内蒙古自治区2000国家大地坐标框架的建立及实时服务     

于欣 《现代测绘》2014,(6):36-38

启用2000大地坐标系的必要性;内蒙古2000国家大地坐标框架建立。  相似文献   

过去2000年全球典型暖期特征与机制的模拟研究   总被引：1，自引：0，他引：1  

王志远  刘健 《第四纪研究》2014,34(6)

本文利用美国国家大气研究中心(NCAR)的通用地球系统模式(Community Earth System Model,简称CESM)的低分辨率版本(CESM1.0.3,T31_g37)在国际国内率先进行了多组过去2000年瞬变积分模拟试验,在与历史重建资料和观测资料进行对比验证的基础上,对过去2000年中的典型暖期(中世纪暖期与现代暖期)的特征和成因机制进行了初步探讨,结果表明:中世纪暖期太阳辐射加强是导致其“暖化”的主要原因之一,而温室气体浓度的激增是现代全球变暖的最主要原因;在中世纪暖期,自然因子(包括太阳辐射和火山活动)对降水量的影响之和比温室气体的影响高一个数量级;而在现代暖期,温室气体对降水量的影响比自然因子(包括太阳辐射和火山活动)对降水量的影响之和高一个数量级;在不同外强迫条件下的海表温度变化在热带太平洋区域截然不同,即自然因子影响下为类-拉尼娜态,而温室气体影响下为类-厄尔尼诺态;无论在中世纪暖期还是现代暖期,相对于1000～1850年的平均情况,沃克(Walker)环流均处于增强状态.  相似文献   

2000—2020年中国省际人口迁移格局的演化特征及影响因素     

古恒宇  劳昕  温锋华  赵志浩 《地理学报》2022,77(12):3041-3054

准确认识和把握21世纪前20年中国人口迁移的地理格局和影响因素,是推动新型城镇化建设及区域均衡发展的关键科学问题。借助特征向量空间滤波泊松伪最大似然估计（ESF PPML）引力模型,基于第六次和第七次全国人口普查数据、2005年和2015年全国1%人口抽样调查数据,研究了2000—2020年中国省际人口迁移的时空演化特征及影响因素。主要结论为：① 2000—2020年间人口迁移格局总体稳定,具有较强的不平衡性和网络溢出效应,大量人口从中部、西部、东北地区迁移至东部地区;② 人口迁移格局稳中有变,不平衡程度和空间集聚程度逐渐减弱,人口迁移和人口分布显现出南北分异趋势,东北地区人口迁出强度不断增强; ③ 传统引力模型因素（人口规模、地理距离）、地区社会经济发展因素（工资差异、科技教育投入占比、医疗水平）、社会网络因素、环境舒适度（PM_2.5浓度）以及生活成本（住宅价格占比）共同影响人口迁移格局;④ 区域经济差异对省际人口迁移的影响作用逐步弱化,人口迁移逐渐转变为对工资收入、高质量公共服务、环境舒适度等多因素考虑的决策过程,生活成本逐渐对人口迁移产生显著影响。  相似文献   

Optical Spectroscopy and Near-Infrared Observations of Comet C/2000 Wm1 (Linear) in December 2001 from Chile and Brazil     

Picazzio  Enos  De Almeida  Amaury A.  Churyumov  Klim I.  Andrievski  Sergei M.  Luk'yanyk  Igor V. 《Earth, Moon, and Planets》2002,90(1-4):391-400

We report on the preliminary analysis of the high-resolution spectrum of CometC/2000 WM1 (LINEAR), obtained on Dec. 1, 2001 with the Fiber fed ExtendedRange Optical Spectrograph (FEROS) installed on the 1.52-m telescope of ESO(Chile). Many emission lines of the molecules C₂, C₃, CN, CH, CH⁺,NH₂, CO, CO⁺, H₂O⁺ and, presumably, C₂ ^- were identifiedin the spectral range 400–900 nm. Also, near-infrared photometry was performed on Dec. 2 and 3, with the infraredcamera (CamIV) attached to the 0.60-m Boller and Chivens telescope of the Picodos Dias Observatory (LNA/MCT), Brazil. We report the preliminary and comparativeanalysis of the I-J and J-H color indices.  相似文献   

Hubble Space Telescope imaging of the progenitor sites of six nearby core-collapse supernovae     

J. R. Maund  S. J. Smartt 《Monthly notices of the Royal Astronomical Society》2005,360(1):288-304

The search for the progenitors of six core-collapse supernovae (CCSNe) in archival Hubble Space Telescope ( HST ) WFPC2 pre-explosion imaging is presented. These SNe are 1999an, 1999br, 1999ev, 2000ds, 2000ew and 2001B. Post-explosion imaging of the SNe, with the HST ACS/WFC, has been utilized with the technique of differential astrometry to identify the progenitor locations on the pre-explosion imaging. SNe 1999br, 1999ev, 2000ew and 2001B are recovered in late-time imaging, and estimates of the progenitor locations on the pre-explosion imaging, with subpixel accuracy, have been made. Only the progenitor of the Type II-P SN 1999ev has been recovered, on pre-explosion F555W imaging, at a 4.8σ significance level. Assuming a red supergiant progenitor, the pre-explosion observation is consistent with   M _ZAMS= 15–18 M_⊙  . The progenitors of the other five SNe were below the 3σ detection threshold of the pre-explosion observations. The detection thresholds were translated to mass limits for the progenitors by comparison with stellar evolution models. Pre-explosion observations of the peculiarly faint SN 1999br limit the mass of a red supergiant progenitor to   M _ZAMS < 12 M_⊙  . Analysis has been extended, from previous studies, to include possible detections of high- T _eff, high-mass stars by conducting synthetic photometry of model Wolf–Rayet star spectra. The mass limits for the Type II-P SNe 1999an and 1999br are consistent with previously determined mass limits for this type of SN. The detection limits for the progenitors of the Type Ibc SNe (2000ds, 2000ew and 2001B) do not permit differentiation between high-mass Wolf–Rayet progenitors or low-mass progenitors in binaries.  相似文献   

