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Chilean Observation Network De MeteOr Radars (CONDOR): Multi-Static System Configuration & Wind Comparison with Co-located Lidar 智利气象雷达观测网络(CONDOR):多静态系统配置及与同地激光雷达的风力比较
IF 3.8 3区 地球科学 Q2 METEOROLOGY & ATMOSPHERIC SCIENCES Pub Date : 2024-09-18 DOI: 10.5194/amt-2024-126
Zishun Qiao, Alan Z. Liu, Gunter Stober, Javier Fuentes, Fabio Vargas, Christian L. Adami, Iain M. Reid
Abstract. The Chilean Observation Network De MeteOr Radars (CONDOR) commenced deployment in June 2019 and became fully operational in February 2020. It is a multi-static meteor radar system consisting of three ~1º latitudinally separated stations. The main (central) station is located at the Andes Lidar Observatory (ALO, 30.25º S, 70.74º W) and is used for both transmission and reception. The two remote sites are located to the north and south and are used for reception only. The southern station is located at the Southern Cross Observatory (SCO, 31.20º S, 71.00º W) and the northern station is located at Las Campanas Observatory (LCO, 29.02º S, 70.69º W). The successful deployment and maintenance of CONDOR provide 24/7 measurements of horizontal winds in the mesosphere and lower thermosphere (MLT), and permit the retrieval of spatially resolved horizontal winds, vertical winds, and temperatures. This is possible because of the high meteor detection rates. Over 30,000 quality controlled underdense meteor echoes are detected at the ALO each day and in total ~88,000 events are detected each day over the three sites. In this paper, we present the system configuration of the CONDOR and discuss the validation and initial results of its data products. The motivations of deploying the CONDOR system also include the combination of results with other co-located ground-based instruments at the ALO, which provide uniquely cross-validated and cross-scale observations of the MLT dynamics with multiple scientific goals.
摘要智利气象雷达观测网络(CONDOR)于 2019 年 6 月开始部署,2020 年 2 月全面投入运行。这是一个多静态流星雷达系统,由三个纬度相距约 1º 的站点组成。主(中心)站位于安第斯激光雷达观测站(ALO,南纬 30.25º,西经 70.74º),用于发射和接收。两个偏远站点分别位于北面和南面,仅用于接收。南站位于南十字星天文台(SCO,南纬 31.20º,西经 71.00º),北站位于拉斯坎帕纳斯天文台(LCO,南纬 29.02º,西经 70.69º)。CONDOR 的成功部署和维护提供了对中间层和低温层(MLT)水平风的全天候测量,并允许检索空间分辨率的水平风、垂直风和温度。之所以能够做到这一点,是因为流星探测率很高。ALO 每天检测到超过 30,000 次质量受控的低密度流星回波,三个站点每天共检测到约 88,000 次事件。在本文中,我们将介绍 CONDOR 的系统配置,并讨论其数据产品的验证和初步结果。部署 CONDOR 系统的动机还包括将结果与 ALO 的其他共址地面仪器相结合,这些仪器提供了独特的跨验证和跨尺度的 MLT 动态观测,具有多重科学目标。
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引用次数: 0
Empirical model for backscattering polarimetric variables in rain at W-band: motivation and implications W 波段雨中反向散射偏振变量的经验模型:动机和影响
IF 3.8 3区 地球科学 Q2 METEOROLOGY & ATMOSPHERIC SCIENCES Pub Date : 2024-09-18 DOI: 10.5194/amt-2024-143
Alexander Myagkov, Tatiana Nomokonova, Michael Frech
Abstract. The established relationships between the size, shape, and terminal velocity of raindrops, along with the spheroidal shape approximation (SSA), are commonly employed for calculating radar observables in rain. This study, however, reveals the SSA's limitations in accurately simulating spectral and integrated backscattering polarimetric variables in rain at the W-band. Improving existing models is a complex task that demands high-precision data from both laboratory settings and natural rain, enhanced stochastic shape approximation techniques, and comprehensive scattering simulations. To circumvent these challenges, this study introduces a simpler and more straightforward approach – the empirical scattering model (ESM). The ESM is derived from an analysis of high-quality, low-turbulence Doppler spectra, which were selected from measurements taken with a 94 GHz radar at three different locations between 2021 and 2024. The ESM's primary advantages over the SSA include superior accuracy and the direct incorporation of microphysical effects observed in natural rain. This study demonstrates that the ESM can potentially clarify issues in existing retrieval and calibration methods that use polarimetric observations at the W-band. The findings of this study are not only valuable for experts in cloud radar polarimetry but also for scattering modelers and laboratory experimenters since explaining the presented observations necessitates a more profound understanding of the microphysical properties and processes in rain.
