ESA Earth Home Missions Data Products Resources Applications
EO Data Access
How to Apply
How to Access
ASAR Data Formats Products
Geolocation Grid ADSRs
Doppler Centroid parameters
Chirp parameters
Antenna Elevation pattern
ASAR external characterization data
ASAR external calibration data
Level 0 SPH
Level 0 MDSR
SPH for auxiliary data with N=1 DSDs
Wave Mode Geolocation ADS
ASAR Wave Mode Products Base SPH
Slant Range to Ground Range conversion parameters
Measurement Data Set containing spectra. 1 MDSR per spectra.
Ocean Wave Spectra
Map Projection parameters
ASAR Image Products SPH
Measurement Data Set 1
Auxilliary Products
ASA_XCH_AX: ASAR External characterization data
ASA_XCA_AX: ASAR External calibration data
ASA_INS_AX: ASAR Instrument characterization
ASA_CON_AX: ASAR Processor Configuration
Browse Products
ASA_WS__BP: ASAR Wide Swath Browse Image
ASA_IM__BP: ASAR Image Mode Browse Image
ASA_GM__BP: ASAR Global Monitoring Mode Browse Image
ASA_AP__BP: ASAR Alternating Polarization Browse Image
Level 0 Products
ASA_WV__0P: ASAR Wave Mode Level 0
ASA_WS__0P: ASAR Wide Swath Mode Level 0
ASA_MS__0P: ASAR Level 0 Module Stepping Mode
ASA_IM__0P: ASAR Image Mode Level 0
ASA_GM__0P: ASAR Global Monitoring Mode Level 0
ASA_EC__0P: ASAR Level 0 External Characterization
ASA_APV_0P: ASAR Alternating Polarization Level 0 (Cross polar V)
ASA_APH_0P: ASAR Alternating Polarization Level 0 (Cross polar H)
ASA_APC_0P: ASAR Alternating Polarization Level 0 (Copolar)
Level 1 Products
ASA_IMS_1P: ASAR Image Mode Single Look Complex
ASA_IMP_1P: ASAR Image Mode Precision Image
ASA_IMM_1P: ASAR Image Mode Medium Resolution Image
ASA_IMG_1P: ASAR Image Mode Ellipsoid Geocoded Image
ASA_GM1_1P: ASAR Global Monitoring Mode Image
ASA_APS_1P: ASAR Alternating Polarization Mode Single Look Complex
ASA_APP_1P: ASAR Alternating Polarization Mode Precision Image
ASA_APM_1P: ASAR Alternating Polarization Medium Resolution Image product
ASA_WSS_1P: Wide Swath Mode SLC Image
ASA_WVS_1P: ASAR Wave Mode Imagette Cross Spectra
ASA_WSM_1P: ASAR Wide Swath Medium Resolution Image
ASA_APG_1P: ASAR Alternating Polarization Ellipsoid Geocoded Image
Level 2 Products
ASA_WVW_2P: ASAR Wave Mode Wave Spectra
ASAR Glossary Terms
Sea Ice Glossary
Land Glossary
Oceans Glossary
Geometry Glossary
ASAR Instrument Glossary
Acronyms and Abbreviations
ASAR Frequently Asked Questions
The ASAR Instrument
Instrument Characteristics and Performance
Inflight Performance Verification
Preflight Characteristics and Expected Performance
Instrument Description
Internal Data Flow
ASAR Instrument Functionality
Payload Description and Position on the Platform
ASAR Products and Algorithms
Auxiliary Products
Common Auxiliary Data Sets
Auxiliary Data Sets for Level 1B Processing
Summary of Auxiliary Data Sets
Instrument-specific Topics
Level 2 Product and Algorithms
Level 2 Product
ASAR Level 2 Algorithms
Level 1B Products
ASAR Level 0 Products
Level 0 Instrument Source Packet Description
Product Evolution History
Definitions and Conventions
Organisation of Products
ASAR Data Handling Cookbook
Hints and Algorithms for Higher Level Processing
Hints and Algorithms for Data Use
ASAR Characterisation and Calibration
The Derivation of Backscattering Coefficients and RCSs in ASAR Products
External Characterisation
Internal Calibration
Pre-flight Characterisation Measurements
ASAR Latency Throughput and Data Volume
Data Volume
Products and Algorithms Introduction
Child Products
The ASAR User Guide
Image Gallery
Further Reading
How to Use ASAR Data
Software Tools
How to Choose ASAR Data
Special Features of ASAR
Geophysical Coverage
Principles of Measurement
Scientific Background
Geophysical Measurements
ASAR Product Handbook
ASAR instrument characterization data
Wave Mode processing parameters
ASAR processor configuration data
Main Processing parameters
ASA_WVI_1P: ASAR Wave Mode SLC Imagette and Imagette Cross Spectra
Product Terms
RADAR and SAR Glossary
Level 1B Products
Summary of Applications vs Products
Site Map
Frequently asked questions
Terms of use
Contact us

