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Solar radiation measurements compared to simulations at the BSRN Iza?a station. Mineral dust radiative forcing and efficiency study

机译:太阳辐射测量与BSRN Iza?a站的模拟结果的比较。矿物粉尘辐射强迫与效率研究

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1 This paper presents a comparative study of shortwave downward radiation (SDR) measurements and simulations, obtained with the radiative transfer model LibRadtran, at the Baseline Surface Radiation Network (BSRN) site of Iza?a Atmospheric Observatory (IZA, Spain). The analysis is based on cloud-free days between March 2009 and August 2012 (386 days), including aerosol-free and Saharan mostly pure mineral dust conditions and comparing the day-to-day, annual, and interannual variability. The observed agreement between simulations and measurements is excellent: the variance of daily measurements overall agrees within 99 with the variance of daily simulations, and the mean bias (simulations-measurements) is -0.30 ± 0.24 MJm~(-2)(-1.1 ± 0.9) for global, -0.16±0.34 MJm~(-2)(-0.4±0.9) for direct, and +0.02±0.25 MJm~(-2)(+0.9±9.2) for diffuse SDR. Furthermore, the diurnally averaged aerosol radiative forcing (?DF) and radiative forcing efficiency (?DF~(eff)) due to Saharan mostly pure mineral dust events has been computed at Iza?a Observatory. The mean ?DF values are -7 ± 1, -96 ± 5, and 44 ±2 Wm-2 for global, direct, and diffuse BSRN SDR, respectively (mean aerosol optical depth, AOD, at 500 nm of 0.18 ± 0.01), whereas the mean ?DF~(eff) values are -59 ± 6, -495 ± 11, and 230 ±8 Wm-2 per unit of AOD at 500 nm for global, direct, and diffuse BSRN SDR, respectively. These values highlight the importance of scattering processes for mineral dust aerosols: the ratio between ?DF and the corresponding SDR without aerosols is ~ 2.5 for diffuse SDR versus 0.2 for direct SDR. This illustrates the significant potential of mineral dust particles to cool the Earth-atmosphere system.
机译:[1] 本文介绍了在伊萨大气观测站(西班牙伊扎)基线表面辐射网络 (BSRN) 站点使用辐射传输模型 LibRadtran 获得的短波下向辐射 (SDR) 测量和模拟的比较研究。该分析基于2009年3月至2012年8月(386天)之间的无云天数,包括无气溶胶和撒哈拉沙漠大部分纯矿物尘埃条件,并比较了日、年和年际变化。模拟和测量之间的一致性非常好:每日测量的方差总体上与每日模拟的方差一致在99%以内,平均偏差(模拟-测量)为-0.30±0.24 MJm~(-2)(-1.1 ± 0.9%),-0.16±0.34 MJm~(-2)(-0.4±0.9%),直接和+0.02±0.25 MJm~(-2)(+0.9±9.2%)。此外,昼夜平均气溶胶辐射强迫(?DF)和辐射强迫效率(?由于撒哈拉主要是纯矿物尘埃事件,DF~(eff))已在伊萨阿天文台计算。平均值 ?对于全局、直接和漫射 BSRN SDR,DF 值分别为 -7 ± 1、-96 ± 5 和 44 ±2 Wm-2(500 nm 处的平均气溶胶光学深度 AOD,为 0.18 ± 0.01),而平均值 ?DF~(eff) 值分别为 -59 ± 6、-495 ± 11 和 230 ±8 Wm-2/单位 AOD 在 500 nm 处的 BSRN SDR。这些值突出了矿物粉尘气溶胶散射过程的重要性:?对于弥散性 SDR,DF 和相应的无气溶胶 SDR 为 ~ 2.5%,而直接 SDR 为 0.2%。这说明了矿物尘埃颗粒冷却地球大气系统的巨大潜力。

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