Radar interferometry and its application to changes in the Earth's surface

Радарная интерферометрия и её применение к изменениям поверхности Земли
D. Massonnet, K. L. Feigl
1998-11-01

ERS-1 ERS-2 JERS-1 RADARSATinterferogramradar interferometrysurface deformation measurementsynthetic aperture radar
Geophysical applications of radar interferometry to measure changes in the Earth's surface have exploded in the early 1990s. This new geodetic technique calculates the interference pattern caused by the difference in phase between two images acquired by a spaceborne synthetic aperture radar at two distinct times. The resulting interferogram is a contour map of the change in distance between the ground and the radar instrument. These maps provide an unsurpassed spatial sampling density (∼100 pixels km −2 ), a competitive precision (∼1 cm), and a useful observation cadence (1 pass month −1 ). They record movements in the crust, perturbations in the atmosphere, dielectric modifications in the soil, and relief in the topography. They are also sensitive to technical effects, such as relative variations in the radar's trajectory or variations in its frequency standard. We describe how all these phenomena contribute to an interferogram. Then a practical summary explains the techniques for calculating and manipulating interferograms from various radar instruments, including the four satellites currently in orbit: ERS‐1, ERS‐2, JERS‐1, and RADARSAT. The next chapter suggests some guidelines for interpreting an interferogram as a geophysical measurement: respecting the limits of the technique, assessing its uncertainty, recognizing artifacts, and discriminating different types of signal. We then review the geophysical applications published to date, most of which study deformation related to earthquakes, volcanoes, and glaciers using ERS‐1 data. We also show examples of monitoring natural hazards and environmental alterations related to landslides, subsidence, and agriculture. In addition, we consider subtler geophysical signals such as postseismic relaxation, tidal loading of coastal areas, and interseismic strain accumulation. We conclude with our perspectives on the future of radar interferometry. The objective of the review is for the reader to develop the physical understanding necessary to calculate an interferogram and the geophysical intuition necessary to interpret it.
1
Applications demonstrated include deformation from earthquakes, volcanoes, glaciers, landslides, subsidence, agriculture impacts, postseismic relaxation, tidal loading, and interseismic strain accumulation.
2
Interferograms provide very high spatial sampling density (~100 pixels km−2), precision (~1 cm), and observation cadence (1 pass month−1).
3
Interferograms record crustal movements, atmospheric perturbations, soil dielectric changes, and topographic relief, but are also sensitive to technical effects (satellite trajectory and frequency variations).
4
Practical methods are described for calculating and manipulating interferograms from existing satellites (ERS‑1, ERS‑2, JERS‑1, RADARSAT) and for assessing uncertainty and artifacts.
5
Radar interferometry computes interferograms from phase differences between two SAR images to map changes in ground-to-radar distance.

Radar interferogram maps of changes in the Earth's surface derived from spaceborne synthetic aperture radar

Measurement, interpretation, and application of surface-change signals in interferograms including deformation (earthquakes, volcanoes, glaciers), subsidence, landslides, atmospheric and dielectric effects, noise/artifacts, uncertainty assessment, and processing techniques

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1998-11-01
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D. Massonnet
K. L. Feigl
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