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METHODS FOR THE SURFACE REFLECTANCE RETRIEVAL FROMCHRIS/PROBADATA OVER LANDAND INLAND WATERS

机译:利用陆地/内陆水域的克里斯/概率数据反演表面反射的方法

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The Compact High Resolution Imaging Spectrometerrn(CHRIS) on board the Project for On–Board Autonomyrn(PROBA) platform system provides the first high spa-tialrnresolution hyperspectral/multiangular remote sensingrndata from a satellite system, what represents a new sourcernof information for Earth Observation purposes. Whenrndealing with the retrieval of surface reflectance from suchrnkind of hyperspectral data, a radiative transfer approachrnis commonly preferred. However, since CHRIS 2003rnand 2004 data present reported calibration problems inrnseveral bands, especially in the near–infrared region, arnstandard atmospheric correction based on radiative trans-ferrnmodels should not be performed. A dedicated at-mosphericrncorrection algorithm for CHRIS/PROBA datarnover land is presented in this work. It consists in therncombination of radiative transfer and empirical line ap-proachesrnto atmospheric correction, in order to retrievernsurface reflectance images free from both the atmo-sphericrndistortion and artifacts due to mis–calibration.rnThe atmospheric optical parameters and the updated setrnof calibration coefficients are obtained jointly in an au-tonomousrnprocess, without the need for any ancillaryrndata. Results from the application of the algorithm tornCHRIS/PROBA data from the two ESA Spectra bAR-raxrnCampaign (SPARC) held at the Barrax study site (LarnMancha, Spain) in 2003 and 2004 are presented in thisrnwork, focusing on the validation of the final surface re-flectancernusing in–situ measurements acquired simulta-neouslyrnto PROBA overpasses. Besides, the first ver-sionrnof an atmospheric correction module for inland wa-ters,rnwhich is currently under development, is also pre-sented,rnas well as the first results obtained from its appli-cationrnto data from the Rosarito reservoir. The potentialrnof CHRIS/PROBA data for Earth observation purposes isrnshown.
机译:车载自主项目(PROBA)平台系统上的紧凑型高分辨率成像光谱仪(CHRIS)提供了来自卫星系统的首个高空间分辨率的高光谱/多角度遥感数据,这代表了用于地球观测的新Sourcernof信息。当要从这类高光谱数据中检索表面反射率时,通常首选辐射传输方法。但是,由于CHRIS 2003rnand 2004的数据显示了几个波段的校准问题,尤其是在近红外区域,因此不应执行基于辐射透射率模型的标准大气校正。在这项工作中,提出了一种专用的CHRIS / PROBA数据大气土地大气校正算法。它包括辐射传递和经验线到大气校正的组合,以便检索没有因校准错误而导致的大气反射和畸变的表面反射图像。联合获得大气光学参数和更新的setrnof校准系数在自动过程中,不需要任何辅助数据。应用此算法得出的结果来自2003年和2004年在Barrax研究地点(西班牙LarnMancha)举行的两次ESA Spectra bAR-raxrnCampaign(SPARC)的撕裂CHRIS / PROBA数据,着重于最终表面的验证使用原位测量获得的反射信号与PROBA立交桥同时获得。此外,还初步提出了正在开发中的内陆污水大气校正模块的第一个版本,以及从罗萨里托水库的应用数据获得的第一批结果。显示了用于地球观测的潜在的CHRIS / PROBA数据。

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