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4th INTERNATIONAL CONFERENCE
of PALAEOGEOGRAPHY
ABSTRACTS
Beijing, China
September, 2019
31
Lisco Stefania Nunzia1, Acquafredda Pasquale1, Gallicchio Salvatore1, Sabato Luisa2, Bonifazi
Andrea3, Cardone Frine2, Corriero Giuseppe2, Gravina Maria Flavia2, Pierri Cataldo2 and Moretti
Massimo1
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K-12
Hyperpycnal Flows and Deposits
Carlos Zavala1,2
(1. Departamento de Geología, Universidad Nacional del Sur, San Juan 670, 8000 Bahía Blanca,
Argentina,. 2.GCS Argentina SRL, Molina Campos 150, 8000 Bahía Blanca, Argentina)
Abstract: A hyperpycnal flow forms when a relatively dense land derived gravity flow
enters in a marine or lacustrine water reservoir. As a consequence of its excess in
density, the flow plunges in coastal areas generating a highly dynamic and often long-
lived dense underflow. Depending on the characteristics of the parent flow (flow
duration and flow rheology) and basin salinity the resulting deposits (hyperpycnites)
can be very variable. According to flow duration, land derived gravity flows can be
classified in short lived or long-lived flows. Short lived gravity flows last for minutes
or hours, and are mostly related to small mountainous river discharges, alluvial fans,
collapse of natural dams, landslides, volcanic eruptions, jökulhlaups, etc. Long lived
gravity flows last for days, weeks or even months, and are mostly associated to medium
to large size river discharges. Concerning the rheology of the incoming flow,
32
hyperpycnal flows can be initiated by non-Newtonian (cohesive debris flows),
Newtonian supercritical (lahars, hyperconcentrated flows, and concentrated flows) or
Newtonian subcritical flows (bedload, sandy or muddy dominated sediment laden
turbulent flows). Once plunged, non-Newtonian and Newtonian supercritical flows
require steep slopes to accelerate, allow the incorporation of ambient water and develop
flow transformations to evolve into a turbidity current and travel basinward. Their
resulting deposits are difficult to differentiate from those related to intrabasinal
turbidites. On the contrary, long lived Newtonian subcritical flows are capable of
transfer huge volumes of sediment, freshwater and organic matter far from the coast
even along gentle or flat slopes. In marine settings, the buoyant effect of interstitial
freshwater in bedload and sandy dominated hyperpycnal flows can result in lofting due
to density reversal. Since the excess of density in muddy hyperpycnal flows is provided
by silt-clay sediments in turbulent suspension, lofting is not possible even in
marine/saline basins. Muddy dominated hyperpycnal flows can also erode the basin
bottom during its travel basinward, allowing the incorporation and transfer of
intrabasinal sediments and organic matter. Long lived hyperpycnal flow deposits
exhibit typical characteristics that allow a clear differentiation respect to those related
to intrabasinal turbidites. Main features include (1) complex beds with gradual and
recurrent changes in sediment grain size and sedimentary structures, (2) mixture of
extrabasinal and intrabasinal components, (3) internal and discontinuous erosional
surfaces and (4) lofting rhythmites in marine/saline basins.
Keywords: Hyperpycnal flows, hyperpycnites, turbidites, sediment gravity flows
Carlos Zavala
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K-13
Growth and form of Conophyton (Maslov) — A radical
reinterpretation inspired by occurrences of Mg Silicates in the
modern microbialites of Lakes Clifton and Preston, Western
Australia
Robert V. Burne 1, 2
(1. Research School of Earth Sciences, Australian National University, Canberra, ACT
Australia
2. School of Earth and Environmental Science, University of Queensland, St Lucia,
Australia)
AbstractSConophyton (Maslov) is a stromatolite form composed of cylindroidal colonies
of nested conical laminae. The majority of fossil Conophytons are dolomitic. The
remains of the microbial communities responsible for their construction are rarely
found, but, where present, there are virtually always in areas of chert within the
Conophyton. Well-preserved Conophytons, up to 4m tall and with basal diameters of
up to 50cm are exposed in the Proterozoic Atar Formation of Mauritanea. Here
many occur in growth position as fields of individual columns spaced between 5