摘要雨滴的大小、形状和末端速度之间的既定关系以及球形近似(SSA)通常用于计算雨中的雷达观测值。然而,本研究揭示了 SSA 在准确模拟 W 波段雨中的光谱和综合后向散射偏振变量方面的局限性。改进现有模型是一项复杂的任务,需要从实验室环境和自然降雨中获取高精度数据、增强随机形状近似技术和综合散射模拟。为了规避这些挑战,本研究引入了一种更简单、更直接的方法--经验散射模型(ESM)。ESM来自对高质量、低湍流多普勒频谱的分析,这些频谱选自2021年至2024年期间在三个不同地点使用94 GHz雷达进行的测量。与 SSA 相比,ESM 的主要优势包括精度更高,并直接纳入了在自然降雨中观测到的微物理效应。这项研究表明,ESM 有可能澄清使用 W 波段偏振观测数据的现有检索和校准方法中存在的问题。这项研究的结果不仅对云雷达偏振测量专家很有价值,而且对散射建模人员和实验室实验人员也很有价值,因为要解释这些观测结果,就必须更深入地了解雨的微物理特性和过程。
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引用次数: 0
Increasing aerosol optical depth spatial and temporal availability by merging datasets from geostationary and sun-synchronous satellites 通过合并来自地球静止卫星和太阳同步卫星的数据集,提高气溶胶光学深度的时空可用性
IF 3.8 3区 地球科学 Q2 METEOROLOGY & ATMOSPHERIC SCIENCES Pub Date : 2024-09-16 DOI: 10.5194/amt-17-5455-2024
Pawan Gupta, Robert C. Levy, Shana Mattoo, Lorraine A. Remer, Zhaohui Zhang, Virginia Sawyer, Jennifer Wei, Sally Zhao, Min Oo, V. Praju Kiliyanpilakkil, Xiaohua Pan
Abstract. This comprehensive study analyzed aerosol products from six low-Earth orbit (LEO) and geostationary Earth orbit (GEO) sensors. LEO sensors like the MODerate resolution Imaging Spectroradiometer (MODIS) and VIsible InfraRed Suite (VIIRS) provide one to two daily global measurements, while GEO sensors (Advanced Himawari Imager: AHI, Advanced Baseline Imager: ABI) offer high-frequency data (∼ 10 min) over specific regions. The combination of LEO and GEO capabilities offers expanded coverage of the global aerosol system if aerosol retrievals are applied consistently across all sensors and packaged in an easy-to-use product. The Dark Target aerosol retrieval algorithm was applied to the six sensors, and the resulting Level 2 aerosol optical depth (AOD) products were gridded and merged into a Level 3 quarter-degree latitude–longitude grid with a 30 min temporal resolution, providing the necessary consistency and packaging. Validation of this packaged Level 3 AOD product against Aerosol Robotics NETwork (AERONET) measurements across global locations showcased the merged product's robustness with a correlation coefficient of 0.83, revealing a global mean bias of approximately ±0.05, with 65.5 % of retrievals falling within an expected uncertainty range, underlining the reliability of the dataset. The new gridded Level 3 dataset significantly improved daily global coverage to nearly 45 %, overcoming the limitations of individual sensors, which typically range from 12 % to 25 %. Furthermore, this merged dataset approximates the diurnal cycle of AOD observed by AERONET, thus offering insights into diurnal signatures retrieved elsewhere. The resulting dataset's high spatiotemporal resolution and improved global coverage, especially in regions covered by GEO sensors (Americas and Asia), make it a valuable tool for diverse applications. Tracking aerosol transport from phenomena like wildfires and dust storms is gaining precision, enabling enhanced air quality forecasting and hindcasting. Additionally, the study positions the merged dataset as a significant asset for evaluating and intercomparing regional or global model simulations, which was previously unattainable in such a gridded format. The dataset and fusion framework layout in this study have the potential to include data from recently (future) launched other GEO (FCI, AMI) and LEO (PACE, VIIRS-JPSS) sensors.
摘要这项综合研究分析了来自六个低地轨道(LEO)和地球静止轨道(GEO)传感器的气溶胶产品。低地轨道传感器,如中分辨率成像分光仪(MODIS)和VIIRS(VIsible InfraRed Suite),每天提供一到两次全球测量数据,而地球同步轨道传感器(高级向日葵成像仪:AHI,高级基线成像仪:ABI)则提供特定区域的高频数据(10 分钟)。如果在所有传感器上一致应用气溶胶检索,并将其打包成易于使用的产品,那么低地轨道和地球同步轨道能力的结合将扩大全球气溶胶系统的覆盖范围。黑暗目标 "气溶胶检索算法应用于六个传感器,由此产生的二级气溶胶光学深度(AOD)产品被网格化,并合并为具有 30 分钟时间分辨率的三级四分之一度经纬度网格,从而提供了必要的一致性和包装。根据气溶胶机器人网络(AERONET)在全球各地的测量结果,对这一打包的三级 AOD 产品进行了验证,结果表明合并后的产品非常可靠,相关系数为 0.83,显示全球平均偏差约为±0.05,65.5%的检索结果在预期的不确定性范围内,凸显了数据集的可靠性。新的网格化三级数据集将每日全球覆盖率大幅提高到近45%,克服了单个传感器通常在12%到25%之间的局限性。此外,合并后的数据集近似于 AERONET 观测到的 AOD 日周期,从而为其他地方检索到的日特征提供了启示。合并后的数据集具有较高的时空分辨率,并扩大了全球覆盖范围,特别是在地球同步轨道传感器覆盖的地区(美洲和亚洲),因此是一种可用于多种应用的宝贵工具。对野火和沙尘暴等现象产生的气溶胶迁移的跟踪越来越精确,从而能够加强空气质量预报和后向预测。此外,该研究还将合并数据集定位为评估和相互比较区域或全球模型模拟的重要资产,这在以前的网格格式中是无法实现的。本研究的数据集和融合框架布局有可能包括最近(未来)发射的其他地球同步轨道(FCI、AMI)和低地轨道(PACE、VIIRS-JPSS)传感器的数据。
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引用次数: 0
Laminar gas inlet – Part 2: Wind tunnel chemical transmission measurement and modelling 层流气体入口 - 第 2 部分:风洞化学传输测量和建模
IF 3.8 3区 地球科学 Q2 METEOROLOGY & ATMOSPHERIC SCIENCES Pub Date : 2024-09-16 DOI: 10.5194/egusphere-2024-2390
Da Yang, Emmanuel Assaf, Roy Mauldin, Suresh Dhaniyala, Rainer Volkamer
Abstract. Aircraft-based measurements of gas-phase species and aerosols provide crucial knowledge about the composition and vertical structure of the atmosphere, enhancing the study of atmospheric physics and chemistry. Unlike aircraft-based aerosol particle sampling systems, the gas loss mechanisms and transmission efficiency of aircraft-based gas sampling systems are rarely discussed. In particular, the gas transmission of condensable vapors through these sampling systems requires systematic study to clarify the key factors of gas loss and to predict and improve gas sampling efficiency quantitatively. An aircraft gas inlet for aircraft-based laminar sampling of condensable vapors is described in part 1 (Yang et al., 2024), which describes the inlet dimensions, flow analysis and modelling, along with initial gas transmission estimates. Here we test and characterize the complete inflight sampling system using for gas-phase measurements of 𝐻2𝑆𝑂4 in a high-speed wind tunnel, and conduct detailed computer fluid dynamics (CFD) simulations to assess inlet performance under a range of flight conditions. The gas transmission efficiency of 𝐻2𝑆𝑂4 through different sampling lines was measured using Chemical Ionization Mass Spectrometry (CIMS), and the experimental results are reproduced by the CFD simulations of flow and mass diffusion using a mass accommodation coefficient, 𝛼𝑖 = 0.70 ± 0.05 for 𝐻2𝑆𝑂4 on inlet lines. The experimental data and simulation results show consistently that gas transmission efficiency increases with an increased sampling flow rate. The simulation results further indicate that sampling efficiency can continue to improve to a certain level after the sampling flow enters the turbulent flow regime, up to Reynolds numbers, Re ~ 6000. A decrease in transmission is predicted only for higher Re numbers. These results challenge the widely held assumption that laminar flow core sampling is the best strategy for sampling condensable vapors. The gas-phase 𝐻2𝑆𝑂4 transmission efficiency can be optimized (increased by a factor ~2) by minimizing residence time, rather than maintaining laminar flow; this benefit extends to other condensable vapors and applies over the full range of operating conditions of the aircraft inlet system. For a sticky species (𝛼𝑖 > 0.25), the laminar diffusivity is important to predict the transmission efficiency via the aircraft inlet section, while for less sticky species (𝛼𝑖 < 0.25) the gas-phase diffusivity plays a minor role in predicting the gas transmission efficiency in the sampling line.
