Excitation of seasonal polar motion by atmospheric and oceanic angular momentums

A quantitative study on the seasonal polar motion excitated by the atmospheric angular momentum (AAM) and the oceanic angular momentum (0AM) has been carried out using numerical models. The results show that for the prograde and retrograde components of the seasonal polar motion (the annual polar motion and the semiannual polar motion) , the sum of excitations by both the AAM and the 0AM is closer to the observed results rather than that of the AAM only. This reflects a significant contribution of the 0AM to the seasonal polar motion.     

Statistical property of the Chandler wobble excitation function

The Chandler wobble excitation function (hereinafter, geodetic excitation) is obtained by removing the seasonal components and low frequency components with periods from several years to decades from the polar motion excitation function derived from SPACE2002 series. The geophysical excitation functions of the individual AAM, OAM, HAM, and two combined excitations of the AAM OAM and AAM OAM HAM at ld, 5d, lm and 3m intervals are statistically tested for the hypothesis of the normality, and then tested for the hypotheses of identical distribution between the geodetic and the geophysical excitations. The results show that, among the total 16 components of the two combined excitation functions at ld, 5d, lm and 3m intervals, most follow random normal processes, the hypotheses of identical distribution between the geodetic excitation and the two combined excitation are acceptable, while most of the hypotheses of identical distribution between the geodetic excitation and the individual excitations of the AAM, OAM, and HAM are rejectable. These results elucidate from a new point of view, that the excitations from AAM, OAM, and HAM are the main sources of the Chandler wobble, and the Chandler wobble excitation function is of a random normal property.     

Oceanic Cd/P ratio and nutrient utilization in the glacial Southern Ocean

During glacial periods, low atmospheric carbon dioxide concentration has been associated with increased oceanic carbon uptake, particularly in the southern oceans. The mechanism involved remains unclear. Because ocean productivity is strongly influenced by nutrient levels, palaeo-oceanographic proxies have been applied to investigate nutrient utilization in surface water across glacial transitions. Here we show that present-day cadmium and phosphorus concentrations in the global oceans can be explained by a chemical fractionation during particle formation, whereby uptake of cadmium occurs in preference to uptake of phosphorus. This allows the reconstruction of past surface water phosphate concentrations from the cadmium/calcium ratio of planktonic foraminifera. Results from the Last Glacial Maximum show similar phosphate utilization in the subantarctic to that of today, but much smaller utilization in the polar Southern Ocean, in a model that is consistent with the expansion of glacial sea ice and which can reconcile all proxy records of polar nutrient utilization. By restricting communication between the ocean and atmosphere, sea ice expansion also provides a mechanism for reduced CO2 release by the Southern Ocean and lower glacial atmospheric CO2.     

地球自转对大气海洋运动的响应

分析了地球自转的年际变化和异常变化,说明它们与热带太平洋的大气、海洋大尺度范围的年际变化——厄尔尼诺(ElNio)事件相当一致,而地球自转的异常变慢稍迟后于厄尔尼诺事件.可能由于伴随着厄尔尼诺事件大气角动量异常增加,引起了地球自转的变慢.可用天文测时资料的归算,监视日长年际变化的极小值,来预测厄尔尼诺事件的发生.     

A local positive feedback of the tropical Pacific ocean-atmosphere system on interdecadal timescales

SINCE THE 1990S, THE CLIMATIC VARIABILITY ON INTERDE- CADAL TIME SCALES BECAME THE FOCUS OF THE INTERNATIONAL CLIMATOLOGY RESEARCH MISSIONS[1―3]. ON TIME SCALES OF A DECADE OR MORE, THE OCEAN CIRCULATION PREDOMINATEDHEAT BALANCE AND HYDROLOGICAL CYCLE, S…     

A strong source of methyl chloride to the atmosphere from tropical coastal land

Methyl chloride (CH3Cl), the most abundant halocarbon in the atmosphere, has received much attention as a natural source of chlorine atoms in the stratosphere. The annual global flux of CH3Cl has been estimated to be around 3.5 Tg on the grounds that this must balance the loss through reaction with OH radicals (which gives a lifetime for atmospheric CH3Cl of 1.5 yr). The most likely main source of methyl chloride has been thought to be oceanic emission, with biomass burning the second largest source. But recent seawater measurements indicate that oceanic fluxes cannot account for more than 12% of the estimated global flux of CH3Cl, raising the question of where the remainder comes from. Here we report evidence of significant CH3Cl emission from warm coastal land, particularly from tropical islands. This conclusion is based on a global monitoring study and spot measurements, which show enhancement of atmospheric CH3Cl in the tropics, a close correlation between CH3Cl concentrations and those of biogenic compounds emitted by terrestrial plants, and OH-linked seasonality of CH3Cl concentrations in middle and high latitudes. A strong, equatorially located source of this nature would explain why the distribution of CH3Cl is uniform between the Northern and Southern hemispheres, despite their differences in ocean and land area.     

