中国物理海洋学研究70年:发展历程、学术成就概览   总被引：2，自引：2，他引：0  

魏泽勋  郑全安  杨永增  刘克修  徐腾飞  王凡  胡石建  谢玲玲  李元龙  杜岩  周磊  林霄沛  胡建宇  朱建荣  李均益  张正光  侯一筠  刘泽  田纪伟  黄晓冬  管玉平  刘志宇  杨庆轩  赵玮  宋振亚  刘海龙  董昌明  于卫东  连涛  陈朝晖  史久新  雷瑞波  刘煜  于福江  尹宝树  陈戈  王岩峰  李整林  熊学军  汪嘉宁  李晓峰  王永刚 《海洋学报》2019,41(10):23-64

本文概略评述新中国成立70年来物理海洋学各分支研究领域的发展历程和若干学术成就。中国物理海洋学研究起步于海浪、潮汐、近海环流与水团，以及以风暴潮为主的海洋气象灾害的研究。随着国力的增强，研究领域不断拓展，涌现了大量具有广泛影响力的研究成果，其中包括:提出了被国际广泛采用的“普遍风浪谱”和“涌浪谱”，发展了第三代海浪数值模式；提出了“准调和分析方法”和“潮汐潮流永久预报”等潮汐潮流的分析和预报方法；发现并命名了“棉兰老潜流”，揭示了东海黑潮的多核结构及其多尺度变异机理等，系统描述了太平洋西边界流系；提出了印度尼西亚贯穿流的南海分支(或称南海贯穿流)；不断完善了中国近海陆架环流系统，在南海环流、黑潮及其分支、台湾暖流、闽浙沿岸流、黄海冷水团环流、黄海暖流、渤海环流，以及陆架波方面均取得了深刻的认识；从大气桥和海洋桥两个方面对太平洋–印度洋–大西洋洋际相互作用进行了系统的总结；发展了浅海水团的研究方法，基本摸清了中国近海水团的分布和消长特征与机制，在大洋和极地水团分布及运动研究方面也做出了重要贡献；阐明了南海中尺度涡的宏观特征和生成机制，揭示了中尺度涡的三维结构，定量评估了其全球物质与能量输运能力；基本摸清了中国近海海洋锋的空间分布和季节变化特征，提出了地形、正压不稳定和斜压不稳定等锋面动力学机制；构建了“南海内波潜标观测网”，实现了对内波生成–演变–消亡全过程机理的系统认识；发展了湍流的剪切不稳定理论，提出了海流“边缘不稳定”的概念，开发了海洋湍流模式，提出了湍流混合参数化的新方法等；在海洋内部混合机制和能量来源方面取得了新的认识，并阐述了混合对海洋深层环流、营养物质输运等过程的影响；研发了全球浪–潮–流耦合模式，推出一系列海洋与气候模式；发展了可同化主要海洋观测数据的海洋数据同化系统和用于ENSO预报的耦合同化系统；建立了达到国际水准的非地转(水槽/水池)和地转(旋转平台)物理模 型实验平台；发展了ENSO预报的误差分析方法，建立了海洋和气候系统年代际变化的理论体系，揭示了中深层海洋对全球气候变化的响应；初步建成了中国近海海洋观测网；持续开展南北极调查研究；建立了台风、风暴潮、巨浪和海啸的业务化预报系统，为中国气象减灾提供保障；突破了国外的海洋技术封锁，研发了万米水深的深水水听器和海洋光学特性系列测量仪器；建立了溢油、危险化学品漂移扩散等预测模型，为伴随海洋资源开发所带来的风险事故的应急处理和预警预报提供科学支撑。文中引用的大量学术成果文献(每位第一作者优选不超过3篇)显示，经过70年的发展，中国物理海洋学研究培养了一支实力雄厚的科研队伍，这是最宝贵的成果。这支队伍必将成为中国物理海洋学研究攀登新高峰的主力军。  相似文献   

基于Landsat数据的近30年上海大陆岸线变化分析          下载免费PDF全文

钱静  栾奎峰  陆雪骏  朱卫东  邱振戈 《海洋测绘》2020,40(5):63-68

为了研究上海大陆岸线的最新变化,以5年为间隔,选取1988~2019年间的近30年多期Landsat遥感影像,采用多尺度分割和光谱分割相结合的分割方法,提取影像中研究区域的水边线,并利用同年不同时相的水边线和平均大潮高潮位数据进行潮位校正,获取相对准确的海岸线位置。使用线性回归速率方法(LRR)对大陆岸线的外扩距离和速度变化进行了统计,同时对上海大陆岸线长度和面积的时空变化进行了分析。结果表明,从1988~2019年,上海大陆岸线总长度增加了10.4km,增幅达5.19%,长度变化呈“减增减”的趋势。海岸线的平均外扩距离为1.35km,平均LRR值为50m/年,外扩距离最大处位于南汇嘴。上海大陆沿岸总的新增土地总面积达到220.39km²。  相似文献   

