The temperature of nonspherical circumstellar dust grains

The temperatures of prolate and oblate spheroidal dust grains in the envelopes of stars of various spectral types are calculated. Homogeneous particles with aspect ratios a/b≤10 composed of amorphous carbon, iron, dirty ice, various silicates, and other materials are considered. The temperatures of spherical and spheroidal particles were found to vary similarly with particle size, distance to the star, and stellar temperature. The temperature ratio T _d(spheroid)/T _d(sphere) depends most strongly on the grain chemical composition and shape. Spheroidal grains are generally colder than spherical particles of the same volume; only iron spheroids can be slightly hotter than iron spheres. At a/b≈2, the temperature differences do not exceed 10%. If a/b≥4, the temperatures can differ by 30–40%. For a fixed dust mass in the medium, the fluxes at wavelengths λ≥100 are higher if the grains are nonspherical, which gives overestimated dust masses from millimeter observations. The effect of grain shape should also be taken into account when modeling Galactic-dust emission properties, which are calculated when searching for fluctuations of the cosmic microwave background radiation in its Wien wing.     

Radio galaxies with a 'double-double' morphology – II. The evolution of double-double radio galaxies and implications for the alignment effect in FRII sources

A double-double radio galaxy (DDRG) is defined as consisting of a pair of double radio sources with a common centre. In this paper we present an analytical model in which the peculiar radio structure of DDRGs is caused by an interruption of the jet flow in the central AGN. The new jets emerging from the restarted AGN give rise to an inner source structure within the region of the old, outer cocoon. Standard models of the evolution of FRII sources predict gas densities within the region of the old cocoon that are insufficient to explain the observed properties of the inner source structure. Therefore additional material must have passed from the environment of the source through the bow shock surrounding the outer source structure into the cocoon. We propose that this material is warm clouds (∼10⁴ K) of gas embedded in the hot IGM which are eventually dispersed over the cocoon volume by surface instabilities induced by the passage of cocoon material. The derived lower limits for the volume filling factors of these clouds are in good agreement with results obtained from optical observations. The long time-scales for the dispersion of the clouds (∼10⁷ yr) are consistent with the apparently exclusive occurrence of the DDRG phenomenon in large (≳700 kpc) radio sources, and with the observed correlation of the strength of the optical/UV alignment effect in z ∼1 FRII sources with their linear size.     

荔枝草对鱼油的抗氧化作用

针对鱼油产品的易氧化问题,研究了荔枝草的抗氧化能力,发现荔枝草提取物在室温下（２８℃）是一种良好的鱼油抗氧化剂,其抗氧化有效成分集中于花和叶中,以酚灰主,极性较弱,乙酸乙酯可以将该成分有效地提取出来。比较对鱼油的抗氧化荔枝草石油醚提取物和茶多要不要相当,但其溶解性远好于茶多酚,尽管远逊于ＴＢＨＱ,仍不失为一种良好的天然抗氧化剂,具有较高的开发应用价值     

21世纪全球油气资源形势和海上多波地震技术展望

首先综述了现在对全球油气资源量的估计和对 2 1世纪全球油气资源发展形势的预测。表明2 1世纪全球油气资源不会枯竭。未来 10 0年 ,不是世界上有没有油气可供开采 ,而是环境允不允许和在多大程度上允许以及用多大的成本开采的问题。在所有情况下 ,技术进步都起着关键的作用。然后从油气勘探角度对技术进步中的一项主要技术———多分量地震的历史、现状和发展作了评述 ,并结合国家 86 3项目关于海上多波地震技术研究的状况提出了进一步实施的设想     

井筒电加热改善水平井蒸汽吞吐效果机理实验

针对稠油水平井蒸汽吞吐面临入井渗流阻力大、产量水平低、吞吐递减率高、采收率偏低等问题,提出了电加热辅助水平井蒸汽吞吐方法.首先根据水平井蒸汽吞吐过程中的电加热与蒸汽复合传热特征,建立了电加热辅助蒸汽吞吐三个阶段的(注汽阶段、焖井阶段、生产阶段)储层升温解析模型,在此基础上,设计并开展了电加热辅助蒸汽吞吐和常规水平井吞吐...     

