Fulop, Reka-H., Fink, David, Yang, Bin, Codilean, Alexandru T., Smith, Andrew ORCID: 0000-0002-9193-2617, Wacker, Lukas, Levchenko, Vladimir and Dunai, Tibor J. (2019). The ANSTO - University of Wollongong in-situ C-14 extraction laboratory. Nucl. Instrum. Methods Phys. Res. Sect. B-Beam Interact. Mater. Atoms, 438. S. 207 - 214. AMSTERDAM: ELSEVIER SCIENCE BV. ISSN 1872-9584

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Abstract

We present our first C-14 in-situ results for calibration and system blanks from the recently completed Australian Nuclear Science and Technology Organisation (ANSTO) University of Wollongong (UOW) in-situ C-14 extraction system. System performance parameters and quality is evidenced by low C-14 blanks and good reproducibility for multiple targets from different reference materials. The C-14 extraction scheme exploits the high temperature phase transformation of quartz to cristobalite in order to quantitatively extract the carbon as CO2. The in-situ C-14 extraction system comprises three independently operated and modular units that are used for initial in-vacuo removal of meteoric C-14, followed by offline high-temperature heating of quartz to release trapped cosmogenic in-situ C-14, and finally CO2 gas purification and mass measurement. The design allows for rapid sample throughput of about 6 samples per week with samples masses ranging between 0.5 and 4 g of clean quartz. Other features include single-pass catalytic oxidation using mixed copper (LII) oxide as catalyst, use of UHV-compatible components and of vacuum annealed copper tubing. We present results for sets of purified quartz samples prepared from CRONUS-A, CRONUS-R and CRONUS-N inter-comparison materials, with final averages consistent with published values. Following extraction and cleaning, CO2 gas aliquots for some of the samples were analysed using the ETH Zurich CO2 gas ion source at the ETH MICADAS AMS facility in addition to CO2 being graphitised using the ANSTO laser-heated graphitisation micro-furnace and then analysed on ANSTO's ANTARES AMS facility. System blanks using either CO2 or graphite ion-sources at both facilities are on the order of similar to 1 x 10(4) atoms.

Item Type: Journal Article
Creators:
CreatorsEmailORCIDORCID Put Code
Fulop, Reka-H.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Fink, DavidUNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Yang, BinUNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Codilean, Alexandru T.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Smith, AndrewUNSPECIFIEDorcid.org/0000-0002-9193-2617UNSPECIFIED
Wacker, LukasUNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Levchenko, VladimirUNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Dunai, Tibor J.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
URN: urn:nbn:de:hbz:38-140838
DOI: 10.1016/j.nimb.2018.04.018
Journal or Publication Title: Nucl. Instrum. Methods Phys. Res. Sect. B-Beam Interact. Mater. Atoms
Volume: 438
Page Range: S. 207 - 214
Date: 2019
Publisher: ELSEVIER SCIENCE BV
Place of Publication: AMSTERDAM
ISSN: 1872-9584
Language: English
Faculty: Unspecified
Divisions: Unspecified
Subjects: no entry
Uncontrolled Keywords:
KeywordsLanguage
COSMOGENIC C-14; METEORITES; BEHAVIOR; CARBON; QUARTZ; BE-10Multiple languages
Instruments & Instrumentation; Nuclear Science & Technology; Physics, Atomic, Molecular & Chemical; Physics, NuclearMultiple languages
Refereed: Yes
URI: http://kups.ub.uni-koeln.de/id/eprint/14083

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