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首页> 外文期刊>Remote Sensing of Environment: An Interdisciplinary Journal >A spatio-temporal active-fire clustering approach for global burned area mapping at 250 m from MODIS data
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A spatio-temporal active-fire clustering approach for global burned area mapping at 250 m from MODIS data

机译:来自MODIS数据250米的全球烧毁区域映射的时空活动灭火途径

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This paper presents the generation of a global burned area mapping algorithm using MODIS hotspots and near-infrared reflectance within ESA's Fire_cci project. The algorithm is based on a hybrid approach that combines MODIS highest resolution (250 m) near-infrared band and active fire information from thermal channels. The burned area is detected in two phases. In the first step, pixels with a high probability of being burned are selected in order to reduce commission errors. To do that, spatio-temporal active-fire clusters are created to determine adaptive thresholds. Finally, a contextual growing approach is applied from those pixels to the neighbouring area to fully detect the burned patch and reduce omission errors. The algorithm was used to obtain a time series of global burned area dataset (named FireCC151), covering the 2001-2018 period. Validation based on 1200 sampled sites covering the period from 2003 to 2014 showed an average omission and commission errors of 67.1% and 54.4%. When using longer validation periods, the errors were found smaller (54.5% omission and 25.7% commission for the additional 1000 African sampled sites), which indicates that the product is negatively influenced by temporal reporting accuracy. The inter-comparison carried out with previous Fire_cci versions (FireCC141 and FireCC150), and NASA's standard burned area product (MCD64A1 c6) showed consistent spatial and temporal patterns. However, the new algorithm estimated an average BA of 4.63 Mkm(2), with a maximum of 5.19 Mkm(2) (2004) and a minimum of 3.94 Mkm(2) (in 2001), increasing current burned area estimations. Besides, the new product was found more sensitive to detect smaller burned patches. This new product, called FireCC151, is publicly available at: http://cci.esa.int/data, last accessed on September 2019.
机译:本文介绍了在ESA的Fire_CCI项目中使用MODIS热点和近红外反射率的全局烧毁区域映射算法。该算法基于混合方法,其将MODIS最高分辨率(250米)近红外频带和来自热通道的主动火灾信息组合。在两个阶段中检测到烧毁区域。在第一步中,选择具有燃烧概率的像素以减少佣金错误。为此,创建时空活动 - 灭火集群以确定自适应阈值。最后,从那些对相邻区域的那些像素应用上下文生长方法以完全检测烧坏的补丁并减少遗漏误差。该算法用于获得全局烧毁区域数据集的时间序列(名为FireCC151),涵盖2001-2018期间。基于1200个采样站点的验证,涵盖2003年至2014年的计划,平均遗漏和佣金误差为67.1%和54.4%。在使用更长的验证期时,发现错误较小(54.5%省略和25.7%的佣金为另外1000个非洲采样站点),这表明该产品受到时间报告准确性的负面影响。使用以前的Fire_CCI版本(FireCC141和FireCC150)和NASA的标准烧毁区域产品(MCD64A1 C6)进行的相互比较显示了一致的空间和时间模式。但是,新算法估计平均BA为4.63 mkm(2),最大为5.19米(2)(2)(2004),最小值为3.94 mkm(2)(2001年),增加电流烧毁区域估计。此外,新产品被发现更敏感,以检测较小的烧坏斑块。这个名为FireCC151的新产品可在公开上获取:http://cci.esa.int/data,上次访问于2019年9月。

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