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AU781580B2 - Process for radar measurements of the movement of city areas and landsliding zones - Google Patents
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AU781580B2 - Process for radar measurements of the movement of city areas and landsliding zones - Google Patents

Process for radar measurements of the movement of city areas and landsliding zones Download PDF

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AU781580B2
AU781580B2 AU71806/00A AU7180600A AU781580B2 AU 781580 B2 AU781580 B2 AU 781580B2 AU 71806/00 A AU71806/00 A AU 71806/00A AU 7180600 A AU7180600 A AU 7180600A AU 781580 B2 AU781580 B2 AU 781580B2
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phase
relation
pixel
atmospheric
residuals
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Alessandro Ferretti
Claudio Prati
Fabio Rocca
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Politecnico di Milano
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AUSTRALIA
Patents Act 1990 COMPLETE SPECIFICATION STANDARD PATENT Applicant(s): POLITECNICO DI MILANO Invention Title: PROCESS FOR RADAR MEASUREMENTS OF THE MOVEMENT OF CITY AREAS AND LANDSLIDING ZONES The following statement is a full description of this invention, including the best method of performing it known to me/us: 1A, "Process for radar measurements of the movement of city areas and landsliding zones."
DESCRIPTION
The present invention relates to a process for measuring the movement of city areas and landsliding zones.
As is already known, a synthetic aperture radar or SA. produces a bidimensional image. One dimension of the image is called range and it is a m=asurement of the line-of-sight distance from the radar to the object illuminated. The other dimension is called azimuth and is perpendicular to the range, The measuring operation and the range accuracy are obtained by means of a synthetic apere radar determining as precise as possible the time that has passed from the transmission of one pulse by the radar to receiving the echo of the illuminated object, The range accuracy is determined by the length of the pulse transmitted. Shorter time pulses ensure a finer resolution.
To obtain a fine resolution of the azimuth it is necessary to use a large physical antenna so that the electromagnetic wave transmitted and received:.
is as similar as possible to a pulse (in the ideal ease the pulse has the shape of a Dirac delta)- Similar to optical systems (such as telescopes), that need large apertures to obtain fine resolutions of the image, also a SAR-type radar, of normal precision, that works at a much lower frequency than those of the optical systems, needs an enormous antenna with enormo4s apertures (hundreds of metres), that cannot be installed on any platform. Nevertheless a SAR-type radar installed on an aeroplane can collect information during the flight and then elaborate it as if it were an antenna. The distance that the aeroplane covers, simulating the length of the antenna, is called synthetic aperture, The SAR-type radar consists of a coherent radar, that is a radar which measures both the module and the phase of the electromagnetic wave 2 reflected, operating at a frequency which is =sally between 400 M~hz and Ghz 2 and is, as previously said, installed on 4eroplanes, and also on orbiting satellites at a height between 250 and 800 Km.
The antenna of the radar is directed towards the earth orthogonally to S the direction of the movement of the platform (aeroplane or satellite) with an angle, called "Offniadir", between 20 and 80 degrees in relation to the direction of Nadir, that is, perpendicularly to the earth.
With said systcm, resolution cells or grids of the earth surface can be generated with a spatial resolution of a few mnetres. Said cells present a minimum grid of resolution, that is, they have ft spacing within which it is possible to distinguish two objects to illuminate, The most important characteristic of SAR is that it is a coherent image system, It is therefore possible to measure the range difference in two or more SAR images (SA.R interferometer) of the same surface with an accuracy of a fraction of the SAR wavelength, Using focusing techniques that preserve the phase, images are obtained in which every element of the image (pixel) is associated with a complex number resulting from the comnbination of the backs cattering of all the objects belonging to the same ground resolution cell and the phase rotation due to the path.
The phase of every pixel is given by the sum of two terms: the fist is the phase of the scatterer s and the second is given by *r 4=r/X where r is the radar resolution cell distance and X is the radar wavelength (with X. c/(21rf), where f is the operating frequency of the radar and c is the speed of the light). The second phase term contains millions of cycles because the w~velengths are a few centimetres and the radar sensor resolution cell distance is a few hundred krns, while the displacement connected to the scatterers; is fundamentally random and therefore the phaqe of a single SAR image is practically unusable- However, if we consider the phase difference between two SAR images taken from slightly different viewing angles, the phase term due to the scatterers is cancelled (at least in first approximation if the angle difference is small) and the residual phase term results =4Ar/. where Ar is the difference of the paths between the sensors and the same ground resolution cell, The phase term still contains a very high number of cycles, that is known apart from the high integer multiple of 27r, but passing from one resolution cell to an adjacent one, the variation of the phase is usually small enough not to present ambiguity of 2T. The phase thus deduced is called the interferometric phase and the variation information Ar (which is measured in fractions of wavelength between pixel of the SAP, image is connected thereto. Knowing the position of the two sensors, the measure of Ar can be used to find the relative elevation between the pixel of the image and therefore generate a digital elevation model ("Digital Elevation Model" or DEM), that is, an electronic reading is taken of the topography of the Earth's surface. On the other hand, if the topography is known, that is a DEM of the area of interest is available (there are special data banks from which one can take these digital models), its contribution to S .the interferometric phase can be eliminated and possible small surface displacements can be detected. In the case of the satellites ERS-1 and ERS-2 (twin satellites sent into orbit by the European Space Agency, the first, ERS- 20 1, in 1991, the second, ERS-2, in 1995, operating at a frequency of 5.3 GHz, characterised by a 35-day revolution period and by a 20-meter grid resolution), for example, from one passage to the next of the platform (ERS- 1 and ERS-2 follow each other at a distance of one day), or of one of the two satellites, several scatterers do not change their behaviour, that is, they keep a. high coherence and therefore the cancellation of their phases is practically perfect. This means that the phase measures obtained by means of this technique can measure movements that are even a few millimetres of the SEarth's topography.
Nevertheless, the present techniques of differential interferometry have some limits. In fact after a few days, in extended zones, the scatterers lose 4 coherence, that is the scatterers do not remain similar to themselves after a period of time and therefore coherent zones with dimensions exceeding a few resolution cells cannot be identified. In addition, the wavelength of the incident signal and the displacement of it are function of atmospheric conditions. These cause phase rotations that cannot be distinguished from the movements of the ground that are required to be measured.
