First arrival cycle-based calculation methods of in situ sound speed and attenuation in sediments

The acoustic properties of seafloor sediments are of great importance in geoacoustic modeling, detecting, and oceanic engineering. The methods based on the first arrival cycle are investigated to calculate sound speed and attenuation of sediment more precisely in in situ measurements. The comparison of different data analysis methods based on the first arrival cycle approach for in situ measurement results in the following conclusions: (1) the calculated methods can help find the effective cycles and reduce the errors in calculating sound speed and attenuation; (2) using this approach, the point judgment method-based data analysis has the same effectiveness as the cross-correlation method-based data analysis in calculating group sound speed and has the same effectiveness in calculating attenuation in the time domain as the spectrum analysis method-based data analysis has in calculating attenuation in frequency domain; and (3) measurement in water can help not only calibrate the transmitting distance but also can calculate the time delay for the sound speed and the attenuation loss in the transmitting process. Finally, theoretical calculation was used to calculate the measured results, indicating a good agreement, which supports that first arrival cycle-based calculated methods can be used to analyze the measured data and the effective density fluid model can be used to analyze more acoustic properties and invert several physical properties in this experiment.     

Investigation of the correlation between morphology and luminosity for two classes of main galaxies

Using an apparent-magnitude limited Main galaxy sample of the Sloan Digital Sky Survey Data Release 7(SDSS DR7), we investigate the correlation between morphologies and luminosity for the Main galaxy sample. Our Main galaxy sample is divided into two classes: Main galaxies only with TARGET_GALAXY flag (bestPrimtarget = 64), and ones also with other flags. It is found that for the second class Main galaxies, the early-type proportion monotonously increases with increasing luminosity nearly in the whole luminosity region. But for the first class Main galaxies, the early-type proportion increases with increasing luminosity only within a certain luminosity region (−22.2 < M _r  < −19.8). In the high luminosity region (M _r  < −22.2), the early-type proportion of the first class Main galaxies even decreases dramatically with increasing luminosity. We also analyze the correlation between morphologies and luminosity of galaxies around the peak of the redshift distribution ( 0.07 ≤ z ≤ 0.08 ). In such a narrow redshift region, we still observe strong correlation between morphologies and luminosity, which shows that this correlation is fundamental.     

冕洞与太阳活动周及地磁活动的演化关系

本文用1970－1995年的冕洞资料，分析了冕洞的分布规律，磁场极性的演化特征和冕洞的地磁效应，以及它们与太阳黑子周期的演化关系，得到了一些有意义的结论。特别指出赤道冕洞和极区冕洞具有相反的演化规律和不同的特征。     

Seven-frequency VLBI Observations of the GHz-Peaked-Spectrum Source OQ 208

We present quasi-simultaneous VLBI images of the GHz-Peaked-Spectrum radio source OQ 208 obtained with the Very Long Baseline Array at 1.4,1.7,2.3,5.0,8.4,15.4GHz and the European VLBI Network at 6.7 GHz.The low frequency(1.4,1.7 and 2.3GHz)ob- servations reveal a weak and extended steep-spectrum component at about 30mas away at position angle-110°,which may be a remnant emission.The radio structure of OQ 208 con- sists of two mini-lobes at 5.0,6.7,8.4 and 15.4 GHz.Our spectral analysis further confirms that the southwest lobe undergoes free-free absorption and finds that the free-free absorption is stronger in the inner region.By fitting the 8.4 GHz images from 1994 to 2005,we obtain a separation speed of 0.031±0.006 mas yr~(-1)between the two mini-lobes.This indicates a jet proper motion of 0.105±0.020 c and a kinematic age of 219±42 yr for the radio source.     

RFI Test Observations at a Candidate Ska Site in China

Radio frequency interference (RFI) test observations were carried out at one of the candidate Square Kilometre Array (SKA) sites in Guizhou province, following the “RFI Measurement Protocol for Candidate SKA Sites” (hereafter RFI protocol). All data (raw and calibrated) are preserved in some suitable format, such as that set by the international RFI working group of the Site Evaluation and Selection Committee (SESC). An RFI test in December 2003 was performed according to Mode 1 of the RFI Protocol, in order to identify technical difficulties which might arise during a co-ordinated RFI measurement campaign over a period of 1 year. In this paper we describe the current equipment, observational technique and data presentation. The preliminary results demonstrate that the RFI situation at Dawodang depression in Guizhou province makes it quite a promising location for the proposed SKA. Furthermore, the first session of the RFI monitoring program, which was made in May 2004, showed that a complete RFI measurement including both modes 1 and 2 of the RFI Protocol would take about 2 weeks. The possible ways to minimize some limitations of the current equipment are also discussed, which will enable us to meet the RFI protocol.     