摘要飞机对气相物种和气溶胶的测量提供了有关大气组成和垂直结构的重要知识,从而加强了对大气物理和化学的研究。与飞机气溶胶粒子采样系统不同,人们很少讨论飞机气体采样系统的气体损失机制和传输效率。特别是可凝蒸汽通过这些采样系统的气体传输问题,需要进行系统研究,以明确气体损失的关键因素,并定量预测和提高气体采样效率。第 1 部分(Yang 等人,2024 年)介绍了用于飞机层流采样可冷凝蒸汽的飞机气体入口,其中描述了入口尺寸、流动分析和建模,以及气体传输的初步估计。在这里,我们在高速风洞中使用𝐻2𝑆𝑂4 的气相测量方法对完整的机上采样系统进行了测试和鉴定,并进行了详细的计算机流体动力学(CFD)模拟,以评估一系列飞行条件下的进气口性能。利用化学电离质谱法(CIMS)测量了𝐻2𝑆𝑂4 通过不同采样管路的气体传输效率,并使用质量容纳系数𝛼𝑖 = 0.70 ± 0.05 对𝐻2𝑆𝑂4 在入口管路上的流动和质量扩散进行了 CFD 模拟,从而再现了实验结果。实验数据和模拟结果一致表明,气体传输效率随着采样流量的增加而提高。模拟结果进一步表明,采样流进入湍流状态后,采样效率会继续提高到一定水平,最高可达雷诺数 Re ~ 6000。只有在雷诺数较高时,传输效率才会下降。这些结果对人们普遍认为层流岩心取样是冷凝蒸汽取样的最佳策略这一假设提出了质疑。气相𝐻2𝑆𝑂4 的传输效率可以通过最大限度地缩短停留时间而不是保持层流来优化(提高约 2 倍);这一优势也适用于其他可冷凝蒸汽,并且适用于飞机进气系统的所有工作条件。对于粘性较大的物质(𝛼𝑖 >0.25),层流扩散率对于预测通过飞机入口部分的传输效率非常重要,而对于粘性较小的物质(𝛼𝑖 <0.25),气相扩散率在预测采样管路中的气体传输效率方面作用较小。
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引用次数: 0
Methane retrieval from MethaneAIR using the CO2 proxy approach: a demonstration for the upcoming MethaneSAT mission 利用二氧化碳替代方法从 MethaneAIR 提取甲烷:为即将到来的 MethaneSAT 任务进行演示
IF 3.8 3区 地球科学 Q2 METEOROLOGY & ATMOSPHERIC SCIENCES Pub Date : 2024-09-16 DOI: 10.5194/amt-17-5429-2024
Christopher Chan Miller, Sébastien Roche, Jonas S. Wilzewski, Xiong Liu, Kelly Chance, Amir H. Souri, Eamon Conway, Bingkun Luo, Jenna Samra, Jacob Hawthorne, Kang Sun, Carly Staebell, Apisada Chulakadabba, Maryann Sargent, Joshua S. Benmergui, Jonathan E. Franklin, Bruce C. Daube, Yang Li, Joshua L. Laughner, Bianca C. Baier, Ritesh Gautam, Mark Omara, Steven C. Wofsy
Abstract. Reducing methane (CH4) emissions from the oil and gas (O&G) sector is crucial for mitigating climate change in the near term. MethaneSAT is an upcoming satellite mission designed to monitor basin-wide O&G emissions globally, providing estimates of emission rates and helping identify the underlying processes leading to methane release in the atmosphere. MethaneSAT data will support advocacy and policy efforts by helping to track methane reduction commitments and targets set by countries and industries. Here, we introduce a CH4 retrieval algorithm for MethaneSAT based on the CO2 proxy method. We apply the algorithm to observations from the maiden campaign of MethaneAIR, an airborne precursor to the satellite that has similar instrument specifications. The campaign was conducted during winter 2019 and summer 2021 over three major US oil and gas basins. Analysis of MethaneAIR data shows that measurement precision is typically better than 2 % at a 20×20 m2 pixel resolution, exhibiting no strong dependence on geophysical variables, e.g., surface reflectance. We show that detector focus drifts over the course of each flight, likely due to thermal gradients that develop across the optical bench. The impacts of this drift on retrieved CH4 can mostly be mitigated by including a parameter that squeezes the laboratory-derived, tabulated instrument spectral response function (ISRF) in the spectral fit. Validation against coincident EM27/SUN retrievals shows that MethaneAIR values are generally within 1 % of the retrievals. MethaneAIR retrievals were also intercompared with retrievals from the TROPOspheric Monitoring Instrument (TROPOMI). We estimate that the mean bias between the instruments is 2.5 ppb, and the latitudinal gradients for the two data sets are in good agreement. We evaluate the accuracy of MethaneAIR estimates of point-source emissions using observations recorded over the Permian Basin, an O&G basin, based on the integrated-mass-enhancement approach coupled with a plume-masking algorithm that uses total variational denoising. We estimate that the median point-source detection threshold is 100–150 kg h−1 at the aircraft's nominal above-surface observation altitude of 12 km. This estimate is based on an ensemble of Weather Research and Forecasting (WRF) large-eddy simulations used to mimic the campaign's conditions, with the threshold for quantification set at approximately twice the detection threshold. Retrievals from repeated basin surveys indicate the presence of both persistent and intermittent sources, and we highlight an example from each case. For the persistent source, we infer emissions from a large O&G processing facility and estimate a leak rate between 1.6 % and 2.1 %, higher than any previously reported emission levels from a facility of its size. We also identify a ruptured pipeline that could increase total basin emissions by 2 % if left unrepaired; this pipeline was discovered 2 weeks before it was found by its operator
