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GreenHouse gas Observations of the Stratosphere and Troposphere (GHOST): an airborne shortwave-infrared spectrometer for remote sensing of greenhouse gases

机译:平流层和对流层的温室气体观测:用于遥感温室气体的机载短波红外光谱仪

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GHOST is a novel, compact shortwave-infrared grating spectrometer, designed for remote sensing of tropospheric columns of greenhouse gases (GHGs) from an airborne platform. It observes solar radiation at medium to high spectral resolution (better than 0.3 nm), which has been reflected by the Earth's surface using similar methods to those used by polar-orbiting satellites such as the JAXA GOSAT mission, NASA's OCO-2, and the Copernicus Sentinel-5 Precursor. By using an original design comprising optical fibre inputs along with a single diffraction grating and detector array, GHOST is able to observe COsub2/sub absorption bands centred around 1.61 and 2.06 μm (the same wavelength regions used by OCO-2 and GOSAT) whilst simultaneously measuring CHsub4/sub absorption at 1.65 μm (also observed by GOSAT) and CHsub4/sub and CO at 2.30 μm (observed by Sentinel-5P). With emissions expected to become more concentrated towards city sources as the global population residing in urban areas increases, there emerges a clear requirement to bridge the spatial scale gap between small-scale urban emission sources and global-scale GHG variations. In addition to the benefits achieved in spatial coverage through being able to remotely sense GHG tropospheric columns from an aircraft, the overlapping spectral ranges and comparable spectral resolutions mean that GHOST has unique potential for providing validation opportunities for these platforms, particularly over the ocean, where ground-based validation measurements are not available. In this paper we provide an overview of the GHOST instrument, calibration, and data processing, demonstrating the instrument's performance and suitability for GHG remote sensing. We also report on the first GHG observations made by GHOST during its maiden science flights on board the NASA Global Hawk unmanned aerial vehicle, which took place over the eastern Pacific Ocean in March 2015 as part of the CAST/ATTREX joint Global Hawk flight campaign.
机译:GHOST是一种新颖的紧凑型短波红外光栅光谱仪,设计用于从机载平台遥感对流层温室气体(GHG)。它观测中至高光谱分辨率(低于0.3 nm)的太阳辐射,该辐射已使用与极轨卫星类似的方法(例如JAXA GOSAT任务,NASA的OCO-2和哥白尼前哨5前体。通过使用包含光纤输入,单个衍射光栅和检测器阵列的原始设计,GHOST能够观察到中心围绕1.61和2.06μm(与OCO-所使用的波长区域相同)的CO 2 吸收带2和GOSAT),同时测量1.65μm处的CH 4 吸收(也可通过GOSAT观察)和2.30μm处的CH 4 和CO(Sentinel-5P观察)。随着全球居住在城市地区的人口增加,预计排放将越来越集中于城市,因此提出了弥合小规模城市排放源与全球温室气体变化之间的空间比例差距的明确要求。除了通过能够从飞机上遥感GHG对流层柱而在空间覆盖方面获得的好处之外,重叠的光谱范围和可比的光谱分辨率还意味着GHOST具有独特的潜力,可以为这些平台(尤其是在海洋上)提供验证机会基于地面的验证测量不可用。在本文中,我们提供了GHOST仪器,校准和数据处理的概述,展示了该仪器的性能以及对GHG遥感的适用性。我们还报告了GHOST在NASA全球鹰无人飞行器上进行的首次科学飞行期间首次进行的温室气体观测,这是CAST / ATTREX联合全球鹰飞行运动的一部分,于2015年3月在东部太平洋上空进行。

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