CN102323571B - Distribution method of satellite-borne dual-antenna SAR (Synthetic Aperture Radar) interferometric calibrator with comprehensive overall parameter - Google Patents

Abstract

The deployment method of the spaceborne dual-antenna SAR interferometric scaler based on the overall parameters, based on the analysis of the interference sensitivity matrix, makes full use of the given satellite orbit, SAR radar system and other parameter information in the overall design, and gives the full rank of the sensitivity matrix The constraints on the layout of the scaler and the deployment rules of the scaler; the present invention combines the analysis of the spaceborne SAR coverage performance and the analysis of the interference sensitivity matrix, so that the formulation of the deployment rules of the interference scaler can be obtained from the overall It is considered at the design stage to provide important guidance for subsequent calibration work; the present invention uses parameters such as satellite orbit elements, so it realizes the analysis of calibration device layout rules for each latitude region in the world, and provides global DEM data measurement. Engineering realization provides a basis for decision-making, which has important theoretical significance and engineering practical value.

Description

The spaceborne double antenna SAR of comprehensive population parameter interferes scaler to lay method

Technical field

The present invention relates to a kind of spaceborne double antenna interference synthetic aperture radar (InSAR) ground calibration device and lay method, belong to the signal processing technology field.

Background technology

Space-borne interference synthetic aperture radar (InSAR) is the comparatively active technology of in recent years synthetic-aperture radar development field development, has round-the-clock, round-the-clock feature, is widely used in topographical height measurement.There are spaceborne double antenna SAR and Distributed Spaceborne SAR in more typical spaceborne InSAR system, and the former realizes that difficulty is little because system is relatively simple, and cost is lower, has obtained larger development.

Interferometric parameter is the key concept of interfering height-finding system, comprises satellite altitude, oblique distance, base length, baseline inclination angle and interferometric phase.Interferometric parameter is determining the interference performance of InSAR system, and its precision directly has influence on the earth's surface elevation of final extraction or the precision of deformation, and therefore accurate interferometric parameter calibration is very important and essential.

The at present calibration of interferometric parameter mainly contains two kinds of methods: based on the interferometric parameter calibration of phase correction; Interferometric parameter calibration based on Sensitivity equation.

First method is based on the interferometric parameter calibration of phase correction, utilize Sensitivity equation to set up the relation of the difference of interferometric parameter error and interferometric phase and fixed phase, the method of employing solving equations is obtained the estimated value of interferometric parameter error, utilize this estimated value that the interferometric parameter error is proofreaied and correct, and the interferometric parameter after use proofreading and correct interferes height reconstruction, and then improves and interfere altimetry precision.Second method is utilized Sensitivity equation to set up the interferometric parameter error and is interfered relation between measurement of higher degree error, on this basis, adopt the method for solving equations that the interferometric parameter error is estimated, and then utilize the parameter error estimated value that interferometric parameter is proofreaied and correct.Research majority based on these two kinds of methods is applied to airborne interference SAR system now, that calibrates is regional smaller, geometric relationship is fairly simple, and spaceborne double antenna interference SAR is along earth orbital operation, zone to be calibrated relates to global a plurality of latitude zone, and satellite altitude, mapping swath width and substar place earth radius all can change when satellite worked in different latitude.In order in overall design process, Accurate Analysis to interfere calibration system to be interfered the impact of performance, be convenient in the world each latitude zone population parameter still to be tested is interfered calibration analysis, the Parameter of Overall Design such as satellite orbit parameter, SAR systematic parameter need to be incorporated into and interfere in the calibration process.

Summary of the invention

Purpose of the present invention: overcome the deficiencies in the prior art, provide a kind of spaceborne double antenna SAR of comprehensive Parameter of Overall Design to interfere scaler to lay method, the method makes overall design and interferes calibration closely to connect, can and interfere calibration to carry out l-G simulation test as unified integral body with overall design, SAR imaging processing, interference processing, both improved interference SAR system overall design quality, and given from overall angle again and interfere calibration that important references is provided.

Technical solution of the present invention: a kind of spaceborne double antenna SAR of comprehensive Parameter of Overall Design interferes scaler to lay method, to analyze borne SAR to the coverage condition on ground according to population parameter, the method of recycling sensitivity matrix analysis draws the ground calibration device and lays rule, and obtain the latitude and longitude information of each scaler by coordinates transformation method, can analyze for each latitude zone, the whole world, realize the interference calibration analysis for global range.

Principle of the present invention is: the ultimate principle that the spaceborne double antenna SAR of given first interferes calibration.Figure 1 shows that the principle of interference figure of spaceborne double antenna InSAR, h _InSARThe earth's core distance for the terrain object place can obtain following expression according to geometric relationship among the figure:

Wherein, f () is the height conversion relation; X is interferometric parameter, comprises satellite altitude H, oblique distance r ₁, base length B, baseline inclination angle theta _bAnd interferometric phase

In the interferometry process, above-mentioned parameter can affect the precision of digital elevation model (DEM) data all with error, usually will utilize ground control point (GCP:Grond Control Point) that these parameters are calibrated, and namely interferes calibration.

Figure 2 shows that the InSAR system interferes the schematic diagram of calibration, establishes the parameter error in the data acquisition

The interferometric parameter that then obtains is expressed as

$\hat{X}=X+\mathrm{\ΔX}---\left(2\right)$

For certain impact point in the mapping band, the linearization error model of its height reconstruction error is

In the mapping band, lay L scaler, and the elevation of known each scaler is h _i, i=1,2 ..., L can obtain the poor of the reconstruction elevation of each scaling point and actual elevation, and matrix equation can be expressed as

Δ＝F·ΔX+M (4)

Wherein,

Be the vertical error of i scaling point, i=1,2 ..., L; M is the linearization error matrix;

Be sensitivity matrix, the concrete form of sensitivity matrix is suc as formula shown in (5),

The interferometric parameter error can be obtained by the finding the solution of system of linear equations of formula (4), is expressed as: Δ X=F ⁺Δ.Wherein, F ⁺Generalized inverse for sensitivity matrix F.Can realize thus the interference calibration of spaceborne double antenna InSAR system.Fig. 2 has provided concrete realization flow.

In the interferometry of reality, the position of ground calibration device can't accurately be known, all with certain error, and interferometric parameter is also with certain stochastic error, therefore observation data Δ band is made an uproar, when finding the solution overdetermined equation (4), error can pass to by certain weight interferometric parameter X, the degree of propagation of error depends on the conditional number of sensitivity matrix F, and the situation that lays of the conditional number of sensitivity matrix and ground calibration device has much relations, must carry out scaler by certain constraint condition for this reason and lay, just can guarantee the calibration precision of interferometric parameter.Namely meeting under certain geometrical constraint condition, making conditional number C (F) minimum of sensitivity matrix F.C (F) computing method are suc as formula (6),

C(F)＝||F|| ₂·||F ⁺|| ₂ (6)

Wherein || F|| ₂With || F ⁺|| ₂Difference representing matrix F and F ⁺2 norms.

The present invention introduces population parameter and interferes calibration, can carry out the analysis that scaler lays rule for each latitude area of global range, will based on the wave beam covering analyzing of satellite orbit parameter and unified based on the interference calibration of sensitivity matrix analysis in same set of coordinate system, be the key point that realizes the method.Used coordinate system should reflect the physical process of spaceborne double antenna InSAR work in overall design analysis and the digital emulation, therefore needs comparatively complete coordinate system framework, so that interfere sensitivity matrix also can represent in this coordinate frame.

Fig. 3 has provided the space geometry graph of a relation of spaceborne double antenna interference SAR, has clearly reflected the inner link between ellipsoid earth model, satellite orbit, major-minor SAR antenna and the ground scene, can provide being defined as follows of each coordinate system accordingly:

(1) earth inertial coordinates system E _O: true origin is at the earth centre of sphere, and X-axis in the plane, is pointed to the first point of Aries under the line, and Z axis points to the positive arctic along the axis of rotation of the earth, and Y-axis in the plane, meets right-hand rule relation with X, Z axis under the line.

(2) body-fixed coordinate system E _G: true origin is at the earth centre of sphere, and in the plane, by first branch of Greenwich meridian, Z axis points to the positive arctic along the axis of rotation of the earth to X-axis under the line, and Y-axis in the plane, meets right-hand rule relation with X, Z axis under the line.

(3) satellite orbit coordinate system E _V: true origin is the earth centre of sphere (being positioned at the satellite orbit plane), and X-axis is in the satellite orbit plane, and forward points to pericenter, Z axis is perpendicular to the satellite orbit plane, forward points to the angular-momentum vector direction of satellite, and Y-axis is in the satellite orbit plane, and direction is determined by the right-hand rule.

(4) satellite platform coordinate system E _R: true origin is at centroid of satellite, and X-axis is in the satellite orbit plane, and forward points to the design heading of satellite, and Z axis is perpendicular to the satellite orbit plane, and forward points to the angular-momentum vector direction of satellite, and Y-axis is in the satellite orbit plane, and direction is determined by the right-hand rule.

(5) satellite celestial body coordinate system E _E: true origin is at centroid of satellite, and X-axis is along satellite celestial body y direction, and forward points to the Live Flying direction of satellite, and Y-axis and Z axis are respectively along two other principal axis of inertia direction of satellite celestial body.

(6) main antenna coordinate system E _A: true origin is at the antenna phase center point, and the X-axis forward points to the Live Flying direction of satellite, and Y-axis is along antenna boresight, and forward points to the ground direction of bowl.

(7) satellite synchronization scene coordinate system E _SS: as shown in Figure 4, true origin is the ground aiming point of main antenna beam center, and XOY plane and earth's spheroid are tangential on the O point, the X-axis positive dirction is pointed to the satellite flight direction, the normal that Z axis is ordered at O along earth's spheroid, forward deviate from the ground direction of bowl, and Y direction is determined by the right-hand rule.

(8) earth synchronization scenarios coordinate system E _SE: as shown in Figure 4, true origin is the ground aiming point of main antenna beam center, and XOY plane and earth's spheroid are tangential on the O point, the X-axis forward points to the due east direction, the Y-axis positive dirction is pointed to direct north, and the normal that Z axis is ordered at O along earth's spheroid, forward deviate from the ground direction of bowl.As we know from the figure, earth synchronization scenarios coordinate system E _SeRotate to an angle around Z axis and can obtain satellite synchronization scene coordinate system Ess.

