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CALIPSO lidar observations of the optical properties of Saharan dust: A case study of long-range transport

机译:CALIPSO激光雷达对撒哈拉尘埃光学特性的观察:以远距离传输为例

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An extensive dust storm originating on 17 August 2006 in North Africa was observed and tracked by the Cloud-Aerosol Lidar and Infrared Pathfinder Satellite Observations (CALIPSO) lidar. Over the next several days, the dust layer moved westward across the Atlantic Ocean and into the Gulf of Mexico. The initial stages of the event were examined using a sequence of CALIPSO measurements. The first of these was acquired very near the source on 18 August. Successive measurements were made over the Atlantic Ocean on 19 and 20 August, at respective locations approximately ~1300 km and ~2400 km from the source region. The later stages of the event were assessed using measurements acquired by the NASA Langley Research Center airborne HSRL over the Gulf of Mexico on 28 August. Within the free troposphere, the intrinsic optical properties of the dust remain relatively unchanged for the first 3 d of transport over the Atlantic Ocean. This is consistent with previous in situ measurements that have shown that there is little change in the size distribution of dust as it crosses the Atlantic. After the 10 d journey to the Gulf of Mexico, some changes are seen in the lidar ratios, the backscatter color ratio, and the optical depth ratio. The linear depolarization ratio appears to remain essentially constant (~0.32) at all four locations mentioned above, demonstrating a notable consistency in the dust particle nonsphericity. The measured 532 nm lidar ratios are 41 ± 3, 41 ± 4, 41 ± 6 and 45.8 ± 0.8 sr, respectively, at locations near the source, over the Atlantic Ocean, and in the Gulf of Mexico. The corresponding 1064 nm lidar ratios are 52 ± 5, 55 ± 5, 54 ± 13 and 44 ± 8.3 sr. The 532 nm lidar ratios are consistent with previous measurements and with CALIPSO's prelaunch models. The lidar ratios retrieved at 1064 nm are somewhat larger than would be expected on the basis of existing modeling studies. The backscatter color ratios are 0.74 ± 0.07, 0.75 ± 0.08, 0.72 ± 0.04 and 0.62 ± 0.01, and the optical depth ratios are 0.97 ± 0.02, 1.01 ± 0.05, 0.93 ± 0.17 and 0.62 ± 0.13, respectively.
机译:2006年8月17日在北非发起了一场大范围的沙尘暴,并由Cloud-Aerosol激光雷达和红外探路者卫星观测(CALIPSO)激光雷达进行了跟踪。在接下来的几天中,尘埃层向西移动,穿过大西洋并进入墨西哥湾。使用CALIPSO测量序列检查了事件的初始阶段。其中第一个是在8月18日非常接近源头的时候获得的。于8月19日至20日在大西洋上进行了连续测量,分别位于距源区约1300 km和2400 km的位置。事件的后期阶段是使用8月28日在墨西哥湾上空的NASA兰利研究中心机载HSRL获得的测量值进行评估的。在自由对流层内,尘埃的固有光学性质对于在大西洋上空传输的前3天保持相对不变。这与以前的现场测量结果一致,该测量结果表明,尘埃越过大西洋,其尺寸分布几乎没有变化。到达墨西哥湾10天后,激光雷达比率,反向散射色比率和光学深度比率发生了一些变化。线性去极化比在上述所有四个位置似乎基本保持恒定(约0.32),这表明尘埃颗粒非球形性具有明显的一致性。在源附近,大西洋上空和墨西哥湾中,测得的532 nm激光雷达比分别为41±3、41±4、41±6和45.8±0.8 sr。相应的1064 nm激光雷达比为52±5、55±5、54±13和44±8.3 sr。 532 nm激光雷达比率与之前的测量以及CALIPSO的预发射模型一致。在1064 nm处获得的激光雷达比比根据现有模型研究预期的要大一些。背向散射色比为0.74±0.07、0.75±0.08、0.72±0.04和0.62±0.01,光学深度比分别为0.97±0.02、1.01±0.05、0.93±0.17和0.62±0.13。

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