冬季菲律宾周围对流活动与北太平洋风暴轴联系的数值模拟   总被引：2，自引：1，他引：1  

胡增臻  黄荣辉 《大气科学》1998,22(1):46-56

通过利用IAP 2-L AGCM进行的数值模拟,进一步揭示了冬季菲律宾周围对流活动异常对北太平洋风暴轴变化的影响及其二者联系的物理机制和物理过程。结果表明:当菲律宾周围对流活动增强时,在500 hPa等压面图上强迫产生一个自赤道西太平洋开始,经我国东部、堪察加半岛、白令海,到美国西海岸的异常波列;位于西太平洋的经向三圈环流增强,位置北移;在风暴轴的西半部和东端斜压性增强;从而导致了北太平洋风暴轴增强、北抬、东伸。  相似文献   

广西1997年气候影响评价     

周玲萍  黄雪松 《气象研究与应用》1998,19(1):21-27

１９９７年度（１９９６年１２月至１９９７年１１月）,广西各地年平均气温１６．６～２３．３℃,属正常;年降水量１２５９．５～２８２５．３ｍｍ,正常到偏多２～５成;年日照时数８５２．８～２１３９．３ｈ,大部地区比常年偏少２００～５００ｈ。１９９７年度,广西主要气候事件及其影响以洪涝和寒露风最为突出,其次是大风和冬旱;日照不足,降水偏多,洪涝及寒露风灾害严重,全年气候条件对工农业生产的影响弊多利少,属偏差年景。  相似文献   

Carbonation and melting reactions in the system CaO–MgO–SiO2–CO2 at mantle pressures with geophysical and petrological applications     

Peter J. Wyllie  Wuu -Liang Huang 《Contributions to Mineralogy and Petrology》1976,54(2):79-107

Bowen's petrogenetic grid was based initially on a series of decarbonation reactions in the system CaO-MgO-SiO₂-CO₂ with starting assemblages including calcite, dolomite, magnesite and quartz, and products including enstatite, forsterite, diopside and wollastonite. We review the positions of 14 decarbonation reactions, experimentally determined or estimated, extending the grid to mantle pressures to evaluate the effect of CO₂ on model mantle peridotite composed of forsterite(Fo)+orthopyroxene(Opx)+clinopyroxene(Cpx). Each reaction terminates at an invariant point involving a liquid, CO₂, carbonates, and silicates. The fusion curves for the mantle mineral assemblages in the presence of excess CO₂ also terminate at these invariant points. The points are connected by a series of reactions involving liquidus relationships among the carbonates and mantle silicates, at temperatures lower (1,100–1,300° C) than the silicate-CO₂ melting reactions (1,400–1,600° C). Review of experimental data in the bounding ternary systems together with preliminary data for the system CaO-MgO-SiO₂-CO₂ permits construction of a partly schematic framework for decarbonation and melting reactions at upper mantle pressures. The key to several problems in the peridotite-CO₂ subsystem is the intersection of a subsolidus carbonation reaction with a melting reaction at an invariant point near 24 kb and 1,200°C. There is an intricate series of reactions between 25 kb and 35 kb involving changes in silicate and carbonate phase fields on the CO₂-saturated liquidus surfaces. Conclusions include the following: (1) Peridotite Fo+Opx+Cpx can be carbonated with increasing pressure, or decreasing temperature, to yield Fo+Opx+Cpx+Cd (Cd=calcic dolomite), Fo+Opx+Cd, Fo+Opx+Cm (Cm=calcic magnesite), and finally Qz+Cm. (2) Free CO₂ cannot exist in subsolidus mantle peridotite with normal temperature distributions; it is stored as carbonate, Cd. (3) The CO₂ bubbles in peridotite nodules do not represent free CO₂ in mantle peridotite along normal geotherms. (4) CO₂ is as effective as H₂O in causing incipient melting, our preferred explanation for the low-velocity zone. (5) Fusion of peridotite with CO₂ at depths shallower than 80 km produces basic magmas, becoming more SiO₂-undersaturated with depth. (6) The solubility of CO₂ in mantle magmas is less than about 5 wt% at depths to 80 km, increasing abruptly to about 40 wt% at 80 km and deeper. (7) Deeper than 80 km, the first liquids produced are carbonatitic, changing towards kimberlitic and eventually, at considerably higher temperatures, to basic magmas. (8) Kimberlite and carbonatite magmas rising from the asthenosphere must evolve CO₂ at depths 100-80 km, which contributes to their explosive emplacement. (9) Fractional crystallization of CO₂-bearing SiO₂-undersaturated basic magmas at most pressures can yield residual kimberlite and carbonatite magmas.  相似文献   

