Abstract

Complex processes govern spatiotemporal distribution of precipitation within the high-mountainous headwater regions (commonly known as the upper Indus basin (UIB)), of the Indus River basin of Pakistan. Reliable precipitation simulations particularly over the UIB present a major scientific challenge due to regional complexity and inadequate observational coverage. Here, we present a statistical downscaling approach to model observed precipitation of the entire Indus basin, with a focus on UIB within available data constraints. Taking advantage of recent high altitude (HA) observatories, we perform precipitation regionalization using K-means cluster analysis to demonstrate effectiveness of low-altitude stations to provide useful precipitation inferences over more uncertain and hydrologically important HA of the UIB. We further employ generalized linear models (GLM) with gamma and Tweedie distributions to identify major dynamic and thermodynamic drivers from a reanalysis dataset within a robust cross-validation framework that explain observed spatiotemporal precipitation patterns across the Indus basin. Final statistical models demonstrate higher predictability to resolve precipitation variability over wetter southern Himalayans and different lower Indus regions, by mainly using different dynamic predictors. The modeling framework also shows an adequate performance over more complex and uncertain trans-Himalayans and the northwestern regions of the UIB, particularly during the seasons dominated by the westerly circulations. However, the cryosphere-dominated trans-Himalayan regions, which largely govern the basin hydrology, require relatively complex models that contain dynamic and thermodynamic circulations. We also analyzed relevant atmospheric circulations during precipitation anomalies over the UIB, to evaluate physical consistency of the statistical models, as an additional measure of reliability. Overall, our results suggest that such circulation-based statistical downscaling has the potential to improve our understanding towards distinct features of the regional-scale precipitation across the upper and lower Indus basin. Such understanding should help to assess the response of this complex, data-scarce, and climate-sensitive river basin amid future climatic changes, to serve communal and scientific interests.

Highlights

  • The trans-Himalayan and transboundary Indus River flows approximately 3200 km across its 1.12 million square kilometer basin to descend into the Arabian Sea (FAO 2011)

  • Snow and glacial melt within the upper Indus basin (UIB) mainly govern the hydrological regime of the Indus River (e.g., Tahir et al 2011; Archer and Fowler 2004), which sustains the livelihood of nearly 215 million downstream inhabitants (Latif et al 2018; Lutz et al 2016)

  • Based upon station precipitation analysis, we identify three major seasons that cover the winter period spanning from December through March (WS, DJFM), the pre-monsoon spanning from April to June (PMS, AMJ), and the summer monsoon season that spans from July to September (MS, JAS)

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Summary

Introduction

The trans-Himalayan and transboundary Indus River flows approximately 3200 km across its 1.12 million square kilometer basin to descend into the Arabian Sea (FAO 2011). An accurate knowledge of the spatial and temporal distribution of precipitation is largely unknown in the high altitudes (HA) of the UIB (Immerzeel et al 2015; Hewitt 2005; Winiger et al 2005). This lack of certainty in precipitation characteristics stems from an insufficient number of HA meteorological observatories, inaccuracies in available HA measurements (Rasmussen et al 2012), concerns about the data quality (Hewitt 2011; Winiger et al 2005), and serious constraints on transboundary data sharing due to regional politics (Dahri et al 2016). It should be noted that most of the observatories with long-term records are sparsely located in the low altitudes, while short-term and inconsistent observations of the HA limit our understanding about the regional orography

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