FN Archimer Export Format PT J TI Heat flow in the Western Mediterranean: Thermal anomalies on the margins, the seafloor and the transfer zones BT AF Poort, Jeffrey Lucazeau, Francis Le Gal, Virginie Dal Cin, Michaela LEROUX, Estelle Bouzid, Abderrezak RABINEAU, Marina Palomino, Désirée Battani, Anne Akhmanov G., Grigory Ferrante G., Matilde Gafurova R., Dina Si Bachir, Roza Koptev, Alexander Tremblin, Maxime Bellucci, Massimo PELLEN, Romain Camerlenghi, Angelonghi MIGEON, Sebastien Alonso, Belen Ercilla, Gemma Yelles-Chaouche A., Karim Khlystov M., Oleg AS 1:1;2:2;3:1,3;4:4;5:5;6:6;7:7;8:8;9:3;10:9;11:4;12:9;13:6;14:1;15:1;16:7;17:5;18:4;19:10;20:11;21:11;22:6;23:12; FF 1:;2:;3:;4:;5:PDG-REM-GM-LGS;6:;7:;8:;9:;10:;11:;12:;13:;14:;15:;16:;17:;18:;19:;20:;21:;22:;23:; C1 Sorbonne Université, CNRS, Institut des Sciences de la Terre de Paris, ISTeP, Paris, France Université de Paris, Institut de Physique du Globe de Paris, CNRS, Paris, France IFP Energies nouvelles, Geosciences, Rueil-Malmaison, France Istituto Nazionale di Oceanografia e di Geofisica Sperimentale (OGS), Trieste, Italy IFREMER, 1625 Route de Sainte-Anne, 29280 Plouzané, France Centre de Recherche en Astronomie Astrophysique et Géophysique (CRAAG), Alger, Algeria Institut Universitaire Européen de la Mer (IUEM), Université de Bretagne Occidentale, Laboratoire Domaines Océaniques, UMR CNRS 6538, Plouzané, France Spanish Institute of Oceanography (IEO), Oceanographic Center of Málaga, Málaga, Spain UNESCO Centre on Marine Geology and Geophysics, Moscow State University, Geology Faculty, Moscow, Russia Université Côte d'Azur, CNRS, Observatoire de la Côte d'Azur, IRD, Géoazur UMR 7329, Valbonne, France Institut de Ciències del Mar (ICM), CSIC, Continental Margins Group, Barcelona, Spain Limnological Institute, Siberian Branch of the Russian Academy of Sciences, Irkutsk, Russia C2 UNIV PARIS 06, FRANCE IPGP, FRANCE IFP ENERGIES NOUVELLES, FRANCE OGS, ITALY IFREMER, FRANCE CRAAG, ALGERIA CNRS, FRANCE IEO, SPAIN UNESCO, RUSSIA UNIV NICE, FRANCE ICM CSIC, SPAIN RUSSIAN ACAD SCI, RUSSIA SI BREST SE PDG-REM-GM-LGS UM LGO IN WOS Ifremer UPR copubli-france copubli-europe copubli-univ-france copubli-int-hors-europe copubli-sud IF 3.548 TC 16 UR https://archimer.ifremer.fr/doc/00588/70052/67992.pdf LA English DT Article CR WESTMEDFLUX BO L'Atalante DE ;Heat flow;Western Mediterranean Sea;Liguro-Provencal basin;Algero-Balearic basin;Continental margins;Oceanic crust AB The Western Mediterranean basin has been formed by Miocene back-arc extension and is underlain by a thin and young lithosphere. This young lithosphere is warm, as testified by an overall elevated offshore heat flow. Heat flow within the Western Mediterranean is, however, highly variable and existing data are unevenly distributed and poorly studied in the central part of the Liguro-Provençal and Algero-Balearic basins. This central part is floored by a young oceanic crust, bordered by different continental margins, cut by transform faults, and filled by up to 8 km of sediments. We present a total of 148 new heat flow data collected during the MedSalt and WestMedFlux cruises in 2015 and 2016 and aligned along seven regional profiles that show an important heat flow variability on the basin-scale, but also locally on the margins. A new heat flow map for the Western Mediterranean outlines the following regional features: (1) a higher average heat flow in the Algero-Balearic basin compared to the Liguro-Provençal basin (94 ± 13 mW/m2 and 78 ± 16 mW/m2, respectively), and (2) a regional thermal asymmetry in both basins, but with opposed heat flow trends. Up to 20% of this heat flow difference can be explained by sediment blanketing, but age and heterogeneity of ocean crust due to an asymmetric and polyphased opening of the basins are believed to have given the major thermal imprint. Estimates of the age of the oceanic crust based on the new heat flow suggest a considerably younger West Algerian basin (16–23 Ma) compared to the East Algerian basin and the West Sardinia oceanic floor (31–37 Ma). On the margins and ocean-continent transitions of the Western Mediterranean the new heat flow data point out the existence of two types of local anomalies (length scale 5–30 km): (1) locally increased heat flow up to 153 mW/m2 on the Gulf of Lion margin results from thermal refraction of large salt diapirs, and (2) the co-existing of both low (<50 mW/m2) and high (>110 mW/m2) heat flow areas on the South Balearic margin suggests a heat redistribution system. We suspect the lateral heat advection is resulting from a regional fluid circulation in the sediments associated to the widespread Plio-Pleistocene volcanism on the South Balearic margin. PY 2020 PD JAN SO Marine Geology SN 0025-3227 PU Elsevier BV VL 419 UT 000508490400012 DI 10.1016/j.margeo.2019.106064 ID 70052 ER EF