江淮气旋发生发展和暴雨过程及有关预报问题的研究   总被引：3，自引：0，他引：3  

黄士松  林元弼  韦统健 《大气科学》1976,(1):27-41

本文就一次典型过程作为例子,分析了江淮气旋发生发展和暴雨过程的特点,指出有利于江淮气旋发生发展的高空天气形势,地面一些中尺度低压和暴雨核的演变与气旋发展的互相联系。发现气旋区内可存在若干个中尺度低压,这些中尺度低压可先于或后于暴雨核生成而出现,并可增强、减弱或合并。文中计算了潜热释放的加热对涡度制造的贡献,指出潜热加热对气旋发展起着极为重要的作用。作者对于影响气旋发展的因子进行了讨论,并对如何根据湿度场、流场和降水分布(或卫星云图)特征来预报江淮气旋提出建议。  相似文献   

1982年12月2日耀斑随时间变化的半经验模型     

方成  黄佑然  胡菊  甘为群 《中国天文和天体物理学报》1986,(4)

我们利用南京大学太阳塔中的多波段光谱仪,在H_α、H_β和CaⅡ H、K三个波段同时拍到了1982年12月2日日面S15W11处的一个SB级耀斑的光谱。本文给出其中七个时刻的谱线轮廓及有关参数的序列。在非局部热动平衡条件下计算了耀斑随时间变化的半经验模型,结果显示了色球耀斑的演化过程。利用模型得到了一些色球物质蒸发参数,结果同根据SMM的X射线观测所作的估计相一致。  相似文献   

Estimation of the chord length and relative height of tracking stations from single pass satellite ranging data     

Miao-fu He  Chu-gang Feng  Cheng Huang 《Chinese Astronomy and Astrophysics》1986,10(4):336-341

We describe here a technique of determining the chord length and the relative height between two laser tracking stations using single-pass satellite ranging data over very short arcs. Numerical examples show that this technique can supplement the conventional technique which requires data over much longer arcs by providing a capability for checking the accuracy of the geodetic network of laser tracking stations.  相似文献   

Diurnal variation of nitric oxide emission flux from a mangrove wetland in Zhangjiang River Estuary,China     

Juan Chen  Fei-Hua Wu  Qiang Xiao  Zhang-Hua Yang  Sheng-Kai Huang  Jian Wang  Yu-Guang Wu  Xue-Jun Dong  Zhen-Ming Pei  Hai-Lei Zheng 《Estuarine, Coastal and Shelf Science》2010

The diurnal variation of nitric oxide (NO) emission fluxes from a Kandelia obovata and Avicennia marina mangrove wetland were studied in the Zhangjiang River Estuary Mangrove National Nature Reserve using a dynamic chamber-based technique and a chemiluminescent analyzer. Results from field experiments show that NO emission from K. obovata and A. marina sampling sites reached maximal values of 1.07 ng N m⁻² s⁻¹ and 1.23 ng N m⁻² s⁻¹, respectively after the night tide. Meanwhile NO emission maintained at a steady lower level in daytime for both wetland sites. In laboratory experiments, NO emission from the mangrove wetland soil samples treated with simulated tides in the darkness exhibited higher values than those in the light, therefore it seems that tides and darkness could increase NO emission from mangrove wetlands, while intensive light, high temperature, and dryness in the daytime decreased NO emission. Compared with K. obovata soil samples, the diurnal average NO emission rate of the A. marina site was significantly higher, which was closely related to relatively higher diurnal average CO₂ emission rate, soil available nitrogen content and soil net nitrification rate of the A. marina site. Moreover, soil samples of the A. marina site were more responsive to simulated tides and the addition of nitrogen than those of the K. obovata site.  相似文献   

