<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article  PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd"><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article"><front><journal-meta><journal-id journal-id-type="publisher-id">JCC</journal-id><journal-title-group><journal-title>Journal of Computer and Communications</journal-title></journal-title-group><issn pub-type="epub">2327-5219</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/jcc.2016.43014</article-id><article-id pub-id-type="publisher-id">JCC-64149</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Computer Science&amp;Communications</subject></subj-group></article-categories><title-group><article-title>
 
 
  Channel Error Estimation Methods Comparison under Different Conditions for Multichannel HRWS SAR Systems
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Tingting</surname><given-names>Jin</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Xiaolan</surname><given-names>Qiu</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Donghui</surname><given-names>Hu</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Chibiao</surname><given-names>Ding</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib></contrib-group><aff id="aff1"><addr-line>Institute of Electronics, Chinese Academy of Sciences, Beijing 100190, China</addr-line></aff><pub-date pub-type="epub"><day>02</day><month>03</month><year>2016</year></pub-date><volume>04</volume><issue>03</issue><fpage>88</fpage><lpage>94</lpage><history><date date-type="received"><day>2</day>	<month>November</month>	<year>2015</year></date><date date-type="rev-recd"><day>accepted</day>	<month>26</month>	<year>February</year>	</date><date date-type="accepted"><day>2</day>	<month>March</month>	<year>2016</year></date></history><permissions><copyright-statement>&#169; Copyright  2014 by authors and Scientific Research Publishing Inc. </copyright-statement><copyright-year>2014</copyright-year><license><license-p>This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/</license-p></license></permissions><abstract><p>
 
 
   Multichannel synthetic aperture radar (SAR) in azimuth can resolve the contradiction between high resolution and wide swath faced with traditional SAR imaging. However, channel errors will degrade the performance of imaging. This paper compares the performances of four channel error estimation algorithms under different clutter distributions and SNR conditions. Further, explanations are given for performance differences of the four algorithms, which provide evidence for method selection in engineering applications. 
 
</p></abstract><kwd-group><kwd>Synthetic Aperture Radar (SAR)</kwd><kwd> High Resolution and Wide Swath (HRWS)</kwd><kwd> Multi-Channel in Azimuth</kwd><kwd> Channel Error Estimation</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Conventional SAR system suffers from the limitation of achieving high resolution and wide swath (HRWS) simultaneously [<xref ref-type="bibr" rid="scirp.64149-ref1">1</xref>]-[<xref ref-type="bibr" rid="scirp.64149-ref10">10</xref>]. Multichannel in azimuth HRWS SAR, combined with digital beam forming (DBF) technique [<xref ref-type="bibr" rid="scirp.64149-ref2">2</xref>] [<xref ref-type="bibr" rid="scirp.64149-ref7">7</xref>], can effectively deal with this problem. Channel mismatch, caused by central electronic equipment, antenna array and satellite platform, and so on, will seriously affect the image quality in multichannel SAR systems. So channel error estimation and compensation becomes very crucial [<xref ref-type="bibr" rid="scirp.64149-ref2">2</xref>].