Climatic control on river discharge simulations,Zackenberg River drainage basin,northeast Greenland

A spatially distributed, physically based, hydrologic modeling system (MIKE SHE) was applied to quantify intra‐ and inter‐annual discharge from the snow and glacierized Zackenberg River drainage basin (512 km²; 20% glacier cover) in northeast Greenland. Evolution of snow accumulation, distribution by wind‐blown snow, blowing‐snow sublimation, and snow and ice surface melt were simulated by a spatially distributed, physically based, snow‐evolution modelling system (SnowModel) and used as input to MIKE SHE. Discharge simulations were performed for three periods 1997–2001 (calibration period), 2001–2005 (validation period), and 2071–2100 (scenario period). The combination of SnowModel and MIKE SHE shows promising results; the timing and magnitude of simulated discharge were generally in accordance with observations (R² = 0·58); however, discrepancies between simulated and observed discharge hydrographs do occur (maximum daily difference up to 44·6 m³ s^?1 and up to 9% difference between observed and simulated cumulative discharge). The model does not perform well when a sudden outburst of glacial dammed water occurs, like the 2005 extreme flood event. The modelling study showed that soil processes related to yearly change in active layer depth and glacial processes (such as changes in yearly glacier area, seasonal changes in the internal glacier drainage system, and the sudden release of glacial bulk water storage) need to be determined, for example, from field studies and incorporated in the models before basin runoff can be quantified more precisely. The SnowModel and MIKE SHE model only include first‐order effects of climate change. For the period 2071–2100, future IPCC A2 and B2 climate scenarios based on the HIRHAM regional climate model and HadCM3 atmosphere–ocean general circulation model simulations indicated a mean annual Zackenberg runoff about 1·5 orders of magnitude greater (around 650 mmWE year^?1) than from today 1997–2005 (around 430 mmWE year^?1), mainly based on changes in negative glacier net mass balance. Copyright © 2007 John Wiley & Sons, Ltd.     

海洋科技在21世纪海上丝绸之路建设中的作用

21世纪海上丝绸之路建设在海洋经济活动、海上综合保障等方面对海洋科技领域提出了新命题。在分析我国海洋技术优势领域的基础上,围绕科技创新政策伙伴关系、培育创新品牌、推进海洋经济和产业发展等方面,深入阐述了海洋科技领域在21世纪海上丝绸之路建设中的支撑作用,同时提出具体工作思路。     

SUSTAINABLE DEVELOPMENT FACING CHALLENGESIN 21ST CENTURY

ISUSTAINABLE DEVELOPMENT IS UNDER UN－guiding human forward．he author pointed out manyCEASINGCHALLENGES times that sustainable developmentwas a correctstrategic selectlonforhumanfuture and It representedaThe Zlst Century has come，people have many newdevelopmentoutlook，strategic vie呷olntandvalueforecasts and long for a wonde山lprospect．The 21st（CHEN，1997；200a；200b）．Century lsa bio－sclentmc era，an economic global－The authoralso pointed out th…     

New magnetic field measurements of β Cephei stars and slowly pulsating B stars

We present the results of the continuation of our magnetic survey with FORS 1 at the VLT of a sample of B‐type stars consisting of confirmed or candidate β Cephei stars and Slowly Pulsating B (hereafter SPB) stars, along with a small number of normal B‐type stars. A weak mean longitudinal magnetic field of the order of a few hundred Gauss was detected in three β Cephei stars and two stars suspected to be β Cephei stars, in five SPB stars and eight stars suspected to be SPB stars. Additionally, a longitudinal magnetic field at a level larger than 3σ has been diagnosed in two normal B‐type stars, the nitrogen‐rich early B‐type star HD 52089 and in the B5 IV star HD 153716. Roughly one third of β Cephei stars have detected magnetic fields: Out of 13 β Cephei stars studied to date with FORS 1, four stars possess weak magnetic fields, and out of the sample of six suspected β Cephei stars two show a weak magnetic field. The fraction of magnetic SPBs and candidate SPBs is found to be higher: Roughly half of the 34 SPB stars have been found to be magnetic and among the 16 candidate SPBs eight stars possess magnetic fields. In an attempt to understand why only a fraction of pulsating stars exhibit magnetic fields, we studied the position of magnetic and non‐magnetic pulsating stars in the H‐R diagram. We find that their domains in the H‐R diagram largely overlap, and no clear picture emerges as to the possible evolution of the magnetic field across the main sequence. It is possible that stronger fields tend to be found in stars with lower pulsating frequencies and smaller pulsating amplitudes. A somewhat similar trend is found if we consider a correlation between the field strength and the v sin i ‐values, i.e. stronger magnetic fields tend to be found in more slowly rotating stars (© 2009 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)     

