Abstract

In this paper, we presented a method for retrieving sea surface wind speed (SSWS) from Sentinel-1 synthetic aperture radar (SAR) horizontal-horizontal (HH) polarization data in extra-wide (EW) swath mode, which have been extensively acquired over the Arctic for polar monitoring. In contrast to the conventional algorithm, i.e., using a geophysical model function (GMF) to retrieve SSWS by spaceborne SAR, we introduced an alternative retrieval method based on a GMF-guided neural network. The SAR normalized radar cross section, incidence angle, and wind direction are used as the inputs of a back propagation (BP) neural network, and the output is the SSWS. The network is developed based on 11,431 HH-polarized EW images acquired in the marginal ice zone (MIZ) of the Arctic from 2015 to 2018 and their collocated scatterometer wind measurements. Verification of the neural network based on the testing dataset yields a bias of 0.23 m/s and a root mean square error (RMSE) of 1.25 m/s compared to the scatterometer wind data for wind speeds less than approximately 30 m/s. Further comparison of the SAR retrieved SSWS with independent buoy measurements shows a bias and RMSE of 0.12 m/s and 1.42 m/s, respectively. We also analyzed the uncertainty of the retrieval when reanalysis model wind direction data are used as inputs to the neural network. By combining the detected sea ice cover information based on SAR data, sea ice and marine-meteorological parameters can be derived simultaneously by spaceborne SAR at a high spatial resolution in the Arctic.

Highlights

  • The retrieval of sea surface wind by spaceborne synthetic aperture radar (SAR) has been studied for a few decades

  • We presented a method for retrieving sea surface wind speed (SSWS) from S1 EW data in HH polarization based on a back propagation (BP) neural network

  • Unlike the data acquired over other sea areas where most EW mode data are a combination of VV and vertical−horizontal (VH) polarizations, the EW data acquired in the Arctic are a combination of HH and HV polarizations for intensive monitoring of sea ice

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Summary

Introduction

The retrieval of sea surface wind by spaceborne synthetic aperture radar (SAR) has been studied for a few decades. Different GMFs for C-band radar (often called CMOD) data with vertical-vertical (VV) polarization have been proposed and are widely exploited to acquire sea surface wind fields at a high spatial resolution, e.g., from the CMOD4, CMOD5, and CMOD5.N to the currently used CMOD7 [1,2,3,4,5] and CMOD_IFR2 [6]. When spaceborne SAR satellites operating at different microwave frequencies from C-band are in orbit, the functions in (1) must be refined to make them suitable for retrieving sea surface wind fields, e.g., the LMOD [13] for the L-band Advanced Land Observing Satellite (ALOS)/Phased Array L-band synthetic aperture radar (PALSAR) and the XMOD [14] for the X-band TerraSAR-X and TanDEM-X. Compared with ASCAT (2277 S1 images from June to December 2018 in the Arctic MIZ)

Methods
S1 Data Acquired in the Arctic
ASCAT Wind Data
In Situ Data
Collocation of S1 Data with in situ Data
Establishing and Training the BP Neural Network
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Findings
Conclusion
Full Text
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