El Nino演变不同阶段东亚大气环流年际异常型的数值模拟   总被引：4，自引：4，他引：4       下载免费PDF全文

孙旭光  杨修群 《地球物理学报》2005,48(3):501-510

给定1948～1999年逐月变化的全球观测的海表温度分布，使用全球大气环流模式（CCM3/NCAR）模拟了大气对海表温度变化的响应，利用SVD和合成检验方法，分析了El Nino发展阶段夏季、成熟阶段冬季以及衰亡阶段夏季东亚大气环流的年际异常型.结果表明：El Nino发展阶段夏季，中国东北、朝鲜半岛以及日本海附近为高度负异常中心，西太平洋副高偏弱、偏东，东亚夏季风增强；El Nino成熟阶段冬季，东亚大槽加强，东亚北部冬季风加强；El Nino衰亡阶段夏季，西太平洋副高偏强、偏南、西伸，东亚夏季风减弱；El Nino事件在其衰亡阶段夏季与东亚大气环流异常的关系最紧密，其次是成熟阶段冬季，最后是发展阶段夏季.模拟的El Nino演变不同阶段东亚大气环流年际异常型易于解释以往研究中观测分析揭示的由El Nino造成的我国东部气温和降水异常型.  相似文献   

http://www.sciencedirect.com/science/article/pii/S1674987114000267   总被引：6，自引：6，他引：0  

James M.Dohm  Shigenori Maruyama 《地学前缘(英文版)》2015,6(1):95-101

Habitable Trinity is a newly proposed concept of a habitable environment.This concept indicates that the coexistence of an atmosphere(consisting largely of C and N),an ocean(H and O).and a landmass(supplier of nutrients) accompanying continuous material circulation between these three components driven by the Sun is one of the minimum requirements for life to emerge and evolve.The life body consists of C,0,H,N and other various nutrients,and therefore,the presence of water,only,is not a sufficient condition.Habitable Trinity environment must be maintained to supply necessary components for life body.Our Habitable Trinity concept can also be applied to other planets and moons such as Mars,Europa,Titan,and even exoplanets as a useful index in the quest for life-containing planetary bodies.  相似文献   

浙江慈溪市土地生态质量调查和评估          下载免费PDF全文

刘军保  陈智渊  潘卫丰 《江苏地质》2011,35(3):296-301

土壤、大气、水和农产品质量共同构成土地生态质量的内涵。通过慈溪市基本农田质量调查试点项目,开展了高精度土壤地球化学调查和农产品、灌溉水、大气质量调查,建立了土地生态质量评估模型。以土壤地球化学质量评估为基础,进行了大气、水、农产品综合质量评估,以及慈溪市农用地土地生态质量评价。评价显示,慈溪市农用地土地生态质量绝大部分优良,只有局部如城市周边等地存在生态风险。试点成果为浙江省国土资源特别是基本农田的数量、质量和生态管护并重的精细化管理提供了示范和依据。  相似文献   

Convective vortices on Mars: a reanalysis of Viking Lander 2 meteorological data, sols 1-60   总被引：1，自引：0，他引：1  

T.J. Ringrose  M.C. Towner 《Icarus》2003,163(1):78-87

Dust devil data from Mars is limited by a lack of data relating to diurnal dust devil behaviour. Previous work looking at the Viking Lander meteorological data highlighted seasonal changes in temporal occurrence of dust devils and gave an indication of typical dust devil diameter, size, and internal dynamics. The meteorological data from Viking Lander 2 for sols 1 to 60 have been revisited to provide detailed diurnal dust devil statistics. Results of our analysis show that the Viking Lander 2 experienced a possible 38 convective vortices in the first 60 sols of its mission with a higher occurrence in the morning compared to Earth, possibly as a result of turbulence generated by the Lander body. Dust devil events have been categorised by statistical confidence and intensity. Some initial analysis and discussion of the results is also presented. Assuming a similar dust loading to the vortices seen by Mars Pathfinder, it is estimated that the amount of dust lofted in the locality of the Lander is approximately 800 ± 10 kgsol⁻¹km⁻².  相似文献   

