Recent Updates on Alpine-Himalayan Belt High Resolution Surface Velocities with Sentinel-1 InSAR and GNSS Observations
- 1COMET, School of Earth and Environment, University of Leeds, LS2 9JT, UK
- 2COMET, School of Earth and Environment, University of Oxford, OX1 3AN, UK
- 3GNS Science, Lower Hutt, New Zealand
The Alpine-Himalayan Belt (AHB) includes 75 percent of all earthquakes that have killed more than 10,000 people in the past century. Geodetic measurements of crustal deformation provide important information for studying earthquake hazards, indicating how the strain is accumulating and illuminating the mechanics of large-scale continental deformation.
The COMET-LiCSAR InSAR processor was designed to automatically produce InSAR products on a global scale [1]. Processed data are made freely available to the community (https://comet.nerc.ac.uk/comet-lics-portal/). With the recent expansion of the system, we aim at generating high-resolution velocity field for the entire AHB. The area is covered by 644 ascending and descending frames. We have processed 130,000 Sentinel-1 epochs in this region and generated more than half a million interferograms. The average length of the connected small baseline network is 6 years. In some sub-regions such as the Anatolia, Caucuses, Iran, Tibet and Tianshan, more than 80 percent of all Sentinel-1 acquisitions are processed.
In this study, we first used the LiCBSAS approach [2] to invert for the LOS displacement time-series and velocities. Next, following the VELMAP approach [3], we used the LOS velocities and the GNSS data to solve for the velocities in nodes of a spherical triangle mesh as well as the InSAR reference frame adjustment parameters. This results in the InSAR LOS velocities in a Eurasian reference frame. We finally decomposed these referenced LOS velocities into the east-west and vertical velocities. While the vertical velocities are mainly dominated by the anthropogenic displacements such as water pumping, or any other environmental parameters such as permafrost, the east-west velocity field exhibits the features of the long-wavelength deformation along the major faults in central, east and west of the AHB.
References:
[1] Lacecky et al., 2020 https://doi.org/10.3390/rs12152430
[2] Morishita et al., 2020 https://doi.org/10.3390/rs12030424
[3] Wang and Wright, 2012 https://doi.org/10.1029/2012GL051222
How to cite: Maghsoudi, Y., Wright, T., Lazecký, M., Ou, Q., Elliott, J., Watson, A., Rollins, C., Hooper, A., Fang, J., Shen, L., Watson, S., and Parsons, B.: Recent Updates on Alpine-Himalayan Belt High Resolution Surface Velocities with Sentinel-1 InSAR and GNSS Observations, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-15348, https://doi.org/10.5194/egusphere-egu23-15348, 2023.
