《岩石矿物学杂志》2010,29(4):355-366

大坪金矿区闪长岩体中发育多条煌斑岩脉,并且多伴随石英脉出现。在岩石化学组成上,SiO2含量为44.86%~54.10%、K2O/Na2O在0.56~2.09之间,属钾玄质系列;岩石富集大离子亲石元素(Sr、U、Rb和Ba)和轻稀土元素(LREE)、相对亏损高场强元素(Ta、Nb和Ti),且Ta、Nb和Ti具"TNT"负异常;δEu值为0.72~1.36,负Eu异常不明显;87Sr/86Sr值范围为0.706 6~0.707 4,均值0.707 1,高于原始地幔现代值0.704 5;143Nd/144Nd值范围为0.512 4~0.512 5,均值0.512 4,低于原始地幔现代值0.512 638;εNd值范围为-2.5~-4.2,均值-3.98。Nb/Ta比值为48.96~82.58(平均62.99),远高于原始地幔值的17.5±2.0;Zr/Hf比值为20.45~47.53(平均39.57),略高于原始地幔值的36.27±2.0;Nb/Ta和Zr/Hf都远大于陆壳值11和33。表明煌斑岩源区可能来自早期俯冲洋壳或造山带根部拆沉组分脱水形成富集流体在地幔源区发生交代作用形成的富集地幔,岩浆在上升侵位过程中受到地壳物质的混染较弱,形成于碰撞后的板内构造环境。  相似文献   

阿尔泰造山带花岗岩时空演变、构造环境及地壳生长意义——以中国阿尔泰为例   总被引：23，自引：0，他引：23  

王涛  童英  李舢  张建军  史兴俊  李锦轶  韩宝福  洪大卫 《岩石矿物学杂志》2010,29(6):595-618

阿尔泰造山带横跨中、俄、哈、蒙四国边界,是中亚造山带主要组成部分,发育大量的花岗岩等侵入体。本文研究总结这些岩体的时空演变、成因类型和构造环境,并探讨其增生造山和地壳生长意义。依据锆石年龄,这些岩体可大致分为早中古生代的470～440Ma(中晚奥陶世)和425～360Ma(晚志留世—晚泥盆世)、晚古生代的355～318Ma(早石炭世)和290～270Ma(早二叠世)以及早中生代245～190Ma(中晚三叠世—早侏罗世)3个阶段5个期次,其中425～360Ma花岗岩可进一步细分为425～390Ma和380～360Ma两个峰期。早中古生代(470～360Ma)花岗岩体分布广泛,主要为钙碱性I型,多具不同程度变形,其中470～440Ma岩体变形极强(片麻岩体)。它们为同造山俯冲增生产物,形成于活动陆缘俯冲(470～440Ma)、继续俯冲弧后盆地伸展(420～390Ma)到聚合碰撞(380～360Ma)的过程中。早石炭世岩体发育于造山带南部,为不变形圆形状或不规则状,具典型碱性花岗岩特征,为晚(后)造山产物。早二叠世岩体主要发育于阿尔泰造山带南部,少量分布于造山带内部,多为圆形,不变形,少量变形岩体集中在额尔齐斯构造带内,成因类型以I、A型为特点,伴生有大量基性岩脉(体),显示为后造山底侵伸展环境。早中生代岩体为不变形圆形或不规则状,具有高分异I型和S型花岗岩特征,伴有稀有金属矿产,具有板内环境特点。花岗岩体同位素填图显示,阿尔泰中部块体岩体具有较低的εNd(t)值和老的Nd同位素模式年龄(1～1.3Ga),暗示存在古老地壳基底;由北向南εNd(t)值增高,模式年龄变年轻,显示陆壳向南生长,其中水平和垂向生长率分别为18%～28%和7%～8%。中生代时期阿尔泰造山带保留水平增生结构,没有发生大规模构造块体垂向叠覆。阿尔泰造山带经历了古陆缘构造演化,奥陶纪—志留纪陆缘俯冲,泥盆纪陆弧及陆缘边缘裂解、弧后盆地形成,晚泥盆世最终洋盆闭合及早石炭世各块体拼合的演化过程。该研究表明增生造山带中同样存在构造演化的阶段性;中亚增生造山作用不仅具有弧前增生,而且还存在陆缘裂解再拼合作用。  相似文献