Performing step of the present invention is as follows:

The first step is found the solution satellite Covering time t ₀:

Can set up following system of equations according to geometric relationship shown in Figure 5,

${\mathrm{<figure-callout\; id="0"\; label="t"\; filenames="HDA0000065297460000021.png,HDA0000065297460000031.png"\; state="\{\{state\}\}">t</figure-callout>}}_0=\mathrm{\&tau;}+\sqrt{\frac{a^3}{\mathrm{\&mu;}}}(E-e\sin E)---\left(7\right)$

$E=2\arctan [\tan \frac{\mathrm{\&phi;}}{2}/{\left(\frac{1+e}{1-e}\right)}^{\frac{1}{2}}]---\left(8\right)$

δ＝arcsin[sin(ω+φ)sini] (9)

λ＝Ω+arctan[tan(ω+φ)cosi]-[G ₀+ω _e(t ₀-t _p)] (10)

Λ _P-λ＝arccos[(cosψ-sinδsinΦ _P)/cosδcosΦ _P] (11)

Wherein τ is the moment of satellite process pericenter, and a represents the major semi-axis of elliptical orbit, and e represents orbital eccentricity, ω is argument of perigee, and i is orbit inclination, and Ω represents the red footpath of ascending node, above six parameter general name satellite orbit six key elements will have overall design to provide.μ represents gravitational field gravitational constant, ω _eBe earth spin rotating speed, ω _e=7.2921158 * 10 ^-5Rad/s, G ₀Be t _pThe sidereal hour angle of moment Greenwich, Λ _P, Φ _PRepresent respectively geocentric longitude and geocentric latitude that terrain object P is ordered, above-mentioned parameter is known quantity.δ, λ represent respectively t ₀Geocentric latitude and the geocentric latitude of moment substar, ψ is substar N _SAnd the earth's core angle between the impact point P, E represent inclined to one side pericenter angle, and φ represents true pericenter angle, and these parameters are unknown quantity, can find the solution by above-mentioned system of equations.Formula (7) is for describing the Kepler's equation of satellite position and time relationship, and formula (8) represents the relation at very near heart angle and partially near heart angle, and formula (9-11) is set up according to the spherical trigonometry relation, specifically can be referring to Fig. 5.O represents the earth centre of sphere among the figure, and N represents the earth's axis arctic, and G represents Greenwich meridian and equatorial node, and D represents the perigee, S _mBe satellite position, P is t ₀The ground aiming point at moment antenna beam center, N _SBe substar.

Utilize numerical computation method can find the solution above-mentioned system of equations, obtain satellite Covering time t ₀

Substar N _SAnd the earth's core angle ψ computing method between the impact point P are as follows:

$\mathrm{\&psi;}=\arcsin \left(\frac{a}{R_e}\sin {\mathrm{\&theta;}}_A\right)---\left(12\right)$

R wherein _eRepresent local earth radius, θ _AExpression antenna beam centre visual angle.

Second step calculates the main antenna wave beam at the coverage condition on ground, obtains the longitude and latitude of the ground aiming point of beam center, near-end wave beam line and far-end wave beam line, and calculates mapping swath width, specifically is calculated as:

If the main antenna centre visual angle is θ _A, distance is Δ θ to beam angle _Ar,

(2.1) the longitude Λ of calculating main antenna beam center aiming point ₀With latitude Φ ₀

At first utilize following formula Calculation of Satellite pole of orbit radius vector r:

$r=\frac{a(1-e^2)}{1-e\cos \mathrm{\&phi;}}---\left(13\right)$

Can calculate t thus ₀Satellite is at earth inertial coordinates system E constantly _OIn position (x _Os, y _Os, z _Os), shown in (14):

$\left(\begin{array}{c}{x}_{\mathrm{os}}\\ y_{\mathrm{os}}\\ z_{\mathrm{os}}\end{array}\right)=A_{\mathrm{OV}}\&CenterDot;\left(\begin{array}{c}r\cos \mathrm{\&phi;}\\ r\sin \mathrm{\&phi;}\\ 0\end{array}\right)---\left(14\right)$

A wherein _OVBe satellite orbit coordinate system E _VTo earth inertial coordinates system E _OTransition matrix.

Then set up main antenna coordinate system E _AMiddle any point (x _a, y _a, z _a) at body-fixed coordinate system E _GIn coordinate.Because the Y-axis of antenna coordinate system overlaps with antenna boresight, so the main antenna aiming point is at coordinate system E _AIn coordinate be (0, y, 0), aiming point is at body-fixed coordinate system E _GIn coordinate (x _Go, y _Go, z _Go) be:

$\left(\begin{array}{c}{x}_{\mathrm{go}}\\ y_{\mathrm{go}}\\ z_{\mathrm{go}}\end{array}\right)=A_{\mathrm{GO}}{A}_{\mathrm{OV}}{A}_{\mathrm{VR}}{A}_{\mathrm{RE}}{A}_{\mathrm{EA}}\left(\begin{array}{c}0\\ y\\ 0\end{array}\right)+A_{\mathrm{GO}}\left(\begin{array}{c}{x}_{\mathrm{os}}\\ y_{\mathrm{os}}\\ z_{\mathrm{os}}\end{array}\right)+A_{\mathrm{GO}}{A}_{\mathrm{OV}}{A}_{\mathrm{VR}}{A}_{\mathrm{RE}}\left(\begin{array}{c}{x}_e\\ y_e\\ z_e\end{array}\right)---\left(15\right)$

(x wherein _e, y _e, z _e) be that antenna phase center is with respect to satellite celestial body coordinate system E _EPosition vector, (x _Os, y _Os, z _Os) for satellite at earth inertial coordinates system E _OIn position vector, A _GOEarth inertial coordinates system E _OTo body-fixed coordinate system E _GTransition matrix, A _OVSatellite orbit coordinate system E _VTo earth inertial coordinates system E _OTransition matrix, A _VRSatellite platform coordinate system E _RTo satellite orbit coordinate system E _VTransition matrix, A _RESatellite celestial body coordinate system E _ETo satellite platform coordinate system E _RSatellite platform coordinate system E _RTransition matrix, A _EATo be θ by the main antenna centre visual angle _AThe antenna coordinate of determining is tied to satellite celestial body coordinate system E _ETransition matrix.With (x _Go, y _gO, z _Go) substitution ellipsoid model of globe equation:

$\frac{x_{\mathrm{go}}^2}{E_a^2}+\frac{y_{\mathrm{go}}^2}{E_a^2}+\frac{z_{\mathrm{go}}^2}{{\mathrm{<figure-callout\; id="2"\; label="E\; b"\; filenames="HDA0000065297460000062.png,HDA0000065297460000071.png"\; state="\{\{state\}\}">E</figure-callout>}}_b^{}}=1---\left(16\right)$

E wherein _aAnd E _bBe respectively major semi-axis and the minor semi-axis of earth's spheroid.Solve an equation and to try to achieve y (get less in two solutions, cast out larger solution), can obtain aiming point at body-fixed coordinate system E simultaneously _GIn coordinate (x _Go, y _Go, z _Go), aiming point longitude Λ is then arranged ₀For:

$\tan {\mathrm{\&Lambda;}}_0=\frac{y_{\mathrm{go}}}{x_{\mathrm{go}}}---\left(17\right)$

Aiming point latitude Φ ₀For:

$\sin {\mathrm{\&Phi;}}_0=\frac{z_{\mathrm{go}}}{\sqrt{x_{\mathrm{go}}^2+y_{\mathrm{go}}^2+z_{\mathrm{go}}^2}}---\left(18\right)$

(2.2) longitude and latitude (Λ of the ground aiming point of calculating main antenna near-end wave beam line _N, Φ _N), the longitude and latitude (Λ of the ground aiming point of far-end wave beam line _F, Φ _F);

The longitude of near-end wave beam line ground aiming point is:

$\tan {\mathrm{\&Lambda;}}_N=\frac{y_{\mathrm{go}}^N}{x_{\mathrm{go}}^N}---\left(19\right)$

The latitude of near-end wave beam line ground aiming point is:

$\sin {\mathrm{\&Phi;}}_N=\frac{z_{\mathrm{go}}^N}{\sqrt{{\left(x_{\mathrm{go}}^N\right)}^2+{\left(y_{\mathrm{go}}^N\right)}^2+{\left(z_{\mathrm{go}}^N\right)}^2}}---\left(20\right)$

Wherein

That the ground aiming point of main antenna near-end wave beam line is at body-fixed coordinate system E _GIn coordinate vector, the computation process of its computation process and main antenna beam center aiming point is similar, difference is for calculating transition matrix A _EAAntenna look angle, use main antenna centre visual angle θ in the step (2.1) _A, use the near-end view angle theta herein _AN, θ as shown in Figure 6 _AN=θ _A-Δ θ _Ar/ 2.

The longitude of far-end wave beam line ground aiming point is:

$\tan {\mathrm{\&Lambda;}}_F=\frac{y_{\mathrm{go}}^F}{x_{\mathrm{go}}^F}---\left(21\right)$

The latitude of far-end wave beam line ground aiming point is:

$\sin {\mathrm{\&Phi;}}_F=\frac{z_{\mathrm{go}}^F}{\sqrt{{\left(x_{\mathrm{go}}^F\right)}^2+{\left(y_{\mathrm{go}}^F\right)}^2+{\left(z_{\mathrm{go}}^F\right)}^2}}---\left(22\right)$

Wherein That the ground aiming point of main antenna far-end wave beam line is at body-fixed coordinate system E _GIn coordinate vector, the computation process of its computation process and main antenna beam center aiming point is similar, difference is for calculating transition matrix A _EAAntenna look angle, use main antenna centre visual angle θ in the step (2.1) _A, use the far-end view angle theta herein _AF, θ as shown in Figure 6 _AF=θ _A+ Δ θ _Ar/ 2.