Impact of climate and socioeconomic changes on fire carbon emissions in the future: Sustainable economic development might decrease future emissions

Fires and their associated carbon and air pollutant emissions have a broad range of environmental and societal impacts, including negative effects on human health, damage to terrestrial ecosystems, and indirect effects that promote climate change. Previous studies investigated future carbon emissions from the perspective of response to climate change and population growth, but the compound effects of other factors like economic development and land use change are not yet well known. We explored fire carbon emissions throughout the 21st century by changing five factors (meteorology, biomass, land use, population density, and gross domestic product [GDP] per capita). Compared to the historical period (2006–2015), global future fire carbon emissions decreased, mainly caused by an increase in GDP per capita, which leads to improvement in fire management and capitalized agriculture. We found that the meteorological factor has a strong individual effect under higher warming cases. Fires in boreal forests were particularly expected to increase because of an increase in fuel dryness. Our research should help climate change researchers consider fire-carbon interactions. Incorporating future spatial changes under diverse scenarios will be helpful to develop national mitigation and adaptation plans.     

塔里木河源流山区径流模拟及不确定性研究

自然环境恶劣、站点稀少、观测困难是干旱区水文系统研究面临的基本问题。特殊的自然地理条件给水文过程带来了极大的复杂性和不确定性,也阻碍了干旱区水文过程和机理研究的发展。选取塔里木河源区开都河流域为研究区,采用分布式水文模型MIKE SHE模拟大尺度资料稀缺地区水文过程,将流域内气象、水文站点数据与遥感数据相结合,利用气象、土壤类型、土地利用和地表覆盖、数字高程(DEM)和降雨等资料,模拟流域水文过程;在出山口径流数据的基础上对模型进行率定和验证;分析了模型中的不确定性的来源,探讨模型优化方法。结果表明,MIKE SHE模型能在水文、气象站点稀少,土壤及水文地质数据缺乏的条件下,模拟开都河流域的日径流过程,但精度仍有待提高;通过分析识别出了隐含于模型结构、输入及参数等3个方面的8种不确定性来源。     

岱海水位下降原因分析

应用ＧＩＳ软件ＡＲＣ／ＩＮＦＯ,建立太湖流域海面－地面变化信息系统,并与数据采集系统,图像处理系统和计算机系统相结合,研究对本区人类社会经济发展,区域规划,工程建设和人民生活产生重大影响的气候,海面,地面变化和区域环境变迁。采用长江三角洲地区邻近海域２１世纪前半期地区性ＲＳＬ上升幅度预测方案进行研究,结果表明：随着海面的不断上升和太湖流域地面沉降的加剧,２０００年和２０５０年,太湖流域处于高潮位以     

巴黎气候会议对全球长期目标的新发展

巴黎气候会议（COP21）达成了包括《巴黎协定》在内的重要成果,丰富和深化了应对气候变化的一揽子长期目标。1.5℃温升控制目标意味着全球管控气候风险的政治意愿得到强化,减缓温室气体排放的路径得到初步勾勒。在未来的科学评估和政治谈判中,全球各区域甚至是各个排放大国的排放空间、排放路径和减缓需求将会进一步清晰化和定量化,还会丰富和深化自上而下的国际气候合作规则,结合当前以国家自主决定贡献（INDC）为特征的、主要以自下而上方式推进全球气候治理的新模式,将对发展中国家、尤其是发展中排放大国的排放配额与发展空间产生重要影响,并进一步影响各国制定其国家贡献目标与行动的自主性。