Habitability analyses of aquatic bacteria     

Md. Nurul Haider  Masahiko Nishimura  Minoru Ijichi  Ching-chia Yang  Wataru Iwasaki  Kazuhiro Kogure 《Journal of Oceanography》2018,74(2):197-207

Habitability is defined as an ability of an organism to inhabit different environments. Habitability of organisms, however, cannot be inferred from analyses such as a whole genome or community structures. A recently developed database, the MetaMetaDB, gives us information from what kind of environments one particular 16S rRNA sequence data has ever been obtained, and thus enables us to infer the habitability of the bacterium in question. In order to check the applicability of this database to study the habitability of aquatic bacteria, samples collected at two Naka River stations, one estuarine station from Naka River Estuary, two coastal stations at Oarai in Ibaraki Prefecture, Japan and one station in the Kuroshio Current of the western North Pacific were examined. The phylotypes were tracked against the MetaMetaDB and it was reasonably found that the low-salinity stations were dominated by sequences with “freshwater and groundwater”, “human” and “wastewater” habitat identities, while the high-salinity stations were dominated by those with a “marine” identity. The phylotypes of low-salinity stations with a particular habitat identity were absent or rare in the high-salinity stations and vice versa. The MetaMetaDB also showed that sequences of Cyanobacteria or related phylogenetic groups may be present in the human gut, as well as the probable distribution of the relatives (ancestors/descendants/siblings) of some bacteria. These overall findings proved that the MetaMetaDB is useful as a new tool to infer microbial habitability and it gives us new information on the possible origin and ecology of microorganisms in the environments.  相似文献   

Tide-related Changes in mRNA Abundance of Aromatases and Estrogen Receptors in the Ovary and Brain of the Threespot Wrasse <Emphasis Type="Italic">Halichoeres trimaculatus</Emphasis>     

Dae-Ju Oh  Sung-Pyo Hur  Selma Bouchekioua  Yuki Takeuchi  Shingo Udagawa  Neelakanteswar Aluru  Yong-Ju Park  Ji-Gweon Park  Se-Jae Kim  Thomas W. Moon  Mathilakath M. Vijayan  Akihiro Takemura 《Ocean Science Journal》2018,53(2):239-249

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Dark energy cosmological models with cosmic string     

T. Vinutha  V. U. M. Rao  Bekele Getaneh  Molla Mengesha 《Astrophysics and Space Science》2018,363(9):188

In this paper we have studied the anisotropic Kantowski-Sachs, locally rotationally symmetric (LRS) Bianchi type-I and LRS Bianchi type-III geometries filled with dark energy and one dimensional cosmic string in the Saez-Ballester theory of gravitation. To get physically valid solution we take hybrid expansion law of the average scale factor which is a product of power and exponential type of functions that results in time dependent deceleration parameter (\(q\)). The equation of state parameter of dark energy (\(\omega _{\mathit{de}}\)) has been discussed and we have observed that for the three models it crosses the phantom divide line (\(\omega _{\mathit{de}} = -1\)) and shows quintom like behavior. The density of dark energy (\(\rho _{\mathit{de}}\)) is an increasing function of redshift and remains positive throughout the evolution of the universe for the three models. Moreover in Kantowski-Sachs and LRS Bianchi type-I geometries the dark energy density dominates the string tension density (\(\lambda \)) and proper density (\(\rho \)) throughout the evolution of the universe. The physical and geometrical aspects of the statefinder parameters (\(r,s\)), squared speed of sound (\(v_{s}^{2} \)) and \(\omega _{\mathit{de}}\)–\(\omega ^{\prime }_{\mathit{de}}\) plane are also discussed.  相似文献   

An on Orbit Determination of Point Spread Functions for the <Emphasis Type="Italic">Interface Region Imaging Spectrograph</Emphasis>     

Hans Courrier  Charles Kankelborg  Bart De Pontieu  Jean-Pierre Wülser 《Solar physics》2018,293(9):125

