Figures & data
Figure 2. Spatial and temporal baseline diagrams of interferograms obtained from (a) ascending; and (b) descending images.
![Figure 2. Spatial and temporal baseline diagrams of interferograms obtained from (a) ascending; and (b) descending images.](/cms/asset/79571676-b605-4edf-b7a0-6b0a8ad88828/tgrs_a_2170125_f0002_oc.jpg)
Figure 3. Proposed flow chart for the analysis of InSAR time series of the unstable slopes of Maoergai Reservoir.
![Figure 3. Proposed flow chart for the analysis of InSAR time series of the unstable slopes of Maoergai Reservoir.](/cms/asset/6c2da6dc-b58d-4f0b-a398-d2eb610568bd/tgrs_a_2170125_f0003_oc.jpg)
Figure 4. (a) SBAS-InSAR displacement rate results of the Maoergai reservoir in ascending orbiting; (b)sbas-InSAR displacement rate results of the Maoergai reservoir in descending orbiting; (c) Geometric distortion of the ascending orbiting; (d) Geometric distortion of the descending orbiting.
![Figure 4. (a) SBAS-InSAR displacement rate results of the Maoergai reservoir in ascending orbiting; (b)sbas-InSAR displacement rate results of the Maoergai reservoir in descending orbiting; (c) Geometric distortion of the ascending orbiting; (d) Geometric distortion of the descending orbiting.](/cms/asset/2d51a513-8b7a-4c5c-919d-f63d7855ac53/tgrs_a_2170125_f0004_oc.jpg)
Figure 5. Average displacement rate of unstable slopes (MEG01–13 detected in the ascending data and MEG14–20 detected in the descending data).
![Figure 5. Average displacement rate of unstable slopes (MEG01–13 detected in the ascending data and MEG14–20 detected in the descending data).](/cms/asset/772bff6e-3509-4cdb-aa56-38e7bdfdb90b/tgrs_a_2170125_f0005_oc.jpg)
Figure 6. Time series displacement curves of landslides (a) MEG06; (b) MEG13; (c) MEG15; and (d) MEG19.
![Figure 6. Time series displacement curves of landslides (a) MEG06; (b) MEG13; (c) MEG15; and (d) MEG19.](/cms/asset/421f6b2e-6e2f-44d6-8e8f-69ae1131beeb/tgrs_a_2170125_f0006_oc.jpg)
Figure 8. Correlation between cumulative displacements and influencing factors derived from gray correlation analysis.
![Figure 8. Correlation between cumulative displacements and influencing factors derived from gray correlation analysis.](/cms/asset/6035fa35-7507-4115-8f81-ea9a63a30339/tgrs_a_2170125_f0008_oc.jpg)
Figure 9. (a) Reservoir water level time series after resampling; (b) CWT of MEG02; (c) CWT of MEG09; (d) CWT of MEG13; (e) CWT of MEG15; (f) CWT of MEG18. 5% significance level relative to red noise is shown as a coarse contour. The wavelets are not fully localized in time and there may be edge pseudo-effects out of the cone of influence (COI).
![Figure 9. (a) Reservoir water level time series after resampling; (b) CWT of MEG02; (c) CWT of MEG09; (d) CWT of MEG13; (e) CWT of MEG15; (f) CWT of MEG18. 5% significance level relative to red noise is shown as a coarse contour. The wavelets are not fully localized in time and there may be edge pseudo-effects out of the cone of influence (COI).](/cms/asset/635bd8db-b516-456a-8af1-25e44338f8dd/tgrs_a_2170125_f0009_oc.jpg)
Figure 10. Results from cross-wavelet transform (XWT) for the reservoir non-linear displacements with reservoir water level. The black line separates ascending orbiting results (above) from descending orbiting results (below). 5% significance level relative to red noise is shown as a coarse contour. The wavelets are not fully localized in time and there may be edge pseudo-effects out of the cone of influence (COI).
![Figure 10. Results from cross-wavelet transform (XWT) for the reservoir non-linear displacements with reservoir water level. The black line separates ascending orbiting results (above) from descending orbiting results (below). 5% significance level relative to red noise is shown as a coarse contour. The wavelets are not fully localized in time and there may be edge pseudo-effects out of the cone of influence (COI).](/cms/asset/abc20a35-5cf6-4b3a-a089-6da8b57132a6/tgrs_a_2170125_f0010_oc.jpg)
Data availability statement
All relevant data are available from the authors upon reasonable request. Some datasets that support the findings of this study are available in [https://scihub.copernicus.eu/dhus/#/home], [https://earthexplorer.usgs.gov/], [https://disc.gsfc.nasa.gov/].