黄海透光层悬浮半导体矿物组成及其促进微生物胞外电子传递过程初探     

刘佳  孙元  任桂平  鲁安怀  李艳  丁竑瑞 《岩石矿物学杂志》2020,39(1):96-104

在地球上最为活跃的海洋透光层体系中,矿物-微生物交互作用的形式十分丰富。系统采集了黄海近海透光层水体样品,测试分析发现其中分布大量悬浮半导体矿物及微生物群落。通过电感耦合等离子质谱仪(ICP-MS)、环境扫描电子显微镜(ESEM)及配有的EDX能谱仪,从宏观到微区对悬浮颗粒矿物的化学元素组成进行了测试分析,发现其主要矿物组成元素为Si、O、Na、K、Ca、Al等,且含有较高含量的Mn、Fe、Ti等金属元素;通过X射线衍射光谱(XRD)、拉曼光谱(Raman)测试从整体到局部分析悬浮颗粒矿物的物相组成,发现其主要组成矿物为石英、钠长石、方解石、云母和绿泥石等,还有锐钛矿、金红石、板钛矿、针铁矿等铁、钛金属氧化物半导体矿物。通过16S rRNA高通量测序分析海水中主要微生物群落为Proteobacteria、Actinobacteria、Bacteroidetes、Planctomycetes、Woeseia、Fluviicola等,并通过构建双室反应体系对海水微生物与悬浮矿物间氧化还原作用及胞外电子传递过程进行了表征,结果显示增加海水悬浮矿物作为电子受体后,体系开路电压由330. 80 mV提升至426. 59 mV,提升比率达130%,最大输出功率由8. 376 9 mW/m^2提升至12. 096 8 mW/m^2,为原体系的1. 44倍。实验研究表明,海水透光层悬浮矿物能有效参与并促进微生物胞外电子传递过程,为后续深入研究基于电子能量传递利用的半导体矿物-微生物协同作用以及元素循环调控机制奠定初步基础。  相似文献   

A Review for the Thermophysics and the Yarkovsky and YORP Effects of Asteroidstwo     

Jiang Hao-xuan  Ji Jiang-hui 《Chinese Astronomy and Astrophysics》2019,43(1):1-22

The thermophysics of asteroids has become an important frontier for the research of asteroids in recent years. In this paper, we have introduced the thermophysical models commonly used in this field, by using these thermophysical models and combining with the data observed by the space or ground-based IR telescopes, some thermophysical parameters of asteroids, such as the thermal inertia, geometric albedo, effective diameter, surface roughness, and surface temperature, etc., can be derived. We have mentioned also the shape model and IR observation of asteroids, as well as the obtained thermophysical parameters for a part of asteroids. These thermophysical parameters can be further applied to studying the asteroids’ Yarkovsky effect, YORP effect, and so on, even can provide the relevant information for the spacecraft landing on the asteroid surface and the return mission of a spacecraft after the asteroid sampling.  相似文献   

关于我国海洋可再生能源产业化发展的思考          下载免费PDF全文

王项南  贾宁  薛彩霞  王冀  麻常雷 《海洋开发与管理》2019,36(12):14-18

为推动我国海洋可再生能源产业发展,文章论述国内和国际海洋可再生能源开发利用在资源量、政策和技术等方面的发展现状,分析我国现阶段发展海洋可再生能源存在的主要问题,并提出未来我国海洋可再生能源产业化在顶层规划、关键核心技术、公共服务平台和标准体系建设、技术示范应用、成果转化以及国际合作等方面的发展建议,从而促进我国生态文明和海洋强国建设。  相似文献   

基于岩体塑性位错理论的龙门山区域构造系统演化过程     

师皓宇  黄辅琼  马念杰  王永建  马骥  邹光华  彭瑞 《地质学报》2020,94(12):3581-3589

青藏高原对四川盆地的挤压作用导致了龙门山断裂带的形成及其山脉的隆起。本文以龙门山附近区域板块运动以及深部岩体力学特性为背景，采用FLAC3D软件模拟再现了时间跨度为700万年的龙门山区域构造系统演化过程。研究结果表明：在板块运动作用下，F1、F2和F3断层依次形成，贯通的断层对地表的抬升具有较强的控制作用，当断层贯通于地表后，龙门山及其以西的川西高原持续隆起，平均抬升速率约为138mm/yr，而龙门山断裂带以东的川西坳陷只有较小的抬升量，从而导致川西高原抬升8996 m, 致使该区域产生6000m左右的落差，模拟的地形特征与目前的龙门山地形地貌基本相似。依据模拟结果与实测资料，绘制了龙门山断裂带形成及其附近区域地形地貌的演化过程图，呈现了板块挤压、断层塑性位错、地表侵蚀和沉积作用等因素共同作用对地形地貌的塑造过程。  相似文献   

中国深层地热能开采的地质条件评价     

庞忠和  罗霁  程远志  段忠丰  天娇  孔彦龙  李义曼  胡圣标  汪集旸 《地学前缘》2020,27(1):134-151

深层地热能是指深度大于3 000 m的地热能。我国深层地热能资源丰富,但是开采条件怎么样呢?本文基于地热地质学原理,结合岩石力学等相关学科的理论,提出一种对深层地热能开采条件进行评价的指标体系,对各单一指标采用专家打分的方法赋值,继而采用模糊数学定量计算和评估深层地热能资源开发的难易程度。该方法考虑了深层地热能开发利用中的增强地热系统(EGS)的环境安全问题,即传统的“刚性造储”可能带来的诱发地震等不利于地热能行业健康发展的因素,倡导“柔性造储”和广义EGS理念,强调储层属性和地物理场的整合,针对我国地热能分布与构造活动关系密切、地壳总体上活动性强、地应力高、地震频发等构造型地热特点,是对以往评价方法的补充和拓展。该方法充分利用了专家知识,发挥了模糊数学综合评估作用,给出的量化结果易于对比和使用,可以更好地支持决策。本文基于新的评估方法,利用现有的深部地热研究及勘探成果,评估了中国大陆地区九个区域深层地热能开发的难易程度,评价区包括西藏南北地堑系、云南西部火山型地热区、青海东部共和盆地以及东北、华北等。从本文的结果可以看出,我国深层地热能开采的地质条件复杂,开采难度较大。  相似文献   

多向不规则波浪作用下群墩结构上爬高的计算研究     

季新然  邹丽  任智源  柳淑学 《海洋学报》2019,41(3):35-43

波浪的方向分布对波浪的传播及其与工程结构物的作用都具有明显影响，目前现有的研究大多是基于单向波浪进行的。为了研究方向分布对群墩结构上的爬高影响，基于规则波浪与群墩作用的理论解，结合多向不规则波浪的造波方法，建立了多向不规则波浪与群墩作用的计算模型，同时进行了物理模型试验对模型的有效性进行了验证。系统地对群墩周围及表面上的波浪爬高进行了计算分析，结果表明，方向分布对波浪爬高具有较大的影响，且不同位置处的影响并不相同，在实际的工程设计中如果按照单向波浪计算，可能低估或者高估群墩周围的爬高。  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