齐家-古龙地区页岩油参数井泉头组—青山口组沉积微相特征

沉积微相发育特征对页岩油赋存及开发潜力具有重要的影响.以松辽盆地北部齐家-古龙地区松页油1井和松页油2井泉头组四段上部—青山口组二三段下部岩心为研究对象,通过大比例尺岩心观察和精细描述,以岩心岩性、层理构造、化石、含有物、电性特征为依据,开展沉积微相研究.研究认为,松页油1井和松页油2井岩心中,主要发育湖泊相沉积,分为浅湖和半深湖—深湖2种沉积亚相,可进一步识别出浅湖滩坝砂、介壳滩、泥质浅湖、半深湖—深湖泥和油页岩5种沉积微相.青一段下部主要发育半深湖—深湖亚相,浅湖亚相主要分布在青一段上部、青二三段下部和泉四段上部层位.泥质浅湖微相、半深湖—深湖泥微相以及油页岩微相均是有利于页岩油形成的沉积微相类型.     

An estimation of internal soliton forces on a pile in the ocean

Internal soliton forces on oil-platform piles in the ocean are estimated with the Morison Formula. Different from sur- face wave forces, which change only in magnitude along a pile, internal soliton forces can be distributed over the entire pile in the water and they change not only in magnitude but also in direction with depth. Our calculations show that the maximum total force caused by a soliton with its associated current of 2.1 m s-1 is nearly equal to the maximum total force exerted by a surface wave with a wavelength of 300 m and a wave-height of 18 m. The total internal soliton force is large enough to affect the operations of marine oil platforms and other facilities. Therefore, the influence of internal solitons should not be neglected in the design of oil platforms.     

基于细粒岩石类型对玛湖凹陷下二叠统风城组烃源岩分类评价

准噶尔盆地玛湖凹陷风城组页岩油勘探取得巨大突破,但是按照普遍认可的页岩油烃源岩评价标准,本区的烃源岩品质并不理想。为了科学评价玛湖凹陷烃源岩品质特征,本文在系统的岩心观察和有机地球化学分析的基础上,揭示烃源岩的形成环境,并按照矿物组成对烃源岩分类评价。玛湖凹陷风城组细粒岩主要沉积于正常半深湖、咸化半深湖、半咸化半深湖、含热液半深湖和滨浅湖环境中,各环境中细粒岩的有机质特征存在一定区别,其中半咸化半深湖有机质较为富集,w(TOC)均值在1%左右。进一步结合有机质类型判别图解,表明咸化半深湖和含热液半深湖有机质来源以湖泊生物为主,而其他环境中存在湖泊和陆源混合有机质来源。基于有机质生烃潜力评价和成熟度(V_re=0.74%)估算,表明目前风城组烃源岩中有机质正处于大量排烃的成熟阶段,且确定了细粒岩中的烃类为原生烃。由于不同矿物组成的烃源岩吸附能力的差异,按照陆相泥质烃源岩和碳酸盐质烃源岩开展分类评价,结果表明风城组沉积了累计厚度近250 m的的有效烃源岩,且富含以藻类体为主的有机质。     

德州气候变化与建筑物防腐

利用德州11县市1951～2005年温度、降水资料,计算气候干燥度,1981～2005年与1951～1980年相比全市干燥度由1.45增大到1.64,已由原来的半湿润气候变化为半干旱气候。各县市降水量呈减少趋势,平均每10年减少19.64mm;气温呈上升趋势,平均每10年升高0.11℃,冬季升高0.30℃,冬季增温显著,北部县市已由原来的冰冻区变化为微冻区,全市均为微冻区。由于气候条件变化,相应场地环境类别与腐蚀介质指标的调整系数标准应作调整改变,场地环境类别由Ⅱ类转变为Ⅰ类,腐蚀介质指标的调整系数均取0.9。