</p><p>This paper mainly deals with the problem of channel errors in multi-channel HRWS SAR systems. In recent years many algorithms have been put forward to estimate the channel errors. The four main methods are time- domain correlation method (TDCM) [<xref ref-type="bibr" rid="scirp.64149-ref3">3</xref>], orthogonal subspace method (OSM) [<xref ref-type="bibr" rid="scirp.64149-ref4">4</xref>], signal subspace comparison method (SSCM) [<xref ref-type="bibr" rid="scirp.64149-ref5">5</xref>] [<xref ref-type="bibr" rid="scirp.64149-ref6">6</xref>] and antenna pattern method (APM) [<xref ref-type="bibr" rid="scirp.64149-ref5">5</xref>] [<xref ref-type="bibr" rid="scirp.64149-ref6">6</xref>]. Some simple comparisons of these methods have also been done [<xref ref-type="bibr" rid="scirp.64149-ref5">5</xref>] [<xref ref-type="bibr" rid="scirp.64149-ref6">6</xref>]. However, the performances of the estimation methods have only been compared under the Gaussian clutter scenes without theoretical analysis. In this paper, comprehensive comparison is done under different SNR conditions and different clutter distributions. In addition, theoretical analysis is given to explain the differences. The results and analysis will provide evidence for method selection in real engineering applications.</p></sec><sec id="s2"><title>2. Echo Model</title><p>The geometric model of an actual multi-channel SAR system is shown in <xref ref-type="fig" rid="fig1">Figure 1</xref>.<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/64149x4.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/64149x5.png" xlink:type="simple"/></inline-formula>and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/64149x6.png" xlink:type="simple"/></inline-formula> denote the antenna position measurement error along X, Y, and Z axis, respectively.</p><p>Taking the channel errors caused by several factors into account [<xref ref-type="bibr" rid="scirp.64149-ref2">2</xref>], the total magnitude error and phase error of the mth channel can be denoted as <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/64149x7.png" xlink:type="simple"/></inline-formula> and<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/64149x8.png" xlink:type="simple"/></inline-formula>. Echo of the mth channel can be expressed as:</p><disp-formula id="scirp.64149-formula97"><label>, (1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/64149x9.png"  xlink:type="simple"/></disp-formula><p>where</p><disp-formula id="scirp.64149-formula98"><label>. (2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/64149x10.png"  xlink:type="simple"/></disp-formula></sec><sec id="s3"><title>3. Error Estimation Methods</title><p>Since channel magnitude errors can be estimated and compensated by simple channel balancing [<xref ref-type="bibr" rid="scirp.64149-ref5">5</xref>], this paper mainly concerns channel phase error estimation methods.</p><sec id="s3_1"><title>3.1. Time-Domain Correlation Method (TDCM)</title><p>The TDCM is presented in [<xref ref-type="bibr" rid="scirp.64149-ref3">3</xref>]. This estimation algorithm is operated in time-domain. Firstly, the echoes received by adjacent channels are multiplied in time-domain to get the interferometry</p><disp-formula id="scirp.64149-formula99"><label>, (3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/64149x11.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/64149x12.png" xlink:type="simple"/></inline-formula> is the echo of the mth channel, and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/64149x13.png" xlink:type="simple"/></inline-formula> denoted the slow-time.</p><p>From the principle of the average cross correlation method in the baseband Doppler centroid estimation, there is</p><disp-formula id="scirp.64149-formula100"><label>, (4)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/64149x14.png"  xlink:type="simple"/></disp-formula><fig id="fig1"  position="float"><label><xref ref-type="fig" rid="fig1">Figure 1</xref></label><caption><title> Geomentry of a multichannel SAR system</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/64149x15.png"/></fig><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/64149x16.png" xlink:type="simple"/></inline-formula> is the Doppler centroid.</p><p>Assume that the first channel is the reference channel, phase error of the mth channel is</p><disp-formula id="scirp.64149-formula101"><label>. (5)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/64149x17.png"  xlink:type="simple"/></disp-formula></sec><sec id="s3_2"><title>3.2. Orthogonal Subspace Method (OSM)</title><p>The OSM is presented in [<xref ref-type="bibr" rid="scirp.64149-ref4">4</xref>]. This algorithm utilizes the orthogonality between the signal subspace and noise subspaces after eigenvalue decomposition, which is processed in Doppler domain.