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We introduce the concepts and techniques relevant to determining evidence for the so-called Head-Tail asymmetry from neutron-induced nuclear recoil tracks in the DRIFT-II dark matter detector. The back-to-back dual TPC arrangement in DRIFT makes this detector ideal for Head-Tail tests, allowing systematic errors to be reduced. The detection of Head-Tail asymmetry can open a powerful new means of searching for a galactic signature from WIMPs.

Techniques for Head-Tail directional recoil measurements in the DRIFT-II dark matter detector