The purpose of this section is to discuss the problem known as scalloping, and the process used to correct it, known as descalloping. Scalloping

A radar system can be operated in burst mode such that the sensor is on for a period of time, then off, then on again, and so on, effectively imaging the region of interest in a series of bursts, where each burst consists of a certain number of echoes. In comparison with the conventional strip-mode imaging methods, burst mode operation enables a reduced power consumption and data rate at the expense of the resolution and image quality achieved.

Since a sensor operating in burst mode does not view a scene continuously, achieving uniform image quality over the imaged extent is more difficult for a burst mode imaging system than for a continuous mode one. In particular, burst mode images are subject to cyclic radiometric banding effects as described below.

During azimuth compression, the data in each burst must be adjusted by the proper azimuth gain correction function. This is due to the fact that the return energy from a single scatterer is modulated in azimuth according to that portion of the antenna gain pattern used in the burst imaging event, an effect known as scalloping Ref. [2.11 ] (see figure2.34 Below). In other words, different point targets are illuminated by different positions of the azimuth gain pattern yielding different integrated powers. The amount of scalloping corresponds to the energy difference from the beginning to the end of the processing bandwidth and is generally measured in decibels (dB).

Figure 2.34 Return Energy From a Single Scatterer (3 bursts shown)
One method to correct for azimuth scalloping across individual bursts involves applying descalloping functions which are inversely proportional to the predicted antenna gain pattern function, thus resulting in a constant magnitude in azimuth across the corrected burst, as shown in figure2.35 a. In this figure, the uncompensated burst energy is drawn as the solid line, and the descalloping (correction) function is drawn as the dotted line. Consequentially, the radiometry is rendered flat in azimuth along the full image extent (figure2.35 b).

However, an inaccurate estimation of the fractional Doppler centroid frequency leads to a misapplication of each of the azimuth descalloping functions to its corresponding burst image return signal. As a result, the output signal level is rendered non-constant across the azimuth burst as shown in figure2.36 a below. In this figure, the Doppler centroid error ( f Derror ) causes a cyclic rotation in the uncompensated burst energy function along azimuth (as shown in the solid line), resulting in an incorrect application of the descalloping function (shown as the dotted line).This radiometric variation in azimuth across each burst results in a cyclic radiometric pattern known as residual scalloping across the full image in azimuth, as depicted in figure2.36 b.

Figure 2.35 The application of a suitable correction function to an azimuth burst with an accurate Doppler centroid frequency estimate

Figure 2.36 The application of a suitable correction function to an azimuth burst in the presence of a Doppler centroid frequency estimation error Methods for Scalloping Correction Azimuth Descalloping Function Application

There are two possible methods that may be selected for calculating the descalloping function: the Inverse Beam Pattern Method and the Constant SNR method.

Inverse Beam Pattern Descalloping Method One method to correct for scalloping across azimuth involves applying weighting functions which are inversely proportional to the azimuth antenna gain function. This technique shall be referred to as the Inverse Beam Pattern Method for descalloping.

