@article {Cameselle,
	title = {{Large-scale margin collapse during Messinian early sea-level drawdown: The SW Valencia Trough, NW Mediterranean}},
	journal = {Basin Research},
	year = {Submitted},
	keywords = {for review purposes only},
	doi = {10.1111/bre.12170},
	author = {Cameselle, Alejandra L and Urgeles, R}
}
@book {Sassa2014,
	title = {{Landslide Science for a Safer Geoenvironment}},
	volume = {2},
	year = {2014},
	pages = {483{\textendash}489},
	publisher = {Springer International Publishing},
	organization = {Springer International Publishing},
	address = {Cham},
	keywords = {ardizzone, cardinali f, f, fiorucci f, geological layers slip ellipsoid, GIS, guzzetti, i, marchesini m, santangelo m, slope stability open source},
	isbn = {978-3-319-05049-2},
	doi = {10.1007/978-3-319-05050-8},
	url = {http://link.springer.com/10.1007/978-3-319-05050-8},
	author = {Marchesini, Ivan and Mergili, Martin and Rossi, Mauro and Santangelo, Michele and Cardinali, Mauro and Ardizzone, Francesca and Fiorucci, Federica and Schneider-muntau, Barbara and Fellin, Wolfgang and Guzzetti, Fausto},
	editor = {Sassa, Kyoji and Canuti, Paolo and Yin, Yueping}
}
@article {Cameselle2014,
	title = {{Late Miocene sedimentary architecture of the Ebro Continental Margin (Western Mediterranean): implications to the Messinian Salinity Crisis}},
	journal = {International Journal of Earth Sciences},
	volume = {103},
	number = {2},
	year = {2014},
	pages = {423{\textendash}440},
	keywords = {Ebro, Erosion, Mediterranean, Messinian, Miocene, Sea level},
	issn = {1437-3254},
	doi = {10.1007/s00531-013-0966-5},
	url = {http://link.springer.com/10.1007/s00531-013-0966-5},
	author = {Cameselle, Alejandra L and Urgeles, R and De Mol, B and Camerlenghi, Angelo and Canning, Jason C}
}
@article {Cameselle2013,
	title = {{Late Miocene sedimentary architecture of the Ebro Continental Margin (Western Mediterranean): implications to the Messinian Salinity Crisis}},
	journal = {International Journal of Earth Sciences},
	volume = {103},
	number = {2},
	year = {2013},
	month = {nov},
	pages = {423{\textendash}440},
	abstract = {The Messinian Salinity Crisis (MSC) resulted from a significant multi-phase drop and subsequent reflooding of the Mediterranean Sea from 5.96 to 5.33 Ma. Well-developed drainage networks, characterized by step-like profiles and abrasion platforms, are associated to this event. The Ebro Continental Margin (Western Mediterranean) presents an additional complexity since the capture of the drainage of the adjacent subaerial Ebro Basin took place sometime prior to the Messinian stage. Using 3D seismic reflection data, this work provides new insights into the origin of the step-like profile of the Messinian erosional surface (MES) and timing of the capture of the subaerial Ebro Basin. The results obtained indicate a sedimentary-active continental slope and delta progradation during Middle-Late Miocene, in a normal regressive context associated to a pre-Messinian proto-Ebro River. The mature development attained by the Messinian Ebro River network during the MSC corroborates that the capture of the Ebro Basin occurred prior to the MSC. The configuration of the clinoforms below the MES suggests that deltaic sediments of the Messinian Paleo-Ebro River deposited during the Tortonian and initial Messinian sea-level drawdown. The MES formed at the top of the Tortonian Highstand, where a fluvial network was deeply carved, and in the topset region of the Messinian Falling Stage Systems Tract, where minor erosion occurred. Fluvial deposits are outstandingly preserved on the main valleys of the MES. Therefore, the step-like profile of the MES was not created during Zanclean inundation, but during the latest stages of the main Messinian sea-level fall and lowstand. {\textcopyright} 2013 Springer-Verlag Berlin Heidelberg.},
	keywords = {Ebro, Erosion, Mediterranean, Messinian, Miocene, Sea level},
	issn = {1437-3254},
	doi = {10.1007/s00531-013-0966-5},
	url = {http://www.scopus.com/inward/record.url?eid=2-s2.0-84894260158\&partnerID=tZOtx3y1},