(2.3) cross the width W that the constantly calculation of longitude ﹠ latitude mapping of the ground aiming point of corresponding antenna proximal end wave beam line and far-end wave beam line of top is with according to satellite:

W＝ψ _NF·R _e (23)

ψ wherein _NFCorresponding the earth's core angle between the ground aiming point for antenna proximal end wave beam line and far-end wave beam line.

Can obtain ψ according to spherical trigonometry relation among Fig. 5 _NFComputing formula:

ψ _NF＝arccos[sin(Φ _N)sin(Φ _F)+cos(Φ _N)cos(Φ _F)cos(Λ _F-Λ _N)] (24)

The 3rd step, utilize mapping swath width W that second step tries to achieve and satellite system parameter for InSAR system made sensitivity matrix, described satellite system parameter comprises satellite altitude H, base length B, baseline inclination angle theta _bAccording to the constraint condition that scaler is laid, to try to achieve scaler and lay parameter, the described parameter that lays comprises distance d between scaler number L, first scaler and the substar ₁And the distance interval delta d between the scaler, it is as follows that scaler lays the calculation of parameter step:

(3.1) set up the sensitivity matrix F of spaceborne double antenna interference SAR:

Wherein

The ground elevation f at expression the i scaler place is to the susceptibility of interferometric parameter X, and described interferometric parameter X comprises satellite altitude H, main antenna oblique distance r ₁, base length B, baseline inclination angle theta _bAnd interferometric phase

(illustrate: In follow-up formula, be not used for calculating, only be used for

The expression of this symbol.)

$\frac{\&PartialD;f}{\&PartialD;H}=\frac{H+R_e-{\mathrm{<figure-callout\; id="1"\; label="r"\; filenames="HDA0000065297460000031.png,HDA0000065297460000071.png"\; state="\{\{state\}\}">r</figure-callout>}}_1\cos \mathrm{\&theta;}}{\sqrt{{(H+R_e)}^2+{{\mathrm{<figure-callout\; id="1"\; label="r"\; filenames="HDA0000065297460000031.png,HDA0000065297460000071.png"\; state="\{\{state\}\}">r</figure-callout>}}_1}^2-2(H+R_e){\mathrm{<figure-callout\; id="1"\; label="r"\; filenames="HDA0000065297460000031.png,HDA0000065297460000071.png"\; state="\{\{state\}\}">r</figure-callout>}}_1\cos \mathrm{\&theta;}}}---\left(26\right)$

$\frac{\&PartialD;f}{\&PartialD;{\mathrm{<figure-callout\; id="1"\; label="r"\; filenames="HDA0000065297460000031.png,HDA0000065297460000071.png"\; state="\{\{state\}\}">r</figure-callout>}}_1}=\frac{1}{R_e+h}\{(R_e+H)\&CenterDot;[\frac{({\mathrm{\&Delta;r}}^2-B^2)\sin \mathrm{\&theta;}}{2{\mathrm{<figure-callout\; id="1"\; label="Br"\; filenames="HDA0000065297460000031.png,HDA0000065297460000071.png"\; state="\{\{state\}\}">Br</figure-callout>}}_1\cos (\mathrm{\&theta;}-{\mathrm{\&theta;}}_b)}-\cos \mathrm{\&theta;}]+r_1\}---\left(27\right)$

$\frac{\&PartialD;f}{\&PartialD;B}=\frac{(H+R_e)\&CenterDot;({\mathrm{<figure-callout\; id="2"\; label="B"\; filenames="HDA0000065297460000062.png,HDA0000065297460000071.png"\; state="\{\{state\}\}">B</figure-callout>}}^2+{2\mathrm{<figure-callout\; id="1"\; label="r"\; filenames="HDA0000065297460000031.png,HDA0000065297460000071.png"\; state="\{\{state\}\}">r</figure-callout>}}_1\&CenterDot;\mathrm{\&Delta;r}+{\mathrm{\&Delta;r}}^2)\sin \mathrm{\&theta;}}{2(R_e+h){\mathrm{<figure-callout\; id="2"\; label="B"\; filenames="HDA0000065297460000062.png,HDA0000065297460000071.png"\; state="\{\{state\}\}">B</figure-callout>}}^2\cos (\mathrm{\&theta;}-{\mathrm{\&theta;}}_b)}---\left(28\right)$

$\frac{\&PartialD;f}{\&PartialD;{\mathrm{\&theta;}}_b}=\frac{(H+R_e)\&CenterDot;{\mathrm{<figure-callout\; id="1"\; label="r"\; filenames="HDA0000065297460000031.png,HDA0000065297460000071.png"\; state="\{\{state\}\}">r</figure-callout>}}_1\sin \mathrm{\&theta;}}{R_e+h}---\left(29\right)$

Wherein Re is local earth radius, and h is the height that scaler place terrain object arrives the earth ellipsoid face, and θ is main antenna visual angle corresponding to scaler place, and Δ r is that the major-minor antenna is poor to the oblique distance of terrain object.

(3.2) be located at the interior edge of mapping band distance to uniformly-spaced laying L scaler, change the distance d between first scaler and the substar ₁And the distance interval delta d between each scaler, adopt numerical analysis method to calculate (L, d ₁, Δ d), under the condition that satisfies formula (31), make conditional number C (F) minimum of sensitivity matrix F.

$\left\{\begin{array}{c}{D}_N\&le;{\mathrm{<figure-callout\; id="1"\; label="d"\; filenames="HDA0000065297460000031.png,HDA0000065297460000071.png"\; state="\{\{state\}\}">d</figure-callout>}}_1<D_N+W/2\\ \max (\frac{D_F+D_N-2{\mathrm{<figure-callout\; id="1"\; label="d"\; filenames="HDA0000065297460000031.png,HDA0000065297460000071.png"\; state="\{\{state\}\}">d</figure-callout>}}_1}{2(L-1)},{\mathrm{\&Delta;d}}_{\min })<\mathrm{\&Delta;d}\&le;\frac{D_F-d_1}{L-1}\end{array}\right.---\left(31\right)$

D wherein _NExpression mapping band near-end distance, D _FExpression mapping band distal end distance, Δ d _MinHave at least in the expression (26-30) one can not carry out at the scaling point place that linearization represents minimally apart from the interval.

The 4th goes on foot, and calculates the longitude and latitude of each scaler;

(4.1) according to the 3rd distance d that goes on foot between scaler number L, first scaler and the substar of obtaining ₁And the distance interval delta d between the scaler, calculate each scaler at satellite synchronization scene coordinate system E _SSIn position vector;

If the distance of L scaler is respectively d _i, i=1 ..., L, i.e. i scaler shown in Fig. 7 and substar N _SBetween arc length, then each scaler is at satellite synchronization scene coordinate system E _SSIn position vector be V _SS=(0, d _i-d ₀, 0), i=1 ..., L, wherein d ₀Be the ground aiming point of main antenna beam center and the distance between the substar, i.e. P shown in Fig. 7 and N _SBetween arc length, computation process is as follows:

d ₀＝ψ ₀·R _e (32)

ψ wherein ₀Be the earth's core angle between beam center ground aiming point and the substar, can do following calculating according to the spherical trigonometry relation:

ψ ₀＝arccos[sin(Φ ₀)sin(δ)+cos(Φ ₀)cosδcos(Λ ₀-λ)] (33)

(4.2) with scaler at satellite synchronization scene coordinate system E _SSIn position vector be transformed into earth synchronization scenarios coordinate system E _SEIn,

V _SE＝A _ESV _SS (34)

A wherein _ESFor by satellite synchronization scene coordinate system E _SSTo earth synchronization scenarios coordinate system E _SETransition matrix.

(4.3) each scaler position coordinates is transformed into body-fixed coordinate system E _GIn, and then calculate the longitude and latitude of each scaler, process is as follows,

$\left(\begin{array}{c}{x}_{\mathrm{gi}}\\ y_{\mathrm{gi}}\\ z_{\mathrm{gi}}\end{array}\right)=A_{\mathrm{GS}}\left(\begin{array}{c}{x}_{\mathrm{ss},i}\\ y_{\mathrm{ss},i}\\ z_{\mathrm{ss},i}\end{array}\right),i=1,\&CenterDot;\&CenterDot;\&CenterDot;,L---\left(35\right)$

A _GSBe corresponding transition matrix, the longitude of i scaler and latitude are respectively suc as formula (36) and (37):

$\tan {\mathrm{\&Lambda;}}_{\mathrm{GCP},i}=\frac{y_{\mathrm{gi}}}{x_{\mathrm{gi}}},i=1,\&CenterDot;\&CenterDot;\&CenterDot;,L---\left(36\right)$

$\sin {\mathrm{\&Phi;}}_{\mathrm{GCP},i}=\frac{z_{\mathrm{<figure-callout\; id="2"\; label="gi\; x\; gi"\; filenames="HDA0000065297460000062.png,HDA0000065297460000071.png"\; state="\{\{state\}\}">gi</figure-callout>}}}{\sqrt{x_{\mathrm{gi}}^{}}},i=1,\&CenterDot;\&CenterDot;\&CenterDot;,L---\left(37\right)$

The present invention's advantage compared with prior art is:

(1) the present invention combines the overall system design parameter with the sensitivity matrix analysis, makes the overall design of spaceborne double antenna interference SAR and interferes calibration to combine and study, can the sophisticated systems performance evaluation, and the optimization system design.

(2) the present invention is based on satellite orbit parameter and SAR systematic parameter to interfering calibration to be analyzed, adopted ellipsoid earth model and perfect coordinate-system, can carry out calibration analysis for each latitude zone, the whole world, and obtain the concrete latitude and longitude information of scaler.

(3) the present invention carries out satellite beams covering and calibration analysis under perfect coordinate system framework, overall design, interfere that processing, interference are calibrated etc. can be carried out comprehensive simulating and verify.

