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ABSTRACTS / RESUMES - Comitato Glaciologico Italiano

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island lands, answering the top part of the most actively<br />

growing morphostructures (Alat and Mishovdag ridges,<br />

Kharamin range and oth.), These island lands were later<br />

experienced mainly the horizontal and vertical development,<br />

not being covered by sea. The relief becomes complicated.<br />

The mud volcanism and corresponding forms of<br />

relief develop. The tectonic deformation becomes revived<br />

and formed newly. Beginning from Late Khvalin the relief<br />

of the territory gains the present outlines and peculiarities<br />

and it is very interesting that even the sinclinal basins are<br />

covered by sea alternately. It did not happen before. The<br />

sea left the limits of mentioned territory only during the<br />

deep regression which occured several times (between in<br />

Tiirkanian time and before). The change of situation took<br />

place repeatedly during 20 thousand years there which it is<br />

impossible not to be affected on the development of relief<br />

of the mentioned territory. A great help in reestablishment<br />

the quantitative indecies of quaternary movements exerted<br />

the sea terraces (about 14 levels). Palaeotectono-geomorphological<br />

course of development of the territory<br />

shows the succession and mobility the display of the latest<br />

and present movements and development of relief.<br />

VATCHE P. TCHAKERIAN\ PATRICK P. PEASE 1<br />

& NEIL W. TINDALE 2<br />

Geomorphology and sediments of the Wahiba sand sea,<br />

Sultanate of Oman<br />

1 Department of Geography, Texas A&M University,<br />

College Station, TX 77843, USA<br />

2 Departments of Meteorology and Oceanography,<br />

Texas A&M University, College Station, TX 77843, USA<br />

Geomorphological, geochemical and mineralogical analyses<br />

of terrestrial sediment samples and aerosol dust were<br />

undertaken in an effort to understand the geomorphology<br />

and cycling of sediment through the Wahiba sand sea (erg)<br />

in northeastern Oman. Sediment transport in the region is<br />

associated with the geomorphic development of the erg<br />

and the production, transport, and flux of desert dust material<br />

from the Oman desert into the Arabian sea. The<br />

Wahiba erg covers over 12,000 km 2 along the northeastern<br />

coast of Oman. It is bordered by mountains on the north,<br />

wadis on the west and east, and the Arabian Sea along the<br />

southeast. Most of the erg is comprised of a linear, northsouth<br />

trending draa system. The remaining areas are covered<br />

by transverse dunes, barchanoid dunes, sand ridges,<br />

and nabkha fields. Terrestrial sample collection included<br />

surface sediment samples from the Wahiba erg, surrounding<br />

wadis and sabkhas, and bedrock material. Aerosol<br />

dust was collected on paper filters from a ship-borne<br />

platform over the Arabian Sea for a semi-continuous one<br />

year period. Sediment samples and aerosol filters were<br />

analyzed for major and trace elements using elemental neu-<br />

372<br />

tron activation analysis. Both short and long irradiation times<br />

were used to quantify a wide range of elements. Mineralogy<br />

was obtained with a combination of optical microscopy<br />

and wavelength dispersive x-ray spectrometry.<br />

The geochemistry and mineralogy of dune samples were<br />

compared with those of wadi sediments and bedrock outcrops<br />

in an attempt to define ultimate and proximate provenance<br />

for the Wahiba sediments. This analysis suggested<br />

that sediment sources for the erg came from multiply provenances<br />

of varying lithologies contributed sediment to the<br />

erg. Landsat Thematic Mapper (TM) imagery was used to<br />

further extend the boundaries of the mineralogic sample<br />

sites beyond the sample points. Regions where the composition<br />

of sediments was determined from in situ chemical<br />

data were linked to specific pixel regions on the imagery.<br />

A combination of classification and band ratio techniques,<br />

designed to enhance contrasts inherent in the spectral responses<br />

of different mineral types, was employed to locate<br />

axes of variability in the spectral signatures and identify<br />

mineralogical boundaries as well as transport pathways.<br />

Geochemical signatures from Wahiba samples were also<br />

compared with those of aeolian dust samples. This comparison<br />

was an attempt to determine the relative contribution<br />

of Wahiba sediments to the regions atmospheric dust concentration.<br />

These data are also important factors in the understanding<br />

of global climate variability. This is because<br />

aerosols with a significant atmospheric residence time may<br />

impact radiation budgets. Also, the flux of mineral matter<br />

is a potentially important factor in the biological productivity<br />

of the Arabian Sea.<br />

BELAY TEGENE<br />

Soil-geomorphic units on piedmont slopes of<br />

Wurgo valley, Welo Highlands, Ethiopia<br />

Department of Geography, University of Addis Abeba,<br />

p.o. box 1176, Addis Ababa, Ethiopia<br />

An investigation of soil distribution in a piedmont valley of<br />

a mountainous cathchment in the Welo highlands led to<br />

the identification of clearly defined soil-geomorphic units.<br />

Luvic Phaoezems are associated to divergent footslopes,<br />

while Haplic Phaoezems occupied convergent footslopes,<br />

and Eutric Vertisols mantled alluvial toeslopes.<br />

The main characteristics of divergent footslopes-Luvic<br />

Phaoezems consociation were concave slopes, saprolite parent<br />

materials, truncated soils with stony surfaces and<br />

Ap/Bt/Cr horizon arrangements.<br />

The convergent footslopes-Haplic Phaoezems consociation<br />

is marked by gentler slopes, colluvial parent materials,<br />

deep young soils and A/Bw/Bb horizon sequences.<br />

The alluvial toeslope-Vertisols consociation is characterized<br />

by gentle to near level surfaces, alluvial parent materials,<br />

deep uniform A horizons, cracking clays and<br />

AIACICr or AIAC/Bb horizon arrangements.

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