To apply the correction effectively, the Doppler centroid frequency must be known accurately.

The weighting functions derived using the Inverse Beam Pattern method emphasise the outer looks to equalise the power, thereby maximising the equivalent number of looks, or speckle reduction, over azimuth.

Constant signal-to-noise ratio (SNR) Descalloping Method Bamler's "Optimum Look Weighting for Burst-Mode and ScanSAR Processing" ( Ref. [2.11 ] ) has developed a set of antenna pattern correction functions for burst mode and ScanSAR processing. The functions are derived to satisfy the following criteria in the multi-look azimuth processing case:

  • The image signal energy becomes constant over azimuth,
  • The noise energy becomes constant over azimuth, and
  • The equivalent number of looks (which describes the amount of speckle reduction obtained by a weighted multi-look process) is maximised over azimuth.
The first and second criteria results in a constant signal-to-noise ratio (SNR) over azimuth. By allowing a variation in the signal image level in the derivation of the constant SNR weighting functions, the sensitivity of residual scalloping to Doppler centroid frequency estimation error is reduced. Note that in the case of only two azimuth looks, the signal image level is fixed as there are no degrees of freedom available to maximise.

In addition, the constant SNR method generates weighting functions which de-emphasise the outer looks, so that the equivalent number of looks is not maximised. Doppler Centroid Frequency Estimation in the context of Burst Mode Data

An accurate estimate of the Doppler centroid frequency is necessary to reduce the effect of residual scalloping, as shown in figure.2.36
For both the Inverse Beam Pattern method and the Constant SNR method, the sensitivity to Doppler centroid errors decreases as the number of looks increases. Notes

Ref 2.10
An approximation in the ASAR implementation of this method is described as follows. The correction at each azimuth location is proportional to the inverse of the midpoint of the azimuth beam pattern over the portion of the beam pattern used in focussing the image at that azimuth location. This is assumed to approximate, at each azimuth location, the inverse of the integral of the azimuth beam pattern over the portion of the beam pattern used in focussing the image at that azimuth location. References

Ref 2.11
Bamler R, "Optimum Look Weighting for Burst-Mode and ScanSAR Processing", IEEE Transactions on Geoscience and Remote Sensing Vol. 33 No. # pp. 722-725, May 1995. ScanSAR Beam Merging

ScanSAR multi-beam processing consists of generating independent beam images (called beam buffers) and subsequently combining them into a single output line, as shown in figure2.37 below:

Figure 2.37 Merging Beam Buffers

The beam buffers overlap in range so, in general, the data should be merged to allow the output image line to be continuous.

Data in the merged line is either copied directly from one beam, or the merged line data is a blend of pixels from the so called blend region of the two beams.

Therefore, the beam merging algorithm consists of three primary steps described ago. Determine a reference point in the blend region

The reference point of the blend region is defined as the pixel corresponding to the range at which the elevation beam patterns for near and far beam intersect. Therefore, the blend region necessarily falls inside the overlap region, which is the region defined by the first pixel of the far beam and the last pixel of the near beam, as indicated in the figure2.38 below. Determine the limits of the blend region

The nominal size of the blend region, say N (even number), is specified in a PF-ASAR input parameter file. A number of N/2 points are extracted on either side of the reference point for each (near and far) beam, so the reference point is precisely the centre of the blend region. If necessary, N will be clipped against the limits of the overlap region.

Figure 2.38 The Blend Region and its Reference Point Merge the data in the two beams corresponding to the blend region according to a predefined rule

The merging formula used to complete this third step is designed so that the signal-to-noise ratio of the imagery of the merged data tends to be maximised.

