Mots-clés
Australie ; Calcaire ; Dissolution karstique ; Distribution spatiale ; Karst ; Météorisation ; Niveau marin ; Nullarbor Plain ; Paléokarst ; Roche carbonatée ; Réseau karstique ; Topographie ; Trou souffleur ; Western AustraliaAustralia ; Blowhole ; Carbonate dissolution ; Carbonate rock ; Karst ; Karst network ; Limestone ; Palaeokarst ; Sea level ; Spatial distribution ; Topography ; Weathering ; Western AustraliaAustralia ; Australia Occidental ; Caliza ; Disolución kárstica ; Distribución espacial ; Karst ; Meteorización ; Nivel del mar ; Paleokarst ; Red kárstica ; Roca carbonatada ; TopografíaOrigin and karst geomorphological significance of the enigmatic Australian Nullarbor Plain blowholes
Auteur(s) et Affiliation(s)
DOERR, S.H.
School of the Environment and Society, Univ., Swansea, Royaume-Uni
DAVIES, R.R.
School of Earth Sciences, Victoria Univ., Wellington, Nouvelle-Zelande
LEWIS, A.
Terradat UK Ltd, Cardiff, Royaume-Uni
PILKINGTON, G.
CEGSA (Cave Exploration Group, South Australia), Rundle Mall, Australie
WEBB, J.A.
Environmental Geoscience, La Trobe Univ., Victoria, Australie
ACKROYD, P.J.
CEGSA (Cave Exploration Group, South Australia), Rundle Mall, Australie
BODGER, O.
School of Medicine, Univ., Swansea, Royaume-Uni
Description :
To elucidate blowhole distribution and mode of formation the AA. : (1) correlated existing location data with Shuttle Radar Topography Mission (SRTM) data, which distinguishes the subtle undulations (<10m per km) of the landscape, (2) surveyed blowhole morphology and (3) determined their rock surface hardness. The distribution of these enigmatic blowholes is not correlated with present topography. Blowholes are often connected to typically shallow cavities, which exhibit numerous ‘cupolas’ (dome-shaped pockets) in their ceilings. Hardness measurements indicate that salt weathering is not their main cause. The observations suggest that blowholes do not develop downwards, but occur where a cupola breaks through the surface. Lowering of the land surface is suggested to be the main cause for this breakthrough. Although cupolas may undergo some modification under the current climate, they, as well as the shallow caves they are formed in, are likely to be palaeokarst features formed under a shallower water table and wetter conditions in the past. The findings presented have implications for theories of dissolutional forms development in caves worldwide.
Type de document :
Article de périodique
Source :
Earth surface processes and landforms, issn : 0197-9337, 2012, vol. 37, n°. 3, p. 253-261, nombre de pages : 9, Références bibliographiques : 28 ref.
Date :
2012
Editeur :
Pays édition : Royaume-Uni, Chichester, Wiley
Langue :
Anglais
Anglais
Droits :
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Tous droits réservés © Prodig - Bibliographie Géographique Internationale (BGI)