| Literature DB >> 31836809 |
Ibrar Ul Hassan Akhtar1,2, H Athar3,4.
Abstract
Major threat that Pakistan faces today is water scarcity and any significant change in water availability from storage reservoirs coupled with below normal precipitation threatens food security of more than 207 million people. Two major reservoirs of Tarbela and Mangla on Indus and Jhelum rivers are studied. Landsat satellite's data are used to estimate the water extents of these reservoirs during 1981-2017. A long-term significant decrease of 15-25% decade-1 in water extent is found for Tarbela as compared to 37-70% decade-1 for Mangla, mainly during March to June. Significant water extents reductions are observed in the range of -23.9 to -53.4 km2 (1991-2017) and -63.1 to -52.3 km2 (2001-2010 and 2011-2017) for Tarbela and Mangla, respectively. The precipitation amount and areas receiving this precipitation show a significant decreasing trend of -4.68 to -8.40 mm year-1 and -358.1 to -309.9 km2 year-1 for basins of Mangla and Tarbela, respectively. The precipitation and climatic oscillations are playing roles in variability of water extents. The ensuing multiple linear regression models predict water extents with an average error of 13% and 16% for Tarbela and Mangla, respectively.Entities:
Year: 2019 PMID: 31836809 PMCID: PMC6910943 DOI: 10.1038/s41598-019-54872-x
Source DB: PubMed Journal: Sci Rep ISSN: 2045-2322 Impact factor: 4.379
Figure 1Study area showing the Tarbela-Indus and Mangla-Jhelum reservoirs, associated basins and sub-basins of PUIRB. Tarbela is the only major reservoir in PUIRB stretching from Gilgit in north Karakoram to eastern and central Himalaya in disputed Kashmir and in north western India. Mangla reservoir is spread across Azad and Jammu Kashmir and considerably smaller in term of basin size. The ALOS GDEM based topography shows the diversification of ecosystem that exists in basins of both reservoirs. Two Landsat satellite grids show the image foot prints. Landsat satellite data were obtained from the Earth Resources Observation and Science (EROS) Center of the United States Geological Survey, USA (https://earthexplorer.usgs.gov/) and ALOS GDEM data were obtained from ALOS Science Project, Earth Observation Research Center (EORC), Japan Aerospace Exploration Agency (JAXA) (https://www.eorc.jaxa.jp/ALOS/en/aw3d30/).
Figure 2Optical Landsat satellites series data (3, 5, 7 and 8) are used to extract the WEs for Tarbela and Mangla reservoirs covering 37 years (1981–2017). (a) Shows extracted WEs from multispectral Landsat imagery based on NDWI and conversion to vector layer. (b) MET and AGR seasons based temporal evolution of WEs for Tarbela (1992–2017) and for Mangla (1993–2017). Four out of six seasons show major reduction in WEs for Tarbela & Mangla starting from Pre Rabi to Pre Kharif (WDs to Pre MS) covering December to June. Landsat satellite data were downloaded from the Earth Resources Observation and Science (EROS) Center of the United States Geological Survey, USA (https://earthexplorer.usgs.gov/).
Figure 3The WEs of Tarbela and Mangla reservoirs at (a) monthly and (b) seasonal scale during 1981–2017. (a) Monthly WEs show less variable curve representing the water storage in Tarbela as compared to Mangla during 1981–2017. This is mainly attributed to hydro-meteorological regimes in the respective basins. Driest/Wettest months recorded are May, 2010/ Sep, 2005 and Apr, 2000/ Sep, 2014 for Tarbela and Mangla, respectively. (b) The MET and AGR seasons also showed distinct WE behavior for both reservoirs.
