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1.
根据2018年4月(春季)和10月(秋季)在舟山群岛外海域进行的渔业资源调查资料,分析了鱼类的种类组成、数量分布和优势种,并用典范对应分析方法分析了其与水文环境之间的关系。结果表明,舟山群岛外海域鱼类有106种,隶属于12目47科80属,春、秋季鱼类质量密度分别为210.50 kg/km2和829.06 kg/km2,尾数密度分别为8.08×103 ind/km2和165.94×103 ind/km2。春季鱼类资源密度在调查海域的西北部较高,东部较低,而秋季鱼类资源密度在东部海域较高,西北部海域较低。两个季节的鱼类优势种更替明显,春季优势种为黄鮟鱇(Lophius litulon)、日本红娘鱼(Lepidotrigla japonica)、细条天竺鲷(Apogon lineatus),秋季为细条天竺鲷、日本发光鲷(Acropom japonicum)。鱼类种数呈现显著的季节和空间变化,但是都以西部以及西北部靠近近岸岛屿的海域种类数较高,大部分鱼类栖息在50~80 m水深海域。典范对应分析结果表明,表层温度、底层温度、表层盐度是影响调查海域鱼类种类组成和数量分布的主要环境因子。 相似文献
2.
Seasonal timing of stratospheric final warming associated with the intensity of stratospheric sudden warming in preceding winter 总被引:1,自引:0,他引:1
The association of seasonal timing of stratospheric final warming events(SFWs) in spring and the occurrence of major and minor stratospheric sudden warming events(SSWs) in midwinter were investigated through statistical analysis, parallel comparison, and composite analysis, based on the NCEP-NCAR reanalysis dataset covering 1958–2012. It was found that the intensity and occurrence of winter SSW events can largely affect the timing of spring SFWs. Specifically, the SFW onset dates tend to be later(earlier) after the occurrence(absence) of winter major SSWs. However, the occurrence or absence of minor SSWs does not change the frequency of early and late SFWs. A parallel comparison of the temporal evolution of the anomalous circulation and planetary-waves between major SSW and minor SSW winters indicates that the stratospheric polar vortex(polar jet) will keep being anomalously stronger 30 days after major SSW onset. And the associated significant negative Eliassen-Palm(EP) flux anomalies can persist for as long as 45 days after major SSW events. In contrast, the circulation anomalies around the occurrence of minor SSW events can last only a few days. To further verify the possible influence of the occurrence of major SSWs on the seasonal timing of SFWs, composite analysis was performed respectively for the 21 major-SSW years, 15 minor-SSW years, and the 15 non-SSW years. Generally, planetary-wave activity in the extratropical stratosphere tends to be stronger(weaker) and the westerly polar jet is anomalously weaker(stronger) in major-SSW(non-SSW) winters. But in the following spring, the planetary-wave activity is weaker(stronger) accompanied with an anomalously stronger(weaker) stratospheric polar vortex. In spring after minor-SSW years, however, the stratospheric polar vortex and the westerly polar jet exhibit a state close to climatology with relatively gentle variations. 相似文献
3.
本博士论文在前人构建的陆面水文过程模型TOPX和区域气候模式RIEMS的耦合模式的框架基础上,针对耦合模式中RIEMS对降水和蒸散发的模拟精度较低,RIEMS和TOPX模式之间尺度不匹配等几个核心问题进行了深入细致的研究:对天气雷达资料的定量估测降水方面的研究获得了对沂沭河流域最佳的Z-R关系,并通过雷达雨量计联合校正法得到较高精度的面降雨量;采用集合卡尔曼滤波同化算法对雷达反演的面雨量及区域气候模式RIEMS的降水输出进行了数据同化方案研究,获得了更好的降水模拟效果;在RIEMS和水文模型TOPX构成的耦合模型中加入同化方案,实现了流域降水的实例模拟研究,结果表明使用同化方案明显改善了水文模拟效果。 相似文献
4.
