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HF radar is widely used to measure ocean currents and, to a somewhat lesser extent, to provide estimates of wave height and the
directional spectrum of surface gravity waves. Its two principal forms ΓΆΒ?Β?HF surface wave radar and HF sky wave radar ΓΆΒ?Β?exploit
the corresponding propagation modes to sample the space-time geometry of the ocean surface over regions of the order 104 km2
and106 km2 respectively, with spatial resolution typically 100-101 km, sensing echo contributions from metre-scale phenomena up
to synoptic-scale and updating on a timescale of seconds or minutes. Surprisingly, despite the proliferation of HF radar systems, with
perhaps 500 HF radars presently in operation, on every continent, the scope of the standard remote sensing missions has remained
almost unchanged since the first commercial systems were deployed some 40 years ago. This contrasts with the intrinsic measurement
capabilities afforded by developments in radar and computing technology, which have improved by orders of magnitude. To counter
this conservatism, the HF radar research group at the University of Adelaide is pursuing an ambitious research program seeking to
expand the palette of missions, using state-of-the-art computer modelling of a wide variety of oceanic and atmospheric processes,
together with advanced electromagnetics, to establish the associated HF radar signatures and to develop advanced signal processing
techniques for extraction of this information from radar echoes in real-time. In several cases, the predictions have been validated
with experimental measurements. This paper will review these recent developments, illustrated by examples including the detection
of internal waves, the observation of nonlinear wave interactions including the Benjamin-Feir instability and Fermi-Pasta-Ulam
recurrence, the non-adiabatic wave field response to tropical convective cells, and the prospect of detecting algal blooms and related
surfactant effects.