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FLEX (Fluorescence Explorer) Feasibility study

机译:FLEX(荧光浏览器)可行性研究

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The fluorescence signal emitted from vegetation is directly linked to the photosynthesis and as such may be usedrnas an indicator for plant functioning, stress and vitality. Observation of solar induced fluorescence from space isrnproposed by measuring the weak signal contribution in the Fraunhofer line wavelengths.rnThe scientific requirements have been studied in detail, looking to aspects such as the selection of Fraunhoferrnlines, the solar induced fluorescence radiance, measurement accuracy, spatial resolution, atmosphere influencernetc. This has resulted in instrument requirements, that are the basis for a trade off study of optical observationrntechniques. The main choice was between applying a grating spectrometer or a filter spectrometer, each of whichrnhave advantages and disadvantages for Fraunhofer line detection (FLD). From both spectrometer types arnpreliminary optical design has been made. A model has been developed to evaluate the different configurationsrnfor S/N, integration time, radiance level etc.rnIn the study the feasibility of Fraunhofer line detection from space is demonstrated, albeit, that the observationrnstrategy will depend on the real amount of the solar excited fluorescence intensity.rnThe main conclusions of the study are:rn- The atmospheric effects on Fraunhofer Line Detection (FLD) are mainly the Rotational RamanrnScattering (RRS). The hereby induced "filling in" of the Fraunhofer lines can be predicted with goodrnaccuracy and can be removed with appropriate models.rn- The signal modelling shows, that depending of the intensity of solar induced fluorescence of vegetationrnmeasuring of fluorescence from space is feasible with reasonable integration times, albeit that thernstrategy of "scene freezing" might be necessary.rn- It is of great importance to acquire on short term reliable data on the fluorescence intensity ofrnvegetation, caused by solar excitation.rn- Two possible spectrometer configurations can be used, an imaging spectrometer or a filter spectrometerrndepending on different spectral and spatial measurement strategies.rnThe results of the study are a good starting point for further development of a passive spaceborne fluorosensor.
机译:从植物发出的荧光信号直接与光合作用相关,因此可以用作植物功能,胁迫和活力的指标。通过测量弗劳恩霍夫谱线波长中的微弱信号贡献,提出了从空间观测太阳致荧光的方法。rn已研究了科学要求,并从诸如弗劳恩霍夫谱系的选择,太阳致荧光辐射率,测量精度,空间分辨率等方面进行了研究。 ,气氛影响等。这导致仪器的需求,这是权衡光学观察技术研究的基础。主要选择是在使用光栅光谱仪或滤光片光谱仪之间,每种方法对于Fraunhofer线检测(FLD)都有优点和缺点。从这两种光谱仪类型,已经进行了初步的光学设计。已经开发了一个模型来评估信噪比,积分时间,辐射水平等的不同配置。在研究中证明了Fraunhofer线从太空探测的可行性,尽管观测策略将取决于实际的太阳激发量这项研究的主要结论是:rn-大气对弗劳恩霍夫线检测(FLD)的影响主要是旋转拉曼散射(RRS)。由此可以准确预测弗劳恩霍夫系的“充满”现象,并可以通过适当的模型将其消除。rn-信号模型表明,取决于太阳光诱导的植物荧光强度,从空间上测量荧光是可行的,而且要合理。积分时间,尽管可能需要进行“场景冻结”的策略。rn-短期获取由太阳激发引起的植被荧光强度的可靠数据非常重要。rn-可以使用两种可能的光谱仪配置,取决于不同光谱和空间测量策略的成像光谱仪或滤光片光谱仪。研究结果为进一步开发无源星载氟传感器提供了良好的起点。

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