Description of drawings

Fig. 1 is the geometric relationship figure of spaceborne interferometric SAR system;

Fig. 2 is for interfering the theory diagram of calibration;

Fig. 3 is spaceborne double antenna interference SAR space geometry graph of a relation;

Fig. 4 is the graph of a relation of earth synchronization scenarios coordinate system and satellite synchronization scene coordinate system;

Fig. 5 is that satellite covers and the comprehensive schematic diagram of orbital elements;

Fig. 6 is satellite-borne SAR wave beam coverage diagram;

Fig. 7 is that scaler lays schematic diagram;

Fig. 8 is the realization flow figure of the inventive method;

Fig. 9 a-Fig. 9 e is the curve map that each interferometric parameter susceptibility changes with distance;

Figure 10 is d ₁Interfere the sensitivity matrix conditional number with the curve map of adjacent scaler interval variation under the fixing situation;

Figure 11 interferes the minimal condition number of sensitivity matrix with d in the certain situation of scaler number ₁The curve map that changes;

Figure 12 is the curve map that sensitivity matrix minimal condition number changes with the scaler number.

Symbolic representation is as follows among the figure: S among Fig. 1 _m, S _sRepresent respectively two SAR antennas on the satellite, S _mBe main antenna, S _sBe slave antenna, B represents the length of baseline, θ _bBe the baseline inclination angle, θ is antenna look angle corresponding to terrain object point, and H is satellite altitude, R _eBe local earth radius, r ₁, r ₂Represent that respectively two antenna phase centers are to the oblique distance of terrain object point, h _InSARThe earth's core distance for impact point.V among Fig. 3 _sBe satellite velocity vector, camber line T ₁T ₂T ₃Be the ground trace of sub-satellite point, A, B are respectively far-end and the near-end of observation band.N represents the earth's axis arctic among Fig. 5, and G represents Greenwich meridian and equatorial node, S _mBe satellite position, P is the ground aiming point at antenna beam center, N _SBe substar, Λ _P, Φ _PRepresent respectively longitude and latitude that P is ordered, δ represents the latitude of sub-satellite point, and E represents inclined to one side pericenter angle, and φ represents true pericenter angle, and Ω represents the red footpath of ascending node, and ω is argument of perigee.Δ θ among Fig. 6 _ArRepresent the main antenna distance to beam angle, R _nBe mapping band near-end oblique distance, R _fBe far-end oblique distance, R _MidBe the oblique distance at beam center place, W is mapping swath width, Λ ₀, Φ ₀Be respectively longitude and the latitude of ground aiming point.D among Fig. 7 _iBe i the distance that scaler is corresponding.

Embodiment

The below utilizes concrete spaceborne double antenna InSAR parameter to test to verify that the spaceborne double antenna InSAR of comprehensive population parameter interferes scaler to lay the validity of method.

Table 1 has provided the orbit parameter of satellite, and table 2 has provided main SAR systematic parameter.

Table 1 satellite orbit parameter

Satellite orbit parameter	Numerical value
		Semi-major axis of orbit a/km	6886.856
Orbital eccentricity e	0.000726
		Orbit inclination i/ °	97.63898
Argument of pericentre ω/°	209.6589
		The red footpath Ω of ascending node/°	218.8837
Time of pericenter passage τ/s	0.0

Table 2 SAR systematic parameter

Systematic parameter	Numerical value
		Signal wavelength lambda/m	0.03
The main antenna view angle theta A/°	28.4
		Beam angle/°	7.3
Base length B/m	200.0
		The baseline inclination angle theta b/°	45.0

As shown in Figure 8, the present invention's step when the spaceborne double antenna InSAR of analysis interferes scaler to lay rule is as follows:

Step (1): zone to be analyzed is equator, and establishing latitude is north latitude 0.25 degree, can be 1347.26 seconds in the hope of the satellite Covering time according to formula (7)-(11).

Step (2.1): according to the satellite Covering time, orbital elements, SAR systematic parameter are tried to achieve the aiming point longitude and latitude of main antenna beam center on ground according to formula (13-18) and are (0.248088 ° ,-64.158359 °);

Step (2.2): distance is to beam angle Δ θ _Ar=7.3 °, near-end antenna look angle θ _AN=24.75 °, far-end antenna look angle θ _AF=32.05 °, calculate the intersection point longitude and latitude on antenna beam near-end and far-end and ground according to formula (19-22), be respectively:

(Λ _N，Φ _N)＝(-64.366509°，0.285488°)

(Λ _F，Φ _F)＝(-63.933913°，0.207757°)

Step (2.3): with the above results substitution formula (23) and (24), calculating mapping swath width W is 48.9275Km.

Step 3: the susceptibility of at first analyzing spaceborne double antenna interference SAR according to formula (26-30), provide its sensitivity curve, shown in Fig. 9 a-Fig. 9 e, select accordingly main interferometric parameter and carry out calibration analysis, can find out that by the sensitivity curve that Fig. 9 a-Fig. 9 e provides the interference survey is high very little to the satellite altitude susceptibility, main interferometric parameter is main antenna oblique distance, base length, baseline inclination angle and interferometric phase.

To different scaler numbers (here from L=2), utilize formula (25-30) to set up sensitivity matrix, be optimized calculating according to formula (31), try to achieve minimal condition corresponding to each L value and count C _L(F), L=2 ..., 30 and corresponding d ₁With Δ d value.Figure 10 and Figure 11 have provided respectively the sensitivity matrix conditional number with Δ d and d ₁Change curve, can draw accordingly in the situation that the scaler number is certain, scaler distributes overstepping the bounds of propriety loose along mapping band, the sensitivity matrix conditional number is less, namely near the low coverage end, each scaler is evenly distributed in the whole mapping band first scaler as far as possible as far as possible.

Choose C _L(F), L=2 ..., the minimum value C in 30 _Min(F), its corresponding scaler number is L _Opt, L _OptCorresponding allocation optimum is d _{1, opt}With Δ d _Opt, the scaler that obtains thus optimum lays and is configured to (L _Opt, d _{1, opt}, Δ d _Opt).Figure 12 has provided the change curve of sensitivity matrix minimal condition number with the scaler number, and can draw the scaler number by figure is that 8 o'clock sensitivity matrix conditional numbers are minimum, so L _Opt=8.This moment d ₁Be 134.474Km, Δ d is 6115.9m.Can get allocation optimum is:

L _opt＝8

d _1，opt＝134.474Km

Δd _opt＝6115.9m

Step (4.1): the distance that can be calculated main antenna beam center ground aiming point place by population parameter and coordinate system translation operation is 158.0162Km, i.e. d ₀=158.0162km, then the position vector of each scaling point in satellite synchronization scene coordinate system is as shown in table 3.

Table 3 scaling point is position vector in satellite synchronization scene coordinate system

The scaling point sequence number	Position vector/m
		1	(0，-23542.10，0)
2	(0，-16552.47，0)
		3	(0，-9562.84，0)
4	(0，-2573.21，0)
		5	(0，4416.41，0)
6	(0，11406.04，0)
		7	(0，18395.67，0)
8	(0，25385.30，0)

Step (4.2) and (4.3): the angle of Calculation of Satellite velocity and due east direction, and then try to achieve the transition matrix A that arrives earth synchronization scenarios coordinate system in the satellite synchronization scene coordinate system _ES, recycling formula (34-37) is calculated the latitude and longitude information of each scaler, and is as shown in table 4.

Table 4 scaler latitude and longitude information

The scaling point sequence number	(longitude/°, latitude/°)
		1	(-64.366509，0.255488)
2	(-64.304710，0.248669)
		3	(-64.242910，0.241851)
4	(-64.181111，0.235032)

5	(-64.119311，0.228213)
		6	(-64.057512，0.221394)
7	(-63.995712，0.214576)
		8	(-63.933913，0.207757)

In a word, the present invention combines the design of the population parameters such as satellite orbit parameter and radar system parameter with interference calibrating method based on the sensitivity matrix analysis, provided spaceborne double antenna interference SAR scaler and laid method.Carry out the satellite covering analyzing based on population parameter, give and interfere calibration that necessary data message is provided, and then set up spaceborne double antenna interference SAR sensitivity matrix, lay scheme according to interfering the high constraint condition analysis to the sensitivity matrix conditional number of survey to obtain optimum scaler.The present invention combines overall design and interference calibration, and can in overall design, take into full account and interfere calibration to the improvement of system performance, and for interfering the Project Realization of calibrating that reference is provided.By above-mentioned test, can obtain optimum scaler number, lay the interval and specifically lay the position, validity of the present invention has been described.

The non-elaborated part of the present invention belongs to techniques well known.

Claims (3)