Figure 4ERA and APH data based linear trends for Mangla-Jhelum basin, Tarbela-Indus basin and overall basin. The ERA based Tp and APH based Ap show a significant decrease of 5.38 mm year−1, 4.68 mm year−1, 8.40 mm year−1 and 319 km2 year−1, 310 km2 year−1 and 358 km2 year−1, respectively. Two very strong El Niño events of 1982–1983 and 1997–1998 reduced Tp (from 481 mm year−1 to 292 mm year−1 and 591 mm year−1 to 446 mm year−1 for 1982–1983 and 1997–1998). A similar decrease in Tp has been observed for Mangla-Jhelum basin during 1982–1983 and 1997–1998 (from 358 mm year−1 to 292 mm year−1 and 438 mm year−1 to 346 mm year−1, respectively). The Ap also decreased from 50233 km2 year−1 to 42442 km2 year−1 and 48286 km2 year−1 to 39758 km2 year−1 for Tarbela during 1982–1983, and 1997–1998. Mangla also shows a decrease in Ap during 1982–1983, 1997–1998 and 2007 (44180 km2 year−1 to 38432 km2 year−1, 40199 km2 year−1 to 34740 km2 year−1 and 36543 km2 year−1 to 30230 km2 year−1, respectively). Strength of ENSO phases are represented by VS (very strong), S (strong), M (moderate), W (weak) and N (neutral).
Figure 5Correlation analysis of WEs with ERA and APH based Tp and Ap & COs. Filled bars show that correlation is significant at 95% confidence level. Overall basin shows least significant and negative correlations with precipitation and COs. The Tarbela reservoir shows negative significant correlations with precipitation from mid to end of the year. However, positive correlations are observed with NAO and ENSO and negative correlations with IOD during winter to early summer. Mangla reservoir shows significant correlations with precipitation but for different months. Significant positive correlations are observed for ENSO and IOD only.
Figure 6The MK and Sen’s slope trend analysis for ERA and APH based Tp and Ap at sub-basin scales. Bars with four-point star represent the significant trends at 95% confidence level. The ERA Tp and Ap show decreasing trends mostly in Mangla and some of Tarbela sub-basins during post WD and pre MS. Most of the significant decreasing trends are observed for APH Tp and Ap throughout the sub-basins of PUIRB during post WD, pre MS and MS seasons.
Multiple linear regression models are developed to predict the WEs of the Tarbela and Mangla reservoirs.
| Reservoirs | Predictors | Numbers of variables | Fitting Model | Criteria | MLR Models | |||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| ANOVA | RMSE (km2) | Model Equation | Number of Significant Predictors | Most Influential Predictor | ||||||||
| R² | Adj R² | df | Training | Validation | ||||||||
| Tarbela | Years, ENSO, NAO, IOD, ERA Tp and ERA Ap | 78 | Best Model Forward | Best Adjusted R² In: P value 0.05 Out: P Value 0.10 P value 0.05 | 0.56 0.52 | 0.53 0.57 0.49 | 61 63 66 | 35.0 35.9 | 72.9 122.6 60.2 | WE = 159.9-0.007×APH Ap-2.57×ERA Tp GB520P+2.48×ERA Tp GL5P-0.039×ERA Ap GL5+0.023×ERA Ap GG20P+0.009×ERA Ap GB520P+0.036×ERA Ap GL5P-0.027×ERA Ap GG20D-0.037×ERA Ap GB520D+0.035×ERA Ap GL5D WE = 27.4-0.006×APH Ap+0.64×ERA Tp T17+0.74×ERA Tp T21+0.027×ERA Ap T3-0.03×ERA Ap T15+0.027×ERA Ap T17 WE = 160.1-0.66×ERA Tp T15+0.94×ERA Tp T17-0.79×ERA Tp T25+0.043×ERA Ap T3-0.007×ERA Ap GB520P+0.0005×ERA Ap GG20D | 10 6 6 | ERA Tp GB520P ERA Ap T3 |