</p><p>Channel phase errors are estimated by minimize the cost function:</p><disp-formula id="scirp.64149-formula102"><label>, (6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/64149x18.png"  xlink:type="simple"/></disp-formula><p>where <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/64149x19.png" xlink:type="simple"/></inline-formula> is the array steering vector, and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/64149x20.png" xlink:type="simple"/></inline-formula> is a square matrix whose diagonal elements are phase errors in exponential form. S<sub>n</sub> corresponds to the noise subspace, whose column vectors are noise eigenvectors.</p><p>Let the first channel be the reference channel, and denote<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/64149x21.png" xlink:type="simple"/></inline-formula>. The estimation of phase errors can be expressed as</p><disp-formula id="scirp.64149-formula103"><label>, (7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/64149x22.png"  xlink:type="simple"/></disp-formula><p>where.<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/64149x23.png" xlink:type="simple"/></inline-formula> (8)</p></sec><sec id="s3_3"><title>3.3. Signal Subspace Comparison Method (SSCM)</title><p>The SSCM is expressed in [<xref ref-type="bibr" rid="scirp.64149-ref5">5</xref>]. This algorithm makes use of the fact that the space spanned by the signal subspace eigenvectors is the same as the space spanned by the array steering vector</p><disp-formula id="scirp.64149-formula104"><label>. (9)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/64149x24.png"  xlink:type="simple"/></disp-formula><p>Let <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/64149x25.png" xlink:type="simple"/></inline-formula> (10)</p><p>According to the uniqueness of orthogonal projection operator, we can get</p><disp-formula id="scirp.64149-formula105"><label>. (11)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/64149x26.png"  xlink:type="simple"/></disp-formula><p>Let<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/64149x27.png" xlink:type="simple"/></inline-formula>, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/64149x27.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/64149x28.png" xlink:type="simple"/></inline-formula>, then</p><disp-formula id="scirp.64149-formula106"><label>. (12)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/64149x29.png"  xlink:type="simple"/></disp-formula></sec><sec id="s3_4"><title>3.4. Antenna Pattern Method (APM)</title><p>The APM is expressed in [<xref ref-type="bibr" rid="scirp.64149-ref6">6</xref>]. This algorithm estimates the channel phase errors by combining with the antenna pattern.</p><p>Let<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/64149x30.png" xlink:type="simple"/></inline-formula>. Ignoring the effect of noise, from the first column of the correlation matrix, there is</p><disp-formula id="scirp.64149-formula107"><label>. (13)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/64149x31.png"  xlink:type="simple"/></disp-formula><p>Then the relative phase error of the mth channel can be expressed by</p><disp-formula id="scirp.64149-formula108"><label>. (14)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/64149x32.png"  xlink:type="simple"/></disp-formula></sec></sec><sec id="s4"><title>4. Performance Comparison and Analysis</title><p>In this section, experiment is done to compare the performance of the above mentioned four algorithms. The parameters are listed in <xref ref-type="table" rid="table1">Table 1</xref>, where M is the number of channels, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/64149x33.png" xlink:type="simple"/></inline-formula>is the antenna size in azimuth, <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/64149x33.