“…Satellite scatterometers generally provide high-quality vector winds over the global ocean surface, such that they have been widely used in the study of TC structure and location [10][11][12][13]. Notably the Ku-band pencil-beam scatterometers, such as SeaWinds onboard QuikSCAT [14], OSCAT onboard the Indian Oceansat-2 [15] and SCATSat-1 satellites [16], and HSCAT on the Chinese HY-2 satellite series [17], are with wide observation swaths of ~1800 km, making them more likely to acquire the entire TC structure in a single overpass than the C-band fixed fan-beam scatterometers, e.g., Advanced Scatterometers (ASCAT) onboard the MetOp satellite series [18]. However, due to signal saturation in the (co-polarized) radar backscatter measurements, both C-and Ku-band scatterometer extreme wind speeds show large errors.…”