Another problem is the physical structure of the single scatterer that influences the phase variation in function of the observation direction and therefore of the baseline, that is of the distance between the two satellites projected orthoganally to the view line. If the stable scatterer is a surface that S•backscatterers and that occupies the entire resolution cell in the range, the ~phase of the radar echo loses correlation in correspondence with the so called critical baseline (for example in the case of satellites of the ERS type *the critical baseline is about 1200 metres). When instead the scatterer is pointwise or is a corner reflector, the phase remains unvaried for much greater baselines.
According to the present invention, there is provided a process for identifying permanent scatterers being scatterers whose electromagnetic characteristics remain unaltered over time, in radar 20 measurements comprising a plurality N of synthetic aperture radar (SAR) o.images, the process comprising: forming N-l differential interferograms in relation to a main or ~master image using a digital elevation model (DEM); for every pixel of the image of step selected on the statistical properties of the modulus of the reflectivity, generating a temporal series of the interferometric phases, and then determining differences between temporal series that belong to neighbouring pixels; for every differential temporal series of step calculating the linear phase components in relation to the baseline and the phase components connected to a predetermined displacement model, in relation to the time; associating the relative error between the precise elevation of the pixel supplied from said DEM with the linear phase component of step in relation to the baseline; associating the relative movement of the pixel in the direction of the SAR with the polynominal phase variation in relation to the time of step forming phase residuals by subtracting the contributions calculated at steps and after a phase unwrapping procedure on the sparse grid of the previously selected pixels; analysing the spectral power density of the phase residuals and 1) if the residuals relating to each single image are spatially correlated, attributing said residuals to atmospheric artefacts and removing said artefacts; and if the further residual dispersion relating to each single image is too large, discarding the pixel.
In one embodiment, the process further comprises: given a number of permanent scatterers per surface unit> after processing the phase residuals, determining the atmospheric artefact of 20 every single image and subtracting the atmospheric artefacts so determined oo•from the reference DEM to improve its vertical precision.
o oo Thanks to the present invention, a process can be made for identifying ,t the stable scatterers in time, called PS (regardless of the atmospheric conditions and of the type of platform on which the SAR radar is positioned), which can determine the movement of city areas and landsliding zones.
As well, a process can be provided which makes it possible, from the phase dispersion of the PS, to estimate the dimension and construct a network of natural reflectors suitable for identifying the orbital position of any satellite or aeroplane that illuminates the natural network of said PS, or to measure the movements of the PS or of the atmospheric artefact.
The invention also provides a process for making radar measurements, including identifying permanent scatterers according to process described above.
The characteristics and advantages of the present invention may be further ascertained from the following detailed description of an embodiment thereof, illustrated as non-limiting example in the enclosed drawings, in which: Figure 1 shows a geometric image of the interferometry SAR in the case of one single cell; Figure 2 illustrates some interferograms referring to a specific area; Figure 3 shows a three-dimensional graph of nine interferograms in 0 0. function of the baseline; Figure 4 shows four examples relative to four different pixels of an interferogram of Figure 3; Figure 5 illustrates a three-dimensional graph of nine interferograms in function of the time; Figure 6 shows four examples relative to four different pixels of an o interferogram of Figure Figure 7 illustrates the differential contributions of the atmosphere of the single images compared to the main image ("master"); o• Figure 8 shows an estimation of the atmospheric contribution present on the master image; Figure 9 illustrates a real example of the localisations and of the spatial densities of the stable scatterers (called PS) over a three-year time; Figure 10 shows a real example of the present invention made on the Valle del Bove (Etna); and Figure 11 is a colour representation that illustrates a real example of the subsidence rates of the Valle del Bove (Etna).
In Figure 1 the phase difference between two SAR images takcen from slightly different viewing angles is shown.
According to what is illustrated in said Figure, there are noted one axis of the x-co-ordinates5, representing sea level or another reference surface, one axis of the ordinates, representing the height of sea level, or another reference surface; three points 101, 102, 103; 4 horizontal line 108 passing through point 101; a vertical line 104, parallel tq the axis of the ordinates, indicating the distance 11W1 between the axis of the x-co-ordinatcS and the horizontal line 108; a topographic line 105; an acute angle 8; the distance between points 10 1 and 102, in a normal direction to the view line (called baseline) will be indicated with a segment 111 having length B; the distance 109 between points 10 1 and 103 is indicated with p; the distance 110 between points 102 and 103 is indicated with p±A&p.
If two receiving and tr~nsmitting tadar antennae, 101 and 102, which illuminate the same surface zone 103 simultaneously are considered, and point 101 is placed at a distance p from the ground and point 102 at a ::::*distance p-iAp from the ground, the displacement of the illumination path is calculated as 4 n~pAk with X as length of incident and reflected wave. It can be noted that the phase difference depends both on the geometric view and the height of point 103 above the reference surface (axis of the xcoordinates). Therefore, if the geometric view can be controlled or is at least known with sufficient accuracy, the topography 105 in relation to point 103 (called q) can be extrapolated from the measure of the phase difference O1q with a precision of several metres, specifically using the expression p sinG Figu.re 2 oliows the interferograms of a specific area generated through *.:the usual computer program Using a main image, called "master", and nine secondary images, called "slaves" Each interferogram is cha ractenised in that it has a different baseline, an axis of the x-coordinates indicating the 8 direction of azimuth and an axis of the ordinates, indicating the range direction.
The nine different differential interferograms are made by subtracting from the phase difference of every pixel the contribution of the topography, and using an existing DEM, that is using digital models which are available on the market, with a better vertical accuracy than 50 m.
The reference DEM can also be generated from the high coherence interferometric couples. For example in the case of satellites ERS-1 and ERS-2 the couples of images taken at the distance of a day can be used because after a brief period of time from the passage of said satellites, said zones do not modify their stable scatterers. These couples of images generate high coherence interferometric couples.
In Figure 3, which uses the baseline and distance values of the radar (slant range), nine interferograms of Figure 2 are shown, generated by the same master image, positioned three-dimensionally, ordered by increasing baselines.
According to said Figure it can be noted that each interferogram is referred to the same ground surface area, but has a different baseline.
Fourpoints, called pixels, are identified with 112, 113, 114 and 115, 20 belonging to a specific interferogram.
