数字滤波技术在潮汐观测中的应用研究

潮汐是重要的海洋物理要素。瞬时变化的海面高度信息除了包含潮汐信息外,还包括波浪等高频干扰信息,因此需要对干扰信息进行滤除。如何从获取到的海面瞬时高度变化中提取出潮汐信息就成为一个关键问题。海洋学中通常是通过低通滤波来获取低频的潮汐信息。通过分析常用的3种低通数字滤波的方法,即滑动平均法、快速傅里叶变换法和小波变换法,对3种低通滤波方法应用于潮汐数据处理的效果进行了比较分析,得出滑动平均法在潮汐信息提取中具有较高应用价值的结论。     

综合物化探方法在深冲矿区铀多金属矿勘探中的应用

通过研究深冲铀矿区γ能谱铀异常、氡浓度异常特征和激电异常特征,探索矿区范围岩体、断裂构造和蚀变带与物化探信息显示特征的关系。据此,结合矿区地质特征,总结物化探方法应用效果,矿致异常综合特征。     

西藏盐湖沉积物：一种潜在的铷、铯资源

铷、铯是我国战略性关键矿产资源。西藏盐湖卤水中赋存着丰富的铷、铯资源,但是品位普遍低于10 mg/L。根据热泉与盐湖锂、铷、铯等元素的补给关系和含量差异特征及铷、铯极易被黏土矿物吸附等特点,推测盐湖沉积物中赋存一定规模的铷、铯资源。为验证该推测,本文选取西藏拉果错、聂尔错、依布茶卡、当穹错、扎布耶茶卡等5个典型盐湖,采集卤水和沉积物样品各5件,开展水体中铷、铯含量和沉积物矿物成分分析,结合沉积物分相淋滤实验,得出如下结论：西藏拉果错、当穹错、聂尔错盐湖卤水铷、铯含量和资源量与其补给量差异显著,大量的铷、铯资源消耗于盐湖沉积物中;盐湖沉积物中的铷、铯含量远高于卤水。铷、铯在沉积物水溶相、碳酸盐相中含量较低,主要以吸附形式赋存于黏土矿物(主要为伊利石),吸附点位包括基面位置、难解吸的磨损边缘及层间位置。盐湖沉积物铷、铯资源量远超大型矿床规模,黏土矿物中铷、铯含量高达100 n×10-6,超过固体盐类矿产综合评价指标,相较于现有盐湖钾产品中的铷资源、含铯硅华中的铯资源开发,具有较好的开发利用性,是一种潜在的铷、铯资源。本研究成果有助于完善盐湖铷、铯富集成矿机制,并为高效开发盐湖中的铷、铯资源提供理论支撑。     

利用树轮宽度重建黄河源区1618—2009年5—6月最高气温

利用采集自青海省雪山乡的祁连圆柏建立树轮宽度标准年表,将标准年表与黄河源区内4个气象站各气象要素作相关分析,结果显示整个源区5—6月最高气温与标准年表相关性最显著,相关系数为-0.65。根据相关分析结果,重建了黄河源区1618—2009年5—6月最高气温距平序列,重建方程经过逐一剔除检验,方差解释量达42.2%,具有一定的可靠性。重建序列在近400年间先后经历了8个较暖时间段和8个较冷时间段,暖期时段有1644—1656、1727—1746、1786—1797、1817—1835、1860—1885、1916—1934、1952—1968和1992—2005年,冷期的时段分别为1632—1643、1657—1696、1747—1764、1798—1816、1836—1859、1898—1915、1935—1951和1969—1991年。对比本次重建序列与杂多、青藏高原东部以及长江源的气温重建序列,发现以上序列在公共时段变化趋势一致,另外,一些文献和历史记载也证实了此次重建的可靠性。     

低温雨雪过程的粒子群-神经网络预报模型

利用逐日气温和降水量数据、NCEP/NCAR再分析资料以及预报场资料,通过分析提取我国南方区域持续性低温雨雪过程及其预报因子,使用粒子群-神经网络方法建立非线性的统计集合预报模型 (PSONN-EPM),对我国南方区域持续性低温雨雪过程进行预报试验。结果表明:以过程的冷湿程度及影响范围为标准,将低温雨雪过程分为一般过程和严重过程,并建立不同的预报模型效果较好。通过10 d独立样本预报试验看,基于粒子群-神经网络方法建立的集合预报模型比基于逐步回归方法建立的预报模型的预报平均相对误差小,对严重过程预报能力高于对一般过程预报,且这种非线性统计集合建模方法在建模过程中不需要调整神经网络参数,在实际预报业务中值得尝试。     

柳州夏季一次雨夹冰雹的天气过程分析

利用常规地面观测、柳州地面自动站、FY-2C卫星、柳州和河池的多普勒天气雷达观测资料,对2014年7月22日夏季柳州发生的一次短暂的雨夹冰雹天气过程的环境条件和雷达产品特征进行分析,主要结果如下:受副高和台风外围气流影响,柳州全市出现了37℃以上大范围的高温天气,天气尺度和中尺度的上升运动较弱,局地性质的加热作用导致大气的不稳定度加强而诱发对流云系进一步发展造成的;雷达显示的冰雹云的最大基本反射率因子为65d BZ,强回波区面积小;风速的切变和辐合上升运动小,0℃层高度较高,不利于对流系统的发展和维持。     

