砂质海滩地形动力分类研究进展

海滩状态是一个地形与水动力相互作用的三维地形动力问题.国外对海滩状态的地形动力分类已开展了大量卓有成效的研究工作,既包括波控、小潮、开阔海岸海滩状态的研究,也包括波控、不同潮差海岸海滩类型的研究和岬间海岸海滩类型的研究.文中回顾并概括了自20世纪70年代至今国外在砂质海滩地形动力分类方面代表性的研究工作,这些对于我国的...     

Astrophysical Implications of the Recent Shocked Deuterium Experiments

In the last few years, deuterium has been the focus of a high level of laboratory activity that was sparked by a disagreement on the experimental value of the maximum compression along the Hugoniot. Astrophysically, the uncertainty in the EOS of hydrogen is most consequential in models of the interiors of Jupiter and Saturn since a significant fraction of their mass falls in the region where the EOS uncertainty is largest. We present a study of the range of interior structures allowed by the shock-compression experiments on deuterium and constrained by astrophysical observations of the two planets. We find that the EOS uncertainty must be reduced to less than 3% along the planet’s isentrope to get good interior models of Jupiter. These models provide values for the mass of a core of heavy elements (other than H and He) and the total mass of heavy elements in these planets. The amount and distribution of heavy elements are quite sensitive to the EOS of hydrogen and constitute important clues to their formation process.     

Chromothermal oscillations and collapse of strange stars to black holes: astrophysical implications

We study the effects of temperature on strange stars. It is found that the maximum mass of the star decreases with the increase of temperature, as at high temperatures the equations of state become softer. Moreover, if the temperature of a strange star increases, keeping its baryon number fixed, its gravitational mass increases and its radius decreases. This leads to a limiting temperature, where it turns into a black hole. These features are the result of a combined effect of the change of gluon mass and the quark distribution with temperature. We report on a new type of radial oscillation of strange stars, driven by what we call 'chromothermal' instability. We also discuss the relevance of our findings in the astrophysics of core collapse supernovae and gamma-ray bursts.     

黄土高原滑坡灾害形成动力学机制

受多路径等未模型化误差影响,全球卫星导航系统（global navigation satellite system,GNSS）监测序列中出现的一些异常波动现象会对精准预警产生干扰,甚至造成漏警、误警等严重后果。针对滑坡灾害体的状态特征信息在GNSS解算过程中未被充分利用的问题,分析了GNSS灾害监测中的状态空间模型,提出了一种顾及灾害体状态特征的实时滤波算法,通过滑动窗口大小的自适应调整,对监测点历史历元解算结果进行状态方程建模,并在当前历元参数估计时进行卡尔曼滤波的状态更新,得到更加可信的实时解算序列。黄土滑坡实验表明,与常规结果相比,该算法的浮点解+固定解精度分别在东、北、天方向提升了97.6%、87.5%、89.6%;单固定解精度分别提升了50.0%、14.3%、18.8%;模糊度固定率由97.1%提升至99.9%。该算法在提高解算结果精度的同时,也提升了模糊度的固定率,有效降低了异常序列波动对灾害监测与预警的影响。     

青藏块体东北缘地壳水平运动状态

应用青藏块体东北缘1999～2003年多期GPS观测资料，计算了不同时段GPS点水平运动速率。通过分析发现：甘青块体可分为东部块体和西部块体，东、西部块体的运动状态存在明显的差异；受2001年11月14日昆仑Ms8．1地震的影响，震后地壳运动状态发生了明显的改变。     

Late Holocene slip rate and average recurrence interval of great earthquakes on the Shangzhi segment of the Yilan‐Yitong Fault Zone,northeastern China: Constraints from paleo‐earthquakes and historical written records