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/64149x34.png" xlink:type="simple"/></inline-formula>is the wavelength, PRF<sub>M</sub> is the pulse repetition frequency, and <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/64149x33.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/64149x34.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/64149x35.png" xlink:type="simple"/></inline-formula> is the velocity of platform. <xref ref-type="fig" rid="fig2">Figure 2</xref> shows a brief illustration of transmitting and receiving of the SAR system.</p><p>To compare the four methods discussed above, we use two indexes: estimation deviation and the maximum azimuth ambiguity-to-signal ratio (AASR<sub>MAX</sub>). Estimation deviation means the bias between the real phase error and the estimated phase error. AASR<sub>K</sub> is the ratio of power of kth (k = 1 - 8) ambiguity component to power of the ambiguity free signal after phase error estimation and compensation [<xref ref-type="bibr" rid="scirp.64149-ref3">3</xref>], i.e.</p><disp-formula id="scirp.64149-formula109"><label>. (15)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/64149x36.png"  xlink:type="simple"/></disp-formula><p>Besides, AASR<sub>MAX</sub> is the maximum of AASR<sub>K</sub> (k = 1 - 8).</p><sec id="s4_1"><title>4.1. Estimation Performance Versus SNR</title><p>In this section, clutters are assumed to be Gaussian distribution, and SNR varies from 0 dB to 20 dB. The estimation deviations of eight channels are illustrated in <xref ref-type="fig" rid="fig3">Figure 3</xref>. The maximum estimation deviations and AASR<sub>MAX</sub> are listed in <xref ref-type="table" rid="table2">Table 2</xref> for different SNR.</p></sec><sec id="s4_2"><title>4.2. Performance Comparison under Different Clutter Distributions</title><p>In engineering application, clutter scenario does not obeyideal Gaussian distribution. Log-normal distribution, Weibull distribution and K-distribution are mainly considered as sea clutter model when HRWS SAR detects the seasurface.</p><p>This section mainly compares the performance of the four algorithms when clutter obeys Log-normal distribution, Weibull distribution and K-distribution, respectively. The estimation deviations of eight channels under SNR = 0 dB are illustrated in <xref ref-type="fig" rid="fig4">Figure 4</xref>. The maximum estimation deviations and AASR<sub>MAX</sub> for different clutter distributions and different SNR are listed in <xref ref-type="table" rid="table3">Table 3</xref> and <xref ref-type="table" rid="table4">Table 4</xref>, respectively.</p></sec><sec id="s4_3"><title>4.3. Analysis of the Results</title><p>Without eigenvalue decomposition and matrix inversion, the computational load of TDCM is the lowest. However, TDCM works worse than the other three algorithms under all simulated clutter distributions and SNR, for the deviation is cumulative when the phase error accumulates.</p><p>APM also does not need eigenvalue decomposition and matrix inversion, which is characterized by light computational load. But this method only applies to uniform distribution scenes. When the clutter obeys Weibull distribution and K-distribution, it works worse than OSM and SSCM under low SNR conditions (0 - 10 dB). While under high SNR conditions (&gt;10 dB), the differences of APM, OSM, and SSCM are very small. The frequency spectrums of Weibull distribution and K-distribution are not quite homogeneous, so the performance of APM deteriorates when the noise is relatively large. For Gaussian distribution and Log-normal distribution clutters, the scenarios are homogeneous, so APM works as well as OSM and SSCM.