2019
DOI: 10.1109/jstars.2019.2932019
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Polarimetric Calibration of RISAT-1 Compact-Pol Data

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Cited by 14 publications
(7 citation statements)
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“…On the other hand, according to (8), the calibrated SAR data and the SAR data to be calibrated can be expressed as σ vh1 = 0.095(0.13 + sin 1.5θ 1 ) 1.4 (1 − exp(−1.3(ks) 0.9 ))σ 0 vv1 (10) σ vh2 = 0.095(0.13 + sin 1.5θ 1 ) 1.4 (1 − exp(−1.3(ks) 0.9 ))σ 0 vv2 (11) By dividing (10) with (11) and combining (9), we can obtain Rewriting (12), the relationship between the calibrated SAR data and the SAR data to be calibrated in VV polarization can be expressed as σ vv1 = cos(θ 1 ) 2.2 (0.13 + sin 1.5θ 2 ) 1.4 cos(θ 2 ) 2.2 (0.13 + sin 1.5θ 1 ) 1.4 σ vv2 (13) The derived backscattering coefficients in ( 9) and ( 13) can then be used to calibrate the SAR satellite data to be calibrated.…”
Section: Correction Of Imaging Parameter Differencesmentioning
confidence: 99%
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“…On the other hand, according to (8), the calibrated SAR data and the SAR data to be calibrated can be expressed as σ vh1 = 0.095(0.13 + sin 1.5θ 1 ) 1.4 (1 − exp(−1.3(ks) 0.9 ))σ 0 vv1 (10) σ vh2 = 0.095(0.13 + sin 1.5θ 1 ) 1.4 (1 − exp(−1.3(ks) 0.9 ))σ 0 vv2 (11) By dividing (10) with (11) and combining (9), we can obtain Rewriting (12), the relationship between the calibrated SAR data and the SAR data to be calibrated in VV polarization can be expressed as σ vv1 = cos(θ 1 ) 2.2 (0.13 + sin 1.5θ 2 ) 1.4 cos(θ 2 ) 2.2 (0.13 + sin 1.5θ 1 ) 1.4 σ vv2 (13) The derived backscattering coefficients in ( 9) and ( 13) can then be used to calibrate the SAR satellite data to be calibrated.…”
Section: Correction Of Imaging Parameter Differencesmentioning
confidence: 99%
“…12) This work is licensed under a Creative Commons Attribution 4.0 License. For more information, see https://creativecommons.org/licenses/by/4.0/…”
mentioning
confidence: 99%
“…Different polarimetric decomposition and classification techniques are widely used to extact information from the PolSAR data sets (Kumar et al., 2020; Ullmann et al., 2016), but the polarimetric distortions present in the PolSAR data sets leads to wrong results from the polarimetric decomposition and classification models (Kumar et al., 2021), which in turn result in the ground target misinterpretation (Jung & Park, 2018; Maiti et al., 2021). The most important of the polarimetric distortions is the channel imbalance, crosstalk, and Faraday rotation errors (Babu et al., 2019a). The channel imbalance between the different polarizations occurs mainly due to the gain mismatch between the power amplifiers used for horizontal and vertical transmission of the electromagnetic waves.…”
Section: Introductionmentioning
confidence: 99%
“…These errors relatively contribute to an increased magnitude of cross‐pol images resulting in overestimation of volume scattering properties (Chang et al., 2018). In addition, the amplitude or phase unconformity of different polarization channels cause imbalance in the transmission or reception of antenna gain (Babu et al., 2019). Coming to the influence of imbalance on the PolSAR images, there are two categories: (a) co‐pol channel imbalance and (b) cross‐pol channel imbalance.…”
Section: Introductionmentioning
confidence: 99%