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An International Research and Mobility Exchange Project: Advance Modeling and Observing Solar Radiation of Sea Ice (AMORA)

机译:国际研究和移动交流项目:推进建模与观察海冰太阳辐射(Amora)

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In recent decades, the Arctic sea ice has been observed undergoing a significant change, including a rapid retreat on sea ice extent, a continuously rapid declining on sea ice thickness, and a trend towards younger sea ice. These changes can significantly influence the surface energy balance of the ice-covered Arctic Ocean. To quantify this energy balance and to increase our understanding of mechanisms leading to observed changes in the Arctic Ocean, a project"Advancing Modeling and Observing solar Radiation of sea ice - understanding changes and processes (AMORA)" was initiated and begun in October 2009. AMORA is funded by the Research Council of Norway and will last until 2013. It is organized under a frame of Norwegian-Chinese bilateral collaboration program for advance in climate research. Other international partners from Finland, Germany and USA are actively involved in thisproject. So far, various project tasks have been carried out: (1) in-situ data collections during several National/International research cruises and field campaigns in different Arctic regions(CHINARE-2010; Norwegian R/V Fram Strait Cruise 2011; Norwegian KV Svalbard Cruise 2011; German Polarstern Arctic Cruise 2011); (2) Research mobility and exchange among project partners (Norway and China, Norway and Germany, and Norway and Finland, and China-Finland); (3) Instrumentation exchange and development among partners, and (4) high resolution thermodynamic snow/ice model development. An autonomous observation system for spectral radiation reflection and transmission through sea ice, the so-called spectral radiation buoy (SRB), is in development and due for first deployment in 2012. The data collected from the SRB and ice mass balance buoys (IMBs) along with numerical model studies will help us to better understand the key thermodynamic processes of Arctic sea ice and changes in polar climate, especially on sea ice.
机译:近几十年来,北极海冰已被观察到进行重大变化,包括海冰范围的快速撤退,海冰厚度不断迅速下降,以及较年轻的海冰的趋势。这些变化可以显着影响冰覆盖的北冰洋的表面能平衡。为了量化这种能量平衡,并提高我们对北极海洋的变化的理解,项目“推进建模和观察海冰太阳辐射 - 理解变化和流程(Amora)”的机制是在2009年10月开始的。 Amora由挪威研究委员会资助,将持续到2013年。在挪威 - 中国双边合作方案的框架下,在气候研究的框架下组织。来自芬兰,德国和美国的其他国际合作伙伴正在积极参与这一项目。到目前为止,已经进行了各种项目任务:(1)在不同北极地区的几个国家/国际研究巡航和田野活动期间的原位数据收集(Chinare-2010;挪威R / V Fram Skrait Cruise 2011;挪威kv svalbard巡航2011;德国偏光态北极巡航2011); (2)项目合作伙伴(挪威和中国,挪威和德国,以及挪威和芬兰)之间的研究流动和交流; (3)合作伙伴中的仪器交流和发展,(4)高分辨率热力雪/冰型发展。通过海冰的光谱辐射反射和传输的自主观察系统,所谓的光谱辐射浮标(SRB),正在开发和2012年首次部署。从SRB和ICE质量平衡浮标(IMB)收集的数据随着数值模型的研究将有助于我们更好地了解北极海冰的关键热力学过程和极地气候变化,特别是在海冰上。

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