摘要。减少石油和天然气(O&G)行业的甲烷(CH4)排放对于在短期内减缓气候变化至关重要。MethaneSAT 是一项即将实施的卫星任务,旨在监测全球范围内全流域的石油和天然气排放情况,提供排放率估计值,并帮助确定导致甲烷释放到大气中的基本过程。MethaneSAT 的数据将有助于跟踪各国和各行业设定的甲烷减排承诺和目标,从而为宣传和政策制定工作提供支持。在此,我们介绍一种基于二氧化碳替代方法的甲烷卫星甲烷检索算法。我们将该算法应用于 MethaneAIR 的首次观测活动,MethaneAIR 是该卫星的机载前身,具有类似的仪器规格。该活动于 2019 年冬季和 2021 年夏季在美国三大油气盆地上空进行。对 MethaneAIR 数据的分析表明,在 20×20 平方米的像素分辨率下,测量精度通常优于 2%,对地球物理变量(如地表反射率)没有很强的依赖性。我们的研究表明,探测器的焦点在每次飞行过程中都会发生偏移,这可能是由于整个光学工作台产生的热梯度造成的。通过在光谱拟合中加入一个参数来挤压实验室得出的、表列的仪器光谱响应函数(ISRF),可以在很大程度上减轻这种漂移对检索到的甲烷的影响。与重合的 EM27/SUN 检索结果进行的验证表明,甲烷空气分析仪的数值一般在检索结果的 1%以内。甲烷空气检索值还与 TROPOspheric Monitoring Instrument (TROPOMI) 的检索值进行了相互比较。我们估计仪器之间的平均偏差为 2.5 ppb,两个数据集的纬度梯度非常一致。我们利用在二叠纪盆地(一个石油和天然气盆地)上空记录的观测数据,评估了 MethaneAIR 对点源排放估算的准确性,该估算基于综合质量增强方法和使用总变异去噪的羽状掩蔽算法。我们估计,在飞机标称的地面以上观测高度 12 千米处,点源检测阈值中值为 100-150 千克/小时。这一估算基于气象研究与预报(WRF)大涡模拟集合,用于模拟活动条件,量化阈值约为探测阈值的两倍。反复流域调查的检索结果表明,存在持续源和间歇源,我们将重点介绍每种情况下的一个例子。对于持续源,我们推断是一个大型石油和天然气加工设施排放的,估计泄漏率在 1.6 % 到 2.1 % 之间,高于之前报告的同规模设施的排放水平。我们还发现了一条破裂的管道,如果不及时修复,可能会使盆地的总排放量增加 2%;这条管道是在其运营商发现前两周被发现的,这突出了未来卫星任务定期监测的重要性。这些结果展示了 MethaneAIR 在单次飞行中对大气中甲烷干气摩尔分数进行高精度、精确测量的能力,其空间分辨率很高(20×20 平方米∼),可绘制大片区域(100×100 平方公里∼)的地图。这些结果使人们相信,甲烷卫星能够从空间以前所未有的精细尺度(目标区域面积为 200×200 平方公里,像素大小为 130×400 平方米)进行此类测量,从而提供关于全流域甲烷排放的定量数据。
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引用次数: 0
Independent validation of IASI/MetOp-A LMD and RAL CH4 products using CAMS model, in situ profiles, and ground-based FTIR measurements 利用 CAMS 模型、现场剖面和地面傅立叶变换红外测量,独立验证 IASI/MetOp-A LMD 和 RAL CH4 产品
IF 3.8 3区 地球科学 Q2 METEOROLOGY & ATMOSPHERIC SCIENCES Pub Date : 2024-09-16 DOI: 10.5194/amt-17-5491-2024
Bart Dils, Minqiang Zhou, Claude Camy-Peyret, Martine De Mazière, Yannick Kangah, Bavo Langerock, Pascal Prunet, Carmine Serio, Richard Siddans, Brian Kerridge
Abstract. In this study, we carried out an independent validation of two methane retrieval algorithms using spectra from the Infrared Atmospheric Sounding Interferometer (IASI) that has been aboard the Meteorological Operational Satellite A (MetOp-A) since 2006. Both algorithms, one developed by the Laboratoire de Météorologie Dynamique (LMD), called the non-linear inference scheme (NLISv8.3), and the other by the Rutherford Appleton Laboratory (RAL), referred to as RALv2.0, provide long-term global CH4 concentrations using distinctively different retrieval approaches (neural network vs. optimal estimation, respectively). They also differ with respect to the vertical range covered, where LMD provides mid-tropospheric dry-air mole fractions (mtCH4), and RAL provides mixing ratio profiles from which we can derive total column-averaged dry-air mole fractions (XCH4) and potentially two partial column layers (qCH4). We compared both CH4 products using the Copernicus Atmospheric Monitoring Service (CAMS) model, in situ profiles (range extended using CAMS model data), and ground-based Fourier transform infrared (FTIR) remote-sensing measurements. The average difference (in mtCH4) with respect to in situ profiles for LMD ranges between −0.3 and 10.9 ppb, while for RAL the XCH4 difference ranges between −4.6 and −1.6 ppb. The standard deviation (SD) of the observed differences between in situ measurements and RAL retrievals is 14.1–21.9 ppb, which is consistently smaller than that between LMD retrievals and in situ measurements (15.2–30.6 ppb). By comparing with ground-based FTIR sites, the mean differences are within ±10 ppb for both RAL and LMD retrievals. However, the SD of the differences at the ground-based FTIR stations shows significantly lower values for RAL (11–15 ppb) than for LMD (about 25 ppb). The long-term trend and seasonal cycles of CH4 derived from the LMD and RAL products are further investigated and discussed. The seasonal variation in XCH4 derived from RAL is consistent with the seasonal variation observed by the ground-based FTIR measurements. However, the overall 2007–2015 XCH4 trend derived from RAL measurements is underestimated, if not adjusted, for an anomaly occurring on 16 May 2013 due to a L1 calibration change. For LMD, we see very good agreement at the (sub)tropics (<35° N–35° S) but notice deviations in the seasonal cycle (both in the amplitude and phase) and an underestimation of the long-term trend with respect to the RAL and reference data at higher-latitude sites.