1. The method for laying the spaceborne dual-antenna SAR interferometric scaler of comprehensive overall parameters is characterized in that the realization steps are as follows: The first step is to solve the satellite overhead moment t ₀ ; The second step is to calculate the coverage of the main antenna beam on the ground, obtain the latitude and longitude of the ground aiming point of the beam center, the near-end beamline and the far-end beamline, and calculate the width of the surveying swath. The specific calculation is: (2.1) Calculate the longitude Λ ₀ and latitude Φ ₀ of the aiming point of the main antenna beam center; The longitude _Λ0 of the aiming point is: $\mathrm{<span\; class="notranslate">\; the\; tan</span>}{\mathrm{<span\; class="notranslate">\; \&Lambda;</span>}}_{\mathrm{<span\; class="notranslate">\; 0</span>}}<span\; class="notranslate">\; =</span>\frac{{\mathrm{<span\; class="notranslate">\; the\; y</span>}}_{\mathrm{<span\; class="notranslate">\; go</span>}}}{{\mathrm{<span\; class="notranslate">\; x</span>}}_{\mathrm{<span\; class="notranslate">\; go</span>}}}<span\; class="notranslate">\; -</span><span\; class="notranslate">\; -</span><span\; class="notranslate">\; -</span><span\; class="notranslate">\; (</span>\mathrm{<span\; class="notranslate">\; 17</span>}<span\; class="notranslate">\; )</span>$ The latitude Φ ₀ of the aiming point is: $\mathrm{<span\; class="notranslate">\; sin</span>}{\mathrm{<span\; class="notranslate">\; \&Phi;</span>}}_{\mathrm{<span\; class="notranslate">\; 0</span>}}<span\; class="notranslate">\; =</span>\frac{{\mathrm{<span\; class="notranslate">\; z</span>}}_{\mathrm{<span\; class="notranslate">\; go</span>}}}{\sqrt{{\mathrm{<span\; class="notranslate">\; x</span>}}_{\mathrm{<span\; class="notranslate">\; go</span>}}^{\mathrm{<span\; class="notranslate">\; 2</span>}}<span\; class="notranslate">\; +</span>{\mathrm{<span\; class="notranslate">\; the\; y</span>}}_{\mathrm{<span\; class="notranslate">\; go</span>}}^{\mathrm{<span\; class="notranslate">\; 2</span>}}<span\; class="notranslate">\; +</span>{\mathrm{<span\; class="notranslate">\; z</span>}}_{\mathrm{<span\; class="notranslate">\; go</span>}}^{\mathrm{<span\; class="notranslate">\; 2</span>}}}}<span\; class="notranslate">\; -</span><span\; class="notranslate">\; -</span><span\; class="notranslate">\; -</span><span\; class="notranslate">\; (</span>\mathrm{<span\; class="notranslate">\; 18</span>}<span\; class="notranslate">\; )</span>$ Wherein (x _go , y _go , z _go ) are the coordinates of the aiming point in the ground-fixed coordinate system E _G ; (2.2) Calculate the latitude and longitude (Λ _N , Φ _N ) of the ground aiming point of the near-end beamline of the main antenna, and the latitude and longitude (Λ _F , Φ _F ) of the ground aiming point of the far-end beamline; The longitude of the near beamline ground aiming point is: $\mathrm{<span\; class="notranslate">\; the\; tan</span>}{\mathrm{<span\; class="notranslate">\; \&Lambda;</span>}}_{\mathrm{<span\; class="notranslate">\; N</span>}}<span\; class="notranslate">\; =</span>\frac{{\mathrm{<span\; class="notranslate">\; the\; y</span>}}_{\mathrm{<span\; class="notranslate">\; go</span>}}^{\mathrm{<span\; class="notranslate">\; N</span>}}}{{\mathrm{<span\; class="notranslate">\; x</span>}}_{\mathrm{<span\; class="notranslate">\; go</span>}}^{\mathrm{<span\; class="notranslate">\; N</span>}}}<span\; class="notranslate">\; -</span><span\; class="notranslate">\; -</span><span\; class="notranslate">\; -</span><span\; class="notranslate">\; (</span>\mathrm{<span\; class="notranslate">\; 19</span>}<span\; class="notranslate">\; )</span>$ The latitude of the near-end beamline ground aiming point is: $\mathrm{<span\; class="notranslate">\; sin</span>}{\mathrm{<span\; class="notranslate">\; \&Phi;</span>}}_{\mathrm{<span\; class="notranslate">\; N</span>}}<span\; class="notranslate">\; =</span>\frac{{\mathrm{<span\; class="notranslate">\; z</span>}}_{\mathrm{<span\; class="notranslate">\; go</span>}}^{\mathrm{<span\; class="notranslate">\; N</span>}}}{\sqrt{{<span\; class="notranslate">\; (</span>{\mathrm{<span\; class="notranslate">\; x</span>}}_{\mathrm{<span\; class="notranslate">\; go</span>}}^{\mathrm{<span\; class="notranslate">\; N</span>}}<span\; class="notranslate">\; )</span>}^{\mathrm{<span\; class="notranslate">\; 2</span>}}<span\; class="notranslate">\; +</span>{<span\; class="notranslate">\; (</span>{\mathrm{<span\; class="notranslate">\; the\; y</span>}}_{\mathrm{<span\; class="notranslate">\; go</span>}}^{\mathrm{<span\; class="notranslate">\; N</span>}}<span\; class="notranslate">\; )</span>}^{\mathrm{<span\; class="notranslate">\; 2</span>}}<span\; class="notranslate">\; +</span>{<span\; class="notranslate">\; (</span>{\mathrm{<span\; class="notranslate">\; z</span>}}_{\mathrm{<span\; class="notranslate">\; go</span>}}^{\mathrm{<span\; class="notranslate">\; N</span>}}<span\; class="notranslate">\; )</span>}^{\mathrm{<span\; class="notranslate">\; 2</span>}}}}<span\; class="notranslate">\; -</span><span\; class="notranslate">\; -</span><span\; class="notranslate">\; -</span><span\; class="notranslate">\; (</span>\mathrm{<span\; class="notranslate">\; 20</span>}<span\; class="notranslate">\; )</span>$ in

is the coordinate vector of the ground aiming point of the near-end beamline of the main antenna in the ground-fixed coordinate system E _G ; The longitude of the ground aiming point on the far end beamline is: $\mathrm{<span\; class="notranslate">\; the\; tan</span>}{\mathrm{<span\; class="notranslate">\; \&Lambda;</span>}}_{\mathrm{<span\; class="notranslate">\; f</span>}}<span\; class="notranslate">\; =</span>\frac{{\mathrm{<span\; class="notranslate">\; the\; y</span>}}_{\mathrm{<span\; class="notranslate">\; go</span>}}^{\mathrm{<span\; class="notranslate">\; f</span>}}}{{\mathrm{<span\; class="notranslate">\; x</span>}}_{\mathrm{<span\; class="notranslate">\; go</span>}}^{\mathrm{<span\; class="notranslate">\; f</span>}}}<span\; class="notranslate">\; -</span><span\; class="notranslate">\; -</span><span\; class="notranslate">\; -</span><span\; class="notranslate">\; (</span>\mathrm{<span\; class="notranslate">\; twenty\; one</span>}<span\; class="notranslate">\; )</span>$ The latitude of the far end beamline ground aiming point is: $\mathrm{<span\; class="notranslate">\; sin</span>}{\mathrm{<span\; class="notranslate">\; \&Phi;</span>}}_{\mathrm{<span\; class="notranslate">\; f</span>}}<span\; class="notranslate">\; =</span>\frac{{\mathrm{<span\; class="notranslate">\; z</span>}}_{\mathrm{<span\; class="notranslate">\; go</span>}}^{\mathrm{<span\; class="notranslate">\; f</span>}}}{\sqrt{{<span\; class="notranslate">\; (</span>{\mathrm{<span\; class="notranslate">\; x</span>}}_{\mathrm{<span\; class="notranslate">\; go</span>}}^{\mathrm{<span\; class="notranslate">\; f</span>}}<span\; class="notranslate">\; )</span>}^{\mathrm{<span\; class="notranslate">\; 2</span>}}<span\; class="notranslate">\; +</span>{<span\; class="notranslate">\; (</span>{\mathrm{<span\; class="notranslate">\; the\; y</span>}}_{\mathrm{<span\; class="notranslate">\; go</span>}}^{\mathrm{<span\; class="notranslate">\; f</span>}}<span\; class="notranslate">\; )</span>}^{\mathrm{<span\; class="notranslate">\; 2</span>}}<span\; class="notranslate">\; +</span>{<span\; class="notranslate">\; (</span>{\mathrm{<span\; class="notranslate">\; z</span>}}_{\mathrm{<span\; class="notranslate">\; go</span>}}^{\mathrm{<span\; class="notranslate">\; f</span>}}<span\; class="notranslate">\; )</span>}^{\mathrm{<span\; class="notranslate">\; 2</span>}}}}<span\; class="notranslate">\; -</span><span\; class="notranslate">\; -</span><span\; class="notranslate">\; -</span><span\; class="notranslate">\; (</span>\mathrm{<span\; class="notranslate">\; twenty\; two</span>}<span\; class="notranslate">\; )</span>$ in is the coordinate vector of the ground aiming point of the main antenna's far-end beamline in the ground-fixed coordinate system E _G ; (2.3) Calculate the width W of the surveying strip according to the latitude and longitude of the ground aiming point of the near-end beamline and the far-end beamline of the antenna corresponding to the moment when the satellite passes over the top, W＝ _ΨNF ·R _e (23) where R _e represents the local radius of the earth; Ψ _NF is the angle between the ground aiming points of the near-end beamline and the far-end beamline of the antenna corresponding to the center of the earth: Ψ _NF ＝arccos[sin(Φ _N )sin(Φ _F )+cos(Φ _N )cos(Φ _F )cos(Λ _F -Λ _N )] (24) In the third step, the sensitivity matrix is established for the spaceborne dual-antenna SAR by using the surveying swath width W obtained in the second step and the satellite system parameters. The satellite system parameters include the satellite height H, the baseline length B, and the baseline inclination angle θ _b ; according to For the constraints on the deployment of the scalers, the deployment parameters of the scalers are obtained, and the deployment parameters include the number of scalers L, the ground distance _d between the first scaler and the sub-satellite point, and The ground distance interval Δd between the scalers, and the calculation steps of the scaler layout parameters are as follows: (3.1) Establish the sensitivity matrix F of the spaceborne dual-antenna SAR,

in

Indicates the sensitivity of the ground elevation f at the i-th scaler to the interference parameter X, which includes the satellite height H, the main antenna slant distance r ₁ , the baseline length B, the baseline inclination angle θ _b and the interference phase

