dot
Detailansicht
Katalogkarte GBA
Katalogkarte ISBD
Suche präzisieren
Drucken
Download RIS
Hier klicken, um den Treffer aus der Auswahl zu entfernen
Titel Geothermal heat flux and basal melt rate in the Dome C region inferred from radar reflectivity and thermal modelling.
VerfasserIn Olivier Passalacqua, Catherine Ritz, Frédéric Parrenin, Stefano Urbini, Massimo Frezzotti
Konferenz EGU General Assembly 2017
Medientyp Artikel
Sprache en
Digitales Dokument PDF
Erschienen In: GRA - Volume 19 (2017)
Datensatznummer 250141164
Publikation (Nr.) Volltext-Dokument vorhandenEGU/EGU2017-4640.pdf
 
Zusammenfassung
Basal melt rate is the most important physical quantity to be evaluated when looking for an old-ice drilling site, and it strongly depends on the geothermal heat flux, which is poorly known under the East Antarctic ice sheet. The wetness of the ice-bed interface can be assessed from radar echoes on the bedrock, considering that a wet bedrock has a stronger reflectivity than a dry one. But, as the basal conditions depends on the climatic forcing lagged by the thick ice, the basal ice may be cold today whereas it was in average temperate in the past. Accordingly, the risk of mismatch between present and past conditions must be evaluated, and more generally the geothermal heat flux and basal melt rate in the Dome C region. Here, we run a 1D heat model over the last 800 ka in inverse mode to constrain the value of geothermal heat flux by assessing a critical ice thickness, i.e. the minimum ice thickness that would allow the local melting distribution at present. A regional map of the geothermal heat flux is then inferred on a 80 km×130 km area, and shows a N-S-oriented gradient, with a value range of 48 − 60 mW m−2. The forward model is then emulated by a polynomial function, to compute a time-averaged value of the basal melt rate, spatially variable over the region. Two main subregions appear to be free of basal melting because of the thin overlying ice, and a third one, north of Dome C, because of a low geothermal heat flux.