Having the nine inteferograms available and taking only one point, for "example 112, belonging to one of the interferograms, on the basis of the ~previous formula of 'Oq this has a phase component, relative to a reference pixel, which increases linearly with the baseline in function of the relative *25 height error. Therefore a mono-dimensional signal is made, as hereunder S" described with reference to Figure 4, which represents a sequence of the S. interferometric phases in function of the baseline.
The method is the same for points 113,114 and 115 from which the same number of sequences of the interferometric phases are extracted in function of the baseline.
In Figure 4 four examples relative to four different pixels of an interferogram are shown.
According to what is illustrated in said Figure four diagrams of the interferometric phases 127, 116, 117 and 118 can be noted having as axis of the x-coordinates the baseline variable and as axis of the ordinates the interferometric phase in relation to the master.
Each diagram consists of a multiplicity of points and a straight line which is the result of the interpolation of said points.
The phase linear component is calculated for evey temporal series 127, 116, 117 and 118 in relation to the baseline, that is the inclination a of the straight line of equation C=aB+C (where C is a constant) to the squared minimum is estimated and which minimises the following expression: q S* ±(QI -aB.C) 2 S"-in relation to the baseline by using the following formula: Aq a l 147 In this way the relative topography error can be detected, which is 5*S S..:connected to the inclination a of the interpolated line, which is more suitable for the data extracted from the interferometric phases.
In Figure 5 nine interferograms in function of the time generated by the same master image are shown.
According to what is illustrated in said Figure it can be noted that every inteferogram refers to the same ground surface area, but has a different inst4nt axis t (time).
Four pixels belonging to a specific interferogram are identified with 119, 120, 121 and 122 as well.
Having the nine interferograms available and taking one single point 119, belonging to one of the interferograms, this has a phase relative to a reference pixel which varies linearly in time (having assumed a constant speed subsidence model) and therefore a signal is made, evidently monodimensional, as is hereunder described with reference to Figure 6.
The method is the same for pixels 120, 121 and 122 which give rise to the same number of monodimensional signals.
In Figure 6 four examples relating to four different pixels of an interferogram of Figure 5 are shown.
According to what is illustrated in said Figure four diagrams of the interferometric phases 123, 124, 125 and 126 can be noted, having the time variable as axis of the x-coordinates, and the interferometric phase variable in relation to the master as axis of the ordinates.
20 Each diagram consists of a multiplicity of points and of a straight line which is the result of the interpolation of said points.
Supposing that we have a subsidence model available, that is a sinking ~movement of the earth's crust at a constant speed which occurs in certain zones called geosynclines, the entity of said movement is estimated by 25 determining to the squared minimum the inclination k of the straight line "r--kt which minimises the following expression: 0%ee *q *e 1 In this manner we can find the subsidence speed which is connected to the inclination k of the interpolated straight line which is more suitable for the data extracted from the interferometric phases, Figure 7 represents differential interfere grams having azimuth variable on the x-axis and the range variable on the y-axis.
According to what is illustrated in said interferograins, the phase residuals are made after subtracting, by using a known computer program, the contributions given by the error between the precise elevation of the pixel and that supplied by the reference DEM and the movement of the pixels in the direction of the satellite radar.
Figure 8 shows an estimation of the atmospheric contribution present on the master image, obtained by making an arithmetic average of the phase residuals of Fig. 7.
In said Figure it can be noted that the image presents a graduation scale indicating the phase in raians.
The estimation of the contribution present on the master image can be subtracted, again by using a known computer program, from the differential atmospheric contributions seen in Figure 7 giving as result the atmospheric contribution present on every single image, called Atmospheric Phase Screen CAPS).
Figure 9 shows a real example of the localisation and the density of the stable scatterers in time, According to what is illustrated in said Figure, an axis of the x-coordinates indicating the azimuth direction and an axis of the ordinates indicating the range direction can be noted. The unit for measuring the axes if the pixel.
A plurality of points that identify the stable pixels in time can be noted as well, .:In fact the sequence of the operations described in the previous figures cannot be carried out on all the image pixels, but only on those that keep their physical characteristics (PS) during the interval of time in which all the images of the temporal series have been acquired.
This analysis is carried out in two steps: first, PS candidates are selected on the statistical properties of the modulus of the reflectivity, then the spectral power density of the phase residuals is analysed and if the residuals relating to each single image are spatially correlated, attributed to atmospheric artefacts and removed; if the fiurther residual dispersion relating to each single image is too large the pixel is discarded, When the number of stable scatterers per surface unit is suficient, at least twenty five PS per Km 2 the phase residuals obtained from the subtraction of the phase contribution due to precise elevation of the pixel and movement of the pixel in the direction of the satellite radar, are su~fficient for reconstructing the atmospheric artefact of each single image through a low-pass interpolation on the uniform image grid.
This artefact can therefore be removed froma each SAR image improving the quality of the DEM and therefore using the interferornetric phases, filtered of the atmospheric artefact found with the method previously described, we have an improvement of the degree of correlation of the pixels, classified as PS, Figure 10 shows a real image of the present invention of a temporal series on the Valle del Bove (Etna), According to what is illustrated in said Figure it can be noted that the axis of the ,c-coordinates indicates the azimuth direction, while the axis of the ordinates indicates the range direction. Both axes have the pixel as unit of measure.
A grade indicator indicating the phase in radians can also be noted.
The Figure shows the atmospheric outlines relating to an iroage of the temporal series on the Valle del Bove estimated by interpolating the results obtained in correspondence with the stable scatterers, that is the PS, seen in Figure 9.
Figure I1I shows the subsidence movement in terms of velocity field 13 estimated on the Valle del Bove (Etna) in correspondence with the stable scatterers, that is the PS, of Figure In said Figure an axis of the x-co-ordinates indicating the azimuth direction can be noted and also an axis of the ordinates indicating the range direction. Both axes have pixel 5 as unit of measure.
It can also be noted that the image is composed of a plurality of points, coloured in different manners. This means that the red ones have the value of a subsidence speed of about four centimetres per year while the green ones have the value of zero speed.
It is to be understood that, if any prior art publication is referred to herein, such reference does not constitute an admission that the publication forms a part of the common general knowledge in the art, in Australia or any other country.
For the purposes of this specification it will be clearly understood that the word "comprising" means "including but not limited to", and that the word "comprises" has a corresponding meaning.
*o