Optical Spectroscopy of Comet C/2000 WM1 (LINEAR) at the Guillermo Harro Astrophysical Observatory in Mexico     

Churyumov  Klim I.  Luk'yanyk  Igor V.  Berezhnoi  Alexei A.  Chavushyan  Vahram H.  Sandoval  Lourdes S.  Palma  Alejandro A. 《Earth, Moon, and Planets》2002,90(1-4):361-368

We present a preliminary analysis of medium resolution optical spectra of comet C/2000 WM1 (LINEAR) obtained on 22 November 2001. Theemission lines of the molecules C₂, C₃, CN, NH₂,H₂O⁺ and presumably CO (Asundi and triplet bands) and C₂ ^-were identified in these spectra. By analysing the brightnessdistributions of the C₂, C₃, CN emission lines along theslit of the spectrograph we determined some physical parameters of theseneutrals, such as their lifetimes and expansion velocities inthe coma. The Franck–Condon factors for the CO Asundi bands and C₂ ^- bands were calculated using a Morse potential model.  相似文献   

SN 1998A: explosion of a blue supergiant     

A. Pastorello  E. Baron  D. Branch  L. Zampieri  M. Turatto  M. Ramina  S. Benetti  E. Cappellaro  M. Salvo  F. Patat  A. Piemonte  J. Sollerman  B. Leibundgut  G. Altavilla 《Monthly notices of the Royal Astronomical Society》2005,360(3):950-962

We present spectroscopic and photometric observations of the peculiar Type II supernova (SN) 1998A. The light curves and spectra closely resemble those of SN 1987A, suggesting that the SN 1998A progenitor exploded when it was a compact blue supergiant. However, the comparison with SN 1987A also highlights some important differences: SN 1998A is more luminous and the spectra show bluer continua and larger expansion velocities at all epochs. These observational properties indicate that the explosion of SN 1998A is more energetic than SN 1987A and more typical of Type II supernovae. Comparing the observational data with simulations, we deduce that the progenitor of SN 1998A was a massive star  (∼25 M_⊙)  with a small pre-supernova radius  (≲6 × 10¹² cm)  . The Ba  ii lines, unusually strong in SN 1987A and some faint II-P events, are almost normal in the case of SN 1998A, indicating that the temperature plays a key role in determining their strength.  相似文献   

COPEX和HM2000与APEX型剖面浮标比测试验及资料质量评价     

卢少磊  孙朝辉  刘增宏  许建平 《海洋技术学报》2016,(1):84-92

利用船载CTD仪、国外剖面浮标(APEX)和实验室盐度计等标准仪器设备,在西北太平洋海域对2种型号国产剖面浮标(COPEX和HM2000)进行了现场比测试验,并对观测资料质量进行了定性和定量分析与评价.结果表明:(1) COPEX和HM2000型剖面浮标观测的盐度资料均能达到国际Argo计划提出的±0.01的精度要求;(2)HM2000的最小观测深度离海面1 m以内,最大观测深度基本稳定在2 000 m左右,并能保持在1000 m深度附近漂移,而COPEX的最小观测深度在8～9 m之间,最大观测深度则在1 800～1 900 m之间波动,且漂移深度都在600～800 m之间;(3)COPEX和HM2000都获得了70条以上有效观测剖面.总体而言,两种国产剖面浮标观测的温、盐度资料都是可信、可靠的.但试验中暴露的一些问题和不足仍有待不断改进和完善.  相似文献   

基于作物模型的河南省旱稻干旱风险评估     

薛昌颖 《气象与环境科学》2016,39(2):126-131

采用作物模型与数理统计相结合的方法,利用长期历史气象资料,以作物模型和地理信息系统技术为工具,系统分析了河南地区旱稻生育期水分盈亏情况。以模型模拟的雨养条件下实际蒸散量相对于潜在条件下的蒸散量(即需水量)的亏缺率,即水分亏缺指数,以雨养条件下产量相对于潜在产量的损失率(即灾损指数)作为产量灾损强度评价指标,从受旱程度和产量损失两个角度构建干旱风险评估模型,进行干旱风险评估。结果表明:河南省旱稻生育期集中在6—9月,水分亏缺最多的阶段为出苗—穗分化阶段,水分亏缺指数变化在0.50~0.60,其次是开花—成熟阶段和穗分化—开花阶段,水分亏缺指数变化在0.11~0.43;全生育期水分亏缺指数在0.36~0.50。出苗—穗分化阶段干旱发生的风险最大,其次是开花—成熟阶段,穗分化—开花阶段的最小。河南旱稻生育期干旱风险呈现为由东南向西北逐渐升高的分布,其中三门峡、济源西部一带风险最高,洛阳南部和南阳西北部一带最低,黄河以北大部地区和豫东、豫南地区风险居中。  相似文献   

基于VC++、ObjectARX的边角网平差系统的设计     

陈影  程耀东  闫浩文 《物探与化探》2007,31(1):59-62

在总结以前手算及其他它语言程序优缺点的基础上,充分利用前期工作成果及现有资源,以AutoCAD2000为平台,用VC++及ObjectARX等软件结合测量平差的专业知识,设计了集平差计算和图形显示为一体的辅助设计软件,用以计算坐标的精确值,并绘出边角网网形.  相似文献