7 research outputs found
The formation, alteration and significance of pyrogenic magnetic fabric in mid-paleolithic burnt cave facies
Trabajo presentado en: Magiber XI, 4-7 de septiembre de 2019, Condeixa a NovaB. Bradák acknowledges the financial support of project BU235P18 (Junta de Castilla y Leon, Spain) and the European
Regional Development Fund (ERD)
Saving Bones: a direct comparison of FTIR-ATR, whole bone percent nitrogen, and NIR
89th Annual Meeting of the American-Association-of-Physical-Anthropologists (AAPA), Los Angeles, CA, APR 15-18, 202
Magnetic fabric and archaeomagnetic analyses of anthropogenic ash horizons in a cave sediment succession (Crvena Stijena site, Montenegro)
An archaeomagnetic, rock magnetic and magnetic fabric study has been carried out on seven
anthropogenic ash horizons in theMiddle Palaeolithic sedimentary level XXIV at the rock shelter
of Crvena Stijena (‘Red Rock’), Montenegro. The study has multiple goals, including the
identification of iron bearingminerals formed during combustion, assessment of the suitability
of these combustion features for recording the Earth´s magnetic field direction, revelation of
the magnetic fabric and its significance in the characterization of cave (rock shelter) burnt
facies, and identification of post-burning alteration processes. Magnetite has been identified
as themain ferromagnetic component of the ash. The ash layers exhibit a high thermomagnetic
reversibility in contrast to the irreversible behaviour of their subjacent burnt black layers which
is related to the different temperatures attained. Seven mean archaeomagnetic directions were
obtained with acceptable statistical values indicating that these features recorded the field direction
at the time of burning. However, some of them are out of the expected range of secular
variation for mid-latitude regions suggesting post-burning alterations. The magnetic fabric of
the ash was characterized by anisotropy of low field magnetic susceptibility measurements.
Statistical analysis (box and whisker plot) of the basic anisotropy parameters, such as foliation,
lineation, degree of anisotropy and the shape parameter, along with the alignment of the principal
susceptibilities on stereoplots, revealed variation among the ash units. The diverse, oblate
to prolate, lineated or strongly foliated, quasi-horizontally and vertically oriented fabrics of the
units may indicate different slope processes, such as orientation by gravity, solifluction, run-off
water, quasi-vertical migration of groundwater and post-burning/post-depositional alteration
of the fabric by rockfall impact. In sum, the magnetic characterization of the ash layers has
shown the occurrence of different post-burning alteration processes previously not identified
at the site. Alteration processes in prehistoric combustion features are often identified from
macroscopic observations but our study demonstrates that multiple processes can affect them
and are usually unnoted because they take place on a microscopic scale. Their identification
is critical for a correct chronological and cultural interpretation of a site (e.g. collection of
samples for dating, stratigraphic displacement of remains), especially if significant alterations
are involved. Magnetic methods are therefore a powerful but underutilized tool in palaeolithic
research for the identification and evaluation of taphonomic processes affecting prehistoric
fires.BU235P18 (Junta de Castilla y León, Spain) and the European
Regional Development Fund(ERDF) and the CGL2016-77560-
C2, PID2019-108753GB-C21 and PID2019-105796GB-I00 of the
Agencia Estatal de Investigación (AEI/10.13039/501100011033).
AHL gives thanks to Junta de Castilla y León (Spain) and
European Social Fund for the financial support during her predoctoral
period. Micromorphological investigations by CM are
funded by ERC Consolidator Grant project ERC-2014-CoG-
648871-PALEOCHAR
Lithic raw material units based on magnetic properties: A blind test with Armenian obsidian and application to the Middle Palaeolithic site of Lusakert Cave 1
Classification of lithic artifacts’ raw materials based on macroscopic attributes (e.g., color, luster, texture) has been used to pull apart knapping episodes in palimpsest assemblages by attempting to identify artifacts produced through the reduction of an individual nodule. These classes are termed “raw material units” (RMUs) in the Old World and “minimum analytical nodules” in the New World. RMUs are most readily defined for lithic artifacts in areas with distinctive cherts and other siliceous raw materials, allowing pieces from different nodules to be recognized visually. Opportunities to apply RMUs, however, are strongly limited at sites where lithic material visual diversity is low. The magnetic properties of obsidian, which result from the presence of microscopic iron oxide mineral grains, vary spatially throughout a flow. Consequently, obsidian from different portions of a source (i.e., different outcrops or quarries) can vary in magnetic properties. This raises the possibility that magnetic-based RMUs (mRMUs) for obsidian artifacts could be effective to distinguish individual scatters from multiple production episodes and offer insights into spatial patterning within a site or specific occupation periods. First, we assess the potential of mRMUs using obsidian pebbles from Gutansar volcano in Armenia. Second, we evaluate the validity of this approach based on a double-blind test involving an experimental assemblage of Gutansar obsidian flakes. Cluster analysis can successfully discern flakes from obsidian specimens containing high concentrations of iron oxides. Obsidian with more magnetic material has more opportunities for that material to vary in unique ways (e.g., grain size, morphology, physical arrangement). Finally, we apply the mRMU approach to obsidian artifacts from the Middle Palaeolithic site of Lusakert Cave 1 in Armenia and compare the results to traditional RMU studies at contemporaneous sites in Europe. In particular, we seek – but do not find – differences between retouch flakes (which re