</p><fig id="fig2"  position="float"><label><xref ref-type="fig" rid="fig2">Figure 2</xref></label><caption><title> Illustration of transmitting and receiving of eight-channel SAR system</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/64149x37.png"/></fig><table-wrap id="table1" ><label><xref ref-type="table" rid="table1">Table 1</xref></label><caption><title> Parameters of multi-channel SAR system</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >M</th><th align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/64149x38.png" xlink:type="simple"/></inline-formula>(m)</th><th align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/64149x39.png" xlink:type="simple"/></inline-formula>(m)</th><th align="center" valign="middle" >PRF<sub>M</sub> (Hz)</th><th align="center" valign="middle" ><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/64149x40.png" xlink:type="simple"/></inline-formula>(m/s)</th></tr></thead><tr><td align="center" valign="middle" >8</td><td align="center" valign="middle" >12.16</td><td align="center" valign="middle" >0.054</td><td align="center" valign="middle" >1.054 &#215; 10<sup>4 </sup></td><td align="center" valign="middle" >7.587 &#215; 10<sup>3</sup></td></tr></tbody></table></table-wrap><table-wrap id="table2" ><label><xref ref-type="table" rid="table2">Table 2</xref></label><caption><title> Maximum estimation deviations and AASR<sub>MAX</sub> for four algorithms</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >Performance indicator</th><th align="center" valign="middle" >SNR (dB)</th><th align="center" valign="middle" >TDCM</th><th align="center" valign="middle" >OSM</th><th align="center" valign="middle" >SSCM</th><th align="center" valign="middle" >APM</th></tr></thead><tr><td align="center" valign="middle"  rowspan="4"  >Maximum estimation deviations (degree)</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >−4.5426</td><td align="center" valign="middle" >1.3959</td><td align="center" valign="middle" >1.3959</td><td align="center" valign="middle" >−2.0650</td></tr><tr><td align="center" valign="middle" >5</td><td align="center" valign="middle" >−4.2495</td><td align="center" valign="middle" >0.8181</td><td align="center" valign="middle" >0.8181</td><td align="center" valign="middle" >−0.9042</td></tr><tr><td align="center" valign="middle" >10</td><td align="center" valign="middle" >−4.0334</td><td align="center" valign="middle" >0.4654</td><td align="center" valign="middle" >0.4654</td><td align="center" valign="middle" >0.4852</td></tr><tr><td align="center" valign="middle" >20</td><td align="center" valign="middle" >−3.2007</td><td align="center" valign="middle" >−0.2280</td><td align="center" valign="middle" >−0.2280</td><td align="center" valign="middle" >−0.2215</td></tr><tr><td align="center" valign="middle"  rowspan="4"  >AASRMAX (dB)</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >−38.0153</td><td align="center" valign="middle" >−42.6855</td><td align="center" valign="middle" >−42.6855</td><td align="center" valign="middle" >−39.9564</td></tr><tr><td align="center" valign="middle" >5</td><td align="center" valign="middle" >−37.3947</td><td align="center" valign="middle" >−45.9853</td><td align="center" valign="middle" >−46.3163</td><td align="center" valign="middle" >−44.2362</td></tr><tr><td align="center" valign="middle" >10</td><td align="center" valign="middle" >−38.2960</td><td align="center" valign="middle" >−49.5419</td><td align="center" valign="middle" >−49.5419</td><td align="center" valign="middle" >−50.0598</td></tr><tr><td align="center" valign="middle" >20</td><td align="center" valign="middle" >−39.4288</td><td align="center" valign="middle" >−51.4076</td><td align="center" valign="middle" >−51.4076</td><td align="center" valign="middle" >−51.3883</td></tr></tbody></table></table-wrap><table-wrap id="table3" ><label><xref ref-type="table" rid="table3">Table 3</xref></label><caption><title> Maximum estimation deviations for four algorithms under three clutter distributions</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >Clutter Distribution</th><th align="center" valign="middle" >SNR(dB)</th><th align="center" valign="middle" >TDCM</th><th align="center" valign="middle" >OSM</th><th align="center" valign="middle" >SSCM</th><th align="center" valign="middle" >APM</th></tr></thead><tr><td align="center" valign="middle"  rowspan="3"  >Log-normal distribution</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >−1.8387</td><td