2017 IEEE Radar Conference (RadarConf) 2017
DOI: 10.1109/radar.2017.7944460
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Sentinel-1 SAR system and mission

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Cited by 15 publications
(6 citation statements)
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“…Sentinel 1 instrument noise floor diminishes sensitivity for low σ 0 . Instrument performance for the IW mode has a marked dependence with incidence angle (Torres et al, 2017). In effect, noise floor is about -25 dB at 35°which prevented sensitivity in the VH polarized returned power for the soft crust (Figure 4(a)).…”
Section: Resultsmentioning
confidence: 99%
“…Sentinel 1 instrument noise floor diminishes sensitivity for low σ 0 . Instrument performance for the IW mode has a marked dependence with incidence angle (Torres et al, 2017). In effect, noise floor is about -25 dB at 35°which prevented sensitivity in the VH polarized returned power for the soft crust (Figure 4(a)).…”
Section: Resultsmentioning
confidence: 99%
“…Crust Type 1 Instrument noise floor diminishes sensitivity for weak backscatters. As for Sentinel-1, instrument performance for the IW mode has a marked dependence on the incidence angle [35], with a noise floor better than −28.8 dB at VH at the incidence angle of the observations. ALOS-2/PALSAR-2 noise floor is −36 dB at HH and −46 dB at HV, far beyond the lower backscattering coefficients found in the study area [36].…”
Section: Sampling Site Id Rms Height S [Cm] Correlation Length L [Cm]...mentioning
confidence: 89%
“…Sentinel 1 instrument noise floor reduced sensitivity for low σ 0 such as those measured at VH polarization. Instrument performance for the IW mode has a marked dependence with the incidence angle [31]. In effect, the noise floor is about −25 dB at 35 • and marginally improves to about −27 dB at angles between 39 • and 40 • , which implied a precise VH-polarized returned power from the rougher crusts solely.…”
Section: Discussionmentioning
confidence: 99%