Warm tropical ocean surface and global anoxia during the mid-Cretaceous period

The middle of the Cretaceous period (about 120 to 80 Myr ago) was a time of unusually warm polar temperatures, repeated reef-drowning in the tropics and a series of oceanic anoxic events (OAEs) that promoted both the widespread deposition of organic-carbon-rich marine sediments and high biological turnover. The cause of the warm temperatures is unproven but widely attributed to high levels of atmospheric greenhouse gases such as carbon dioxide. In contrast, there is no consensus on the climatic causes and effects of the OAEs, with both high biological productivity and ocean 'stagnation' being invoked as the cause of ocean anoxia. Here we show, using stable isotope records from multiple species of well-preserved foraminifera, that the thermal structure of surface waters in the western tropical Atlantic Ocean underwent pronounced variability about 100 Myr ago, with maximum sea surface temperatures 3-5 degrees C warmer than today. This variability culminated in a collapse of upper-ocean stratification during OAE-1d (the 'Breistroffer' event), a globally significant period of organic-carbon burial that we show to have fundamental, stratigraphically valuable, geochemical similarities to the main OAEs of the Mesozoic era. Our records are consistent with greenhouse forcing being responsible for the warm temperatures, but are inconsistent both with explanations for OAEs based on ocean stagnation, and with the traditional view (reviewed in ref. 12) that past warm periods were more stable than today's climate.     

极坐标表象与轨道角动量表象

本文主要介绍希尔伯特空间的另两组基矢:极坐标表象和轨道角动量表象以及该二表象间的变换。     

干、湿大气环流模式中地表增温的经向分布及其机制

使用耦合了平板海洋的三维大气环流模式, 探究理想条件下极地增温放大现象的产生机制。实验中关闭海冰和云的辐射效应, 固定地表反照率, 并将海洋经向热量输送设置为零。通过控制地表蒸发的有无, 模拟湿大气和干大气两种情形。模拟结果显示, CO₂浓度加倍后, 湿大气环流模式中存在极地增温放大的现象, 而干大气环流模式中不存在这种现象。在干大气环流模式中, 地表增温幅度基本上不随纬度变化, 即均匀增温。湿大气环流模式中, CO₂浓度加倍导致的直接辐射强迫和水汽反馈导致的辐射效应都是热带比极地更强, 唯一能够解释湿大气中极地增温放大原因的是从赤道向极地的大气能量传输增强。在干大气环流模式中, 从赤道向极地的热量输送及其变化比湿大气弱很多, 因此无法支持极地增温放大现象。干大气中的均匀增温是CO₂的直接辐射强迫和普朗克效应相互竞争的结果。研究结果表明, 与水汽相关的经向热量输送是地球极地增温放大的关键因素, 而在基本上没有水汽的火星上, 可能不会出现极地增温放大现象。     

年际和年代际气候变化的全球时空特征比较

5利用1950－1998年全球海洋同化分析资料和全球大气再分析资料，分析比较了全球海气系统年际和年代际变化的主要时空特征。结果表明：1）全球上层海洋年际变化主要为位于热带太平洋的ENSO模态，年代际变化最显区域中纬度海洋、赤道外热带东太平洋和大西洋及南半球高纬度区域；2）全球大气年际和年代际变化均主要位于中高纬地区尤其是两极地区，在年际时间尺度上，气温异常和气压异常没有明显的对应关系，但在年代际时间尺度上，气温增暖（变冷）常常伴随着气压的降低（升高）；3）在年际时间尺度上，发生在中高纬度陆地地区的大气年际变化和主要发生在热带海洋的上层海洋年际变化没有一致性的内在联系，前主要表现为大气内部（浑沌）变化，而后主要为热带海气相互作用产生的ENSO变化；4）在年代际时间尺度上，全球海洋大气系统大约在20世纪70年代均一致性地经历了一次跃变，其结果导致80年代以来，全球大范围地区（尤其是两极和西伯利亚地区）气温明显偏暖，赤道两侧的热带东太平洋、北美和南美西海岸及非洲西海岸等海域海表温度偏高，伴随着这种全球大范围背景增暖现象，青藏高原北部地区和格陵兰岛气温具有变冷趋势，而中纬度北太平洋和南半球高纬度海域海表温度也表现为降低。     

