Impacts of geoid height on large-scale crustal deformation mapping with InSAR observations

  • Peng Li
  • , Zhen Hong Li
  • , Chuang Shi*
  • , Wan Peng Feng
  • , Cun Ren Liang
  • , Tao Li
  • , Qi Ming Zeng
  • , Jing Nan Liu
  • *Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

Abstract

An ellipsoidal height datum (e.g. WGS84) is required in SAR Interferometric processing, whilst DEMs are often referenced to a geoid datum (e.g. EMG96). Therefore, geoid height error is introduced due to the inconsistency of height datums in InSAR derived displacement maps. In this paper, the relationship between geoid heights and uncertainties in InSAR displacements is investigated using 27 scenes of Envisat ASAR ScanSAR images and 44 scenes of Image-mode images covering the western Altyn Tagh Fault, northern Tibetan Plateau. A typical error of 8.8 m in SRTM DEM leads to 3 mm uncertainty in an InSAR interferogram with a perpendicular baseline of 100 m, whilst a geoid height of 20 m can result in 10 mm uncertainty. Geoid height varies from one place to another, and is highly correlated with topography. The impacts of geoid height on InSAR displacements increase with perpendicular baselines, but SAR images with a small perpendicular baseline may not be available in some cases. In addition, it may also not always be feasible to use a best-fitting plane to remove the impacts of geoid height. It is thus highly recommended in this paper that DEMs with an ellipsoidal height datum should be employed in interferometric processing, particularly when long-wavelength crustal deformation is targeted.

Original languageEnglish
Pages (from-to)1857-1867
Number of pages11
JournalActa Geophysica Sinica
Volume56
Issue number6
DOIs
StatePublished - Jun 2013
Externally publishedYes

Keywords

  • Altyn tagh fault
  • Crustal deformation
  • Geoid height
  • SAR interferometry
  • Wide-swath InSAR

Fingerprint

Dive into the research topics of 'Impacts of geoid height on large-scale crustal deformation mapping with InSAR observations'. Together they form a unique fingerprint.

Cite this