	author = {Cameselle, Alejandra L. and Urgeles, Roger and De Mol, Ben and Camerlenghi, Angelo and Canning, Jason C.}
}
@booklet {Volpi2013,
	title = {{Late Neogene to Recent seafloor instability on the deep Pacific margin of the Antarctic Peninsula}},
	year = {2013},
	month = {mar},
	publisher = {SEPM (Society for Sedimentary Geology)},
	abstract = {17 pages, 12 figures, 1 table},
	keywords = {Antarctic Peninsula, contourite sedimentation, Pacific margin, Slope instability},
	isbn = {isbn: 978-1-56576-287-9},
	url = {http://digital.csic.es/handle/10261/72631},
	author = {Volpi, Valentina and Amblas, David and Camerlenghi, Angelo and Canals, Miquel and Rebesco, M. and Urgeles, Roger}
}
@article {LoIacono2012a,
	title = {{Large, deepwater slope failures: Implications for landslide-generated tsunamis}},
	journal = {Geology},
	volume = {40},
	number = {10},
	year = {2012},
	month = {aug},
	pages = {931{\textendash}934},
	abstract = {Deepwater landslides are often underestimated as potential tsunami triggers. The North Gorringe avalanche (NGA) is a large (\~{}80 km3 and 35 km runout) newly discovered and deepwater (2900 m to 5100 m depth) mass failure located at the northern fl ank of Gorringe Bank on the southwest Iberian margin. Steep slopes and pervasive fracturing are suggested as the main preconditioning factors for the NGA, while an earthquake is the most likely trigger mechanism. Near-fi eld tsunami simulations show that a mass failure similar to the NGA could generate a wave >15 m high that would hit the south Portuguese coasts in \~{}30 min. This suggests that deepwater landslides require more attention in geo-hazard assessment models of southern Europe, as well as, at a global scale, in seismically active margins. {\textcopyright} 2012 Geological Society of America.},
	issn = {0091-7613},
	doi = {10.1130/G33446.1},
	url = {http://www.scopus.com/inward/record.url?eid=2-s2.0-84868693659\&partnerID=tZOtx3y1},
	author = {Lo Iacono, C. and Gr{\`a}cia, E. and Zaniboni, F. and Pagnoni, G. and Tinti, S. and Bartolome, R. and Masson, D. G. and Wynn, R. B. and Lourenco, N. and Pinto de Abreu, M. and Danobeitia, J. J. and Zitellini, N.}
}
@article {Miensopust2011,
	title = {{Lithospheric structures and Precambrian terrane boundaries in northeastern Botswana revealed through magnetotelluric profiling as part of the Southern African Magnetotelluric Experiment}},
	journal = {Journal of Geophysical Research},
	volume = {116},
	number = {B2},
	year = {2011},
	month = {feb},
	pages = {B02401},
	abstract = {Within the framework of the Southern African Magnetotelluric Experiment a focused study was undertaken to gain improved knowledge of the lithospheric geometries and structures of the westerly extension of the Zimbabwe craton (ZIM) into Botswana, with the overarching aim of increasing our understanding of southern African tectonics. The area of interest is located in northeastern Botswana, where Kalahari sands cover most of the geological terranes and very little is known about lithospheric structures and thicknesses. Some of the regional-scale terrane boundary locations, defined based on potential field data, are not sufficiently accurate for local-scale studies. Investigation of the NNW-SSE orientated, 600 km long ZIM line profile crossing the Zimbabwe craton, Magondi mobile belt, and Ghanzi-Chobe belt showed that the Zimbabwe craton is characterized by thick (\~{}220 km) resistive lithosphere, consistent with geochemical and geothermal estimates from kimberlite samples of the nearby Orapa and Letlhakane pipes (\~{}175 km west of the profile). The lithospheric mantle of the Ghanzi-Chobe belt is resistive, but its lithosphere is only about 180 km thick. At crustal depths a northward dipping boundary between the Ghanzi-Chobe and the Magondi belts is identified, and two middle to lower crustal conductors are discovered in the Magondi belt. The crustal terrane boundary between the Magondi and Ghanzi-Chobe belts is found to be located further to the north, and the southwestern boundary of the Zimbabwe craton might be further to the west, than previously inferred from the regional potential field data. Copyright 2011 by the American Geophysical Union.},