利用Scripps海洋研究所0—400m上层海洋热含量资料和美国环境监测中心/国家大气研究中心(National Centers for Environmental Prediction/National Center for Atmospheric Research,NCEP/NCAR)的再分析资料,运用经验正交分解(empirical orthogonal function,EOF)等统计方法,研究在有ENSO影响和去除ENSO影响的情况下,前期春季印度洋热含量如何影响南海夏季风爆发。结果表明,在没有扣除ENSO信号的情况下,热带印度洋热含量EOF分解第一模态呈东西相反变化的空间分布。印度洋东部热含量为正(负)异常、西部为负(正)异常时,南海夏季风爆发较早(晚),印度洋上层热含量主要通过影响热带印度洋上空大气的垂直运动和高低层辐散辐合,进而影响季风纬向环流的强弱,来影响南海夏季风爆发的早晚。在扣除ENSO信号的情况下,印度洋热含量CEOF(conditional EOF)第一模态的空间分布类似于EOF第一模态的空间分布;第二模态表现为除小部分海区外,热带印度洋热含量呈一致变化的海盆模态。这两个模态对南海夏... 相似文献
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7.
Yuan Ma De-Yu Wang Jun Lin Shuo Dai Xue-Fei Zhang National Astronomical Observatories of China / Yunnan Astronomical Observatory Chinese Academy of Sciences Kunming China Purple Mountain Observatory Nanjing China Harvard-Smithsonian Center for Astrophysics Cambridge MA USA 《中国天文和天体物理学报》2010,10(5)
We present a statistical study of decimetric type Ⅲ radio bursts,coronal mass ejections(CMEs),and Hα flares observed in the period from July 2000 to March2005.In total,we investigated 395 decimetric type Ⅲ radio burst events,21% of which showed apparent correlation to CMEs that were associated with Hα flares.We noticed that the Hα flares which were strongly associated with CMEs were gradual events,and82% of them took place before CMEs appeared in the field of view of LASCO C2;that most of the CME-associated radio bursts started in the frequency range around750 MHz with a frequency drifting rate of several hundred MHz s-1,of which both positive and negative ones were recognized; and that the correlation of type Ⅲ radio bursts to CMEs without associated flares is fairly vague,less than 9%. 相似文献
8.
In order to study the origin of the spatial structure of the Northern Hemisphere Annular Mode (NAM),a linear stochastic model is constructed empirically from the output of a GCM run.Optimal stochastic forcing in terms of the maximum variance contribution,which may be potentially related to the maintenance of the NAM,is investigated.Theoretical analysis on the dominant non-modal response to the stochastic forcing shows that this dominance is jointly decided by the properties of forcing and the non-modal grow... 相似文献
9.
Climate variability recorded by n-alkanes of paleolake sediment in Qaidam Basin on the northeast Tibetan Plateau in late MIS3 总被引:1,自引:0,他引:1
PU Yang ZHANG HuCai LEI GuoLiang CHANG FengQin YANG MingSheng ZHANG WenXiang LEI YanBin YANG LunQing & PANG YouZhi State Key Laboratory of Lake Science Environment Nanjing Institute of Geography Limnology Chinese Academy of Sciences Nanjing China Graduate University of Chinese Academy of Sciences Beijing Key Laboratory of Boyang Lake MOE School of Environmental Chemical Engineering Nanchang University Nanchang 《中国科学:地球科学(英文版)》2010,(6)
Here we combine n-alkanes preserved in a shell bar section from Qarhan paleolake, Qaidam Basin with the other sedimentary proxies to elucidate the lake evolution process during the period 39.7 to 17.5 14C ka BP (calibrated age ranges from 43.5 to 22.4 cal. ka BP). In different stages, the n-alkane homologues exhibited different distribution modes indicative of variations in the surrounding vegetation and the hydrologic condition of the lake. The n-alkanes proxies (CPIh, ACLh, Paq) have the same trends as th... 相似文献
10.
Rui-Zhi Yang Jin Chang Jian Wu Purple Mountain Observatory Chinese Academy of Sciences Nanjing China 《中国天文和天体物理学报》2010,10(1)
Results from PAMELA and ATIC indicate that the Kaluza-Klein type dark matter particles could be the annihilation source of the observed excess of electrons and positrons.Assuming the existence of a nearby black hole with 10000–100000 solar masses and a point source boost algorithm,we apply the standard propagation model and find that the results fit the data well. 相似文献