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搭载于第一颗陆地生态系统碳监测卫星(TECIS-1)上的太阳诱导叶绿素荧光成像光谱仪(SIFIS):规格和前景。

The Solar-Induced Chlorophyll Fluorescence Imaging Spectrometer (SIFIS) Onboard the First Terrestrial Ecosystem Carbon Inventory Satellite (TECIS-1): Specifications and Prospects.

机构信息

Key Laboratory of Digital Earth Science, Aerospace Information Research Institute, Chinese Academy of Sciences, Beijing 100094, China.

College of Resources and Environment, University of Chinese Academy of Sciences, Beijing 100049, China.

出版信息

Sensors (Basel). 2020 Feb 3;20(3):815. doi: 10.3390/s20030815.

Abstract

The global monitoring of solar-induced chlorophyll fluorescence (SIF) using satellite-based observations provides a new way of monitoring the status of terrestrial vegetation photosynthesis on a global scale. Several global SIF products that make use of atmospheric satellite data have been successfully developed in recent decades. The Terrestrial Ecosystem Carbon Inventory Satellite (TECIS-1), the first Chinese terrestrial ecosystem carbon inventory satellite, which is due to be launched in 2021, will carry an imaging spectrometer specifically designed for SIF monitoring. Here, we use an extensive set of simulated data derived from the MODerate resolution atmospheric TRANsmission 5 (MODTRAN 5) and Soil Canopy Observation Photosynthesis and Energy (SCOPE) models to evaluate and optimize the specifications of the SIF Imaging Spectrometer (SIFIS) onboard TECIS for accurate SIF retrievals. The wide spectral range of 670-780 nm was recommended to obtain the SIF at both the red and far-red bands. The results illustrate that the combination of a spectral resolution (SR) of 0.1 nm and a signal-to-noise ratio (SNR) of 127 performs better than an SR of 0.3 nm and SNR of 322 or an SR of 0.5 nm and SNR of 472 nm. The resulting SIF retrievals have a root-mean-squared (RMS) diff* value of 0.15 mW m sr nm at the far-red band and 0.43 mW m sr nm at the red band. This compares with 0.20 and 0.26 mW m sr nm at the far-red band and 0.62 and 1.30 mW m sr nm at the red band for the other two configurations described above. Given an SR of 0.3 nm, the increase in the SNR can also improve the SIF retrieval at both bands. If the SNR is improved to 450, the RMS diff* will be 0.17 mW m sr nm at the far-red band and 0.47 mW m sr nm at the red band. Therefore, the SIFIS onboard TECIS-1 will provide another set of observations dedicated to monitoring SIF at the global scale, which will benefit investigations of terrestrial vegetation photosynthesis from space.

摘要

利用卫星观测进行全球太阳诱导叶绿素荧光(SIF)监测为全球尺度监测陆地植被光合作用的状态提供了一种新方法。近几十年来,已经成功开发了几种利用大气卫星数据的全球 SIF 产品。中国第一颗陆地生态系统碳监测卫星“碳星一号”(TECIS-1)将于 2021 年发射,该卫星将搭载一台专门用于 SIF 监测的成像光谱仪。在这里,我们使用了一组广泛的模拟数据,这些数据是由 MODerate resolution atmospheric TRANsmission 5(MODTRAN 5)和 Soil Canopy Observation Photosynthesis and Energy(SCOPE)模型得出的,用于评估和优化 TECIS 卫星上的 SIF 成像光谱仪(SIFIS)的规格,以便进行准确的 SIF 反演。我们推荐使用 670-780nm 的宽光谱范围来获取红光和远红光波段的 SIF。结果表明,光谱分辨率(SR)为 0.1nm,信噪比(SNR)为 127 的组合比 SR 为 0.3nm,SNR 为 322 或 SR 为 0.5nm,SNR 为 472nm 的组合表现更好。反演得到的 SIF 在远红波段的均方根(RMS)差值为 0.15mW m sr nm,在红波段的 RMS 差值为 0.43mW m sr nm。相比之下,上述两种配置在远红波段的 RMS 差值分别为 0.20 和 0.26mW m sr nm,在红波段的 RMS 差值分别为 0.62 和 1.30mW m sr nm。如果光谱分辨率为 0.3nm,那么 SNR 的提高也可以改善两个波段的 SIF 反演。如果 SNR 提高到 450,远红波段的 RMS 差值将为 0.17mW m sr nm,红波段的 RMS 差值将为 0.47mW m sr nm。因此,TECIS-1 卫星上的 SIFIS 将提供另一组专门用于全球尺度 SIF 监测的观测数据,这将有助于从太空研究陆地植被光合作用。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/8f3d/7038700/51cb36842673/sensors-20-00815-g001.jpg

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