| Years, ENSO, NAO, IOD, ERA Tp, ERA Ap, APH Tp and APH Ap | 148 | Best Model Forward | Best Adjusted R² In: P value 0.05 Out: P Value 0.10 P value 0.05 | 0.52 0.56 | 0.45 0.58 0.53 | 120 124 124 | 38.4 36.4 | 108.1 69.9 61.1 | WE = 207.3-4.46×ERA Tp GB520P+4.42×ERA Tp GL5P+0.16×APH Ap T26-0.032×APH Ap GL5-0.017×APH Ap GG20P-0.047×APH Ap GB520P+0.03×APH Ap GL5P+0.008×APH Ap GG20D+0.07×APH Ap GB520D+0.041×Aph Ap GL5D WE = 161.5+12.57×ENSO+1.08×ERA Tp T6-3.27×ERA Tp T25-2.73×ERA Tp GB520P+4.12×ERA Tp GL5D+0.035×ERA Ap T3-0.022×ERA Ap T9-0.012×APH Ap T9 WE = 171.5+16.72×ENSO-0.93×ERA Tp T25+0.016×ERA Ap T3-0.02×ERA Ap GG20D+0.0075×ERA Ap GL5D | 10 8 5 | ERA Tp GB520P ERA Tp T25 | |
| Mangla | Years, ENSO, NAO, IOD, ERA Tp and ERA Ap | 22 | Best Model Stepwise Forward | Best Adjusted R² In: P value 0.05 Out: P Value 0.10 P value 0.05 | 0.37 0.23 0.22 | 0.33 0.22 0.20 | 60 65 66 | 55.3 59.3 59.2 | 78.0 63.0 61.6 | WE = 189.6+5.63×ENSO-15.12×NAO-2.03×ERA Tp-0.11×ERA Ap+2.42×ERA Tp GL5P+0.068×ERA Ap M1-2.17×ERA Ap M4+0.055×ERA Ap M5 WE = 184.9-0.96×ERA Tp M1+0.73×ERA Tp WE = 183.3-16.08×NAO-0.77×ERA Tp M1+0.53×ERA Tp M3 | 8 2 3 | ERA Tp ERA Tp M1 ERA Tp M1 |
| Years, ENSO, NAO, IOD, ERA Tp, ERA Ap, APH Tp and APH Ap | 40 | Stepwise Forward | Best Adjusted R² In: P value 0.05 Out: P Value 0.10 P value 0.05 | 0.44 0.39 | 0.43 0.40 0.36 | 138 144 143 | 47.9 50.1 | 92.5 88.6 77.0 | WE = 172.7-23.3×NAO-1.30×ERA Tp M1+1.11×ERA Tp M3+12.41×APH Tp GL5-11.16×APH Tp GL5D+12.76×APH Ap M4-0.039×APH Ap M5+0.24×APH Ap GL5-0.13×APH Ap GL5P-0.18×APH Ap GL5D WE = 183.9-0.75×ERA Tp M1+2.81×ERA Tp M3-3.07×ERA Tp GL5P+3.92×APH Tp M4-1.62×APH Tp M5 WE = 182.5-1.05×ERA Tp M1+0.70×ERA Tp M3+3.67×APH Tp M4-1.57×APH Tp M5 | 10 5 4 | APH Tp M4 ERA Tp M1 | |
Three different regression models’ approaches are employed using different number of predictor variables at monthly scale. Difference in number of predictors for the Tarbela and Mangla is due to different number of sub-basins. Best models are showed in bold (with highest R2 value). Most influential predictor is also identified based on its maximum contribution to model performance and is displayed in bold in extreme column.
Figure 7Sub-basin characteristics based on distribution and size of glaciated areas using Rudolph glacier inventory. The glaciated area percent contribution at sub-basin scale is used to generate new predictor variables for multiple linear regression models for WE prediction. We have addressed the following question: whether precipitation of glaciated sub-basins play some role in WE variability or not? Detailed information is provided in Extended Table 1. Glacier inventory data was downloaded from http://www.glims.org/RGI/randolph50.html (RGI Consortium (2015). Randolph Glacier Inventory -A Dataset of Global Glacier Outlines: Version 5.0: Technical Report, Global Land Ice Measurements from Space, Colorado, USA. Digital Media. https://doi.org/10.7265/N5-RGI-50).