$\frac{<span\; class="notranslate">\; \&PartialD;</span>\mathrm{<span\; class="notranslate">\; f</span>}}{<span\; class="notranslate">\; \&PartialD;</span>\mathrm{<span\; class="notranslate">\; h</span>}}<span\; class="notranslate">\; =</span>\frac{\mathrm{<span\; class="notranslate">\; h</span>}<span\; class="notranslate">\; +</span>{\mathrm{<span\; class="notranslate">\; R</span>}}_{\mathrm{<span\; class="notranslate">\; e</span>}}<span\; class="notranslate">\; -</span>{\mathrm{<span\; class="notranslate">\; r</span>}}_{\mathrm{<span\; class="notranslate">\; 1</span>}}\mathrm{<span\; class="notranslate">\; cos</span>}\mathrm{<span\; class="notranslate">\; \&theta;</span>}}{\sqrt{{<span\; class="notranslate">\; (</span>\mathrm{<span\; class="notranslate">\; h</span>}<span\; class="notranslate">\; +</span>{\mathrm{<span\; class="notranslate">\; R</span>}}_{\mathrm{<span\; class="notranslate">\; e</span>}}<span\; class="notranslate">\; )</span>}^{\mathrm{<span\; class="notranslate">\; 2</span>}}<span\; class="notranslate">\; +</span>{\mathrm{<span\; class="notranslate">\; r</span>}}_{\mathrm{<span\; class="notranslate">\; 1</span>}}^{\mathrm{<span\; class="notranslate">\; 2</span>}}<span\; class="notranslate">\; -</span>\mathrm{<span\; class="notranslate">\; 2</span>}<span\; class="notranslate">\; (</span>\mathrm{<span\; class="notranslate">\; h</span>}<span\; class="notranslate">\; +</span>{\mathrm{<span\; class="notranslate">\; R</span>}}_{\mathrm{<span\; class="notranslate">\; e</span>}}<span\; class="notranslate">\; )</span>{\mathrm{<span\; class="notranslate">\; r</span>}}_{\mathrm{<span\; class="notranslate">\; 1</span>}}\mathrm{<span\; class="notranslate">\; cos</span>}\mathrm{<span\; class="notranslate">\; \&theta;</span>}}}<span\; class="notranslate">\; -</span><span\; class="notranslate">\; -</span><span\; class="notranslate">\; -</span><span\; class="notranslate">\; (</span>\mathrm{<span\; class="notranslate">\; 26</span>}<span\; class="notranslate">\; )</span>$ $\frac{<span\; class="notranslate">\; \&PartialD;</span>\mathrm{<span\; class="notranslate">\; f</span>}}{<span\; class="notranslate">\; \&PartialD;</span>{\mathrm{<span\; class="notranslate">\; r</span>}}_{\mathrm{<span\; class="notranslate">\; 1</span>}}}<span\; class="notranslate">\; =</span>\frac{\mathrm{<span\; class="notranslate">\; 1</span>}}{{\mathrm{<span\; class="notranslate">\; R</span>}}_{\mathrm{<span\; class="notranslate">\; e</span>}}<span\; class="notranslate">\; +</span>\mathrm{<span\; class="notranslate">\; h</span>}}<span\; class="notranslate">\; \{</span><span\; class="notranslate">\; (</span>{\mathrm{<span\; class="notranslate">\; R</span>}}_{\mathrm{<span\; class="notranslate">\; e</span>}}<span\; class="notranslate">\; +</span>\mathrm{<span\; class="notranslate">\; h</span>}<span\; class="notranslate">\; )</span><span\; class="notranslate">\; \&Center\; Dot;</span><span\; class="notranslate">\; [</span>\frac{<span\; class="notranslate">\; (</span>{\mathrm{<span\; class="notranslate">\; \&Delta;r</span>}}^{\mathrm{<span\; class="notranslate">\; 2</span>}}<span\; class="notranslate">\; -</span>{\mathrm{<span\; class="notranslate">\; B</span>}}^{\mathrm{<span\; class="notranslate">\; 2</span>}}<span\; class="notranslate">\; )</span>\mathrm{<span\; class="notranslate">\; sin</span>}\mathrm{<span\; class="notranslate">\; \&theta;</span>}}{\mathrm{<span\; class="notranslate">\; 2</span>}{\mathrm{<span\; class="notranslate">\; Br</span>}}_{\mathrm{<span\; class="notranslate">\; 1</span>}}\mathrm{<span\; class="notranslate">\; cos</span>}<span\; class="notranslate">\; (</span>\mathrm{<span\; class="notranslate">\; \&theta;</span>}<span\; class="notranslate">\; -</span>{\mathrm{<span\; class="notranslate">\; \&theta;</span>}}_{\mathrm{<span\; class="notranslate">\; b</span>}}<span\; class="notranslate">\; )</span>}<span\; class="notranslate">\; -</span>\mathrm{<span\; class="notranslate">\; cos</span>}\mathrm{<span\; class="notranslate">\; \&theta;</span>}<span\; class="notranslate">\; ]</span><span\; class="notranslate">\; +</span>{\mathrm{<span\; class="notranslate">\; r</span>}}_{\mathrm{<span\; class="notranslate">\; 1</span>}}<span\; class="notranslate">\; \}</span><span\; class="notranslate">\; -</span><span\; class="notranslate">\; -</span><span\; class="notranslate">\; -</span><span\; class="notranslate">\; (</span>\mathrm{<span\; class="notranslate">\; 27</span>}<span\; class="notranslate">\; )</span>$ $\frac{<span\; class="notranslate">\; \&PartialD;</span>\mathrm{<span\; class="notranslate">\; f</span>}}{<span\; class="notranslate">\; \&PartialD;</span>\mathrm{<span\; class="notranslate">\; B</span>}}<span\; class="notranslate">\; =</span>\frac{<span\; class="notranslate">\; (</span>\mathrm{<span\; class="notranslate">\; h</span>}<span\; class="notranslate">\; +</span>{\mathrm{<span\; class="notranslate">\; R</span>}}_{\mathrm{<span\; class="notranslate">\; e</span>}}<span\; class="notranslate">\; )</span><span\; class="notranslate">\; \&Center\; Dot;</span><span\; class="notranslate">\; (</span>{\mathrm{<span\; class="notranslate">\; B</span>}}^{\mathrm{<span\; class="notranslate">\; 2</span>}}<span\; class="notranslate">\; +</span>\mathrm{<span\; class="notranslate">\; 2</span>}{\mathrm{<span\; class="notranslate">\; r</span>}}_{\mathrm{<span\; class="notranslate">\; 1</span>}}<span\; class="notranslate">\; \&Center\; Dot;</span>\mathrm{<span\; class="notranslate">\; \&Delta;r</span>}<span\; class="notranslate">\; +</span>\mathrm{<span\; class="notranslate">\; \&Delta;</span>}{\mathrm{<span\; class="notranslate">\; r</span>}}^{\mathrm{<span\; class="notranslate">\; 2</span>}}<span\; class="notranslate">\; )</span>\mathrm{<span\; class="notranslate">\; sin</span>}\mathrm{<span\; class="notranslate">\; \&theta;</span>}}{\mathrm{<span\; class="notranslate">\; 2</span>}<span\; class="notranslate">\; (</span>{\mathrm{<span\; class="notranslate">\; R</span>}}_{\mathrm{<span\; class="notranslate">\; e</span>}}<span\; class="notranslate">\; +</span>\mathrm{<span\; class="notranslate">\; h</span>}<span\; class="notranslate">\; )</span>{\mathrm{<span\; class="notranslate">\; B</span>}}^{\mathrm{<span\; class="notranslate">\; 2</span>}}\mathrm{<span\; class="notranslate">\; cos</span>}<span\; class="notranslate">\; (</span>\mathrm{<span\; class="notranslate">\; \&theta;</span>}<span\; class="notranslate">\; -</span>{\mathrm{<span\; class="notranslate">\; \&theta;</span>}}_{\mathrm{<span\; class="notranslate">\; b</span>}}<span\; class="notranslate">\; )</span>}<span\; class="notranslate">\; -</span><span\; class="notranslate">\; -</span><span\; class="notranslate">\; -</span><span\; class="notranslate">\; (</span>\mathrm{<span\; class="notranslate">\; 28</span>}<span\; class="notranslate">\; )</span>$ $\frac{<span\; class="notranslate">\; \&PartialD;</span>\mathrm{<span\; class="notranslate">\; f</span>}}{<span\; class="notranslate">\; \&PartialD;</span>{\mathrm{<span\; class="notranslate">\; \&theta;</span>}}_{\mathrm{<span\; class="notranslate">\; b</span>}}}<span\; class="notranslate">\; =</span>\frac{<span\; class="notranslate">\; (</span>\mathrm{<span\; class="notranslate">\; h</span>}<span\; class="notranslate">\; +</span>{\mathrm{<span\; class="notranslate">\; R</span>}}_{\mathrm{<span\; class="notranslate">\; e</span>}}<span\; class="notranslate">\; )</span><span\; class="notranslate">\; \&Center\; Dot;</span>{\mathrm{<span\; class="notranslate">\; r</span>}}_{\mathrm{<span\; class="notranslate">\; 1</span>}}\mathrm{<span\; class="notranslate">\; sin</span>}\mathrm{<span\; class="notranslate">\; \&theta;</span>}}{{\mathrm{<span\; class="notranslate">\; R</span>}}_{\mathrm{<span\; class="notranslate">\; e</span>}}<span\; class="notranslate">\; +</span>\mathrm{<span\; class="notranslate">\; h</span>}}<span\; class="notranslate">\; -</span><span\; class="notranslate">\; -</span><span\; class="notranslate">\; -</span><span\; class="notranslate">\; (</span>\mathrm{<span\; class="notranslate">\; 29</span>}<span\; class="notranslate">\; )</span>$