	issn = {0148-0227},
	doi = {10.1029/2010JB007740},
	url = {http://www.scopus.com/inward/record.url?eid=2-s2.0-79951472921\&partnerID=tZOtx3y1},
	author = {Miensopust, M. P. and Jones, A. G. and Muller, M. R. and Garcia, X. and Evans, R. L.}
}
@article {LoIacono2010,
	title = {{Large-scale bedforms along a tideless outer shelf setting in the western Mediterranean}},
	journal = {Continental Shelf Research},
	volume = {30},
	number = {17},
	year = {2010},
	month = {oct},
	pages = {1802{\textendash}1813},
	abstract = {High-resolution multibeam swath-bathymetry and sediment samples were collected across the outer shelf region of the Columbretes Islands (southern Ebro continental shelf, western Mediterranean Sea). Bathymetric data from the submerged part of the Columbretes volcanic system revealed the presence of three main relict sand bodies along the outer shelf, at 80-116. m depth range, above which asymmetric and slightly asymmetric large and very large 2D and 3D subaqueous dunes were observed. These bed features were recognized, mapped and quantified with the aim of evaluating their potential formation mechanisms in relation to the local hydrodynamic and morphologic settings of the area. Dunes range from 150 to 760. m in wavelength and from tens of centimeters to 3. m in height, and are among the longest ever recognized in an outer shelf region. These bedforms are mostly composed of medium-sized sandy sediments, presumably coming from the degraded relict sand bodies on top of which they have developed, mixed with fine fractions from the recent draping holocenic sediments. The orientation of the dunes is SSW, progressively turning W towards the southernmost sector of the area, following the trend of the shelf-edge. Contemporary hydrodynamic measurements at the Ebro continental shelf-edge show that recorded currents are insufficient to form the observed bedforms and that stronger currents are required for sediment mobilization and dune formation. Based on their morphology and orientation, it is proposed that these bedforms are produced by the action of the southward-flowing Liguro-Proven{\c c}al-Catalan (LPC) geostrophic current. The LPC probably reaches high near-bottom currents during energetic hydrodynamic events through interactions with the seafloor morphology of the study area. Subaqueous dunes are expected to be basically inactive features with respect to present-day processes, although they can be reactivated during high-energy events. The small $Δ$h/${\l}ambda$ ratio measured in the dune fields of the Columbretes shelf revealed that the dune heights fall below the values predicted by the Flemming (1988) global equation, as observed in other outer shelf settings also dominated by unidirectional flows. This may suggest a different morphodynamic character of large dunes formed on outer shelves in a micro-tidal regime. {\textcopyright} 2010 Elsevier Ltd.},
	keywords = {Continental shelf, Geomorphology, Subaqueous dunes, Swath mapping, Western Mediterranean},
	issn = {02784343},
	doi = {10.1016/j.csr.2010.08.005},
	url = {http://www.scopus.com/inward/record.url?eid=2-s2.0-77957596289\&partnerID=tZOtx3y1},
	author = {Lo Iacono, Claudio and Guill{\'e}n, Jorge and Puig, Pere and Rib{\'o}, Marta and Ballesteros, Maria and Palanques, Albert and l{\'\i} Farr{\'a}n, Marcel and Acosta, Juan}
}
@article {Muller2009,
	title = {{Lithospheric structure, evolution and diamond prospectivity of the Rehoboth Terrane and western Kaapvaal Craton, southern Africa: Constraints from broadband magnetotellurics}},
	journal = {Lithos},
	volume = {112},
	year = {2009},
	month = {nov},
	pages = {93{\textendash}105},
