This iconic right-hand, point-break is nestled in an ideal location on the Surf Coast of Victoria to harness both wind and swell. Its reliable conditions have established it as a world-class competition venue and a treasured home-break for countless surfers over the decades. In this article, I'm going to dive into the key elements that have made this wave so legendary.
The Southern Ocean stretching between Australia and Antarctica, and extending west into the South Indian Ocean, is one of the most active zones on the planet for storm activity. These storms are strongest and most frequent from April through September (the Southern Hemisphere's winter months), but swell-producing systems can develop at any time of year.
Storms that develop a strong and well-aimed fetch between 224° SW and 196° SSW are ideal for Bells, as there are no obstructions for inbound swell. Due to the orientation of Bells (generally facing southeastward), incoming swell west of 224° will feel a degree of shadowing by Australia itself - the more west, the more it will be shadowed, and therefore less energy making it into Bells. Swells east of 196° will feel partial shadowing by islands off the coast of Tasmania, then blocked by Tasmania east of 175°.
An offshore underwater ridge stretching to the south will help to refract a greater share of the inbound swell toward the gradually rising rock reef at Bells. While it isn’t a classic point break, the waves often act like one—concentrating their energy at the top of the reef where it peaks. From there, the local bathymetry takes over, guiding the swell as it refracts from the deeper bay into the shallower reef along the point, producing the long, clean right-hand lines Bells is known for.
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