in $R_e+h=\sqrt{{(h+R_e)}^2+r_1^2-2(h+R_e)r_1\cos \mathrm{\&theta;}},$ R _e is the local radius of the earth, h is the height from the ground target at the scaler to the ellipsoid of the earth, θ is the angle of view of the main antenna corresponding to the scaler, Δr is the slant distance difference between the main antenna and the secondary antenna to the ground target, and B is the baseline length, θ _b is the baseline inclination, H is the satellite height, r ₁ is the slant distance of the main antenna; (3.2) Assuming that L calibrators are arranged at equal intervals along the distance in the surveying zone, the ground distance d ₁ between the first calibrator and the sub-satellite point and the ground distance interval between the calibrators are changed Δd, using the numerical analysis method to calculate (L,d ₁ ,Δd), under the condition of satisfying the formula (31), the condition number C(F) of the sensitivity matrix F is minimized; $\left\{\begin{array}{c}{\mathrm{<span\; class="notranslate">\; D.</span>}}_{\mathrm{<span\; class="notranslate">\; N</span>}}<span\; class="notranslate">\; \&le;</span>{\mathrm{<span\; class="notranslate">\; d</span>}}_{\mathrm{<span\; class="notranslate">\; 1</span>}}<span\; class="notranslate">\; <</span>{\mathrm{<span\; class="notranslate">\; D.</span>}}_{\mathrm{<span\; class="notranslate">\; N</span>}}<span\; class="notranslate">\; +</span>\mathrm{<span\; class="notranslate">\; W</span>}<span\; class="notranslate">\; /</span>\mathrm{<span\; class="notranslate">\; 2</span>}\\ \mathrm{<span\; class="notranslate">\; max</span>}<span\; class="notranslate">\; (</span>\frac{{\mathrm{<span\; class="notranslate">\; D.</span>}}_{\mathrm{<span\; class="notranslate">\; f</span>}}<span\; class="notranslate">\; +</span>{\mathrm{<span\; class="notranslate">\; D.</span>}}_{\mathrm{<span\; class="notranslate">\; N</span>}}<span\; class="notranslate">\; -</span>\mathrm{<span\; class="notranslate">\; 2</span>}{\mathrm{<span\; class="notranslate">\; d</span>}}_{\mathrm{<span\; class="notranslate">\; 1</span>}}}{\mathrm{<span\; class="notranslate">\; 2</span>}<span\; class="notranslate">\; (</span>\mathrm{<span\; class="notranslate">\; L</span>}<span\; class="notranslate">\; -</span>\mathrm{<span\; class="notranslate">\; 1</span>}<span\; class="notranslate">\; )</span>}<span\; class="notranslate">\; ,</span>\mathrm{<span\; class="notranslate">\; \&Delta;</span>}{\mathrm{<span\; class="notranslate">\; d</span>}}_{\mathrm{<span\; class="notranslate">\; min</span>}}<span\; class="notranslate">\; )</span><span\; class="notranslate">\; <</span>\mathrm{<span\; class="notranslate">\; \&Delta;d</span>}<span\; class="notranslate">\; <</span>\frac{{\mathrm{<span\; class="notranslate">\; D.</span>}}_{\mathrm{<span\; class="notranslate">\; f</span>}}<span\; class="notranslate">\; -</span>{\mathrm{<span\; class="notranslate">\; d</span>}}_{\mathrm{<span\; class="notranslate">\; 1</span>}}}{\mathrm{<span\; class="notranslate">\; L</span>}<span\; class="notranslate">\; -</span>\mathrm{<span\; class="notranslate">\; 1</span>}}\end{array}\right.<span\; class="notranslate">\; -</span><span\; class="notranslate">\; -</span><span\; class="notranslate">\; -</span><span\; class="notranslate">\; (</span>\mathrm{<span\; class="notranslate">\; 31</span>}<span\; class="notranslate">\; )</span>$ where D _N represents the ground distance at the near end of the surveying zone, D _F represents the ground distance at the far end of the surveying zone, and Δd _min represents at least one of the minimum ground distances that cannot be expressed linearly at the calibration point in equations (26)-(30) interval; The fourth step is to calculate the latitude and longitude of each scaler; Longitude of scaler: $\mathrm{<span\; class="notranslate">\; the\; tan</span>}{\mathrm{<span\; class="notranslate">\; \&Lambda;</span>}}_{\mathrm{<span\; class="notranslate">\; GCP</span>}<span\; class="notranslate">\; ,</span>\mathrm{<span\; class="notranslate">\; i</span>}}<span\; class="notranslate">\; =</span>\frac{{\mathrm{<span\; class="notranslate">\; the\; y</span>}}_{\mathrm{<span\; class="notranslate">\; gi</span>}}}{{\mathrm{<span\; class="notranslate">\; x</span>}}_{\mathrm{<span\; class="notranslate">\; gi</span>}}}<span\; class="notranslate">\; ,</span>\mathrm{<span\; class="notranslate">\; i</span>}<span\; class="notranslate">\; =</span>\mathrm{<span\; class="notranslate">\; 1</span>}<span\; class="notranslate">\; ,</span><span\; class="notranslate">\; \&Center\; Dot;</span><span\; class="notranslate">\; \&Center\; Dot;</span><span\; class="notranslate">\; \&Center\; Dot;</span><span\; class="notranslate">\; ,</span>\mathrm{<span\; class="notranslate">\; L</span>}<span\; class="notranslate">\; -</span><span\; class="notranslate">\; -</span><span\; class="notranslate">\; -</span><span\; class="notranslate">\; (</span>\mathrm{<span\; class="notranslate">\; 36</span>}<span\; class="notranslate">\; )</span>$ Latitude of scaler: $\mathrm{<span\; class="notranslate">\; sin</span>}{\mathrm{<span\; class="notranslate">\; \&Phi;</span>}}_{\mathrm{<span\; class="notranslate">\; GCP</span>}<span\; class="notranslate">\; ,</span>\mathrm{<span\; class="notranslate">\; i</span>}}<span\; class="notranslate">\; =</span>\frac{{\mathrm{<span\; class="notranslate">\; z</span>}}_{\mathrm{<span\; class="notranslate">\; gi</span>}}}{\sqrt{{\mathrm{<span\; class="notranslate">\; x</span>}}_{\mathrm{<span\; class="notranslate">\; gi</span>}}^{\mathrm{<span\; class="notranslate">\; 2</span>}}<span\; class="notranslate">\; +</span>{\mathrm{<span\; class="notranslate">\; the\; y</span>}}_{\mathrm{<span\; class="notranslate">\; gi</span>}}^{\mathrm{<span\; class="notranslate">\; 2</span>}}<span\; class="notranslate">\; +</span>{\mathrm{<span\; class="notranslate">\; z</span>}}_{\mathrm{<span\; class="notranslate">\; gi</span>}}^{\mathrm{<span\; class="notranslate">\; 2</span>}}}}<span\; class="notranslate">\; ,</span>\mathrm{<span\; class="notranslate">\; i</span>}<span\; class="notranslate">\; =</span>\mathrm{<span\; class="notranslate">\; 1</span>}<span\; class="notranslate">\; ,</span><span\; class="notranslate">\; \&Center\; Dot;</span><span\; class="notranslate">\; \&Center\; Dot;</span><span\; class="notranslate">\; \&Center\; Dot;</span><span\; class="notranslate">\; ,</span>\mathrm{<span\; class="notranslate">\; L</span>}<span\; class="notranslate">\; -</span><span\; class="notranslate">\; -</span><span\; class="notranslate">\; -</span><span\; class="notranslate">\; (</span>\mathrm{<span\; class="notranslate">\; 37</span>}<span\; class="notranslate">\; )</span>$ Where (x _gi , y _gi , z _gi ) is the coordinate vector of the i-th scaler in the ground-fixed coordinate system E _G . 2. The method for deploying a spaceborne dual-antenna SAR interferometric scaler with integrated overall parameters according to claim 1, characterized in that: (x _go , y _go , z _go ) in the step (2.1) is calculated as follows: (1) Calculate the position (x _os , y _os , z _os ) of the satellite in the Earth’s inertial coordinate system E _O at time t ₀ ; Use the following formula to calculate the polar vector radius r of the satellite orbit: $\mathrm{<span\; class="notranslate">\; r</span>}<span\; class="notranslate">\; =</span>\frac{\mathrm{<span\; class="notranslate">\; a</span>}<span\; class="notranslate">\; (</span>\mathrm{<span\; class="notranslate">\; 1</span>}<span\; class="notranslate">\; -</span>{\mathrm{<span\; class="notranslate">\; e</span>}}^{\mathrm{<span\; class="notranslate">\; 2</span>}}<span\; class="notranslate">\; )</span>}{\mathrm{<span\; class="notranslate">\; 1</span>}<span\; class="notranslate">\; -</span>\mathrm{<span\; class="notranslate">\; e</span>}\mathrm{<span\; class="notranslate">\; cos</span>}\mathrm{<span\; class="notranslate">\; \&phi;</span>}}<span\; class="notranslate">\; -</span><span\; class="notranslate">\; -</span><span\; class="notranslate">\; -</span><span\; class="notranslate">\; (</span>\mathrm{<span\; class="notranslate">\; 13</span>}<span\; class="notranslate">\; )</span>$ Where a represents the semi-major axis of the satellite's elliptical orbit, e represents the orbital eccentricity, and φ represents the true periapsis angle of the satellite at time t ₀ ; From this, the position (x _os , y _os , z _os ) of the satellite in the Earth’s inertial coordinate system E _O at time t ₀ can be calculated, as shown in equation (14): $\left(\begin{array}{c}{\mathrm{<span\; class="notranslate">\; x</span>}}_{\mathrm{<span\; class="notranslate">\; os</span>}}\\ {\mathrm{<span\; class="notranslate">\; the\; y</span>}}_{\mathrm{<span\; class="notranslate">\; os</span>}}\\ {\mathrm{<span\; class="notranslate">\; z</span>}}_{\mathrm{<span\; class="notranslate">\; os</span>}}\end{array}\right)<span\; class="notranslate">\; =</span>{\mathrm{<span\; class="notranslate">\; A</span>}}_{\mathrm{<span\; class="notranslate">\; OV</span>}}<span\; class="notranslate">\; \&Center\; Dot;</span>\left(\begin{array}{c}\mathrm{<span\; class="notranslate">\; r</span>}\mathrm{<span\; class="notranslate">\; cos</span>}\mathrm{<span\; class="notranslate">\; \&phi;</span>}\\ \mathrm{<span\; class="notranslate">\; r</span>}\mathrm{<span\; class="notranslate">\; sin</span>}\mathrm{<span\; class="notranslate">\; \&phi;</span>}\\ \mathrm{<span\; class="notranslate">\; 0</span>}\end{array}\right)<span\; class="notranslate">\; -</span><span\; class="notranslate">\; -</span><span\; class="notranslate">\; -</span><span\; class="notranslate">\; (</span>\mathrm{<span\; class="notranslate">\; 14</span>}<span\; class="notranslate">\; )</span>$ Where A _OV is the conversion matrix from the satellite orbit coordinate system E _V to