align="center" valign="middle" >−1.7378</td><td align="center" valign="middle" >−1.7378</td><td align="center" valign="middle" >−1.7966</td></tr><tr><td align="center" valign="middle" >10</td><td align="center" valign="middle" >−1.1058</td><td align="center" valign="middle" >−0.5793</td><td align="center" valign="middle" >−0.5793</td><td align="center" valign="middle" >−0.5430</td></tr><tr><td align="center" valign="middle" >20</td><td align="center" valign="middle" >−0.8439</td><td align="center" valign="middle" >−0.2104</td><td align="center" valign="middle" >−0.2104</td><td align="center" valign="middle" >−0.1943</td></tr><tr><td align="center" valign="middle"  rowspan="3"  >Weibull distribution</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >−2.2719</td><td align="center" valign="middle" >2.9642</td><td align="center" valign="middle" >2.9642</td><td align="center" valign="middle" >4.3430</td></tr><tr><td align="center" valign="middle" >10</td><td align="center" valign="middle" >3.3355</td><td align="center" valign="middle" >0.8791</td><td align="center" valign="middle" >0.8791</td><td align="center" valign="middle" >1.0050</td></tr><tr><td align="center" valign="middle" >20</td><td align="center" valign="middle" >4.2251</td><td align="center" valign="middle" >0.2599</td><td align="center" valign="middle" >0.2599</td><td align="center" valign="middle" >0.2721</td></tr><tr><td align="center" valign="middle"  rowspan="3"  >K-distribution</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >5.6282</td><td align="center" valign="middle" >−2.1395</td><td align="center" valign="middle" >−2.1395</td><td align="center" valign="middle" >−3.5778</td></tr><tr><td align="center" valign="middle" >10</td><td align="center" valign="middle" >4.7262</td><td align="center" valign="middle" >−0.7711</td><td align="center" valign="middle" >−0.7711</td><td align="center" valign="middle" >−0.8575</td></tr><tr><td align="center" valign="middle" >20</td><td align="center" valign="middle" >3.9462</td><td align="center" valign="middle" >−0.2767</td><td align="center" valign="middle" >−0.2767</td><td align="center" valign="middle" >−0.2820</td></tr></tbody></table></table-wrap><table-wrap id="table4" ><label><xref ref-type="table" rid="table4">Table 4</xref></label><caption><title> AASR<sub>MAX</sub> for four algorithms under three clutter distributions</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >Clutter Distribution</th><th align="center" valign="middle" >Before error compensation</th><th align="center" valign="middle" >SNR (dB)</th><th align="center" valign="middle" >TDCM</th><th align="center" valign="middle" >OSM</th><th align="center" valign="middle" >SSCM</th><th align="center" valign="middle" >APM</th></tr></thead><tr><td align="center" valign="middle"  rowspan="3"  >Log-normal distribution</td><td align="center" valign="middle"  rowspan="3"  >−25.1927</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >−43.2373</td><td align="center" valign="middle" >−46.0874</td><td align="center" valign="middle" >−46.0874</td><td align="center" valign="middle" >−42.6242</td></tr><tr><td align="center" valign="middle" >10</td><td align="center" valign="middle" >−45.7383</td><td align="center" valign="middle" >−50.1350</td><td align="center" valign="middle" >−50.1350</td><td align="center" valign="middle" >−50.4650</td></tr><tr><td align="center" valign="middle" >20</td><td align="center" valign="middle" >−46.9298</td><td align="center" valign="middle" >−51.5807</td><td align="center" valign="middle" >−51.5807</td><td align="center" valign="middle" >−51.4993</td></tr><tr><td align="center" valign="middle"  rowspan="3"  >Weibull distribution</td><td align="center" valign="middle"  rowspan="3"  >−25.1927</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >−35.1346</td><td align="center" valign="middle" >−38.9284</td><td align="center" valign="middle" >−38.9284</td><td align="center" valign="middle" >−33.5966</td></tr><tr><td align="center" valign="middle" >10</td><td align="center" valign="middle" >−39.1445</td><td