In describing the method, the following notation is used:

xnear(n) = the array of near beam pixel power values;

xfar (n) = the array of far beam pixel power values and;

p = weight rate

For a given value of p, the formula used to calculate the merged pixels is given by:

eq 2.15

xmerged(n) = (1 - (n/N)p) * xnear(n) + ((n/N)p) * xfar(n),

where n =0,1,...,N-1 and p >= 0. The data on the steeper extremities of the beam pattern, where the effects of a bias in the elevation beam pattern correction are more significant, are disregarded while the data on the steeper extremities of the blend region are weighted less by the merging model. This is because the following continuity conditions hold true:

xmerged(0) = xnear(0)

xmerged(N) = xfar (N)

In particular, if xfar(n) = xnear(n) for all n = 0,1,...,N-1, then

xmerged(n) = xfar(n) = xnear(n) for all n = 0,1,...,N-1

The desired merging scenario can be easily selected by simply setting the weight rate parameter, p, as shown in the following table:

Table 2.33 Setting Weight Rates Parameter
Parameter p Weighting
p = 1 current weighting scenario
p > 1 the near beam weighs more(it is favoured)
0 < p < 1 the far beam weighs more(it is favoured)
p = 0 only the far beam contributes to the merged one
p = infinity only the near beam contributes to the merged one Global Monitoring Mode Inverse Filter

The transmitted pulse typically has a rectangular amplitude, and a quadratic phase variation that gives the pulse its linear FM character. For linear FM pulses, increasing the duration of the pulse allows greater frequency variation across the pulse, thus increasing the pulse bandwidth and resulting in a higher resolution after pulse compression. (See the description of range compression in the section on Range-Doppler processing). Linear FM pulses that are used for pulse compression typically have a large time-bandwidth product, at least 100.

For linear FM pulses with a large time-bandwidth product, there is a time-frequency relationship, such that the amplitude spectrum has the same shape as the pulse amplitude in the time domain. For example, the figure below shows the amplitude of the Fourier transform (FFT) of a large time-bandwidth product pulse with a rectangular shape.

Figure 2.39 Pulse spectrum with large time-bandwidth product.

The Fourier transform (FFT) also has a quadratic phase variation that needs to be removed during matched filtering, in order to compress the pulse. In the frequency domain, the matched filter is defined as the conjugate of the Fourier transform of the pulse. For large time-bandwidth product pulses, multiplication of the pulse spectrum by its conjugate removes the quadratic phase variation, and leaves the amplitude approximately unchanged because of the rectangular shape, resulting in the sinc shaped impulse response.

However, in Global Monitoring (GM) Mode where the required resolution is quite low, a relatively short pulse with smaller bandwidth is used. In this case the time-bandwidth product is quite low, on the order of 20, and the time-frequency relationship does not hold as well. For example, the figure below shows the amplitude of the Fourier transform of a pulse used in Global Monitoring Mode. The amplitude is no longer rectangular, and multiplication by the matched filter would worsen the amplitude variation, which affects the shape of the compressed pulse.

imagefull size
Figure 2.40 Pulse spectrum with small time-bandwidth product.

To solve the problem caused by the shape of the amplitude spectrum when the time bandwidth product is low, the variation of the amplitude spectrum is removed by multiplying the pulse spectrum by the inverse of the Fourier transform (IFFT)of the pulse, rather than the conjugate. This removes the amplitude variation of the spectrum during pulse compression, improving the shape of the compressed pulse. ASAR Strip Line Product Processing Introduction

The ASAR Instrument may be operated in one high rate mode continuously (an acquisition segment) for up to ten minutes duration or for up to one orbit duration in a low-rate mode called Global Monitoring (GM) mode. Stripline products contain image data from an entire acquisition segment, up to a maximum of 10 minutes per product for IM, AP, and WS and up to a full orbit (100 minutes) for GM. All medium-resolution and browse products (IMM, IMB, APM, APB, WSM, WSB, GM1, and GMB) are processed as stripline products. The browse products are subsampled versions of the medium-resolution products and are processed at the same time. ( For a further discussion of all of these products refer to the section entitled "Level 1B Image Products" and "Browse Products" , which can both be found in chapter 2 ).