	abstract = {A 1400~km-long, 2-D magnetotelluric (MT) profile, consisting of 69 sites at 20~km intervals, across the western part of the Archaean Kaapvaal Craton, the Proterozoic Rehoboth Terrane and the Late Proterozoic/Early Phanerozoic Ghanzi-Chobe/Damara Belt reveals significant lateral heterogeneity in the electrical resistivity structure of the southern African lithosphere. The lithospheric structures of the Rehoboth Terrane and Ghanzi-Chobe/Damara Belt have not been imaged previously by geophysical methods. Temperature is the primary control on the resistivity of mantle minerals, and the MT derived lithospheric thicknesses therefore provide a very reasonable proxy for the "thermal" thickness of the lithosphere (i.e., the thickness defined by the intersection of a conductive geotherm with the mantle adiabat), allowing approximate present-day geotherms to be calculated. The work indicates the following present-day average lithospheric thicknesses, to a precision of about {\textpm} 20~km, for each of the terranes traversed (inferred geotherms in brackets): Eastern Kimberley Block of the Kaapvaal Craton 220~km (41~mW m- 2), Western Kimberley Block 190~km (44~mW m- 2), Rehoboth Terrane 180~km (45~mW m- 2) and Ghanzi-Chobe/Damara Belt 160~km (48~mW m- 2). A clear relationship between the electrical resistivity structure of the lithosphere and the tectonic stabilisation-age of the terrane is evident. Good agreement between the inferred present-day lithospheric geotherms and surface heat flow measurements indicate the latter are strongly controlled by variations in lithospheric thickness. A significant difference in lithospheric thickness is observed between the Eastern and Western Kimberley blocks, and is consistent with previous seismic tomography images of the Kaapvaal Craton. The present-day lithospheric thickness, and reduced depth extent into the diamond stability field, accounts for the absence of diamondiferous kimberlites in the Gibeon and Gordonia kimberlite fields in the Rehoboth Terrane. Previously published mantle xenolith P-T arrays from the Gibeon, Gordonia and Kimberley fields, however, suggest that the Rehoboth Terrane had equilibrated to a cooler conductive palaeo-geotherm (40-42~mW m- 2 ), very similar to that of Eastern Kimberley Block of the Kaapvaal Craton, at some time prior to the Mesozoic eruption of the kimberlites. The timing and nature of both the thermal equilibration of the Rehoboth Terrane, and the subsequent lithospheric heating/thinning event required to account for its present-day lithospheric structure, are not well constrained. A model consisting of the penetration of heat transporting magmas into the lithosphere, with associated chemical refertilisation, at an early stage of Mesozoic thermalism appears to be the most plausible model at present to account for both the present-day lithospheric structure of the Rehoboth Terrane and an earlier, cooler palaeo-geotherm. Some problems, however, remain unresolved in terms of the isostatic response of the model. Based on a compilation of xenocryst Cr/Ca-in-pyrope barometry observations, the extent of depleted mantle in the Rehoboth Terrane is found to be significantly reduced with respect to the Eastern Kimberley Block: 117~km versus 138-167~km. It appears most likely that the depletion depth in both terranes, at least in the vicinity of kimberlite eruption, is explained by refertilisation of the lower lithospheric mantle. {\textcopyright} 2009.},
	keywords = {Diamond, Geotherm, Lithosphere, Magnetotellurics, Southern Africa, Xenolith},
	issn = {00244937},
	doi = {10.1016/j.lithos.2009.06.023},
	url = {http://www.scopus.com/inward/record.url?eid=2-s2.0-72049130282\&partnerID=tZOtx3y1},
	author = {Muller, M.R. and Jones, A.G. and Evans, R.L. and Gr{\"u}tter, H.S. and Hatton, C. and Garcia, X. and Hamilton, M.P. and Miensopust, M.P. and Cole, P. and Ngwisanyi, T. and Hutchins, D. and Fourie, C.J. and Jelsma, H.A. and Evans, S.F. and Aravanis, T. and Pettit, W. and Webb, S.J. and Wasborg, J.}
}
@article {Goldfinger2008,
	title = {{Late Holocene Rupture of the Northern San Andreas Fault and Possible Stress Linkage to the Cascadia Subduction Zone}},
	journal = {Bulletin of the Seismological Society of America},
	volume = {98},
	number = {2},
	year = {2008},
	month = {apr},
	pages = {861{\textendash}889},