The rotational structure of the B-X system of sulfur dimers in the spectra of Comet Hyakutake (C/1996 B2)     

Sang J. Kim  M.F. A'Hearn  R. Meier 《Icarus》2003,166(1):157-166

We have constructed line-by-line fluorescence models for the ro-vibrational bands of the B-X system of sulfur dimers (S₂). For the first time the detailed rotational lines of the bands are clearly resolved in the high-resolution echelle spectra of Comet Hyakutake (C/1996 B2), which were obtained at the Kitt Peak 4-m telescope on 26.4 March 1996 (UT). In order to construct satisfactory band models of the B-X system, we first compared the models to laboratory spectra available in literature, and then compared the models including Swings effects to the high-resolution spectra of Hyakutake. From the model fits, we derived a rotational temperature of 70±10 K, which should represent a temperature of a coma region close to the nucleus, where most of the S₂ emissions originate. We present previously proposed scenarios for the origin of S₂ in cometary comae, and compare them with our spectral analysis.  相似文献   

Laboratory measurements of the Ka-band (7.5 mm to 9.2 mm) opacity of phosphine (PH₃) and ammonia (NH₃) under simulated conditions for the Cassini-Saturn encounter     

Priscilla N Mohammed 《Icarus》2003,166(2):425-435

Recently, a model for the centimeter-wavelength opacity of PH₃ under conditions characteristic of the outer planets was developed by Hoffman et al. (2001, PhD thesis), based on centimeter wavelength laboratory measurements. New laboratory measurements have been conducted which show that this model is also accurate at low pressures and temperatures, and at millimeter wavelengths such as will be employed in Cassini Ka-band (9.3 mm) radio occultation studies. The opacity of PH₃ in a hydrogen/helium (H₂/He) atmosphere has been measured at frequencies in the Ka-band region at 32.7 GHz (9.2 mm), 35.6 GHz (8.4 mm), 37.7 GHz (8.0 mm), and 39.9 GHz (7.5 mm) at pressures of 0.5, 1, and 2 bar and at temperatures of 295, 209, and 188 K. Additionally, new high-precision laboratory measurements of the opacity of NH₃ in an H₂/He atmosphere have been conducted under the same temperature and pressure conditions described for PH₃. These new measurements better constrain the NH₃ opacity model supporting use of a Ben-Reuven lineshape model. These measurements will also elucidate the interpretation of millimeter wavelength observations conducted with the NRAO/VLA at 43 GHz (7 mm).  相似文献   

Saturn's cloud morphology and zonal winds before the Cassini encounter     

A Sánchez-Lavega  R Hueso  J.F Rojas 《Icarus》2004,170(2):519-523

Analyses of Hubble Space Telescope (HST) images of Saturn obtained from August 2003 to March 2004, with extensive support from ground-based telescopes, have been used to characterize the cloud morphology and motions in its atmosphere few months before the Cassini encounter. We present data on the major meteorological features as potential targets for Cassini observations. We extend our previous measurements of the zonal winds during the 1996-2002 period (A. Sánchez-Lavega et al., 2003, Nature, 423, 623-625), confirming the strong change in the equatorial jet, and the high hemispheric symmetry of the zonal wind pattern.  相似文献   

The role and performance of ground-based networks in tracking the evolution of the ozone layer     

