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ABSTRACTS / RESUMES - Comitato Glaciologico Italiano

ABSTRACTS / RESUMES - Comitato Glaciologico Italiano

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JORGE RABASSA 1, MARCELO ZARATE 2,<br />

TIMOTHY C. PARTRIDGE 3, RODNEY MAUD 4,<br />

MARCELA CIOCCALE 5 & CLAUDIO CARIGNANO 5<br />

Gondwanic relict palaeolandscapes in cratonic areas<br />

of Argentina<br />

1 Cadic-conicet, C.C.92, 9410 Ushuaia, Argentina<br />

2 Conicet-Universidad Nacional de Mar del Plata,<br />

C.C.722, 7600 Mar del Plata, Argentina<br />

3 University of Witwatersrand, p.o. box 1050, Parklands,<br />

Johannesburg 2121, South Africa<br />

4 University of Natal, 68 Ridge Road, Durban 4001, South Africa<br />

5 Conicet-Universidad Nacional de C6rdoba, Av.Velez Sarsfield 299,<br />

5000 C6rdoba, Argentina<br />

Relict landforms (peneplains, pediplains, bornhardts,<br />

rocking stones, core rocks, palaeoweathering profiles, etc.)<br />

of Late Mesozoic-Early Tertiary age, have been identified<br />

since long ago in South Africa and Brazil. Similar<br />

landforms have been recognized in Argentina, following<br />

the South African methodology as summarized by Partridge<br />

& Maud (1987). The works ofDu Toit (1927) and KING<br />

(1967), among many other South African and Brazilian<br />

authors, have been used in the preparation of the theoretical,<br />

conceptual framework for this paper.<br />

During Early Cretaceous times, the present territories of<br />

Argentina, as well as the rest of South America, were still<br />

physically linked to South Africa as part of the Gondwana<br />

Supercontinent. Dominant climate was humid tropicalsubtropical<br />

for most of its emerged lands. Relict landscapes<br />

in Argentina would have been generated during Jurassic-Cretaceous,<br />

up to Palaeocene times, under climatic<br />

conditions which were very different from those existing<br />

today. These relict landforms have been observed in the<br />

Tandilia hills (core stones, rocking stones, palaeoweathering<br />

profiles), the Ventania ranges (silcretes and silicified<br />

slope breccias), the Northern Patagonian Massif (erosional<br />

surfaces, deep palaeoweathering profiles, kaolinization<br />

processes), the Sierras de Cordoba (high «pampas» or erosional<br />

surfaces, core stones, bornhardts, palaeoweathering<br />

profiles) and the Deseado Massif of Southern Patagonia<br />

(extensive erosional surfaces). In Ventania, the densely silicified<br />

Cerro Colorado Breccia fills a drainage network eroded<br />

into the Late Palaeozoic sedimentary rocks. These<br />

breccias have been tentatively correlated with Du Toit's<br />

«High Level Gravels» and their associated siliceous duricrusts<br />

of the Southern Africa Cape region, which age is<br />

bracketed between 63-54.8 Ma, thus providing a minimum<br />

age for the underlying fluvial palaeolandscape. However,<br />

due to other regional interpretations, the breccias may be<br />

even older (Cretaceous). The Pampean intracratonic tectonic<br />

basins, such as the Colorado, Parana, and Macachfn<br />

basins, were initially filled by Cretaceous basalts, related to<br />

the Southern Atlantic rifting process. In the western margin<br />

of the Northern Patagonian Massif, the Jurassic(?)-Cretaceous<br />

erosional surfaces were fluvially eroded and the resulting<br />

drainage landscape was infilled by Palaeocene-Early<br />

Eocene (ca. 55 Ma) volcanics and highly-siliceous pyrocla-<br />

sties, The Sierras de Cordoba high «pampas» are locally<br />

covered by Cretaceous basalts and sedimentary rocks, which<br />

fill shallow depressions carved into the relict erosional<br />

surfaces. However, in the Sierras Pampeana region, the palaeolandforms<br />

have been severely affected by Tertiary Andean<br />

tectonism, and their reconstruction is more difficult.<br />

The preservation of these ancient, relict palaeolandscapes,<br />

which were never buried afterwards and remained as portions<br />

of positive elements since then, is interpreted as a<br />

consequence of their development over hyperstable regions<br />

of Argentina. Their recognition in the field and subsequent<br />

interpretation is of high relevance because: (1) it<br />

explains the cratonic morphogenesis as part of Gondwana<br />

and its persistency for at least 60 Ma; (2) it provides a new<br />

approach in the interpretation of the Pampean and present<br />

submarine-platform, Cretaceous-Early Tertiary tectonic<br />

basins; (3) it offers an appropiate conceptual scheme for<br />

mineral exploration of such ores as kimberlites or bauxites;<br />

(4) it favours the geomorphological interpretation of the<br />

Argentine cratonic regions with a «Gondwanic vision»<br />

that should replace the «Andean vision», until now dominating<br />

the Argentine geological literature.<br />

ZOFIA RACZKOWSKA<br />

Nivation in the Tatras in comparison<br />

with other mountain areas<br />

Department of Geomorphology, Institut of Geography<br />

and Spatial Organization, Polish Academy of Sciences,<br />

cew.Jana 22,30-918 Krac6w, Poland<br />

The geomorphic processes operating around the snow patches<br />

on the high-mountain slopes are presented.<br />

The studies of nivation in the Tatras were carried out on<br />

the northern slopes of the High Tatras, above the timberline<br />

(1500 m a.s.l.), on the slopes developed on granite bedrock.<br />

The studies mainly concerned thermal conditions of<br />

weathering, meltwater runoff, material transport and the<br />

impact of snow patches on the accumulation processes developed<br />

on debris slopes. It is concluded that the key factor<br />

in the intensification of processes is increased moisture<br />

availability rather than the microclimatic effects of snow<br />

patches. If compared with weathering, present-day transport<br />

processes and deposition appear to be more active.<br />

Nevertheless, the activity of the above processes varies<br />

with the meteorological situation.<br />

Erosional effects of snow patches are considerable on slopes<br />

mantled by debris devoid of vegetation cover. The nival<br />

niche backwall retreats 1 to 5 em per year due mainly<br />

to frost action and needle ice. In the lower part of niche<br />

bottom sheet wash and rill erosion was observed.<br />

On debris slopes «accumulation niches» are developing in<br />

places occupied by snow patches, most often in the apex<br />

part of the slope. They are formed due to accreation on de-<br />

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