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中沙,西沙群岛海区表层沉积物中微型腹足类,双壳类的分布 总被引:2,自引:0,他引:2
中沙,西沙群岛海区表层沉积物中微型腹足类、双壳类主要由热带、亚热带种类和广温性种类组成,并以典型的带珊瑚礁型种类为主,见有腹足类176种,双壳类48种,可划分出3个沉积组合类型。温度、水深、底质,海底地貌是控制本区腹足类、双壳类分布的主要环境因素。腹足类、双壳类遗壳埋藏群由原地埋藏类型和异地埋藏类型组成。在珊瑚礁深水处这现任中类型呈明显混合分布。在水深22.90,115m处属原地埋藏的潮间带或浅不 相似文献
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Generalized Inversion Method has been used to estimate the spatial variation of site effects,using the digital data of SH-waves recorded by 63 stations in the Capital Circle Region of China from 2001 to 2006.We gained the site effects of all stations participating in the calculation.We found that the site effect of rock was stabile and about 1.0 from 1.0Hz to 10.0Hz,while the site effect of deposit was high in low frequencies,about 3 ~ 7 from 1.0Hz to 8.0Hz,and the site effect was protuberant at about 5.0Hz,then fell as the frequency increased.The result shows the shape and intensity of station site effects are mainly influenced by the lithology below the station,and possibly also by the local geological structure. 相似文献
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Some observational results of sea storm current 总被引:3,自引:0,他引:3
INTRODUCTIONDr. Hollister, a marine geologist of the Woods Hole Oceanographic Institution, firstpointed out that there was ocean storm current in the ocean. He found out the wavy texture inthe seabed core samples, and suggested that this wavy texture was caused by the high speedsea current in remote antiquity. He then suggested a bold hypothesis that there existed a benthic storm current near the ocean bottom, and presented this hypothesis at the IUGG confer-ence held at San Francisco… 相似文献
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本文建议了一个用于太阳活动区纵向电流计算的新方法,讨论了将该方法用于向量磁场观测分析的可行性。 相似文献
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假定太阳是一颗普通的恒星,对太阳磁场的高分辨率观测,则从内禀磁场强度,尺度谱,面积填充因子,成穴分布趋势,双极分布特征和演化时标等多方面,为类太阳恒星磁场测量提供了一个基本标度,本文综述了与恒星磁场测量有关的,太阳磁场若干观测特征,与类太阳恒星测量结果对比表明,类太阳恒星磁场的内禀强度与太阳磁场接近,但面积填充因子大1-2个数量级,这可能真实地反映了恒星磁场的内禀强度成太阳磁场接近,但面积填充因子 相似文献
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本讨论了从太阳光球向日冕传输磁能和磁复杂性的过程。活动日冕,作为由电磁场和粒子组成的系统,其唯一的开场表面是太阳光球,光球层等离子体的运动和磁场的相互作用,是造成磁能和磁复杂性向日冕传输的主要根据;同时,光球上的耗散过程也对日冕磁能和磁复杂性的积累有不可忽视的贡献。 相似文献
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