Claims (8)

1. A process for identifying permanent scatterers in radar measurements comprising a plurality N of synthetic aperture radar (SAR) images, the process comprising: forming N-I differential interferograms in relation to a main or master image using a digital elevation model (DEM); for every pixel of the image of step selected on the statistical properties of the modulus of the reflectivity, generating a temporal series of the interferometric phases, and then determining differences between temporal series that belong to neighbouring pixels; for every differential temporal series of step calculating the linear phase components in relation to the baseline and the phase :components connected to a predetermined displacement model, in relation to the time; 0 associating the relative error between the precise elevation of the pixel supplied from said DEM with the linear phase component of step in -relation to the baseline; associating the relative movement of the pixel in the direction of the 20 SAR with the polynominal phase variation in relation to the time of step oooe forming phase residuals by subtracting the contributions calculated oo at steps and after a phase unwrapping procedure on the sparse grid of 0 o•0 the previously selected pixels; analysing the spectral power density of the phase residuals and 1) if the residuals relating to each single image are spatially correlated, attributing said residuals to atmospheric artefacts and removing said artefacts; and if the further residual dispersion relating to each single image is too large, discarding the pixel.
2. A process as claimed in claim 1, further comprising: given a number of permanent scatterers per surface unit 25/km 2 after processing the phase residuals, determining the atmospheric artefact of every single image and subtracting the atmospheric artefacts so determined from the reference DEM to improve its vertical precision.
3. A process as claimed in claim 2, wherein steps and are reiterated, using the interferometric phases filtered of the atmospheric artefact according to step
4. A process for making radar measurements, including identifying permanent scatterers according to any one of the preceding claims.
5. A process as claimed in claim 4, used for making radar measurements of movements in city areas.
6. A process as claimed in claim 4, used for making radar measurements of landsliding zones. Oo o
7. A process for identifying permanent scatterers substantially as 20 hereinbefore described with reference to the accompanying drawing.
8. A process for making radar measurements substantially as hereinbefore described with reference to the accompanying drawing. Dated this 8th day of April 2005 POLITECNICO DI MILANO By their Patent Attorneys GRIFFITH HACK Fellows Institute of Patent and Trade Mark Attorneys of Australia.
AU71806/00A 2000-11-24 2000-11-24 Process for radar measurements of the movement of city areas and landsliding zones Ceased AU781580B2 (en)

