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Radar Scattering Features Under High Wind Conditions From Spaceborne Quad-Polarization SAR Observations  id статьи: 3200
Тип публикации
статья в журнале
Язык
En
Журнал
IEEE Transactions on Geoscience and Remote Sensing

ISSN:01962892
Год
2024
Выходные данные
том 62
выпуск
страницы № 4207309
Авторы
Fan, Shengren2
Zhang, Biao3
Perrie, William1
EDN
Абстракт
This study examines the impact of wave breaking (WB) and Bragg scattering on the normalized radar cross section (NRCS) to reveal radar scattering features during high wind conditions. This is conducted by decomposing C-band quasi-synchronous wide-swath quad-polarization synthetic aperture radar (SAR) observations acquired from the RADARSAT Constellation Mission (RCM) and RADARSAT-2 (RS-2). The analysis results clearly demonstrate that the polarization difference (PD) associated with Bragg scattering saturates at high wind speeds, while still maintaining azimuthal modulation. Notably, the radar returns from breaking waves at cross-polarization (HV or VH) exhibit higher sensitivity to wind speeds but lower sensitivity to wind direction, compared to co-polarization (HH or VV). Moreover, our analyses show that WB contributes 40%, 80%, and 90% of VV-, HH-, and HV-polarized NRCS, respectively. This study highlights the unique capabilities provided by collocated RCM and RS-2 observations for investigating radar scattering features under high wind conditions. Results of this study can be further used to develop empirical models for estimating co- and cross-polarization radar backscatters induced by WB under high wind speeds
Ключевые слова
High wind conditions, quad-polarization, synthetic aperture radar (SAR) observations, wave breaking (WB)
Дата занесения
2024-08-24 11:10:05
Scopus
Статус есть
Квартиль Q1
WoS
Статус есть
Квартиль Q1
РИНЦ
Статус нет
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12
количество баллов каждому автору
3
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Финансирование:

42076181

U2106211

FSZU-2020-0005

SOLZSKY2024005