	abstract = {We relate the late Holocene northern San Adreas fault (NSAF) paleoseismic history developed using marine sediment cores along the northern California continental margin to a similar dataset of cores collected along the Cascadia margin, including channels from Barclay Canyon off Vancouver Island to just north of Monterey Bay. Stratigraphic correlation and evidence of synchronous triggering imply earthquake origin, and both temporal records are compatible with onshore paleoseismic data. In order to make comparisons between the temporal earthquake records from the NSAF and Cascadia, we refine correlations of southern Cascadia great earthquakes, including the land paleoseismic record. Along the NSAF during the last \~{}2800 yr, 15 turbidites, including one likely from the great 1906 earthquake, establish an average repeat time of \~{}200 yr, similar to the onshore value of \~{}240 yr. The combined land and marine paleoseismic record from the southern Cascadia subduction zone includes a similar number of events during the same period. While the average recurrence interval for full-margin Cascadia events is \~{}520 yr, the southern Cascadia margin has a repeat time of \~{}220 yr, similar to that of the NSAF. Thirteen of the 15 NSAF events were preceded by Cascadia events by \~{}0-80 yr, averaging 25-45 yr (as compared to \~{}80-400 yr by which Cascadia events follow the NSAF). Based on the temporal association, we model the coseismic and cumulative postseismic deformation from great Cascadia megathrust events and compute related stress changes along the NSAF in order to test the possibility that Cascadia earthquakes triggered the penultimate, and perhaps other, NSAF events. The Coulomb failure stress (CFS) resulting from viscous deformation related to a Cascadia earthquake over \~{}60 yr does not contribute significantly to the total CFS on the NSAF. However, the coseismic deformation increases CFS on the northern San Andreas fault (NSAF) by up to about 9 bars offshore of Point Delgada, most likely enough to trigger that fault to fail in north-to-south propagating ruptures.},
	issn = {0037-1106},
	doi = {10.1785/0120060411},
	url = {http://www.scopus.com/inward/record.url?eid=2-s2.0-42649087275\&partnerID=tZOtx3y1},
	author = {Goldfinger, C. and Grijalva, K. and Burgmann, R. and Morey, A. E. and Johnson, J. E. and Nelson, C. H. and Gutierrez-Pastor, J. and Ericsson, A. and Karabanov, E. and Chaytor, J. D. and Patton, J. and Gr{\`a}cia, E.}
}
@article {Panahi2008,
	title = {{A Low-Power Datalogger Based on CompactFlash Memory for Ocean Bottom Seismometers}},
	journal = {IEEE Transactions on Instrumentation and Measurement},
	volume = {57},
	number = {10},
	year = {2008},
	month = {oct},
	pages = {2297{\textendash}2303},
	abstract = {In the last decade, marine scientific instruments have been in high demand, particularly autonomous instruments that are capable of staying under water for a long time while performing continuous data acquisition and storage. This paper introduces an instrument under development that is used for the study of ocean bottom sublayers and microseismic detection. The power consumption of the equipment has been minimized to increase autonomy, and CompactFlash memory cards have been used as the storage element. Development of such equipment is a joint effort between different disciplines, such as electronics, mechanics, geophysics, underwater communications, etc. The acquisition system was tested both in the laboratory and under real environmental conditions in the summer of 2005, and the results have been evaluated. {\textcopyright} 2008 IEEE.},
	keywords = {Analog-to-digital (A/D) converter, CompactFlash memory, Datalogger, Effective number of bits (ENOB), Ocean bottom seismometer (OBS), Power consumption, Time base},
	issn = {0018-9456},
	doi = {10.1109/TIM.2008.919005},
	url = {http://www.scopus.com/inward/record.url?eid=2-s2.0-52649175960\&partnerID=tZOtx3y1},
	author = {Panahi, S.S. and Ventosa, S. and Cadena, J. and Manuel-Lazaro, A. and Bermudez, A. and Sallar{\`e}s, V. and Piera, J.}
}