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CN112627245B (en) * 2020-12-20 2022-02-08 长江水利委员会长江科学院 Abandoned dreg site surveying and ecological restoration method based on in-situ recognition
CN115453520B (en) * 2022-10-26 2023-01-03 中国电子科技集团公司第十四研究所 Earth surface deformation measurement method and device based on dual-frequency multi-polarization differential interference
CN118584435B (en) * 2024-08-05 2024-11-19 南京信息工程大学 Error correction method and system for radar differential interference pair based on reference plane

Citations (3)

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US5659318A (en) * 1996-05-31 1997-08-19 California Institute Of Technology Interferometric SAR processor for elevation
WO1998002761A1 (en) * 1996-07-11 1998-01-22 Science Applications International Corporation Terrain elevation measurement by interferometric synthetic aperture radar (ifsar)
US5726656A (en) * 1996-12-19 1998-03-10 Hughes Electronics Atmospheric correction method for interferometric synthetic array radar systems operating at long range

Patent Citations (3)

* Cited by examiner, † Cited by third party
Publication number Priority date Publication date Assignee Title
US5659318A (en) * 1996-05-31 1997-08-19 California Institute Of Technology Interferometric SAR processor for elevation
WO1998002761A1 (en) * 1996-07-11 1998-01-22 Science Applications International Corporation Terrain elevation measurement by interferometric synthetic aperture radar (ifsar)
US5726656A (en) * 1996-12-19 1998-03-10 Hughes Electronics Atmospheric correction method for interferometric synthetic array radar systems operating at long range

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