The PF-ASAR will systematically generate output parent products, within the time constraints, that cover an entire acquisition segment by processing a number of separate slices and then joining the slices to form the continuous segment. Most long data segments will be processed using more than one processing computer, in order to meet throughput performance requirements. Each computer will be given a portion of the input data segment to process. The output, referred to as slices, from the different computers are then concatenated to produce one long strip product, referred to as stripline product.

This stripline parent product is stored as a single product in the Archive Facility (ARF) and key information about the product is maintained in the inventory database for access by users. After the segment product is archived, a customer may extract a subset, or child product. If a customer orders a floating scene from within the stripline product the appropriate portion of the archived product, i.e. the measurement data, annotation data, Specific Product Header (SPH) and Main Product Header (MPH), will be extracted to form the requested output product. The extracted subset product may start at any point in the segment and shall not contain any radiometric or geometric discontinuities.

Geometric continuity is achieved by ensuring all PF-ASAR computers establish the same output grid. All PF-ASAR will use the same input parameters (orbit data, earth ellipsoid parameters, centre swath elevation angle, etc.) and the same software to establish the output grid. The projection used for stripline products differs from the normally used for SAR products. SAR products are usually projected such that the first pixel in range is kept at a constant range. For stripline products, however, the ground range projection is designed to allow very long azimuth extent images to be displayed without cutting off any data and with a minimum of black-filled pixels. This is done by keeping the mid-ground range pixels at a constant elevation angle.

Radiometric continuity is achieved by ensuring the Doppler Centroid frequency is continuous along the data segment. The input raw data to the different PF-ASAR computers is overlapped and each PF-ASAR uses the overlap regions (at the beginning and end of the slice) to estimate the Doppler Centroid frequency. The Doppler Centroid frequency that is used within the slice is calculated by interpolation.

The slice size and the overlap depend on the mode (IM, AP, WS or GM). The figure and table below show the minimum and maximum slice sizes and the minimum overlap. The overlap must take into account the amount of data required for Doppler centroid estimation and processing throw away (matched filter throw-away and azimuth skew).

Figure 2.41 Slice Size and Overlap Illustration

Product generation includes the following extra parameters for stripline processing:
  • Slice size
  • Slice number
  • Acquisition start time of the segment
  • Overlap size Slice Size and Overlap

Table 2.34 Slice Size and Overlap
MinimumSlice Size 20.7 sec 37.4 sec 5 sec 30.7 sec
MaximumSlice Size 90 sec 90 sec 90 sec 20 min
MinimumOverlap 2.5 sec 2.5 sec 8.3 sec 54.3 sec Processing Parameters Affected By Strip Line Product Continuity Requirements

ASAR processing requires the calculation and use of a number of processing parameters whose values vary at different rates. Some parameters may be held constant throughout an acquisition segment while other parameters must be recalculated at intervals and then applied to blocks of data or varied smoothly throughout the segment.

Table 2.35 below "Processing Parameters Affecting Stripline Products", identifies processing parameters that are important for stripline processing and groups the parameters depending on their source:

  • signal data - parameters derived from the SAR raw data;
  • auxiliary data - parameters derived from common auxiliary data provided to all ASAR computers;
  • ISP header data - parameters extracted from header of downlink data and may vary throughout data segments.

Table 2.35 Processing Parameters Affecting Stripline Products
Processing Parameters from Signal Data Processing Parameters from Auxiliary Data Processing Parameters from ISP Header Data
I and Q channel statistics along-track pixel spacing/start position First output range sample
Chirp Replica
Antenna Elevation gain correction Slant range/ground range interpolation to output grid
Doppler Centroid Estimate
Doppler Ambiguity Estimate FM Rate I And Q Channel Statistics

Channel statistics are calculated from raw data to determine I and Q channel bias and orthogonality adjustments. These adjustments affect radiometric accuracy. ERS experience indicates that channel bias values are relatively slowly varying, therefore statistical analysis of data from any portion of the data segment could be applied to the entire segment, or the analysis could be repeated using any portion of the segment and yield similar results.