摘要在这项研究中,我们利用 2006 年以来搭载在气象业务卫星 A(MetOp-A)上的红外大气探测干涉仪(IASI)的光谱,对两种甲烷检索算法进行了独立验证。这两种算法,一种由动力学实验室(LMD)开发,称为非线性推理方案(NLISv8.3),另一种由卢瑟福-阿普尔顿实验室(RAL)开发,称为 RALv2.0,均采用截然不同的检索方法(分别为神经网络和最优估计)提供长期的全球甲烷浓度。LMD 提供中对流层干空气摩尔分数(mtCH4),而 RAL 提供混合比剖面,我们可以从中得出柱平均干空气总摩尔分数(XCH4)和可能的两个部分柱层(qCH4)。我们利用哥白尼大气监测服务(CAMS)模型、原地剖面(利用 CAMS 模型数据扩展了范围)和地面傅立叶变换红外(FTIR)遥感测量数据对这两种 CH4 产品进行了比较。LMD 与原位剖面的平均差异(以 mtCH4 为单位)介于 -0.3 和 10.9 ppb 之间,而 RAL 的 XCH4 差异介于 -4.6 和 -1.6 ppb 之间。观测到的原地测量值与 RAL 回收值之间的差异的标准偏差(SD)为 14.1-21.9 ppb,始终小于 LMD 回收值与原地测量值之间的差异(15.2-30.6 ppb)。通过与地基傅立叶变换红外站点进行比较,RAL 和 LMD 回收率的平均差异均在±10 ppb 范围内。不过,地面傅立叶变换红外站的差异标差显示,RAL(11-15 ppb)明显低于 LMD(约 25 ppb)。我们进一步研究和讨论了 LMD 和 RAL 产品得出的 CH4 长期趋势和季节周期。从 RAL 中得出的 XCH4 季节性变化与地面傅立叶变换红外测量观测到的季节性变化一致。但是,如果不对 2013 年 5 月 16 日因 L1 校准变化而出现的异常进行调整,则会低估 RAL 测量得出的 2007-2015 年 XCH4 总体趋势。对于 LMD,我们发现在(亚)热带地区(<北纬 35°-南纬 35°)的一致性非常好,但注意到季节周期(振幅和相位)存在偏差,并且相对于 RAL 和高纬度站点的参考数据,长期趋势被低估。
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引用次数: 0
The role of time averaging of eddy covariance fluxes on water use efficiency dynamics of maize 涡协方差通量的时间平均化对玉米水分利用效率动态的影响
IF 3.8 3区 地球科学 Q2 METEOROLOGY & ATMOSPHERIC SCIENCES Pub Date : 2024-09-16 DOI: 10.5194/amt-17-5477-2024
Arun Rao Karimindla, Shweta Kumari, Saipriya S R, Syam Chintala, BVN P. Kambhammettu​​​​​​​
Abstract. Direct measurement of carbon and water fluxes at high frequencies make eddy covariance (EC) the technique most preferred to characterize water use efficiency (WUE). However, reliability of EC fluxes largely hinges on the energy balance ratio (EBR) and inclusion of low-frequency fluxes. This study is aimed at investigating the role of the averaging period in representing EC fluxes and its propagation into WUE dynamics. Carbon and water fluxes were monitored in a drip-irrigated maize field at 10 Hz frequency and were averaged over 1, 5, 10, 15, 30, 45, 60, and 120 min, considering daytime unstable conditions. The optimal averaging period to simulate WUE fluxes for each growth stage is obtained by considering cumulative frequency (Ogive) curves. A clear departure of EBR from unity was observed during the dough and maturity stages of the crop due to ignorance of canopy heat storage, low-frequency flux losses, and an inadequate averaging period. Deviations in representing water (carbon) fluxes relative to the conventional 30 min average are within ±3 % (±10 %) for 10–120 min averaging and beyond ±3 % (±10 %) for other time averages. Ogive plots show that the optimal averaging period to represent carbon, water, and WUE fluxes is 15–30 min for the sixth leaf and silking stages and is 45–60 min for the dough and maturity stages. Dynamics of WUE considering optimal averaging periods are in the range of μ ± σ: 1.49 ± 0.95, 1.37 ± 0.74, 1.39 ± 0.79, and 3.06 ± 0.69 µmol mmol−1 for the sixth leaf, silking, dough, and maturity stages, respectively. The error in representing WUE by conventional 30 min averaging is marginal (< 1.5 %) throughout the crop period except for the dough stage (12.12 %). We conclude that the conventional 30 min averaging of EC fluxes is not appropriate for representing WUE throughout the crop period. Our findings can help to develop efficient water management strategies by accurately characterizing WUE fluxes from the EC measurements.
