Abstract

Currently, reflectometry-based sea ice detection methods rely on observables extracted from delay-Doppler maps (DDM)s, which are sensitive to ice in the specular zone. Due to the size of the glistening zone, the transition from open seas to sea ice in the specular zone can take up to 10 s for satellite platforms and no methods exist that can process this. In this article, using DDMs collected by TechDemoSat-1, we demonstrate that this transition is comprised of a response that is fixed in the spatial domain, at the ice edge, and moving in the delay-Doppler domain. This is the first observation of persistent nonspecular coherent reflections from sea ice. The delay-Doppler trajectory of the ice response is shown to correspond with a point that is located on the ambiguity free line. Furthermore, the response is point-like as it suffers from delay and Doppler walk suggesting that it originates from a small spatial footprint, i.e., the first (few) Fresnel zone(s). Exploiting these facts, we then propose a technique that integrates the ice response in the spatial domain after preprocessing. This results in the edges of the ice sheet being emphasized as all of the power received during the transition phase maps to the edge of the sheet. We also propose to compensate for the delay-Doppler walk during preprocessing by modifying Woodward's ambiguity function when deconvolution is performed.

Highlights

  • E ARLY work demonstrated that detecting sea ice using airborne [1], [2] and spaceborne (UK-DMC) [3] GNSS-R receivers was possible

  • Using multiple observables extracted from the specular zone, Yan and Huang [6] presented a method for sea ice detection in delay-Doppler map (DDM) collected by TechDemoSat-1 (TDS-1)

  • The shape of the marker indicates the type of DDM corresponding to that epoch: a triangle indicates a clutter-only DDM; a circle indicates a mixed DDM containing clutter and the transitioning ice; and a star indicates a specular ice-only DDM

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Summary

INTRODUCTION

E ARLY work demonstrated that detecting sea ice using airborne [1], [2] and spaceborne (UK-DMC) [3] GNSS-R receivers was possible. Using multiple observables extracted from the specular zone, Yan and Huang [6] presented a method for sea ice detection in DDMs collected by TechDemoSat-1 (TDS-1). These observables describe the spread of the signal, and, if the DDM does not present a significant spread, it is classified as an ice Manuscript received June 11, 2019; revised August 20, 2019; accepted September 20, 2019. We compensate for the spatially variant blurring of χ2 [13] in the DD domain during the deconvolution process Using this method, it is possible to construct ice sheet maps using different receivers, specular point tracks and temporally separate (within reason) DDMs as the integration is performed in the spatial domain. This is the first observation of persistent nonspecular scattering off sea ice in GNSS-R observables

SEA ICE IN DDM SEQUENCES
DYNAMICS ANALYSIS
PROCESSING DDMS
INCOHERENT INTEGRATION
RESULTS
DISCUSSION
VIII. CONCLUSION
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