Using the 2016 Mercury transit of the Sun, we characterize on orbit spatial point spread functions (PSFs) for the Near- (NUV) and Far- (FUV) Ultra-Violet spectrograph channels of NASA’s Interface Region Imaging Spectrograph (IRIS). A semi-blind Richardson–Lucy deconvolution method is used to estimate PSFs for each channel. Corresponding estimates of Modulation Transfer Functions (MTFs) indicate resolution of 2.47 cycles/arcsec in the NUV channel near 2796 Å and 2.55 cycles/arcsec near 2814 Å. In the short (\({\approx}\,1336~\mathring{\mathrm{A}}\)) and long (\({\approx}\,1394~\mathring{\mathrm{A}}\)) wavelength FUV channels, our MTFs show pixel-limited resolution (3.0 cycles/arcsec). The PSF estimates perform well under deconvolution, removing or significantly reducing instrument artifacts in the Mercury transit spectra. The usefulness of the PSFs is demonstrated in a case study of an isolated explosive event. PSF estimates and deconvolution routines are provided through a SolarSoft module.  相似文献   

Template-based classification of SDSS-<Emphasis Type="BoldItalic">GALEX</Emphasis> point sources     

Ayesha Anjum  Mousumi Das  Jayant Murthy  S. B. Gudennavar  Rajesh Gopal  S. G. Bubbly 《Journal of Astrophysics and Astronomy》2018,39(5):61

We have classified a sample of 37,492 objects from SDSS into QSOs, galaxies and stars using photometric data over five wave bands (u, g, r, i and z) and UV GALEX data over two wave bands (near-UV and far-UV) based on a template fitting method. The advantage of this method of classification is that it does not require any spectroscopic data and hence the objects for which spectroscopic data is not available can also be studied using this technique. In this study, we have found that our method is consistent by spectroscopic methods given that their UV information is available. Our study shows that the UV colours are especially important for separating quasars and stars, as well as spiral and starburst galaxies. Thus it is evident that the UV bands play a crucial role in the classification and characterization of astronomical objects that emit over a wide range of wavelengths, but especially for those that are bright at UV. We have achieved the efficiency of 89% for the QSOs, 63% for the galaxies and 84% for the stars. This classification is also found to be in agreement with the emission line diagnostic diagrams.  相似文献   

Maximizing the community exploitation of the VLTI 2nd-generation instruments     

Stefan Kraus  Paulo Garcia  Guy Perrin 《Experimental Astronomy》2018,46(3):511-516

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Response of soil aggregate disintegration to the different content of organic carbon and its fractions during splash erosion     

Hairu Li  Gang Liu  Ju Gu  Hong Chen  Hongqiang Shi  Mohamed A. M. Abd Elbasit  Feinan Hu 《水文研究》2021,35(2):e14060

Aggregate disintegration is a critical process in soil splash erosion. However, the effect of soil organic carbon (SOC) and its fractions on soil aggregates disintegration is still not clear. In this study, five soils with similar clay contents and different contents of SOC have been used. The effects of slaking and mechanical striking on splash erosion were distinguished by using deionized water and 95% ethanol as raindrops. The simulated rainfall experiments were carried out in four heights (0.5, 1.0, 1.5 and 2.0 m). The result indicated that the soil aggregate stability increased with the increases of SOC and light fraction organic carbon (LFOC). The relative slaking and the mechanical striking index increased with the decreases of SOC and LFOC. The reduction of macroaggregates in eroded soil gradually decreased with the increase of SOC and LFOC, especially in alcohol test. The amount of macroaggregates (>0.25 mm) in deionized water tests were significantly less than that in alcohol tests under the same rainfall heights. The contribution of slaking to splash erosion increased with the decrease of heavy fractions organic carbon. The contribution of mechanical striking was dominant when the rainfall kinetic energy increased to a range of threshold between 9 J m⁻² mm⁻¹ and 12 m⁻² mm⁻¹. This study could provide the scientific basis for deeply understanding the mechanism of soil aggregates disintegration and splash erosion.  相似文献   

北太平洋副热带模态水盐度的年代际变化     

胡睿坤  边志刚  刘子洲  刘聪  翟方国  顾艳镇 《中国海洋大学学报(自然科学版)》2020,(2):9-21

副热带模态水(Subtropical Mode Water;STMW)在气候变化中起着重要作用。本文利用全球高分辨率数值模拟结果,研究了北太平洋STMW核心层盐度(Core Layer Salinity;CLS)的年代际变化及其物理机制。结果表明,CLS存在显著的年代际变化,其空间分布则与背景流场分布特征有关。侵蚀区CLS滞后生成区CLS约1~2年,这主要是海流平流输运引起的。生成区内,STMW的季节循环一般可分为生成期(12-4月)、隔离期(5-6月)和侵蚀期(7-11月),生成期混合层盐度(Mixed Layer Salinity;MLS)决定着隔离期和侵蚀期的CLS,而MLS年代际变化则主要由同太平洋年代际涛动存在负相关性的海表面淡水通量的变化引起。  相似文献