The interaction of cosmic radiation with terrestrial matter leads to the in-situ production of cosmogenic nuclides in the exposed surface material. Accelerator mass spectrometry (AMS) enables us to quantitatively measure trace concentrations of in-situ produced radionuclides like 10Be and 26Al. 21Ne can be determined by conventional noble gas mass spectrometry. This ultimately allows the determination of surface exposure ages, erosion rates and other processes of landscape evolution. The availability of a pure and well defined mineral sample is an important prerequisite for surface exposure dating. As the samples taken in the field usually do consist of many different mineral components, a quartz separation technique has to be employed. We present a chemical mineral separation that allows the isolation of a pure quartz fraction, which is quantitatively decontaminated from the atmospheric 10Be contamination lying on the sample.
Print ISSN: 0033-8230
Volume: 89, 11/2001
Pages: 779