A modeling study of relation between cloud amount and SST over western tropical pacific cloudy regions during TOGA COARE

The relationship between cloud amount and sea surface temperature (SST) over western tropical Pacific cloudy regions during TOGA COARE is investigated based on hourly grid simulation data from a two-dimensional coupled ocean-cloud resolving atmosphere model. The model is forced by the large-scale vertical velocity and zonal wind observed and derived from TOGA COARE for a 50-day period. The cloud amount becomes smaller when the ocean surface gets warmer, which is similar to previous relations obtained from observational analyses. As SST increases, the atmospheric temperature increases whereas the surface sensible heat flux decreases. The atmospheric water vapor is not sensitive to SST whereas the surface evaporation flux decreases as SST increases. These indicate that the oceanic effects do not play an important role in determining atmospheric heat and water vapor budgets. The cold atmosphere produces a larger amount of ice clouds that cover a larger area than the warm atmosphere does. The large amounts of ice clouds lead to cooling of the ocean surface through reflecting large amount of solar radiation back to the space. Thus, the negative correlation between the cloud amount and SST only accounts for the important atmospheric effects on the ocean.     

希尔伯特空间的极坐标表象与轨道角动量表象

在讨论希尔伯特空间中的极坐标表象与轨道角动量表象的基础上导出了二表象间的变换关系式.     

转动类体育动作几个知识点的分析

转动普遍存在于体育动作中．在一些体育文献中，对转动的分析不很清楚，有时存在概念上的模糊或逻辑上的混乱．本文从运动学和动力学的角度予以澄清     

The Earth's 'hum' is driven by ocean waves over the continental shelves

Observations show that the seismic normal modes of the Earth at frequencies near 10 mHz are excited at a nearly constant level in the absence of large earthquakes. This background level of excitation has been called the 'hum' of the Earth, and is equivalent to the maximum excitation from a magnitude 5.75 earthquake. Its origin is debated, with most studies attributing the forcing to atmospheric turbulence, analogous to the forcing of solar oscillations by solar turbulence. Some reports also predicted that turbulence might excite the planetary modes of Mars to detectable levels. Recent observations on Earth, however, suggest that the predominant excitation source lies under the oceans. Here I show that turbulence is a very weak source, and instead it is interacting ocean waves over the shallow continental shelves that drive the hum of the Earth. Ocean waves couple into seismic waves through the quadratic nonlinearity of the surface boundary condition, which couples pairs of slowly propagating ocean waves of similar frequency to a high phase velocity component at approximately double the frequency. This is the process by which ocean waves generate the well known 'microseism peak' that dominates the seismic spectrum near 140 mHz (refs 11, 12), but at hum frequencies, the mechanism differs significantly in frequency and depth dependence. A calculation of the coupling between ocean waves and seismic modes reproduces the seismic spectrum observed. Measurements of the temporal correlation between ocean wave data and seismic data have confirmed that ocean waves, rather than atmospheric turbulence, are driving the modes of the Earth.     

Observed oceanic feedback to the atmosphere over the Kuroshio Extension during spring time and its possible mechanism

High-resolution satellite measurements are used to study the air-sea interaction over the Kuroshio Extension （KE） region during spring time. There are two oceanic fronts in the KE region off the east coast of Japan. These fronts are generally associated with strong ocean currents, which may display unstable meander, resulting in remarkable warm sea surface temperature （SST） ridges and cold SST troughs. Analyses of these satellite observations reveal a significantly positive correlation between sea surface wind speed and its underlying SST along these fronts. This positive SST-wind correlation becomes even more significant when strong meanders occur along the fronts. This positive SST-wind correlation indicates an ocean-to-atmosphere feedback over the KE region during spring time. A high-resolution regional atmospheric model is used to investigate the atmospheric response to SST changes along the two fronts.     

An analysis of the polar motion series from VLBI observations

From the reduction of 2893 globally distributed astrometric and geodetic VLBI sessions from August 1979 to the end of 1998, coordinates of 722 radio sources at J2000.0, coordinates and velocities of 128 stations at J1997.0 and about 20 years Earth Orientation Parameters were estimated. From the analysis of the resultant polar motion series, the following are demonstrated: (ⅰ) During the VLBI data span the Markowitz wobble is not exhibited. (ⅱ) The amplitudes of both annual and Chandler wobble show temporal variations, with the former being more obvious than the latter. (ⅲ) Wavelet analysis shows that all the signals in the polar motion series are characterized by temporal variation in amplitudes. If we take any signal as strictly periodic, it is impossible to remove it completely from the polar motion series by least-squares fit because the hypothesis of a constant amplitude conflicts with VLBI measurements. (ⅳ) By applying a filter, the secular polar motion was found to be (2.74±0.01) mas/a towards (83.9±0.3) °W longitude, which is smaller in rate and more westward in direction compared with those determined from optical observations or the combination of optical and space geodetic observations.     