the earth inertial coordinate system E _O ; (2) Calculate the coordinates (x _go , y _go , z _go ) of the ground aiming point in the ground-fixed coordinate system E _G ; Establish the coordinates of any point (x _a , y _a , z _a ) in the main antenna coordinate system E _A in the ground-fixed coordinate system E _G. Since the Y axis of the antenna coordinate system coincides with the antenna line of sight, the main antenna aiming point is at The coordinates in the coordinate system E _A are (0,y,0), and the coordinates (x _go ,y _go ,z _go ) of the aiming point in the ground-fixed coordinate system E _G are: $\left(\begin{array}{c}{\mathrm{<span\; class="notranslate">\; x</span>}}_{\mathrm{<span\; class="notranslate">\; go</span>}}\\ {\mathrm{<span\; class="notranslate">\; the\; y</span>}}_{\mathrm{<span\; class="notranslate">\; go</span>}}\\ {\mathrm{<span\; class="notranslate">\; z</span>}}_{\mathrm{<span\; class="notranslate">\; go</span>}}\end{array}\right)<span\; class="notranslate">\; =</span>{\mathrm{<span\; class="notranslate">\; A</span>}}_{\mathrm{<span\; class="notranslate">\; go</span>}}{\mathrm{<span\; class="notranslate">\; A</span>}}_{\mathrm{<span\; class="notranslate">\; OV</span>}}{\mathrm{<span\; class="notranslate">\; A</span>}}_{\mathrm{<span\; class="notranslate">\; VR</span>}}{\mathrm{<span\; class="notranslate">\; A</span>}}_{\mathrm{<span\; class="notranslate">\; RE</span>}}{\mathrm{<span\; class="notranslate">\; A</span>}}_{\mathrm{<span\; class="notranslate">\; EA</span>}}\left(\begin{array}{c}\mathrm{<span\; class="notranslate">\; 0</span>}\\ \mathrm{<span\; class="notranslate">\; the\; y</span>}\\ \mathrm{<span\; class="notranslate">\; 0</span>}\end{array}\right)<span\; class="notranslate">\; +</span>{\mathrm{<span\; class="notranslate">\; A</span>}}_{\mathrm{<span\; class="notranslate">\; go</span>}}\left(\begin{array}{c}{\mathrm{<span\; class="notranslate">\; x</span>}}_{\mathrm{<span\; class="notranslate">\; os</span>}}\\ {\mathrm{<span\; class="notranslate">\; the\; y</span>}}_{\mathrm{<span\; class="notranslate">\; os</span>}}\\ {\mathrm{<span\; class="notranslate">\; z</span>}}_{\mathrm{<span\; class="notranslate">\; os</span>}}\end{array}\right)<span\; class="notranslate">\; +</span>{\mathrm{<span\; class="notranslate">\; A</span>}}_{\mathrm{<span\; class="notranslate">\; go</span>}}{\mathrm{<span\; class="notranslate">\; A</span>}}_{\mathrm{<span\; class="notranslate">\; OV</span>}}{\mathrm{<span\; class="notranslate">\; A</span>}}_{\mathrm{<span\; class="notranslate">\; VR</span>}}{\mathrm{<span\; class="notranslate">\; A</span>}}_{\mathrm{<span\; class="notranslate">\; RE</span>}}\left(\begin{array}{c}{\mathrm{<span\; class="notranslate">\; x</span>}}_{\mathrm{<span\; class="notranslate">\; e</span>}}\\ {\mathrm{<span\; class="notranslate">\; the\; y</span>}}_{\mathrm{<span\; class="notranslate">\; e</span>}}\\ {\mathrm{<span\; class="notranslate">\; z</span>}}_{\mathrm{<span\; class="notranslate">\; e</span>}}\end{array}\right)<span\; class="notranslate">\; -</span><span\; class="notranslate">\; -</span><span\; class="notranslate">\; -</span><span\; class="notranslate">\; (</span>\mathrm{<span\; class="notranslate">\; 15</span>}<span\; class="notranslate">\; )</span>$ Where ( _x e , y _e , z _e ) is the position vector of the antenna phase center relative to the satellite star coordinate system E _E , ( x _os , y _os , z _os ) is the position vector of the satellite in the earth's inertial coordinate system E _O , A _GO is the transformation matrix from the earth inertial coordinate system E _O to the earth fixed coordinate system E _G , A _OV is the transformation matrix from the satellite orbit coordinate system E _V to the earth inertial coordinate system E _O , A _VR is the satellite platform coordinate system E _R The transformation matrix to the satellite orbit coordinate system E _V , A _RE is the transformation matrix from the satellite star coordinate system E _E to the satellite platform coordinate system E _R , A _EA is the antenna coordinate system E _A determined by the main antenna central viewing angle θ _A to the satellite The transformation matrix of the star coordinate system E _E ; Substitute (x _go ,y _go ,z _go ) into the Earth ellipsoid model equation: $\frac{{\mathrm{<span\; class="notranslate">\; x</span>}}_{\mathrm{<span\; class="notranslate">\; go</span>}}^{\mathrm{<span\; class="notranslate">\; 2</span>}}}{{\mathrm{<span\; class="notranslate">\; E.</span>}}_{\mathrm{<span\; class="notranslate">\; a</span>}}^{\mathrm{<span\; class="notranslate">\; 2</span>}}}<span\; class="notranslate">\; +</span>\frac{{\mathrm{<span\; class="notranslate">\; the\; y</span>}}_{\mathrm{<span\; class="notranslate">\; go</span>}}^{\mathrm{<span\; class="notranslate">\; 2</span>}}}{{\mathrm{<span\; class="notranslate">\; E.</span>}}_{\mathrm{<span\; class="notranslate">\; a</span>}}^{\mathrm{<span\; class="notranslate">\; 2</span>}}}<span\; class="notranslate">\; +</span>\frac{{\mathrm{<span\; class="notranslate">\; z</span>}}_{\mathrm{<span\; class="notranslate">\; go</span>}}^{\mathrm{<span\; class="notranslate">\; 2</span>}}}{{\mathrm{<span\; class="notranslate">\; E.</span>}}_{\mathrm{<span\; class="notranslate">\; b</span>}}^{\mathrm{<span\; class="notranslate">\; 2</span>}}}<span\; class="notranslate">\; =</span>\mathrm{<span\; class="notranslate">\; 1</span>}<span\; class="notranslate">\; -</span><span\; class="notranslate">\; -</span><span\; class="notranslate">\; -</span><span\; class="notranslate">\; (</span>\mathrm{<span\; class="notranslate">\; 16</span>}<span\; class="notranslate">\; )</span>$ Among them, E _a and E _b are the semi-major axis and semi-minor axis of the earth ellipsoid respectively. Solving the equation can obtain y, and at the same time can obtain the coordinates of the aiming point in the ground-fixed coordinate system E _G (x _go , y _go , z _go ). 3. the method for deploying the spaceborne dual-antenna SAR interferometric scaler of the comprehensive overall parameter according to claim 1, is characterized in that: in the described fourth step (x _gi , y _gi , z _gi ) are calculated as follows: (1) According to the number of calibrators L calculated in the third step, the ground distance d ₁ between the first calibrator and the sub-satellite point, and the ground distance interval Δd between the calibrators, calculate each calibration The position vector of the sensor in the satellite synchronous scene coordinate system _ESS ; Assuming that the ground distances of the L scalers are d _i , i=1,..., L respectively, then the position vector of each scaler in the satellite synchronous scene coordinate system E _SS is V _SS =(0,d _i -d ₀ ,0), i=1,..., L, where d ₀ is the ground distance between the ground aiming point at the center of the main antenna beam and the sub-satellite point, the calculation process is as follows: d ₀ =Ψ ₀ ·R _e (32) Where R _e represents the radius of the local Earth, Ψ _o is the angle between the center of the earth and the sub-satellite point at the center of the beam, and can be calculated as follows according to the spherical triangle relationship: Ψ ₀ ＝arccos[sin(Φ ₀ )sin(δ)+cos(Φ ₀ )cosδcos(Λ ₀ -λ)] (33) Where δ and λ represent the geocentric latitude and geocentric longitude of the sub-satellite point at time t ₀ respectively; (2) Convert the position vector of the scaler in the satellite synchronous scene coordinate system E _SS to the geosynchronous scene coordinate system E _SE : V _SE = A _ES V _SS (34) Where A _ES is the conversion matrix from the satellite synchronous scene coordinate system E _SS to the geosynchronous scene coordinate system E _SE ; (3) Transform the position coordinates of each scaler into the ground-fixed coordinate system E _G , the process is as follows: $\left(\begin{array}{c}{\mathrm{<span\; class="notranslate">\; x</span>}}_{\mathrm{<span\; class="notranslate">\; gi</span>}}\\ {\mathrm{<span\; class="notranslate">\; the\; y</span>}}_{\mathrm{<span\; class="notranslate">\; gi</span>}}\\ {\mathrm{<span\; class="notranslate">\; z</span>}}_{\mathrm{<span\; class="notranslate">\; gi</span>}}\end{array}\right)<span\; class="notranslate">\; =</span>{\mathrm{<span\; class="notranslate">\; A</span>}}_{\mathrm{<span\; class="notranslate">\; GS</span>}}\left(\begin{array}{c}{\mathrm{<span\; class="notranslate">\; x</span>}}_{\mathrm{<span\; class="notranslate">\; ss</span>}<span\; class="notranslate">\; ,</span>\mathrm{<span\; class="notranslate">\; i</span>}}\\ {\mathrm{<span\; class="notranslate">\; the\; y</span>}}_{\mathrm{<span\; class="notranslate">\; ss</span>}<span\; class="notranslate">\; ,</span>\mathrm{<span\; class="notranslate">\; i</span>}}\\ {\mathrm{<span\; class="notranslate">\; z</span>}}_{\mathrm{<span\; class="notranslate">\; ss</span>}<span\; class="notranslate">\; ,</span>\mathrm{<span\; class="notranslate">\; i</span>}}\end{array}\right)<span\; class="notranslate">\; ,</span>\mathrm{<span\; class="notranslate">\; i</span>}<span\; class="notranslate">\; =</span>\mathrm{<span\; class="notranslate">\; 1</span>}<span\; class="notranslate">\; ,</span><span\; class="notranslate">\; \&CenterDot;</span><span\; class="notranslate">\; \&CenterDot;</span><span\; class="notranslate">\; \&CenterDot;</span><span\; class="notranslate">\; ,</span>\mathrm{<span\; class="notranslate">\; L</span>}<span\; class="notranslate">\; -</span><span\; class="notranslate">\; -</span><span\; class="notranslate">\; -</span><span\; class="notranslate">\; (</span>\mathrm{<span\; class="notranslate">\; 35</span>}<span\; class="notranslate">\; )</span>$ Among them, A _GS is the corresponding conversion matrix.

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