Mariano Cerca

Dr. Mariano Cerca


Research Focus & Metrics

Academic Career Length

27Years (2000-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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1 November 2016 in Journal of Structural Geology
Verified
Journal Article
Closed access
GSGuido Schreurs
Guido Schreurs
SBSusanne J.H. Buiter
Susanne J.H. Buiter
JBJennifer Boutelier
Jennifer Boutelier
CBCaroline Burberry
Caroline Burberry
JCJean-Paul Callot
Jean-Paul Callot
YYYasuhiro Yamada
Yasuhiro Yamada


1 November 2018 in Engineering Geology
Verified
Journal Article
Closed access
GOG.H. Ochoa-González
G.H. Ochoa-González
DCD. Carreón-Freyre
D. Carreón-Freyre
AFA. Franceschini
A. Franceschini
MCMariano Cerca
Mariano Cerca
PTP. Teatini
P. Teatini

2 March 2016 in Hydrogeology Journal
Verified
Journal Article
Closed access
PDF file
DCD. Carreón-Freyre
D. Carreón-Freyre
MCMariano Cerca
Mariano Cerca
GOG. Ochoa-González
G. Ochoa-González
PTP. Teatini
P. Teatini
FZF. R. Zuñiga
F. R. Zuñiga

1 February 2000 in International Geology Review
Verified
Journal Article
Closed access
MCMariano Cerca
Mariano Cerca
GDGerardo De Jesús Aguirre Díaz
Gerardo De Jesús Aguirre Díaz
MMMargarita López Martínez
Margarita López Martínez
Geologic mapping and new K-Ar and 40Ar/39Ar geochronology of the southeastern Sierra Madre Occidental (SMO), at its intersection with the northern margin of the Mexican Volcanic Belt (MVB), indicate the occurrence of three volcanic groups. The oldest group corresponds to the SMO, and includes 29 to 22 Ma voluminous ignimbrites and 30 Ma andesites and rhyolites. The youngest group includes widespread basaltic-andesitic lava plateaus that yielded ages from 14.6 to 8.8 Ma and are interpreted as the beginning of the MVB. From 22 to 14.6 Ma, volcanic activity in the area was significantly reduced, but did not cease entirely. We refer to the third group as transitional volcanism, which is dominated by andesitic and rhyolitic lava domes but also includes high-grade andesitic ignimbrites. We conclude that the change from volcanism proper of the SMO to that of the MVB was gradual with respect to age and drastic with respect to composition and style, from a voluminous-silicic-ignimbrite domain to a widespread basaltic-andesitic-lava plateau domain. This change may have been related to major plate tectonic reorganizations within the interval from 25 to 12 Ma that involved the waning of subduction of the Farallon plate west of northern Mexico and the associated southward migration of the triple junction of the Pacific-Farallon-North America plates, the subsequent break-up of the Farrallon plate into the Guadalupe and Cocos plates, and the counterclockwise and clockwise rapid rotation of the ridge between them around 16 to 12.5 Ma.