长竹蛏人工育苗技术的初步研究

本文对长竹蛏繁殖习性、胚胎发育和人工育苗技术关键进行研究．结果表明亲贝经暂养可促进性成熟；幼虫对温、盐度的适应较广；变态附着采用缩光培育,未经缩光的附着时间延长,存活率降低;幼虫长至约240μm变态附着,附着量在(0.6～10)×106个/m     

基于地质建造的西南山区成土母质分类方案——以大凉山区为例

为适应生态地质调查和评价工作对成土母质研究的要求,以四川大凉山区为例,提出基于地质建造的成土母质分类方案,即以地质构造演化和地质建造环境为依据,结合残坡积物的成因类型对成土母质进行分类。大凉山区的成土母质可划分为第四纪冲洪积物、新近纪—第四纪砂泥岩类残坡积物、侏罗纪—白垩纪泥质岩类残坡积物、三叠纪砂泥岩类残坡积物、中生代中酸性岩类残坡积物、二叠纪基性—超基性岩类残坡积物、震旦纪—三叠纪砂泥岩类残坡积物、震旦纪—三叠纪碳酸盐岩类残坡积物、元古宙中酸性岩类残坡积物、元古宙火山碎屑岩类残坡积物、元古宙基性—超基性岩类残坡积物、元古宙变质岩类残坡积物等12类。研究表明,大凉山区成土母质和土壤存在差异性,但同一成土母质上的不同土壤类型具有一定相似的地球化学特征,不同成土母质形成的同一种土壤类型存在较大的地球化学差异。因此,基于地质建造的成土母质分类方案既能有效反映不同构造背景和成岩环境下的成土母质差异,又能有效表征成土母质与其上土壤的内在联系。     

鄂尔多斯盆地西缘羊虎沟组物源区分析

鄂尔多斯盆地西缘羊虎沟组物源特征对天然气勘探尤为重要。通过砂岩的碎屑组分、岩屑组分、重矿物组合以及石英阴极发光等研究,认为研究区羊虎沟组受到北部、西南部、南部物源控制,各个方位物源在研究区中部吴忠—马家滩地区汇合。通过砂岩轻、重矿物组合和碎屑组分的Dickinson三角图解,以及泥岩的稀土元素特征等分析,认为研究区羊虎沟组源岩以大陆上地壳岩石为主。研究区北部砂岩物源区为再旋回造山带物源区,泥岩球粒陨石标准化稀土元素配分模式与阿拉善古陆浅变质岩相似,具有亲缘性;西南部及南部砂岩物源区为稳定陆块区和再旋回造山带物源区,泥岩球粒陨石标准化稀土元素配分模式与祁连—北秦岭造山带中浅变质岩相似。综上所述,研究区北部母岩主要为阿拉善古陆的浅变质岩夹少许火山岩,西南部及南部母岩主要为祁连—北秦岭造山带的中浅变质岩,其次为碳酸盐岩和火山岩。     

Flora小行星族自转特性研究

小行星族作为灾变碰撞的残留物,其基础物理性质提供了其母体以及后续演化信息.其中轨道以及自转特性分别反映了Yarkovsky效应以及Yarkovsky-O’Keefe-Radzievskii-Paddack效应(YORP效应)对于小行星族演化的影响.基于小行星光变数据库(Asteroid Lightcurve Database),通过对Flora小行星族自转速率分布进行研究,发现随着直径减小,族成员自转速率倾向于主要集中在3–5 d^-1的范围内.同时,可以注意到Flora小行星族整体表现出更倾向于顺行自转状态的现象,但对于轨道半长轴小于2.2au的成员来说,其顺行自转与逆行自转状态成员数目比接近于近地小行星中顺逆行自转状态源1:3的比例;此外,对于轨道半长轴大于2.2 au且具有顺行自转状态的部分族成员,在轨道半长轴-绝对星等分布中表现出聚集现象,并在聚集区域中有9颗成员展现出类似Slivan状态特征.     

