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The use of SMILES data to study ozone loss in the Arctic winter 2009/2010 and comparison with Odin/SMR data using assimilation techniques

机译:使用SMILES数据研究2009/2010年北极冬季臭氧损失,并使用同化技术与Odin / SMR数据进行比较

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摘要

The Superconducting Submillimeter-Wave Limb-Emission Sounder (SMILES) on board theInternational Space Station observed ozone in the stratosphere with high precisionfrom October 2009 to April 2010.Although SMILES measurements only cover latitudes from 38° S to 65° N,the combination of data assimilation methods and an isentropic advection model allowsus to quantify the ozone depletion in the 2009/2010 Arctic polar winter by making use ofthe instability of the polar vortex in the northern hemisphere.Ozone data from both SMILES and Odin/SMR (Sub-Millimetre Radiometer) for the winterwere assimilated into the Dynamical Isentropic Assimilation Model for OdiN Data (DIAMOND).DIAMOND is an off-line wind-driven transport model on isentropic surfaces.Wind data from the operational analyses of the European Centre for Medium- RangeWeather Forecasts (ECMWF) were used to drive the model.In this study, particular attention is paid to the cross isentropic transport of thetracer in order to accurately assess the ozone loss.The assimilated SMILES ozone fields agree well with the limitation of noise inducedvariability within the SMR fields despite the limited latitude coverage of the SMILESobservations.Ozone depletion has been derived by comparing the ozone field acquired by sequentialassimilation with a passively transported ozone field initialized on 1 December 2009.Significant ozone loss was found in different periods and altitudes from using bothSMILES and SMR data:The initial depletion occurred at the end of January below 550 K with an accumulatedloss of 0.6–1.0 ppmv (approximately 20%) by 1 April.The ensuing loss started from the end of February between 575 K and 650 K.Our estimation shows that 0.8–1.3 ppmv (20–25 %) of O has beenremoved at the 600 K isentropic level by 1 April in volume mixing ratio (VMR).
机译:从2009年10月到2010年4月,国际空间站上的超导亚毫米波无辐射探测器(SMILES)观测到平流层中的臭氧的精度很高。尽管SMILES的测量仅覆盖了38°S至65°N的纬度,同化方法和等熵对流模型使我们能够利用北半球极涡的不稳定性来量化2009/2010北极极地冬季中的臭氧消耗。来自SMILES和Odin / SMR的臭氧数据(次毫米辐射计) OdiN数据的动态等熵同化模型(DIAMOND)吸收了冬季的数据.DIAMOND是等熵表面上的离线风驱动运输模型。欧洲中距离天气预报中心(ECMWF)的运行分析得出的风力数据在本研究中,要特别注意示踪剂的交叉等熵传输,以便准确地尽管SMILES观测的纬度覆盖范围有限,但同化SMILES臭氧场与SMR场内噪声引起的可变性的局限性很好地吻合。通过比较顺序同化获得的臭氧场与被动运输的臭氧场得出了臭氧耗竭的结论。通过使用SMILES和SMR数据,在不同的时期和海拔高度发现了显着的臭氧损失:1月底发生的初始损耗在550 K以下,累积损耗为0.6-1.0 ppmv(约20%),下降幅度为1。 4月。随之而来的损失从2月底开始在575 K和650 K之间。我们的估计显示,到4月1日,在600 K等熵水平上,体积混合比中已除去了0.8–1.3 ppmv(20–25%)的O( VMR)。

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