摘要直接测量高频碳通量和水通量使涡度协方差(EC)成为描述水分利用效率(WUE)的首选技术。然而,EC 通量的可靠性在很大程度上取决于能量平衡比(EBR)和低频通量。本研究旨在探讨平均周期在代表 EC 通量方面的作用及其在 WUE 动态中的传播。考虑到白天的不稳定条件,在滴灌玉米田中以 10 赫兹的频率监测碳通量和水通量,并在 1、5、10、15、30、45、60 和 120 分钟内取平均值。通过考虑累积频率(Ogive)曲线,得出了模拟每个生长阶段 WUE 流量的最佳平均周期。由于忽略了冠层蓄热、低频通量损失和平均期不足,在作物的面团期和成熟期观察到 EBR 明显偏离统一值。相对于传统的 30 分钟平均值,10-120 分钟平均值的水(碳)通量偏差在 ±3 %(±10 %)以内,而其他时间平均值的偏差则超过 ±3 %(±10 %)。曲线图显示,代表碳、水和 WUE 通量的最佳平均时间段在第六片叶和抽丝阶段为 15-30 分钟,在面团和成熟阶段为 45-60 分钟。考虑到最佳平均期,WUE 的动态范围为 μ ± σ:六叶期、生丝期、面团期和成熟期的 WUE 动态值分别为 1.49 ± 0.95、1.37 ± 0.74、1.39 ± 0.79 和 3.06 ± 0.69 µmol mmol-1。除面团期(12.12%)外,传统的 30 分钟平均法在整个作物期表示 WUE 的误差很小(< 1.5%)。我们的结论是,传统的 30 分钟平均分配 EC 通量的方法不适合用来表示作物整个生长期的水分利用效率。我们的研究结果有助于通过EC测量值准确描述WUE通量,从而制定高效的水分管理策略。
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引用次数: 0
Ammonium CI-Orbitrap: a tool for characterizing the reactivity of oxygenated organic molecules 铵 CI-轨道阱:表征含氧有机分子反应性的工具
IF 3.8 3区 地球科学 Q2 METEOROLOGY & ATMOSPHERIC SCIENCES Pub Date : 2024-09-13 DOI: 10.5194/amt-17-5413-2024
Dandan Li, Dongyu Wang, Lucia Caudillo, Wiebke Scholz, Mingyi Wang, Sophie Tomaz, Guillaume Marie, Mihnea Surdu, Elias Eccli, Xianda Gong, Loic Gonzalez-Carracedo, Manuel Granzin, Joschka Pfeifer, Birte Rörup, Benjamin Schulze, Pekka Rantala, Sébastien Perrier, Armin Hansel, Joachim Curtius, Jasper Kirkby, Neil M. Donahue, Christian George, Imad El-Haddad, Matthieu Riva
Abstract. Oxygenated organic molecules (OOMs) play an important role in the formation of atmospheric aerosols. Due to various analytical challenges with respect to measuring organic vapors, uncertainties remain regarding the formation and fate of OOMs. The chemical ionization Orbitrap (CI-Orbitrap) mass spectrometer has recently been shown to be a powerful technique that is able to accurately identify gaseous organic compounds due to its greater mass resolution. Here, we present the ammonium-ion-based CI-Orbitrap (NH4+-Orbitrap) as a technique capable of measuring a wide range of gaseous OOMs. The performance of the NH4+-Orbitrap is compared with that of state-of-the-art mass spectrometers, including a nitrate-ion-based chemical ionization atmospheric pressure interface coupled to a time-of-flight mass spectrometer (NO3--LTOF), a new generation of proton transfer reaction-TOF mass spectrometer (PTR3-TOF), and an iodide-based CI-TOF mass spectrometer equipped with a Filter Inlet for Gases and AEROsols (I−-CIMS). The instruments were deployed simultaneously in the Cosmic Leaving OUtdoors Droplets (CLOUD) chamber at the European Organization for Nuclear Research (CERN) during the CLOUD14 campaign in 2019. Products generated from α-pinene ozonolysis under various experimental conditions were simultaneously measured by the mass spectrometers. The NH4+-Orbitrap was able to identify the widest range of OOMs (i.e., O ≥ 2), from less-oxidized species to highly oxygenated organic molecules (HOMs). Excellent agreement was found between the NH4+-Orbitrap and the NO3--LTOF with respect to characterizing HOMs and with the PTR3-TOF for the less-oxidized monomeric species. OOM concentrations measured by NH4+-Orbitrap were estimated using calibration factors derived from the OOMs with high time-series correlations during the side-by-side measurements. As with the other mass spectrometry techniques used during this campaign, the detection sensitivity of the NH4+-Orbitrap to OOMs is greatly affected by relative humidity, which may be related to changes in ionization efficiency and/or multiphase chemistry. Overall, this study shows that NH4+-ion-based chemistry associated with the high mass resolution of the Orbitrap mass analyzer can measure almost all inclusive compounds. As a result, it is now possible to cover the entire range of compounds, which can lead to a better understanding of the oxidation processes.