行星磁场与卫星引力及其相对运动的统计关系

从知道某些天体具有磁场起，人们就对其磁场的起源提出种种解释，例如有电池说，转子说，化石说，发电机说等等。但由于这些学说都分别与某些观测事实相抵触而未被公认，因此星球磁场的起源一直是未能解决的命题。余先河先生提出，星球的磁场起源可能与所受的引力有关，行星的磁场强度正比于其所受卫星的引力；正比于卫星与行星的引力连线转动的相对角速度。本文对这两方面的命题分别进行了相关分析，得到其相关系数分别为：ｒ＝０．８４８１和ｒ＝０．８４２５，它们都在ａ＝０．０１的信度水平上相关。结果表明余新河关于行星磁场起源的设想是有基础的。本文还对其统计结果和可能机制进行了讨论。     

利用MapReduce进行批量遥感影像瓦片金字塔构建

在分析面向瓦片金字塔并行构建任务分解的基础上,提出了一种利用MapReduce进行批量遥感影像瓦片金字塔并行构建的方法.实验结果表明,该方法不仅在集群上快速、有效地解决了单机上难以解决的大规模批量遥感影像瓦片金字塔的构建操作,而且具有良好的可扩展性.同时,该算法可作为大规模遥感影像并行处理的基础框架,非常容易扩展到高效能影像特征提取、遥感影像融合以及影像增量计算等其他海量遥感影像处理任务中.     

华北地台前寒武花岗岩类、陆壳演化与克拉通形成

通过华北前寒武纪花岗岩类的研究,提出英云闪长岩和奥长花岗岩（Ｔ１Ｔ２）代表不成熟陆壳组成,Ｔ１Ｔ２Ｇ１Ｇ２代表半成熟陆壳组成,花岗闪长岩和花岗岩（Ｇ１Ｇ２）代表成熟陆壳组成。讨论了大陆根的形成与性质。识别出华北地台内１０个太古陆核。讨论了中太古代初始陆核、新太古代陆核;新太古代末两个微大陆尺度的陆核的形成;早元古代两个成熟陆核的构造拼合并形成华北克拉通     

铜镍硫化物矿床的成冈——以诺里尔斯克（俄罗斯）和金川（中国）为例

与超基性岩浆作用有关的铜镍硫化物矿床主要有两种成矿建造,一种为含铬建造,另一种为含铂建造。尖晶石类矿物成分的变化清楚地反映了这两类建造的成矿属性,含铬建造的尖晶石属于铬铁矿－尖晶石系列,含铂建造中则为尖晶石－磁铁矿系列。从含铬建造向含铂建造转变的原因,可以解释为超基性岩艇中硫的作用增加,从而引起反应：４ＦｅＯ＋Ｓ＝ＦｅＳ＋Ｆｅ３Ｏ４（磁铁矿）,同时分散性铂族元素的专属性特征也发生相应变化（Ｒｕ＋Ｏｓ＋Ｉｒ）→（Ｐｔ＋Ｐｄ）。因此,含铬建造中主要富含Ｒｕ、Ｏｓ和Ｉｒ,而含铂建造中则富含Ｐｔ和Ｐｄ。超基性岩浆作用中硫的化学活动性增加与基碱度增加直接有关。因此,含铂的超基性岩大多数情况下与富碱的玄武岩形成共生组合,当富铁熔浆发生硫化作用时,将会导致硫化物与硅酸岩熔浆的不混融,从而形成矿浆,据此,金川含铂铜镍矿石不是矿     

泥鳅对铀的富集、释放和生物富集规律的研究

试验在半静态条件下 ,研究了泥鳅鱼对铀的富集、释放和生物规律。测出泥鳅对铀的生物富集系数 (BCF) ,铀在泥鳅体内的释放过程可用双区一级动力学模型很好地描述 ,并得出表达式。