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Greenhouse gas profiling by infrared-laser and microwave occultation: retrieval algorithm and demonstration results from end-to-end simulations

机译:红外激光和微波掩埋法分析温室气体:端对端模拟的检索算法和演示结果

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摘要

Measuring greenhouse gas (GHG) profiles with global coverage and high accuracy and vertical resolution in the upper troposphere and lower stratosphere (UTLS) is key for improved monitoring of GHG concentrations in the free atmosphere. In this respect a new satellite mission concept adding an infrared-laser part to the already well studied microwave occultation technique exploits the joint propagation of infrared-laser and microwave signals between Low Earth Orbit (LEO) satellites. This synergetic combination, referred to as LEO-LEO microwave and infrared-laser occultation (LMIO) method, enables to retrieve thermodynamic profiles (pressure, temperature, humidity) and accurate altitude levels from the microwave signals and GHG profiles from the simultaneously measured infrared-laser signals. However, due to the novelty of the LMIO method, a retrieval algorithm for GHG profiling is not yet available. Here we introduce such an algorithm for retrieving GHGs from LEO-LEO infrared-laser occultation (LIO) data, applied as a second step after retrieving thermodynamic profiles from LEO-LEO microwave occultation (LMO) data. We thoroughly describe the LIO retrieval algorithm and unveil the synergy with the LMO-retrieved pressure, temperature, and altitude information. We furthermore demonstrate the effective independence of the GHG retrieval results from background (a priori) information in discussing demonstration results from LMIO end-to-end simulations for a representative set of GHG profiles, including carbon dioxide (CO), water vapor (HO), methane (CH), and ozone (O). The GHGs except for ozone are well retrieved throughout the UTLS, while ozone is well retrieved from about 10 km to 15 km upwards, since the ozone layer resides in the lower stratosphere. The GHG retrieval errors are generally smaller than 1% to 3% r.m.s., at a vertical resolution of about 1 km. The retrieved profiles also appear unbiased, which points to the climate benchmarking capability of the LMIO method. This performance, found here for clear-air atmospheric conditions, is unprecedented for vertical profiling of GHGs in the free atmosphere and encouraging for future LMIO implementation. Subsequent work will examine GHG retrievals in cloudy air, addressing retrieval performance when scanning through intermittent upper tropospheric cloudiness.
机译:对流层和平流层下层(UTLS)具有全球覆盖范围,高精度和垂直分辨率的温室气体(GHG)剖面测量是改善自由大气中GHG浓度监测的关键。在这方面,新的卫星任务概念在已经被充分研究的微波掩星技术中增加了红外激光部分,从而利用了低地球轨道(LEO)卫星之间红外激光和微波信号的联合传播。这种协同的组合被称为LEO-LEO微波和红外激光掩星(LMIO)方法,能够从同时测量的红外信号中的微波信号和GHG轮廓中检索热力学曲线(压力,温度,湿度)和准确的海拔高度。激光信号。但是,由于LMIO方法的新颖性,用于GHG分析的检索算法尚不可用。在这里,我们介绍了一种从LEO-LEO红外激光掩星(LIO)数据中检索GHG的算法,该算法在从LEO-LEO微波掩星(LMO)数据中检索热力学特征之后作为第二步应用。我们彻底描述了LIO检索算法,并揭示了与LMO检索到的压力,温度和高度信息的协同作用。我们还将在讨论LMIO端对端模拟的代表性结果(包括二氧化碳(CO),水蒸气(HO))的LMIO端到端模拟的演示结果时,进一步证明背景信息(先验信息)对温室气体检索结果的有效独立性。 ,甲烷(CH)和臭氧(O)。在整个UTLS中,除臭氧外的温室气体都可以很好地回收,而从约10 km到15 km以上的臭氧,则可以很好地回收,因为臭氧层位于平流层下部。在约1 km的垂直分辨率下,GHG取回误差通常小于1%至3%r.m.s.。检索到的剖面图也似乎没有偏见,这表明了LMIO方法的气候基准测试能力。这种性能是在晴空条件下发现的,对于在自由大气中对GHG进行垂直剖析是前所未有的,并为以后的LMIO实施提供了鼓励。随后的工作将检查多云空气中的GHG回收,以解决通过对流层上层高空浑浊进行扫描时的回收性能。

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