align="center" valign="middle" >−47.2660</td><td align="center" valign="middle" >−47.1231</td><td align="center" valign="middle" >−46.1919</td></tr><tr><td align="center" valign="middle" >20</td><td align="center" valign="middle" >−40.1673</td><td align="center" valign="middle" >−51.5414</td><td align="center" valign="middle" >−51.5371</td><td align="center" valign="middle" >−51.7242</td></tr><tr><td align="center" valign="middle"  rowspan="3"  >K-distribution</td><td align="center" valign="middle"  rowspan="3"  >−25.1927</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >−36.2404</td><td align="center" valign="middle" >−39.2750</td><td align="center" valign="middle" >−40.0067</td><td align="center" valign="middle" >−34.1553</td></tr><tr><td align="center" valign="middle" >10</td><td align="center" valign="middle" >−40.6513</td><td align="center" valign="middle" >−46.1806</td><td align="center" valign="middle" >−46.6014</td><td align="center" valign="middle" >−42.3101</td></tr><tr><td align="center" valign="middle" >20</td><td align="center" valign="middle" >−40.3331</td><td align="center" valign="middle" >−50.9115</td><td align="center" valign="middle" >−50.5628</td><td align="center" valign="middle" >−49.9990</td></tr></tbody></table></table-wrap><p>The OSM and SSCM use the signal subspace and noise subspaces after eigenvalue decomposition of the correlation matrix, respectively. Assuming L Doppler bins are used to estimate the phase errors, the computational load of OSM and SSCM are 2 LM<sup>3</sup> and LM<sup>3</sup> + M<sup>3</sup>, respectively. Their performances are best under all simulated clutter distribution and SNR conditions.</p><p>In application, when the scenes are homogeneous, such as agricultural and natural areas, APM can be chosen to estimate the channel phase errors for its accuracy and light computational load. In contrast, for heterogeneous scenes such as urban or sea surfaces, OSM and SSCM are suitable for phase error estimation.</p><fig-group id="fig3"><label><xref ref-type="fig" rid="fig3">Figure 3</xref></label><caption><title> Estimation deviations of eight channels versus SNR for the time-domain correlation method (dashed red), the orthogonal subspace method (dashed green), the signal subspace comparison method (dashed black), the antenna pattern method (dashed blue). SNR = 0 dB corresponds to <xref ref-type="fig" rid="fig3">Figure 3</xref>(a), and SNR = 10 dB corresponds to <xref ref-type="fig" rid="fig3">Figure 3</xref>(b).</title></caption><fig id ="fig3_1"><label> (b)</label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/64149x41.png"/></fig><fig id ="fig3_2"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/64149x42.png"/></fig></fig-group><fig-group id="fig4"><label><xref ref-type="fig" rid="fig4">Figure 4</xref></label><caption><title> Estimation deviations of eight channels under SNR = 0 dB. Log-normal distribution clutter corresponds to <xref ref-type="fig" rid="fig4">Figure 4</xref>(a), Weibull distribution clutter corresponds to <xref ref-type="fig" rid="fig4">Figure 4</xref>(b), and K-distribution clutter corresponds to <xref ref-type="fig" rid="fig4">Figure 4</xref>(c).</title></caption><fig id ="fig4_1"><label>(b)</label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/64149x43.png"/></fig><fig id ="fig4_2"><label> (c)</label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/64149x44.png"/></fig><fig id ="fig4_3"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/64149x45.png"/></fig></fig-group></sec></sec><sec id="s5"><title>5. Conclusion</title><p>In this paper, four channel error estimation methods for multichannel HRWS SAR system are compared under different SNR conditions and clutter distributions. From the simulation results, we can conclude that the estimation deviations are not relevant to real phase error distribution, and only relate to SNR and the clutter distribution. In addition, the performance of time-domain correlation method is poorer than the other three methods. For Doppler-domain methods, the APM works as well as the OSM and SSCM for homogeneous clutter scenes, but worse than OSM and SSCM for heterogeneous surfaces. OSM and SSCM work best for all clutter scenes.