The impact of temperature vertical structure on trajectory modeling of stratospheric water vapor

Abstract

Lagrangian trajectories driven by reanalysis meteorological fields are frequently used to study water vapor (H 2 O) in the stratosphere, in which the tropical cold-point temperatures regulate the amount of H 2 O entering the stratosphere. Therefore, the accuracy of temperatures in the tropical tropopause layer (TTL) is of great importance for understanding stratospheric H 2 O abundances. Currently, most reanalyses, such as the NASA MERRA (Modern Era Retrospective - analysis for Research and Applications), only provide temperatures with ∼1.2 km vertical resolution in the TTL, which has been argued to miss finer vertical structure in the tropopause and therefore introduce uncertainties in our understanding of stratospheric H 2 O. In this paper, we quantify this uncertainty by comparing the Lagrangian trajectory prediction of H 2 O using MERRA temperatures on standard model levels (traj.MER-T) to those using GPS temperatures at finer vertical resolution (traj.GPS-T), and those using adjusted MERRA temperatures with finer vertical structures induced by waves (traj.MER-Twave). It turns out that by using temperatures with finer vertical structure in the tropopause, the trajectory model more realistically simulates the dehydration of air entering the stratosphere. But the effect on H 2 O abundances is relatively minor: compared with traj.MER-T, traj.GPS-T tends to dry air by ∼0.1 ppmv, while traj.MERTwave tends to dry air by 0.2-0.3 ppmv. Despite these differences in absolute values of predicted H 2 O and vertical dehydration patterns, there is virtually no difference in the interannual ariability in different runs. Overall, we find that a tropopause temperature with finer vertical structure has limited impact on predicted stratospheric H 2 O.