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黄土高原冬小麦田光谱特征变化及其与二氧化碳日收支的相关分析
引用本文:李双江,刘志红,刘文兆,高桥厚裕,樋口笃志,桧山哲哉,福岛义宏.黄土高原冬小麦田光谱特征变化及其与二氧化碳日收支的相关分析[J].应用生态学报,2008,19(11):2408-2413.
作者姓名:李双江  刘志红  刘文兆  高桥厚裕  樋口笃志  桧山哲哉  福岛义宏
作者单位:1. 中国科学院水利部水土保持研究所,陕西杨凌,712100;中国科学院研究生院,北京,100039
2. 中国科学院水利部水土保持研究所,陕西杨凌,712100;成都信息工程学院资源环
3. 中国科学院水利部水土保持研究所,陕西杨凌,712100
4. 日本综合地球环境学研究所,日本京都,603-8047
5. 日本千叶大学环境遥感中心,日本千叶,263-8522
6. 日本名古屋大学地球水循环研究中心,日本名古屋,464-8601,境系,成都,610225
基金项目:中国科学院知识创新工程重要方向项目,日本文部科学省资助项目
摘    要:根据光谱辐射仪对黄土高原冬小麦整个生育期光谱反射率的连续观测数据及CO2通量观测数据,对冬小麦田光谱特征变化及其与CO2日收支的相关性进行了分析.结果表明:冬小麦田不同波长光谱反射率和归一化植被指数(NDVI)呈现明显的日变化和季节变化.同一天内,反射率随太阳高度角的变化而变化,变化最大的波段(550 nm左右、700~1 050 nm)表现为峰.不同生育期同一时刻,可见光波段(350~670 nm)反射率变化不大,近红外波段(700~1 050 nm)出现较大差异,在出苗期、分蘖期和越冬期后红边位置向长波方向“红移”;越冬期前出现向短波方向“蓝移” 的现象;但成熟期“蓝移”现象不明显,表现为突变;其他生育时期没有观测到波谱位移.NDVI的日变化呈U型,13:00左右最低,16:00后出现较大波动,与抛物线有较好的拟合效果,小麦生长旺盛时期,对其地面遥感观测应选择在NDVI变化不大的13:00左右进行;整个冬小麦生长季11:00反射率及NDVI以播种后第140天为中心对称,NDVI的季节变化表现为M型,可用四次多项式拟合;在整个小麦生育期中NDVI与CO2的日收支呈极显著负相关,但正午左右的相关性稍差.

关 键 词:光谱仪  反射率  红边位置  CO2收支
收稿时间:2008-2-25

Correlations between spectral characteristics and diurnal CO2 budget of winter wheat field on Loess Plateau.
LI Shuang-jiang,LIU Zhi-hong,LIU Wen-zhao,SUHIRO Takahashi,ATSUSHI Higuchi,TETSUYA Hiyama,YOSHIHIRO Fukushima.Correlations between spectral characteristics and diurnal CO2 budget of winter wheat field on Loess Plateau.[J].Chinese Journal of Applied Ecology,2008,19(11):2408-2413.
Authors:LI Shuang-jiang  LIU Zhi-hong  LIU Wen-zhao  SUHIRO Takahashi  ATSUSHI Higuchi  TETSUYA Hiyama  YOSHIHIRO Fukushima
Abstract:Based on the continuous observation on the spectral reflectance and CO2 flux during the whole growth period of winter wheat, the correlations between the variations of spectral characteristics and the diurnal CO2 budget of winter wheat field on Loess Plateau were analyzed. The results showed that the spectral reflectance at different wavelengths and the NDVI changed with the growth stages of winter wheat, and the diurnal spectral reflectance changed with solar altitude angle, with the wavelengths at which the reflectance changed most being at 550 nm and 700-1 050 nm. At the same time period of different growth stages, the spectral reflectance changed little at 350-670 nm but varied greatly at 700-1 050 nm. The red edge position shifted to longer wavelengths at seedling and tillering stages and by the end of wintering while to shorter wavelengths at the beginning of wintering, but the shift to shorter wavelengths was not obvious at ripening stage. No spectrum shift was observed at other growth stages. The diurnal NDVI changed in U-shape, reaching to the minimum at about 13:00 and fluctuating after 16:00, and the change pattern could be fitted by a parabola. Therefore, for winter wheat field, the best time for remote sensing observation should be selected at about 13:00 when the NDVI changed little, except in winter. After the 140th day of seeding, the reflectance and NDVI at 11:00 were symmetrical, and NDVI changed in M-shape, being able to be simulated by a quartic polynomial. There was a significant negative correlation between the NDVI and the diurnal CO2 budget during the whole growth period of winter wheat, but the correlation was weaker around midday.
Keywords:NDVI
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