Red and orange iron-stained sands of relatively recent age occur widely in both coastal dunefields and continental deserts in the tropics and subtropics. Red desert dune sands have been described from elsewhere ( Figure 1). Not all tropical and subtropical dunes are red, but in general aeolian red sands are more common in these areas than in temperate and high latitudes.The question of the nature and significance of red sediments in general has concerned geologists for many years, since reddening is often an important process associated with diagenesis, and because ancient red sediments occur widely in the geological record (Van Houten, 1973). The debate concerning red sediments has centred around two main questions; first, the nature of the climatic conditions which best favour reddening, and hence the palaeoclimatic inferences which can be drawn from fossil red beds; and, second, the role of time in the reddening process.Several authors have discussed these issues with reference to recent sediments in particular areas (e.g. Norris, 1969; Folk, 1976;Walker, 1979), but little attention has been given to patterns of reddening at the wider global scale.The purpose of this paper is to review the present state of knowledge regarding the nature, origin and palaeoclimatic significance of red dune sands within the context of late Quaternary environmental change. The paper is therefore concerned with reddening of sands under subaerial conditions rather than at high temperature and pressures. Processes of reddening during diagenesis have recently been reviewed by Walker (1976) and Turner (1980) in relation to the general problem of continental red beds. The discussion stems in part from recent investigations carried out by the authors on red dune sands in southern India and northeast Australia. These investigations will be described in more detail elsewhere.
IThe nature of red dune sands .