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Feedback between dust particles and atmospheric processes over West Africa during dust episodes in March 2006 and June 2007

机译:2006年3月和2007年6月沙尘暴期间西非尘埃颗粒与大气过程之间的反馈

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We used the comprehensive model system COSMO-ART to quantify the impact ofmineral dust on the radiative fluxes, the temperature and the feedbackbetween dust particles and their emissions. We simulated two dust stormsover West Africa in March 2006 and in June 2007. Simulations with andwithout coupling of the actual dust concentration with the radiative fluxesand the thermodynamics were carried out for each case. The model results forthe 2006 case were compared with observations of the AMMA campaign.At the surface the shortwave radiative effect of mineral dust can bedescribed by a linear relation between the changes in net surface radiationand the aerosol optical depth (AOD). For an AOD at 450 nm of 1 the averageshortwave radiation reduction amounts ?140 W m?2 during noon. Thelongwave radiative effect of mineral dust is nonlinear, with an averageincrease of +70 W m?2 for an AOD (450 nm) of 1. At the top of theatmosphere the effect of the dust layer with an AOD of 1 on radiative fluxesis not as significant as at the surface. It is slightly positive for theshortwave and approximately 26 W m?2 for the longwave radiation.The height range and the extension of the dust layer determine the effect ofdust particles on the 2 m temperature. When the dust layer is attached tothe surface and lasts for several days it leads to an increase of thesurface temperature even during daytime. In case of an elevated dust layerthere is a decrease in 2 m temperature of up to 4 K during noon.It is shown, that the temperature changes caused by mineral dust may resultin horizontal temperature gradients which also modify near surface winds.Since surface wind thresholds decide the uptake of dust from the surface, afeedback on total emission fluxes is established. The coupled model providesan increase in the total emission fluxes of dust particles by about 16%during the dust storm in March 2006 and 25% during the dust episode inJune 2007.
机译:我们使用综合模型系统COSMO-ART来量化矿物粉尘对辐射通量,温度以及粉尘颗粒及其排放之间的反馈的影响。我们分别于2006年3月和2007年6月对西非的两次沙尘暴进行了模拟。在每种情况下,都进行了实际尘埃浓度与辐射通量和热力学的耦合和不耦合的模拟。将2006年案例的模型结果与AMMA运动的观测结果进行了比较。 在表面,矿物尘埃的短波辐射效应可以通过净表面辐射的变化与气溶胶光学深度(AOD)之间的线性关系来描述。 )。对于450nm处的AOD为1,中午期间平均短波辐射减少量为≤140Wm≤2。矿物粉尘的长波辐射效应是非线性的,当AOD(450 nm)为1时,平均增加+70 W m ?2 。在大气层顶部,具有AOD的粉尘层的效应辐射通量的1不如表面显着。对于短波来说略微为正,对于长波辐射来说为约26 W m ?2 。 尘埃层的高度范围和延伸决定了尘埃颗粒对2 m的影响温度。当灰尘层附着在表面并持续数天时,即使在白天,也会导致表面温度升高。如果尘埃层升高,则中午时分2m的温度会降低,最高可达4K。 表明,矿物尘埃引起的温度变化可能会导致水平温度梯度,这也会改变近地表温度由于表面风阈值决定了表面灰尘的吸收,因此建立了总排放通量的反馈。耦合模型使尘埃颗粒的总排放通量在2006年3月的沙尘暴期间增加了约16%,在2007年6月的沙尘暴期间增加了25%。

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