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Please use this identifier to cite or link to this item: http://apo.ansto.gov.au/dspace/handle/10238/6459

Title: Accelerator Mass spectrometry: revealing subtle signals in ice sheets
Authors: Smith, A
Heikkila, U
Keywords: ACCELERATORS
MASS SPECTROSCOPY
ISOTOPES
ISOTOPE DATING
ANSTO
ANTARCTICA
Issue Date: 13-Feb-2013
Publisher: PAGES
Citation: Smith, A., & Heikkila, U. (13th – 16th February 2013). Accelerator mass spectrometry: revealing
Abstract: Accelerator Mass Spectrometry (AMS) determines the ratio of a rare isotope, normally radioactive and of intermediate half-life, to a stable isotope. AMS permits the detection of individual atoms in a sample and so is an inherently sensitive analytical technique. A well-known example is radiocarbon dating (14C, t1/2 = 5730 a), where measurement of the 14C/12C ratio permits determination of the age of an artifact. Such AMS measurements can be performed rapidly (~ 20 min), at good precision (~ 0.3 ‰), with high sensitivity (< 10-15) and on very small samples (as little a few μg of carbon). Radiometric measurements, by contrast, require much larger sample masses and much longer measurement times in order to obtain good precision. Besides its use as a chronometer, 14C is increasingly used as a tracer in geophysical studies as the amount of carbon required for a measurement has decreased.At ANSTO we routinely measure 14C, 10Be, 26Al and the Actinides by AMS and in 2010 we added 7Be to the list. Here I give some examples from the ice sheets in Greenland and Antarctica of palaeoclimate research I have been involved in. In each case AMS has provided the unique key to unlock these important climate archives. I will discuss 14C studies of atmospheric gases from firn air and ice core bubbles, with the objective of learning more about the natural and anthropogenic sources of the important greenhouse gas methane. Additionally, I will discuss studies of the beryllium isotopes, 7Be (t1/2 = 53 d) and 10Be (t1/2 = 1.4 _ 106 a) in snow and ice, with the objective of improving the use of 10Be as a proxy for Solar variability.
URI: http://pages-igbp.org/download/docs/meeting-products/abstracts/osm4ysm2/OSM2013abstract_book.pdf
http://apo.ansto.gov.au/dspace/handle/10238/6459
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