The Yilan‐Yitong Fault Zone (YYFZ) is considered to be the key branch of the Tancheng‐Lujiang Fault Zone (TLFZ) in northeastern China. Although the Mesozoic and early Cenozoic deformation of the YYFZ has been studied intensively over the past century, few estimates of slip rate and recurrence interval of large earthquakes in the late Quaternary, which are the two most important parameters for understanding the potential seismic hazard of this crucial structure, were obtained. Based on integrated interpretations of high resolution satellite images and detailed geologic and geomorphic mapping, linear landforms were identified, including fault scarps and troughs, along the Shangzhi segment of the YYFZ, which exceeds 25 km in length. Synthesized results of trench excavations and differential GPS measurements of terrace surfaces indicate that two events (E1, E2) occurred along the Shangzhi segment during the late Holocene, which resulted in 3.2 ±0.1 m of total vertical co‐seismic displacement with clear features of thrust motion. ¹⁴C dating of samples suggests that event E1 occurred between 440 ±30 years BP and 180 ±30 years BP and that event E2 occurred between 4 090 ±30 years BP and 3 880 ±30 years BP, which indicates that the minimum vertical slip rate of the Shangzhi segment of the YYFZ has been approximately 0.8 ±0.03 mm/year during the late Holocene. Constraints from paleo events and the slip rate suggest that the average recurrence interval of major earthquakes on the YYFZ is 3 800 ±200 years. Historical documents in Korea show that event E1 possibly corresponds to the earthquake that occurred in AD 1810 (the Qing Dynasty in Chinese history) in the Ningguta area, which had surface‐wave magnitude (Ms) of 6.8–7.5. Studies of kinematics show that the right‐lateral strike‐slip with a reverse component has been dominant along the YYFZ during the late Holocene.     

大嵛山附近海域游泳动物种类组成和资源现状及其变化分析

2006年1月～10月福建闽东大嵛山附近海域游泳动物调查研究结果表明,该海域的游泳动物有97种,其中鱼类51种（软骨鱼1种,硬骨鱼类50种）,隶属于9目24科42属;甲壳类42种,隶属于2目15科20属;头足类4种,隶属于3目3科3属.暖水性种类为33种,占鱼类总种数的64.7%;暖温性鱼类18种,占鱼类总种数的35.3%,未出现冷温性和冷水性鱼类.种类数的季节变化依次呈夏季〉冬季〉秋季〉春季.生物量的季节变化,依次呈夏季〉秋季〉春季〉冬季;而生物量尾数的季节变化,依次呈夏季〉春季〉秋季〉冬季.平均单位网次渔获生物量和密度分别为9.53kg/h和1 319 ind/h.生物量优势种和密度优势种分别为大黄鱼和中华管鞭虾.扫海面积法估算年平均现存资源量为57 370 ind/km^2和404.51kg/km^2.同时,本文对该海域游泳生物的资源结构现状与历史调查数据作了对比分析,并讨论了多样性结构与生物量的季节性变化规律.结果表明,该海域渔业资源有严重衰退的现象,多样性结构与生物量的季节性变化并不具有必然的一致性.     

膨胀地球基本参数的初值及其平均变化率

本文讨论了地球膨胀过程的初始半径R0、膨胀起始时间t0以及半径R、转动惯量I、地表重力加速度g和反映地球内部物质分布状态参数y等膨胀基本参数的平均变化率。研究结果表明,在地球的地质年龄之内,地球膨胀的初始半径R0>4619km,膨胀的起始时间t0>43.8×102Ma,膨胀过程中的地球半径R、物质分布状态参数y、转动惯量I、地表重力加速度g和表面积S随时间的平均变化率分别为:dR/dt=4×10-4m/a,dy/dt=-6.7×1012/a,dI/dt=8.49×1027kg·m~2/a,dg/dt=-1.23×10-10kg·s-2/a和ds/dt=6.41×104m2/a。地球膨胀过程中的半径平均增长率,是首次用天文学方法研究得出,且该值介于其他作者用古地磁、古地理等方法所求得的地球半径增长率若干数值之间。     

马尔可夫链模型在地下水水位预测中的应用

作者将鲁南地区一水文观测孔的９２次地下水水位月平均监测数据,划分了１０种状态范围,运用马尔可夫链模型,对未来地下水水位进行状态范围预测。在与实际监测资料进行对比的基础上,验证了马尔可夫链理论在地下水水位预测中的可行性及可靠性,并对运用中的具体问题进行了探讨。