Towards SHRIMP SI: Developments in Stable Isotope Analysis with SHRIMP

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Towards SHRIMP SI: Developments in Stable Isotope Analysis with SHRIMP Trevor Ireland Research School of Earth Sciences The Australian National University

Acknowledgments Ryan Ickert, Joe Hiess Peter Holden, Ian Williams John Foster, Peter Lanc, Ben Jenkins Electronics and Mechanical Workshops

Overview Historical SIMS, SHRIMP, Stable Isotopes Current SHRIMP II MC Oxygen isotopes Development SHRIMP SI

Stable-Isotope Analysis One of the first applications of SHRIMP Coles et al. (1981; RSES Ann Rept) Duoplasmatron with Ar + primary PbS2 from Galena combined Pb and S isotope analysis S - has higher yield Faraday cup yields ± 0.3 in 20 minutes

S-isotope Analysis Coles et al. noted: A primary Cs + beam will improve this(sensitivity) further work has been deferred in the absence of an in-house sulphide specialist. ion probe has a fearfully short time interval between the decision to sample and getting a final isotopic result

Positive secondaries Cowra granodiorite Core 1050 Ma Rim 420 Ma 50 µm U-Pb in zircon Ti, Mg isotopes in refractory inclusions Grain 1

Stable isotope reprise: S + Sulfide Specialist: Stewart Eldridge O2 - primary; S + secondaries few hundred khz on 32 S + electron multiplier yields ± 1 First routine SIMS VC-2a 188' S-isotope analyses silica +4-9 -18-14 crystal 9 50 µm

Stable Isotopes on SHRIMP II Cs Gun Kimball Physics IGS4 Cs zeolite

Electron Gun Electron beam Energetic (1.5 kev) Non-normal incidence Sustainable charge neutralization no settling

Stable isotope analysis Analytical Issues Fractionation at source slit Magnetic influence Sensitivity to steering Mount influence Electron-induced secondary electrons

Fractionation Dependent on steering ion optics beam dimensions δ 18 O QT1Y bits initial results in 2004

Mass bias at source slit Fractionation ( per bit of O lateral Si steering) S Ca Mass (AMU)

Source slit 28 Si Source slit 28 Si Canberra 35 S Z -53,000 nt St Petersburg 60 N Z +49,800 nt

Source slit 28 Si Source slit 28 Si 30 Si - 30 Si - Canberra 35 S Z -53,000 nt St Petersburg 60 N Z +49,800 nt

Source slit 28 Si Source slit 28 Si 30 Si - 30 Si + 30 Si + 30 Si - Canberra 35 S Z -53,000 nt St Petersburg 60 N Z +49,800 nt

Helmholtz coils

Mount Design 35mm Epoxy S Oxygen isotopes affected by steel rim Ickert and Hiess

Mega Mount Conventional Mount

Mega Mount No fractionation across mount until extraction aperture overlaps the mount edge Also favourable for U-Pb reproducibility Conductivity contrast on mounts an issue

Electron-Induced Secondary Ion Emission e - O 16- EISIE A Sample

EISIE probably related to Cs bombardment gettering vacuum water issue for multiple spots much reduced on Al vs Au coats factor of three reduced typically ca. 0.1 correction

Intra-Grain Measurements

Other Improvements Specialised low-field magnet control Electrometers DVS distributed vacuum monitoring system Automation Flight tube

Al Fight Tube Noted for some time that magnetic domains are present in 306 stainless steel ASI noted irreproducibility in beam refocus tried an Al flight tube Al flight tube installed on SHRIMP II greatly improved refocus (lower aberrations) returned magnetic field to theoretical

Current Status SHRIMP II typically achieves ca. 0.1 internal precision and <0.3 external, single spot precision for O, S, C April-May 2008 4-week stable isotope session; 1 day lost standard calibrations all better than 0.5 both user and automated operation

SHRIMP SI Dedicated stable isotope instrument Improved vacuum reduction in instrumental hydrides Smaller spot sizes down to 1 µm Simpler multiple collector

ION COUNTERS

SHRIMP SI Multiple collector fabrication complete Mass Analyzer fabrication complete Source and primary 60% complete Last machine drawings in by July 2008 Some assembly required

Calendar SHRIMP II Stable Isotopes J5 Building extension Build SHRIMP SI Move SHRIMP II from J3