埃尔塔宁小行星质量的下限估计

埃尔塔宁小行星是一颗２１５ 万年前在南太平洋撞击地球的小行星,它也是目前唯一的深海区与地球碰撞的小行星。根据埃尔塔宁号和Ｐｏｌａｒｓｔｅｒｎ 号海洋调查船在陨击海区勘查的小行星残骸分布密度,我们估计埃尔塔宁小行星质量为２ ．３ ×１０１３ｇ ,对应于它的直径为０ ．２３ 公里。这比Ｋｙｔｅ 等人（１９８８） 估计的质量小了１０ 倍,然而它更接近埃尔塔宁小行星撞击事件的实际情况,可以作为埃尔塔宁小行星质量下限和半径下限更合理的估计值。     

The Eltanin asteroid impact: possible South Pacific palaeomegatsunami footprint and potential implications for the Pliocene–Pleistocene transition

Large asteroid impacts are rare, and those into the deep ocean are rarer still. The Eltanin asteroid impact around 2.51 ± 0.07 Ma occurred at a time of great climatic and geological change associated with the Pliocene–Pleistocene boundary. Numerical models of the event indicate that a megatsunami was generated, although there is debate concerning its magnitude and the region‐wide extent of its influence. We summarise the existing evidence for possible Eltanin megatsunami deposits in Antarctica, Chile and New Zealand, while also examining other potential sites from several locations, mainly around the South Pacific region. In reviewing these data we note that these events were unfolding at the same time as those associated with the Pliocene–Pleistocene boundary and, as such, most of the geological evidence from that time has a climatic interpretation. The potential climatic and geological ramifications of the Eltanin asteroid impact, however, have failed to be considered by most researchers studying this time period. Although we are not advocating that all geological activity at that time is connected with the Eltanin asteroid impact, it raises interesting questions about the role potentially played by such catastrophic events in contributing to or even triggering epochal transitions. Copyright © 2012 John Wiley & Sons, Ltd.     

中国龙卷风的若干特征

应用数理统计方法和通过对观测资料的分析，研究了龙卷风的气候特征；根据近年天气资料，研究了龙卷风发生的天气系统，层结特征，风场和母体云团的特征。     

The Near-Earth Asteroid Size-Frequency Distribution: A Snapshot of the Lunar Impactor Size-Frequency Distribution

It is shown that the size-frequency distribution (SFD) of a time-averaged projectile population derived from the lunar crater SFD of Neukum and Ivanov (in Hazards Due to Comets and Asteroids (T. Gehrels, Ed.), 1994, pp. 359-416, Univ. of Arizona Press, Tucson) provides a convincing fit to the SFD of the current near-Earth asteroid (NEA) population, as deduced from the results of asteroid search programs. Our results suggest that the shape of the SFD of the impactor flux has remained in a steady state since the late heavy bombardment, so that the current NEA population can be viewed as a snapshot of the flux of impactors on the Moon. The number of bodies in the projectile population with diameters of 1 km or more is 700±130, which is in good agreement with recent estimates of the total number of NEAs in this size range. Our results imply that the contribution to the projectile flux from comets is small for diameters below 10 km.     

吉林省南部宇宙尘的化学组成特征

在吉林省南部元古宇石英岩内发现磁性微球粒３９２枚,根据其产状,形貌及一般特征,微结构和化学组成表明为陨石消融型宇宙尘,由４亚４小类组成一个宇宙尘系列,（１）金属球粒;（２）纯铁球粒,（ｂ）ＦＣＮ型（天然不锈钢）球粒;（２）氧化物球粒（ａ）普通铁质宇宙尘（ｂ）铬铁氧化物球粒;（３）玻璃质球粒;（４）氧化物－金属过渡型球粒,其母体要能是一分异的ＦＣＮ型石－铁陨石质陨星体,核部为ＦＣＮ合金,经消融分异作     

早白垩世Ruffordia goepperti的原位孢子及与分散孢子的关系

海金沙特的Ｒｕｆｆｏｒｄｉａ ｇｏｅｐｐｅｒｔｉ（Ｄｕｎｋｅｒ）Ｓｅｗａｒｄ是世界上早白垩世极为重要的蕨类植物。通过对比发现,Ｒｕｆｆｏｒｄｉａ ｇｏｅｐｐｅｒｔｉ原位孢子的形态和细微纹饰与地层中分散孢子Ｃｉｃａｔｒｉｃｏｓｉｓｐｏｒｉｔｅｓ ａｕｓｔｒａｌｉｅｎｓｉｓ（Ｃｏｏｋｓｏｎ）Ｐｏｔｏｎｉｅ和Ｃ．ｍｉｎｏｒ（Ｂｏｌｃｈ．）Ｐｏｃｏｃｋ一致,而且大化石与分散孢子的地史、地理分布范围也相同,