Evaluation of kinetic energy and erosivity potential of simulated rainfall using Laser Precipitation Monitor
Evaluation of kinetic energy and erosivity potential of simulated rainfall using Laser Precipitation Monitor
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DOI:
10.1016/j.catena.2015.09.017
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发表时间:
2016-02
期刊:
影响因子:
6.2
通讯作者:
D. Meshesha;A. Tsunekawa;M. Tsubo;Nigussie Haregeweyn;F. Tegegne
中科院分区:
文献类型:
--
作者:
D. Meshesha;A. Tsunekawa;M. Tsubo;Nigussie Haregeweyn;F. Tegegne
Rainfall kinetic energy is a widely recognized indicator of a raindrop's ability to detach soil particles in rainsplash erosion. However, it is challenging to estimate the kinetic energy (KE) of a given rain event, because it involves analysis of the terminal velocity and drop size distribution (DSD) of raindrops. A preferred alternative is to relate KE to rainfall intensity. Therefore we sought to characterize simulated rainfall, establish a relationship between kinetic energy and intensity as a function of both time (KEt, J m− 2h− 1) and volume (KEvol, J m− 2mm− 1), and examine the erosivity potential of each event. A rainfall simulator and Laser Precipitation Monitor (optical disdrometer) were used to characterize raindrop size, terminal velocity and KE at different rainfall intensities (1.5 to 202 mm h− 1). Values ofKEtranged from 26.67 to 5955 J m− 2h− 1andKEvolranged from 16.10 to 34.85 J m− 2mm− 1, which is comparable to values determined from natural rain of similar intensity ranges. A power-law function and a polynomial function betweenKEtand rainfall intensity had coefficients of determination (R2) of 0.99 and 0.98 (P< 0.0001), respectively. The best-fitting relationship betweenKEvoland intensity was a power-law function (R2= 0.95;P< 0.001). We found that erosivity had a very strong correlation with rainfall depth (R2= 0.99;P< 0.0001) in power-law function. Furthermore, regardless of rainfall intensity, KE is more strongly correlated with raindrop size than volume of raindrop.