摘要含氧有机分子(OOMs)在大气气溶胶的形成过程中发挥着重要作用。由于在测量有机蒸汽方面存在各种分析难题,OOMs 的形成和归宿仍然存在不确定性。最近的研究表明,化学电离轨道阱(CI-Orbitrap)质谱仪是一种功能强大的技术,由于其质量分辨率更高,能够准确识别气态有机化合物。在此,我们介绍了基于铵离子的 CI-Orbitrap (NH4+-Orbitrap),它是一种能够测量多种气态 OOMs 的技术。我们将 NH4+-Orbitrap 的性能与最先进的质谱仪进行了比较,这些质谱仪包括基于硝酸根离子的化学电离常压界面耦合飞行时间质谱仪(NO3--LTOF)、新一代质子转移反应--TOF 质谱仪(PTR3-TOF)以及配备气体和气溶胶过滤器入口的基于碘化物的 CI-TOF 质谱仪(I--CIMS)。在2019年的CLOUD14活动期间,这些仪器同时部署在欧洲核子研究中心(CERN)的宇宙离体液滴室(CLOUD)中。质谱仪同时测量了各种实验条件下α-蒎烯臭氧分解产生的产物。NH4+-Orbitrap 能够识别范围最广的 OOMs(即 O ≥ 2),从氧化程度较低的物种到含氧程度较高的有机分子(HOMs)。NH4+-Orbitrap和NO3--LTOF在表征HOMs方面以及PTR3-TOF在表征氧化程度较低的单体物种方面具有极好的一致性。NH4+-Orbitrap测量的OOM浓度是利用并排测量过程中时间序列相关性较高的OOM得出的校准因子估算的。与本次活动中使用的其他质谱技术一样,NH4+-Orbitrap 对 OOM 的检测灵敏度受相对湿度的影响很大,这可能与电离效率和/或多相化学变化有关。总之,这项研究表明,基于 NH4+ 离子的化学反应与 Orbitrap 质量分析仪的高质 量分辨率相结合,可以测量几乎所有的包容性化合物。因此,现在有可能覆盖整个化合物范围,从而更好地了解氧化过程。
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引用次数: 0
Joint spectral retrievals of ozone with Suomi NPP CrIS augmented by S5P/TROPOMI 利用 S5P/TROPOMI 增强的 Suomi NPP CrIS 对臭氧进行联合光谱检索
IF 3.8 3区 地球科学 Q2 METEOROLOGY & ATMOSPHERIC SCIENCES Pub Date : 2024-09-12 DOI: 10.5194/amt-17-5341-2024
Edward Malina, Kevin W. Bowman, Valentin Kantchev, Le Kuai, Thomas P. Kurosu, Kazuyuki Miyazaki, Vijay Natraj, Gregory B. Osterman, Fabiano Oyafuso, Matthew D. Thill
Abstract. The vertical distribution of ozone plays an important role in atmospheric chemistry, climate change, air pollution, and human health. Over the 21st century, spaceborne remote-sensing methods and instrumentation have evolved to better determine this distribution. We quantify the ability of ozone retrievals to characterize this distribution through a sequential combination of thermal infrared (TIR) and ultraviolet (UV) spectral radiances, harnessing co-located TIR measurements from the Cross-track Infrared Sounder (CrIS) on board the Suomi National Polar-orbiting Partnership (NPP) and UV measurements from the TROPOspheric Monitoring Instrument (TROPOMI), which is on the Sentinel 5-Precursor (S5P) satellite. Using the MUlti-SpEctra, MUlti-SpEcies, MUlti-SEnsors (MUSES) algorithm, the sequential combination of TIR and UV measurements, which follows retrievals from each instrument separately, moderately improves the ability of satellites to characterize global ozone profiles over the use of each instrument/band individually. The CrIS retrievals enhanced by TROPOMI radiances in the Huggins band (325–335 nm) show good agreement with independent datasets both in the troposphere and in the stratosphere in spite of calibration issues in the TROPOMI UV. Improved performance is characterized in the stratosphere from CrIS-TROPOMI, firstly through a modest increase in the degrees of freedom for signal (DFS; often between 0.1–0.2) and secondly through comparisons with the Microwave Limb Sounder (MLS), where a global multi-month-long comparison shows a mean difference ∼×10 lower than either CrIS or TROPOMI individually and R2 values 3 % higher. In the troposphere, CrIS-TROPOMI and CrIS show similar degrees of freedom for signal, with about 2 globally, but these are higher in the tropics partitioned equally between the lower and upper troposphere. CrIS-TROPOMI validation with ozonesondes shows improved performance over CrIS-only validation, with a difference in the tropospheric-column bias of between 30 % and 200 % depending on the season. Cross-comparisons with satellite instruments and reanalysis datasets show similar performances in terms of correlations and biases. These results demonstrate that CrIS and CrIS-TROPOMI retrievals have the potential to improve global satellite ozone retrievals, especially with future developments. If spectral accuracy is improved in future TROPOMI calibration, the degrees of freedom for signal in the stratosphere could double when using bands 1 and 2 of TROPOMI (270–330 nm), while tropospheric degrees of freedom for signal could increase by 25 %.