Geochemical study on oil-cracked gases and kerogen-cracked gases (II)—Discrimination methods between oil-cracked gases and kerogen-cracked gases     

Huang  GuangHui  Zhang  Min  Hu  GuoYi  Xiao  ZhongYao 《中国科学:地球科学(英文版)》2010,52(1):10-18

In the processes of discrimination between oil-cracked gases and kerogen-cracked gases, Behar and Pinzgofer et al.’s results were adopted in the former researches, in which the ratio of C₂/C₃ is basically a constant while the ratio of C₁/C₂ gradually increases in the course of primary cracking of kerogen. Otherwise in the course of secondary cracking of oil, the ratio of C₂/C₃ increases rapidly while C₁/C₂ keeps relatively stable. Our study on analogue experiment shows that, whether it is oil or kerogen, in its process of gas generating by cracking, the ratios of C₂/C₃, C₁/C₂ or C₁/C₃ will all be increased with the growth of thermal conditions. In comparison, the ratio of C₂/C₃, which is affected by genetic type to some comparatively less extent, mainly responds to the maturity of gases, while the value of C₂/C₃ is about 2, and that of C₂/iC₄ is about 10, and the corresponding value of R _o is about 1.5%–1.6%. The influence of gas source on C₂/C₃ is less than that of gas maturity, otherwise C₁/C₂ (or C₁/C₃) is obviously affected by cracking matrices. The ratios of C₁/C₂, C₁/C₃ of oil-cracked gases are less than that of kerogen-cracked gases, under the condition that the ratios of C₂/C₃ are similar in value, so are the value of dryness indexes. There exists wide diffidence between this view and the former discrimination method in theory. The analysis of the spot sample indicates that we can apply the above basic view to dealing efficiently with the problem of the discrimination between oil-cracked gas and kerogen-cracked gas.

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A Model for Contact Binary Systems     

Han-Feng Song Run-Qian Huang Shao-Lan Bi 《中国天文和天体物理学报》2007,7(4):539-550

A model for contact binary systems is presented, which incorporates the following special features: a) The energy exchange between the components is based on the understand-ing that the energy exchange is due to the release of potential, kinetic and thermal energies of the exchanged mass. b) A special form of mass and angular momentum loss occurring in contact binaries is losses via the outer Lagrangian point. c) The effects of spin, orbital rota-tion and tidal action on the stellar structure as well as the effect of meridian circulation on the mixing of the chemical elements are considered. d) The model is valid not only for low-mass contact binaries but also for high-mass contact binaries. For illustration, we used the model to trace the evolution of a massive binary system consisting of one 12M and one 5M star. The result shows that the start and end of the contact stage fall within the semi-detached phase during which the primary continually transfers mass to the secondary. The time span of the contact stage is short and the mass transfer rate is very large. Therefore, the contact stage can be regarded as a special part of the semi-detached phase with a large mass transfer rate. Both mass loss through the outer Lagrangian point and oscillation between contact and semi-contact states can occur during the contact phase, and the effective temperatures of the primary and the secondary are almost equal.  相似文献   

The Origin and Acceleration of ~3He and Heavy Ions in the 2000 July 14 Event     

Gui-Ping Wu  Guang-Li Huang  Yu-Hua Tang  Yu Dai Department of Physics  Southeast University  Nanjing  Purple Mountain Observatory  Chinese Academy of Sciences  Nanjing Department of Astronomy  Nanjing University  Nanjing 《中国天文和天体物理学报》2007,7(1):141-147

1INTRODUCTIONEnrichment of3He and heavy ions(i.e.,Ne,Mg,Si and Fe),characteristic of impulsive?ares,have beenstudied for more than three decades.It is found that they are generally associated with nonthermal energeticelectron-rich events(Reames et al.1988;Reames1999and references therein;Ho et al.2001;Wang et al.2006)and are related to the peculiar ratio of charge to mass(Mazur et al.1996;Reames1999).Althoughthe abundance of3He ions is not correlated with the abundance of heavy ions,s…  相似文献