Each PF-ASAR computer evaluates I and Q channel statistics from its own ISP data. The raw data used for statistics is a subsample of the total raw data taken from samples throughout the input data. The calculated correction factors are applied uniformly for the entire slice. Chirp Replica

The chirp replica is derived by processing the periodic calibration data. Periodic calibration activities performed by the instrument generate calibration data for segments of the SAR antenna in a cyclic manner and downlinks this data interspersed with the imaging data. The pulse replica is derived from the summation of calibration data from all 32 antenna segments received over a period of time.

During stripline processing the chirp replica is updated whenever a new periodic calibration cycle is found in the input data. If a complete set of calibration pulses from 32 antenna segments is not found, then the nominal chirp is used. Antenna Elevation Gain Correction

The antenna elevation gain correction is also derived by processing the periodic calibration data and is also updated whenever a new periodic calibration cycle is found in the input data. If a complete set of calibration pulses from 32 antenna segments is not found, then the nominal antenna elevation gain correction is used.

The antenna elevation pattern is converted to slant range pattern so it can be applied to the range compressed data. This conversion is updated periodically to follow the continuously changing satellite/earth geometry. Doppler Centroid Estimation

Doppler centroid estimation is performed by each PF-ASAR computer using the data at the beginning and end of the slice. Linear interpolation using the two estimates is used to compute Doppler centroid frequency at various positions along the slice.

If the overlap data is missing, Doppler centroid estimation is still done using the data at the beginning and end of the available input data. In this case, the Doppler centroid may not be continuous across the adjacent slices. This is acceptable because there is no valid image at the boundary of the slices.

The Doppler centroid frequency maximum variation is about 1.7 Hz/sec. Over a slice of 20 seconds, the Doppler centroid frequency changes by a maximum of 34 Hz and the variation can be approximated as a linear function over a long period.

The ambiguity estimate is performed once per slice and is then applied throughout that slice.

( For a further discussion of the Doppler centroid frequency, ambiguity, and estimation, see the section entitled "Doppler Centroid Frequency Estimator" ). along-track Pixel Spacing/Start Position

A stripline product is required to have a constant along-track pixel spacing to meet geometric requirements and ease processing of child products (floating scenes extracted from the stripline product). For systematically generated ASAR products (GMM, IMM, WSM, APM, and browse), each output line contains pixels for a specific zero Doppler time and lines are spaced by a constant zero Doppler time interval (rather than constant distance spacing). Therefore each output line must be placed on a grid with a regular time interval referenced to the start time of the stripline product segment.

The Line Time Interval in seconds (the grid spacing along-track) is pre-defined for each product type and subswath and is a constant throughout the orbit to ensure repeatability of grid spacing from one orbit to the next. (It should be noted that the precise pixel spacing in metres will vary depending on the instantaneous velocity of the satellite.)

Each PF-ASAR calculates the zero Doppler start time of the stripline product segment by converting the acquisition time to zero Doppler time.

Each PF-ASAR then calculates the zero Doppler start time and stop time of its output slice. Slant Range/Ground Range (SR/GR) Conversion To Output Grid

The output grid is defined such that the azimuth line of the output product is parallel with the mid swath line, where the mid swath line is the line which has a fixed elevation angle along azimuth. This output grid does not contain any range pixel with a constant range time along azimuth.

As the satellite altitude varies with time, the mid swath line moves closer or farther away from the subsatellite track and the valid data follows the Sampling Window Start Time (SWST).

The number of samples per range lines in the output product is set to be large enough to cover the shift of the valid data along the segment so that no valid data is thrown away.