摘要臭氧的垂直分布在大气化学、气候变化、空气污染和人类健康中发挥着重要作用。21 世纪以来,空间遥感方法和仪器不断发展,以更好地确定这种分布。我们通过热红外(TIR)和紫外(UV)光谱辐射的连续组合,利用苏米国家极轨伙伴关系(NPP)上的跨轨道红外探测仪(CrIS)和哨兵 5 号前兆(S5P)卫星上的 TROPOspheric Monitoring Instrument (TROPOMI)的紫外测量,对臭氧检索描述这种分布的能力进行量化。利用 MUlti-SpEctra、MUlti-SpEcies、MUlti-SEnsors(MUSES)算法,在每种仪器分别进行检索之后,将 TIR 和 UV 测量结果顺序结合起来,与单独使用每种仪器/波段相比,适度提高了卫星描述全球臭氧剖面的能力。尽管 TROPOMI 紫外线存在校准问题,但通过 TROPOMI 在赫金斯波段(325-335 nm)的辐射量增强的 CrIS 检索结果显示,在对流层和平流层与独立的数据集具有良好的一致性。在平流层,CrIS-TROPOMI 的性能有所改善,首先是信号自由度(DFS;通常在 0.1-0.2 之间)略有增加,其次是与微波肢体探测仪(MLS)的比较。在对流层,CrIS-TROPOMI 和 CrIS 显示出相似的信号自由度,全球约为 2,但在对流层下部和对流层上部平分的热带地区自由度更高。CrIS-TROPOMI 与臭氧探测仪的验证结果表明,CrIS-TROPOMI 的性能比仅验证 CrIS 时有所提高,对流层大气柱偏差的差异在 30% 到 200% 之间,具体取决于季节。与卫星仪器和再分析数据集的交叉比较显示,两者在相关性和偏差方面表现相似。这些结果表明,CrIS 和 CrIS-TROPOMI 检索具有改进全球卫星臭氧检索的潜力,特别是在未来的发展中。如果在未来的 TROPOMI 校准中提高光谱精度,使用 TROPOMI 的波段 1 和波段 2(270-330 nm)时,平流层的信号自由度可增加一倍,而对流层的信号自由度可增加 25%。
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引用次数: 0
Mapping the CO2 total column retrieval performance from shortwave infrared measurements: synthetic impacts of the spectral resolution, signal-to-noise ratio, and spectral band selection 绘制短波红外测量的二氧化碳总量柱检索性能图:光谱分辨率、信噪比和光谱波段选择的合成影响
IF 3.8 3区 地球科学 Q2 METEOROLOGY & ATMOSPHERIC SCIENCES Pub Date : 2024-09-12 DOI: 10.5194/amt-17-5373-2024
Matthieu Dogniaux, Cyril Crevoisier
Abstract. Satellites have been providing spaceborne observations of the total column of CO2 (denoted XCO2) for over two decades now, and, with the need for independent verification of Paris Agreement objectives, many new satellite concepts are currently planned or being studied to complement or extend the instruments that already exist. Depending on whether they are targeting natural and/or anthropogenic fluxes of CO2, the designs of these future concepts vary greatly. The characteristics of their shortwave infrared (SWIR) observations notably explore several orders of magnitude in spectral resolution (from λ/Δλ ∼ 400 for Carbon Mapper to λ/Δλ ∼ 25 000 for MicroCarb) and include different selections of spectral bands (from one to four bands, among which there are the CO2-sensitive 1.6 µm and/or 2.05 µm bands). The very nature of the spaceborne measurements is also explored: for instance, the NanoCarb imaging concept proposes to measure CO2-sensitive truncated interferograms, instead of infrared spectra like other concepts, in order to significantly reduce the instrument size. This study synthetically explores the impact of three different design parameters on the XCO2 retrieval performance obtained through optimal estimation: (1) the spectral resolution, (2) the signal-to-noise ratio (SNR) and (3) the spectral band selection. Similar performance assessments are completed for the exactly defined OCO-2, MicroCarb, Copernicus CO2 Monitoring (CO2M) and NanoCarb concepts. We show that improving the SNR is more efficient than improving the spectral resolution to increase XCO2 precision when perturbing these parameters across 2 orders of magnitude, and we find that a low SNR and/or a low spectral resolution yield XCO2 with vertical sensitivities that give more weight to atmospheric layers close to the surface. The exploration of various spectral band combinations illustrates, especially for lower spectral resolutions, how including an O2-sensitive band helps to increase the optical path length information and how the 2.05 µm CO2-sensitive band contains more geophysical information than the 1.6 µm band. With very different characteristics, MicroCarb shows a CO2 information content that is only slightly higher than that of CO2M, which translates into XCO2 random errors that are lower by a factor ranging from 1.1 to 1.9, depending on the observational situation. The performance of NanoCarb for a single pixel of its imager is comparable to those of concepts that measure spectra at low SNR and low spectral resolution, but, as this novel concept would observe a given target several times during a single overpass, its performance improves when combining all the observations. Overall, the broad range of results obtained through this synthetic XCO2 performance mapping hint at the future intercomparison challenges that the wide variety of upcoming CO2-observing concepts will pose.
摘要。二十多年来,卫星一直在对二氧化碳总气柱(XCO2)进行空间观测,由于需要对《巴黎协定》的目标进行独立验证,目前正在计划或研究许多新的卫星概念,以补充或扩展已有的仪器。根据是否针对二氧化碳的自然和/或人为通量,这些未来概念的设计大相径庭。其短波红外(SWIR)观测的特点主要是在光谱分辨率上探索几个数量级(从碳绘图仪的 λ/Δλ ∼ 400 到 MicroCarb 的 λ/Δλ ∼ 25 000),并包括不同的光谱波段选择(从一个波段到四个波段,其中有对 CO2 敏感的 1.6 µm 和/或 2.05 µm 波段)。此外,还探讨了空间测量的性质:例如,纳米碳成像概念建议测量对二氧化碳敏感的截断干涉图,而不是像其他概念一样测量红外光谱,以大幅缩小仪器尺寸。本研究综合探讨了三个不同设计参数对通过优化估计获得的 XCO2 检索性能的影响:(1) 光谱分辨率,(2) 信噪比 (SNR) 和 (3) 光谱带选择。我们还对精确定义的 OCO-2、MicroCarb、Copernicus CO2 Monitoring (CO2M) 和 NanoCarb 概念进行了类似的性能评估。我们发现,在对这些参数进行两个数量级的扰动时,提高信噪比比提高光谱分辨率更有效地提高 XCO2 的精度,而且我们发现,低信噪比和/或低光谱分辨率产生的 XCO2 垂直灵敏度更重视靠近地表的大气层。对各种光谱波段组合的探索表明,特别是对于较低的光谱分辨率,包括一个对氧气敏感的波段如何有助于增加光路长度信息,以及对二氧化碳敏感的 2.05 µm 波段如何比 1.6 µm 波段包含更多的地球物理信息。MicroCarb 具有非常不同的特性,其二氧化碳信息含量仅略高于 CO2M,这意味着 XCO2 随机误差较低,根据观测情况,误差系数从 1.1 到 1.9 不等。NanoCarb 相机单个像素的性能可与那些在低信噪比和低光谱分辨率下测量光谱的概念相媲美,但是,由于这种新概念会在单次飞越过程中对给定目标进行多次观测,因此在综合所有观测结果时,其性能会有所提高。总之,通过这一合成 XCO2 性能图谱所获得的广泛结果,暗示了即将推出的各种二氧化碳观测概念将在未来带来的相互比较挑战。
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引用次数: 0
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Atmospheric Measurement Techniques
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