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A red tide detecting method using spectral angle mapping technology based on MODIS data

机译:基于MODIS数据的光谱角映射技术的赤潮检测方法

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Remote sensing technique has become one of the most important means of red tide detection. Now, there have been a number of successful applications of red tide detections using remote sensing technology in the world. The present detecting technology basically based on the true color images of the ocean, chlorophyll a (CHL-a)maps and sea surface temperature (SST)maps, however, these methods all have some limitations. Red tides can be cased by numerous kinds of phytoplankton or zooplankton. Some of the red tides will case an apparent color change in the ocean, but some will not. So, in the first method, if there is no change in the ocean color pictures, the red tide will not be detected. CHL-a index will increase when the red tide is cased by phytoplankton, that is also the theoretical basis of the method 2, but it will not work when the red tide is cased by zooplankton. Many researches indicated that red tides can arose a rising in SST, but ocean currents and so many other factors can cause the phenomenon as well. It seems that method 3 maybe not the perfect way too. In this paper, the author suggested a process based on the spectral signature and spectral angle mapping (SAM)method to detect red tides. Spectral signature of red tides has three features. Firstly, there are 2 peaks in the wavelength rage of 500nm-800nm, and the second reflection peak in the wavelength rage of 680nm-710nm generally, is the sign to distinguish a red tide from normal sea water. Secondly, the height of the second reflection peak varies with the dominant species which cause the red tide. Last but not the least, the shape of the spectral signature of a certain kind red tide is almost the same, differences only exist in the modular of spectral vector, and that is the theoretical basis of the SAMbased red tides detection process. AS preprocess, minimum noise transform (MNF)and pixel purity index (PPI)should be done to collect the end-members. Then, we can select the end-members in the n-dimensional visualization of ENVI software. By examining the endmembers' spectral signature, people can tell whether it is the red tide pixel or not, even which dominant species are as well with a complete spectral libraries. Finally, with the SAM method, red tide class can be highlighted. It is also very convenient to do the area calculation and change detection after this kind of classification. In conclusion, the method discussed above can be used to detect all kinds of red tides, and with the high temporal resolution of MODIS, it is possible for us to analyze the relationship of the probable influencing factors of red tides and the change of red tide area based on the change detection. That will be helpful to realize the red tide prediction which could minimize the losses caused by red tides.
机译:遥感技术已成为赤潮探测的最重要手段之一。现在,在世界范围内已经有许多成功的利用遥感技术进行赤潮探测的应用。目前的检测技术基本上是基于海洋的真实彩色图像,叶绿素a(CHL-a)图和海面温度(SST)图,但是这些方法都有一定的局限性。赤潮可由多种浮游植物或浮游动物引起。有些赤潮会导致海洋出现明显的颜色变化,而有些则不会。因此,在第一种方法中,如果海洋彩色图片没有变化,则不会检测到赤潮。当浮游植物引起赤潮时,CHL-a指数会增加,这也是方法2的理论基础,但是当浮游动物引起赤潮时,CHL-a指数将不起作用。许多研究表明,赤潮可能引起海表温度升高,但是洋流和许多其他因素也可能导致这种现象。似乎方法3也不是完美的方法。在本文中,作者提出了一种基于光谱特征和光谱角度映射(SAM)方法的检测赤潮的过程。赤潮的光谱特征具有三个特征。首先,在500nm-800nm波长范围内有2个峰,而在680nm-710nm波长范围内通常有第二个反射峰,是区分赤潮和普通海水的标志。其次,第二反射峰的高度随引起赤潮的主要种类而变化。最后但并非最不重要的是,某种赤潮的光谱特征形状几乎相同,差异仅存在于光谱矢量的模数中,这是基于SAM的赤潮检测过程的理论基础。作为预处理,应进行最小噪声变换(MNF)和像素纯度指数(PPI)来收集末端成员。然后,我们可以在ENVI软件的n维可视化中选择末端成员。通过检查末端成员的光谱特征,人们可以分辨出它是否是赤潮像素,甚至哪些优势种也具有完整的光谱库。最后,使用SAM方法,可以突出显示赤潮类别。这种分类后进行面积计算和变化检测也非常方便。总之,以上讨论的方法可用于检测各种类型的赤潮,并且由于MODIS的高时间分辨率,我们有可能分析赤潮的可能影响因素与赤潮变化之间的关系。基于更改检测的区域。这将有助于实现赤潮预测,将赤潮造成的损失降到最低。

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