The valid samples are projected to the output grid using an SR/GR conversion table. PF-ASAR calculates the SR/GR conversion table periodically along the azimuth direction and performs linear interpolation between adjacent SR/GR conversion tables so that a smoothly varying SR/GR can be achieved. FM Rate

The Frequency Modulation (FM) Rate must be updated throughout the segment to maintain geometric continuity. The FM rate varies slowly so that calculations at consecutive portions of the segment do not result in discontinuity for medium-resolution products. It is calculated once per slice. First Output Range Sample

The location of the first valid output range sample is a function of the Sampling Window Start Time (SWST). PF-ASAR calculates the slant range of this first valid sample using the SWST and then projects it to the output grid using the smoothly varying SR/GR conversion table. Level 1B Accuracies

The following two tables define the product geometric accuracies of the Level1B products.

Table 2.36 ASAR High Resolution Image Accuracy
Product Type
IM (Image Mode) AP (Alternating Polarisation Mode) WV (Wave Mode)
Precision Image


Resolution < 28m

ENL = 3.9


Resolution < 30m

ENL = 1.9

Single-Look Complex

Pixel=image spacing

Resolution=6m (Azimuth) and 9m(Slant Range)

Pixel=image spacing

Resolution=12m (Azimuth) and 9m(Slant Range)

Ellipsoid Geocoded


Resolution < 30m

ENL = 3.9


Resolution < 30m

ENL > 1.9

Single-Look Complex Wave Imagette

Pixel=image spacing

Resolution=6m (Azimuth) and 9m(Slant Range)

Table 2.37 ASAR Brows, Medium Resolution and Global Monitoring Image Accuracy
Product Type
IM (Image Narrow swath) AP (Alternating Polarisation) WS (Wide Swath) GM (Global Monitoring)
Medium Resolution Image

Resolution < 150m


ENL = 40

Resolution < 150m


ENL = 50

Resolution < 150m


ENL = 11*

Global Monitoring Image

Resolution < 950m


ENL = 7 to 9*

Browse Image **


ENL = 80


ENL = 75


ENL = 57to 82

Resolution =2000m


ENL = 18 to 21

In the tables, Pixel means pixel spacing, Resolution means spatial resolution, ENL is equvalent number of looks (which affects radiometric resolution). The ENL on some images is dependant on the instrument setting, indicated with one asterisk (*). Browse images are derived from Medium Resolution images.

Table 2.38 Summary of ASAR Predicted Performance with Comparison to ERS
Parameter Unit Image Alternating Polarisation Wide Swath Global Monitoring Wave ERS-1/2
Polarisation VV or HH VV/HH, HH/HV, VV/VH VV or HH VV or HH VV or HH VV
Spatial resolution (a x r) m 27.5 x 28.1 28.7 x 29.7 149 x 145 949 x 977 27.5 x 29.6 27.5 x 28.1
Radiometric resolution dB 1.54 2.46 to 2.50 1.45 to 1.72 1.35 to 1.44 1.54 2.07
PTAR azimuth dB 25.9 to 29.6 19.1 to 28.0 22.3 to 28.6 26.6 to 29.3 27.3 to 29.6 27.8/24.5
PTAR range dB 31.6 to 45.8 26.4 to 40.5 25.0 to 33.9 25.0 to 32.2 31.2 to 45.7 >40
DTAR azimuth dB 22.6 to 24.7 18.1 to 24.5 20.3 to 24.9 24.6 to 27.5 22.6 to 24.7 >25
DTAR range dB 17.1 to 39.4 17.1 to 39.4 17.1 to 30.8 17.1 to 30.8 21.2 to 47.7 >35
Radiometric stability (1sigma) dB 0.32 to 0.40 0.50 to 0.55 0.32 to 0.42 0.46 to 0.53 0.55 to 0.60 0.24/0.27
Radiometric accuracy (3sigma) dB 1.17 to 1.38 1.62 to 1.81 1.20 to 1.45 1.54 to 1.74 1.80 to 1.94 na
Noise Equivalent (sigma-nought) dB -19.6 to -22.1 -19.4 to -21.9 -20.8 to -26.2 -31.5 to -35 -19.8 to -22.4 -26.2/-25.2