Inhibition of carbonate synthesis in acidic oceans on early Mars

Several lines of evidence have recently reinforced the hypothesis that an ocean existed on early Mars. Carbonates are accordingly expected to have formed from oceanic sedimentation of carbon dioxide from the ancient martian atmosphere. But spectral imaging of the martian surface has revealed the presence of only a small amount of carbonate, widely distributed in the martian dust. Here we examine the feasibility of carbonate synthesis in ancient martian oceans using aqueous equilibrium calculations. We show that partial pressures of atmospheric carbon dioxide in the range 0.8-4 bar, in the presence of up to 13.5 mM sulphate and 0.8 mM iron in sea water, result in an acidic oceanic environment with a pH of less than 6.2. This precludes the formation of siderite, usually expected to be the first major carbonate mineral to precipitate. We conclude that extensive interaction between an atmosphere dominated by carbon dioxide and a lasting sulphate- and iron-enriched acidic ocean on early Mars is a plausible explanation for the observed absence of carbonates.     

A short-term sink for atmospheric CO2 in subtropical mode water of the North Atlantic Ocean

Large-scale features of ocean circulation, such as deep water formation in the northern North Atlantic Ocean, are known to regulate the long-term physical uptake of CO2 from the atmosphere by moving CO2-laden surface waters into the deep ocean. But the importance of CO2 uptake into water masses that ventilate shallower ocean depths, such as subtropical mode waters of the subtropical gyres, are poorly quantified. Here we report that, between 1988 and 2001, dissolved CO2 concentrations in subtropical mode waters of the North Atlantic have increased at a rate twice that expected from these waters keeping in equilibrium with increasing atmospheric CO2. This accounts for an extra 0.4-2.8 Pg C (1 Pg = 10(15) g) over this period (that is, about 0.03-0.24 Pg C yr(-1)), equivalent to 3-10% of the current net annual ocean uptake of CO2 (ref. 3). We suggest that the lack of strong winter mixing events, to greater than 300 m in depth, in recent decades is responsible for this accumulation, which would otherwise disturb the mode water layer and liberate accumulated CO2 back to the atmosphere. However, future climate variability (which influences subtropical mode water formation) and changes in the North Atlantic Oscillation (leading to a return of deep winter mixing events) may reduce CO2 accumulation in subtropical mode waters. We therefore conclude that, although CO2 uptake by subtropical mode waters in the North Atlantic--and possibly elsewhere--does not always represent a long-term CO2 sink, the phenomenon is likely to contribute substantially to interannual variability in oceanic CO2 uptake.     

电磁体系角动量守恒的完整物理图像——从对条件改变后的费曼园盘佯谬谈起

本文借助矢量分析工具,针对费曼园盘佯谬中,园盘边缘的带电小球改放在线圈内部的情形,解决了发散困难,在定量计算的基础上,对电磁体系角动量守恒做全面讨论,给出完整的物理图像.     

Variable ageing and storage of dissolved organic components in the open ocean

Seawater dissolved organic matter (DOM) is the largest reservoir of exchangeable organic carbon in the ocean, comparable in quantity to atmospheric carbon dioxide. The composition, turnover times and fate of all but a few planktonic constituents of this material are, however, largely unknown. Models of ocean carbon cycling are thus limited by the need for information on temporal scales of carbon storage in DOM subcomponents, produced via the 'biological pump', relative to their recycling by bacteria. Here we show that carbohydrate- and protein-like substances in the open Atlantic and Pacific oceans, though often significantly aged, comprise younger fractions of the DOM, whereas dissolved lipophilic material exhibits up to approximately 90 per cent fossil character. In contrast to the millennial mean ages of DOM observed throughout the water column, weighted mean turnover times of DOM in the surface ocean are only decadal in magnitude. An observed size-age continuum further demonstrates that small dissolved molecules are the most highly aged forms of organic matter, cycling much more slowly than larger, younger dissolved and particulate precursors, and directly links oceanic organic matter age and size with reactivity.