</p></sec><sec id="s6"><title>Cite this paper</title><p>Tingting Jin,Xiaolan Qiu,Donghui Hu,Chibiao Ding, (2016) Channel Error Estimation Methods Comparison under Different Conditions for Multichannel HRWS SAR Systems. Journal of Computer and Communications,04,88-94. doi: 10.4236/jcc.2016.43014</p></sec></body><back><ref-list><title>References</title><ref id="scirp.64149-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Gebert, N., Krieger, G. and Moreira, A. (2009) Digital Beamforming on Receive: Techniques and Optimization Strategies for High-Resolution Wide-Swath SAR Imaging. IEEE Transactions on Geoscience and Remote Sensing, 45, 564- 592.</mixed-citation></ref><ref id="scirp.64149-ref2"><label>2</label><mixed-citation publication-type="other" xlink:type="simple">Zhang, S.X., Xing, M.D., Xia, X.G., Liu, Y.Y., Guo, R. and Bao, Z. (2013) A Robust Channel-Calibration Algorithm for Multi-Channel in Azimuth HRWS SAR Imaging Based on Local Maximum-Likelihood Weighted Minimum Entropy. IEEE Transactions on Image Processing, 22, 5294-5305. http://dx.doi.org/10.1109/TIP.2013.2274387</mixed-citation></ref><ref id="scirp.64149-ref3"><label>3</label><mixed-citation publication-type="other" xlink:type="simple">Liu, Y.Y., Li, Z.F., Suo, Z.Y. and Bao, Z. (2013) A Novel Channel Phase Bias Estimation Method for Spaceborne Along-Track Multi-Channel HRWS SAR in Time-Domain. IET International Radar Conference, China.</mixed-citation></ref><ref id="scirp.64149-ref4"><label>4</label><mixed-citation publication-type="other" xlink:type="simple">Liu, Y.Y., Li, Z.F., Suo, Z.Y. and Bao, Z. (2010) Adaptive Two-Step Calibra-tion for High Resolution and Wide-Swath SAR Imaging. IET Radar Sonar Navigation, 4, 548-559.</mixed-citation></ref><ref id="scirp.64149-ref5"><label>5</label><mixed-citation publication-type="other" xlink:type="simple">Yang, T.L., Li, Z.F., Liu, Y.Y. and Bao, Z. (2013) Channel Error Estimation Methods for Multichannel SAR Systems in Azimuth. IEEE International Geoscience and Remote Sensing letters, 10, 548-552.  
http://dx.doi.org/10.1109/LGRS.2012.2212873</mixed-citation></ref><ref id="scirp.64149-ref6"><label>6</label><mixed-citation publication-type="other" xlink:type="simple">Yang, T.L., Li, Z.F., Liu, Y.Y., Suo, Z.Y. and Bao, Z. (2013) Channel Error Estimation Methods for Multi-Channel HRWS SAR Systems. IEEE International Geoscience and Remote Sensing Symposium, Australia, 4507-4510.</mixed-citation></ref><ref id="scirp.64149-ref7"><label>7</label><mixed-citation publication-type="other" xlink:type="simple">Kim, J.-H., Younis, M., Prats-Iraola, P., Gabele, M. and Krieger, G. (2013) First Spaceborne Demonstration of Digital Beamforming for Azimuth Ambiguity Suppression. IEEE Trans-actions on Image Processing, 55, 579-590.  
http://dx.doi.org/10.1109/tgrs.2012.2201947</mixed-citation></ref><ref id="scirp.64149-ref8"><label>8</label><mixed-citation publication-type="other" xlink:type="simple">Gebert, N., de Almeida, F.Q. and Krieger, G. (2011) Airborne Demonstration of Multichannel SAR Imaging. IEEE Geoscience and Remote Sensing Letters, 8, 963-967. http://dx.doi.org/10.1109/LGRS.2011.2144563</mixed-citation></ref><ref id="scirp.64149-ref9"><label>9</label><mixed-citation publication-type="other" xlink:type="simple">Zhang, S.X., Xing, M.D., Xia, X.G., Zhang, L., Guo, R., Liao, Y. and Bao, Z. (2014) Multichannel HRWS SAR Imaging Based on Range-Variant Channel Calibration and Mul-ti-Doppler-Direction Restriction Ambiguity Suppression. IEEE Transactions on Geoscience and Remote Sensing, 52, 4306-4327. http://dx.doi.org/10.1109/TGRS.2013.2281329</mixed-citation></ref><ref id="scirp.64149-ref10"><label>10</label><mixed-citation publication-type="other" xlink:type="simple">Li, Z.F., Bao, Z., Wang, H.Y. and Liao, G.S. (2004) Performance Improvement for Constellation SAR Using Signal Processing Techniques. IEEE International Geoscience and Remote Sensing Letters, 1, 436-452.</mixed-citation></ref></ref-list></back></article>