Relations between integrated and monochromatic luminosities of flat-spectrum radio quasars

We employ a sample of 362 flat-spectrum radio quasars (FSRQs) to calculate their integrated luminosities by integrating the spectral energy distribution (SED) constructed with multi-band (radio,IR,optical,UV and X-ray) data.We compare these luminosities with those estimated from monochromatic luminosities by multiplying them by the conventional bolometric correction factors.Our analysis shows that the integrated luminosities calculated from the SED are much larger than the bolometric luminosities estimated ...     

Iron and phosphorus effects on the growth of Cryptomonas sp. (Cryptophyceae) and their availability in sediments from the Pearl River Estuary, China

Based on lab-culture experiments analyzing limitation and combination of iron and phosphorus on the growth of Cryptomonas sp. (Cryptophyceae), and the study of accumulation and release of Fe-bound P in sediment cores collected from the marine region of the Pearl River Estuary, China, reasons for the high frequency of phytoplankton bloom therein are discussed. Results show that the combined effect of Fe and P can obviously accelerate algal development, and the optimum culture conditions maintaining maximum growth rate are 0.05 μM Fe and 50 μM P. Cellular contents of Fe and P is consistent and the P:Fe molar ratio is 159:1. The optimum range of the P:Fe molar ratio in culture experiments for cell incubation is 500–1400. The vertical trends of total Fe and total P variations in sediments are parallel. Fe-bound P is the main species of inorganic sedimentary P. Through continuous leaching with agitation, 34–80% of exchangeable P and 4–23% of exchangeable Fe are concurrently released from the surficial sediments. This is a possible way by which nutrients are made available to phytoplankton. These factors might be responsible for a high frequency of harmful algal blooms in the Pearl River Estuary.     

Contributors to chromium isotope variation of meteorites

We report the results of a comprehensive, high precision survey of the Cr isotopic compositions of primitive chondrites, along with some differentiated meteorites. To ensure complete dissolution of our samples, they were first fused with lithium borate-tetraborate at 1050-1000 °C. Relative to the NIST Cr standard SRM 3112a, carbonaceous chondrites exhibit excesses in ⁵⁴Cr/⁵²Cr from 0.4 to 1.6ε (1ε = 1 part in 10,000), and ordinary chondrites display a common ⁵⁴Cr/⁵²Cr deficit of ∼0.4ε. Analyses of acid-digestion residues of chondrites show that carbonaceous and ordinary chondrites share a common ⁵⁴Cr-enriched carrier, which is characterized by a large excess in ⁵⁴Cr/⁵²Cr (up to 200ε) associated with a very small deficit in ⁵³Cr/⁵²Cr (<2ε). We did not find ⁵⁴Cr anomalies in either bulk enstatite chondrites or in leachates of their acid-digestion residues. This either requires that the enstatite chondrite parent bodies did not incorporate the ⁵⁴Cr anomaly carrier phase during their accretion, or the phase was destroyed by parent body metamorphism. Chromium in the terrestrial rocks and lunar samples analyzed here show no deviation from the NIST SRM 3112a Cr standard. The eucrite and Martian meteorites studied exhibit small deficits in ⁵⁴Cr/⁵²Cr. The ⁵⁴Cr/⁵²Cr variations among different meteorite classes suggest that there was a spatial and/or temporal heterogeneity in the distribution of a ⁵⁴Cr-rich component in the inner Solar System.We confirm the correlated excesses in ⁵⁴Cr/⁵²Cr and ⁵³Cr/⁵²Cr for bulk carbonaceous chondrites, but the new data yield a steeper slope (∼6.6) than that reported in Shukolyukov and Lugmair (2006). The correlated excesses may affect the use of the Mn-Cr chronometer in carbonaceous chondrites. We could not confirm the bulk carbonaceous chondrite Mn-Cr isochron reported by Shukolyukov and Lugmair (2006) and Moynier et al. (2007), mostly because we find much smaller total variations in ε⁵³Cr (∼0.2). All bulk chondrites have small ε⁵³Cr excesses (up to 0.3) relative to the Earth, most likely reflecting the sub-chondritic Mn/Cr ratio of the Earth. The ε⁵³Cr variations in chondrites do seem to grossly correlate with Mn/Cr and yield an initial Solar System ⁵³Mn/⁵⁵Mn value of 5.4(±2.4) × 10⁻⁶, corresponding to an absolute age of 4566.4 (±2.2) Ma.Nuclear interactions with cosmic rays result in coupled excesses in ε⁵⁴Cr and ε⁵³Cr with a ∼4:1 ratio in phases with high Fe/Cr. These are most dramatically demonstrated in the iron meteorite Carbo, showing excesses in ε⁵⁴Cr of up to 140ε. These new results show that the Mn-Cr chronometer should be used with caution in samples/minerals with high Fe/Cr and long cosmic ray exposure ages.