Abstract

Wind speed (u) is a significant constraint in the evapotranspiration modeling over the highly heterogeneous regional surface due to its high temporal-spatial variation. In this study, a satellite-based Wind Speed Avoiding Priestley–Taylor (WAPT) algorithm was proposed to estimate the regional actual evapotranspiration by employing a u-independent theoretical trapezoidal space to determine the pixel Priestley–Taylor (PT) parameter Φ. The WAPT model was comprehensively evaluated with hydro-meteorological observations in the arid Heihe River Basin in northwestern China. The results show that the WAPT model can provide reliable latent heat flux estimations with the root-mean-square error (RMSE) of 46.0 W/m2 across 2013–2018 for 5 long-term observation stations and the RMSE of 49.6 W/m2 in the growing season in 2012 for 21 stations with intensive observations. The estimation by WAPT has a higher precision in the vegetation growing season than in the non-growing season. The estimation by WAPT has a closer agreement with the ground observations for vegetation-covered surfaces (e.g., corn and wetland) than that for dry sites (e.g., Gobi, desert, and desert steppe).

Highlights

  • Terrestrial latent heat flux (LE) is an important component of the land surface water cycle and land surface–atmosphere energy exchange [1–4]

  • Many remote sensing models have been proposed to simulate terrestrial LE based on constraints on water vapor transport and energy balance constraints [2–4,7], such as SEBAL [8], SEBS [9], METRIC [10], TSEB model [11], Gc-TSEB [12], MOD16 [2], feature space methods [13–17]

  • The feature space to estimate LE was introduced by Jiang et al [21,22] with the scatter diagram of TL and vegetation index containing a full range of soil water content and fractional vegetation cover to linear fitting the triangle space with the advantages of no auxiliary atmospheric or ground data

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Summary

Introduction

Terrestrial latent heat flux (LE) is an important component of the land surface water cycle and land surface–atmosphere energy exchange [1–4]. Many remote sensing models have been proposed to simulate terrestrial LE based on constraints on water vapor transport and energy balance constraints [2–4,7], such as SEBAL [8], SEBS [9], METRIC [10], TSEB model [11], Gc-TSEB [12], MOD16 [2], feature space methods [13–17]. Those models have been proven successful for certain weather conditions, underlying surfaces, etc. The feature space model, which employs the triangle or trapezoidal relationship between land surface temperature (TL ) and vegetation index (VI) to represent the constraints of soil available water on LE, is widely accepted.

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