《Comptes Rendus Geoscience》2018,350(7):354-367

In the 1980s, ground-based monitoring of the ozone layer played a key role in the discovery of the Antarctic Ozone Hole as well as in the first documentation of significant winter and spring long-term downward trends in the populated mid-latitude regions. The article summarizes the close-to-hundred-year-long history of ground-based measurements of stratospheric ozone, and more recent observations of constituents that influence its equilibrium. Ozone observations began long before the recognition of the impact of increasing emissions of manmade ozone-depleting substances on ozone and therefore on UV levels, human health, ecosystems and the Earth climate. The historical ozone observations prior to 1980s are used as a reference for the assessments of the state of the ozone layer linked to the enforcement of the Montreal Protocol. In this paper, we describe the worldwide monitoring networks and their ozone observations used to determine long-term trends with an accuracy of a few percent per decade. Since 1989, the ground-based monitoring activities have provided support for the amendments of the Montreal Protocol (MP). They include monitoring of (a) the ozone total column and the vertical distribution at global scale, (b) the ozone-depleting substances (ODS) related to the MP such as chlorofluorocarbons (CFCs), and their decomposition products in the stratosphere, and (c) the atmospheric species playing a role in ozone depletion, e.g., nitrogen oxides, water vapor, aerosols, polar stratospheric clouds. We highlight important accomplishments in the atmospheric monitoring performed by the Global Atmosphere Watch program (GAW) run under the auspices of the World Meteorological Organization (WMO) and by the Network for the Detection of Atmospheric Composition Change (NDACC). We also address the complementary roles of ground-based networks and satellite instruments. High-quality ground-based measurements have been used to evaluate ozone variabilities and long-term trends, assess chemistry climate models, and check the long-term stability of satellite data, including more recently the merged satellite time-series developed for the detection of ozone recovery at global scale, which might be further modified by climate change.  相似文献   

一种新的高精度全球对流层天顶延迟模型     

黄良珂  陈华  刘立龙  姜卫平 《地球物理学报》2021,64(3):782-795

对流层延迟是影响高精度卫星导航定位的关键因素,也是大气科学研究的重要数据.针对已有全球对流层延迟模型的模型方程未同时顾及高程、纬度和季节变化以及模型构建时仅使用单一格网点数据等问题,本文提出了一种对流层天顶延迟(ZTD)全球模型构建的新方法,即引入滑动窗口算法将全球剖分为大小一致的规则窗口,利用2008—2015年全球大地观测系统(GGOS)大气格网产品构建每个窗口同时顾及高程、纬度和季节因子的全球ZTD新模型(GGZTD模型).联合未参与建模的2016年全球GGOS格网产品和2016年全球316个IGS站精密ZTD产品,检验了GGZTD模型的精度和适用性.结果表明:以GGOS大气格网ZTD产品和IGS站ZTD产品为参考值,GGZTD模型在全球的精度分别为3.58 cm和3.62 cm,相对于UNB3m模型和目前标称精度最优的GPT2w模型计算的ZTD信息,GGZTD模型在全球表现出了最优的精度和稳定性,其精度相对于UNB3m模型具有显著的提升(精度提高了30%以上),相对于GPT2w模型仍具有一定的改善;在ZTD计算时GGZTD模型相对于GPT2w模型显著地减少了模型参数,尤其相对于GPT2w-1(减少了99%).GGZTD模型只需输入位置与时间和依赖相对较少的模型参数则能在全球获得高精度和稳定的ZTD信息,极大地提升了模型的计算效率.  相似文献   

南半球平流层极涡崩溃早晚年环流异常特征          下载免费PDF全文

李琳  潘静  李崇银 《地球物理学报》2013,56(6):1825-1834

极涡崩溃是平流层大气环流一个重要的变化过程,本文利用31年的再分析资料研究了南半球平流层极涡崩溃早晚年的异常特征.研究结果表明,南半球平流层极涡崩溃偏早年极涡崩溃前后平流层环流场异常表现为整层一致的变化,即都为正温度异常、正位势高度异常和负纬向风异常;而南半球平流层极涡崩溃偏晚年极涡崩溃前后平流层环流场异常的整层一致性的变化不典型,而在符号上与极涡崩溃偏早年的异常相反.与北半球平流层极涡崩溃前后环流异常相反明显不同,南半球平流层极涡崩溃偏早或偏晚年在极涡崩溃前后的环流异常保持相同的性质.进一步分析表明行星波活动在南极极涡的崩溃过程中起到了重要作用,极涡崩溃早年上传行星波比极涡崩溃晚年强,并且持续时间长.通过波流相互作用,行星波的异常使得极涡崩溃早年和晚年10月的平流层高纬地区分别为位势高度正异常和负异常,环流异常持续保持可能最终影响了南半球平流层极涡的崩溃时间.分析显示南半球极涡崩溃偏晚与La Niña事件之间可能存在一定的联系,但在极涡崩溃偏早年与赤道太平洋海表温度异常(SSTA)并无明显关系.  相似文献