2009
DOI: 10.1111/j.1365-2117.2008.00384.x
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Stratigraphic evolution of the Triassic–Jurassic succession in the Western Southern Alps (Italy): the record of the two‐stage rifting on the distal passive margin of Adria

Abstract: The Triassic–Lower Jurassic succession of the Southern Alps is characterized by rapid thickness changes, from an average of about 5000 m east of Lago Maggiore to about 500 m in the Western Southern Alps. The stratigraphy reflects the Triassic evolution of the Tethyan Gulf and the Early Jurassic rifting responsible for the Middle Jurassic break‐up of Adria from Europe. The succession of the Western Southern Alps starts with Lower Permian volcanics directly covered by Anisian sandstones. The top of the overlying… Show more

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Cited by 48 publications
(81 citation statements)
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“…It cannot be excluded that a grainsize-age relationship not resolved at the precision of our in situ analyses is also superimposed on these discrete cooling events, adding further complexity to the data. We postulate that the ~175 Ma cooling may be due to rift-related exhumation, which would be consistent with the fact that the ~175 Ma ages coincide with or only slightly postdate the termination of documented rift-related activity of faults and shear zones in the western Southern Alps (Berra et al 2009;Mulch et al 2002a).…”
Section: Constraints On the Permian To Jurassic Thermal Evolution Of mentioning
confidence: 58%
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“…It cannot be excluded that a grainsize-age relationship not resolved at the precision of our in situ analyses is also superimposed on these discrete cooling events, adding further complexity to the data. We postulate that the ~175 Ma cooling may be due to rift-related exhumation, which would be consistent with the fact that the ~175 Ma ages coincide with or only slightly postdate the termination of documented rift-related activity of faults and shear zones in the western Southern Alps (Berra et al 2009;Mulch et al 2002a).…”
Section: Constraints On the Permian To Jurassic Thermal Evolution Of mentioning
confidence: 58%
“…These ages cannot therefore be related to exhumation-related cooling and are instead interpreted to record an early post-rift heating-cooling cycle during oceanisation. The ~175 Ma age population coincides with the latest documented stages of activity of rift-related faults (Berra et al 2009) and shear zones (Mulch et al 2002a) within the western termination of the Adriatic margin. As a result, this age population is interpreted to record cooling associated with rift-related exhumation.…”
Section: Discussionmentioning
confidence: 96%
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