Electron
Microprobe/SIMS Determinations of Al in Olivine:
Applictions
to Solar
Wind, Pallasites, and Trace Element Measurements
J M Paque1,
AE Hofmann1, DS Burnett1, Y Guan1, AJG Jurewicz2, DS Woolum3, C Ma1, GR Rossman1
1 Division of Geological
and Planetary
Sciences
California
Institute of
Technology
Pasadena, CA 91125-2500
2 SESE
Arizona
State University
Tempe, AZ 85287
3 Department
of Physics
California
State University, Fullerton
Fullerton, CA 92834
ABSTRACT
Electron probe microanalyser measurements of trace elements with high
accuracy are challenging. Accurate Al measurements in olivine are
required to calibrate SIMS implant reference materials for measurement
of Al in the solar wind. We adopt a combined EPMA/SIMS approach that is
useful for producing SIMS reference materials as well as for EPMA at the
~ 100 µg g-1 level. Even for mounts not polished with
alumina photoelectron spectroscopy shows high levels of Al surface
contamination. In order to minimise electron beam current density, a
rastered 50 × 100 µm electron beam was adequate and minimised
sensitivity to small Al‐rich contaminants. Reproducible analyses of
eleven SIMS‐cleaned spots on San Carlos olivine agreed at
69.3 ± 1.0 µg g-1. The known Al mass fraction was used to
calibrate an Al implant into San Carlos. Accurate measurements of Al
were made for olivines in the pallasites: Imilac, Eagle Station and
Springwater. Our focus was on Al in olivine, but our technique could be
refined to give accurate electron probe measurements for other
contamination‐sensitive trace elements. For solar wind, it is projected
that the Al/Mg abundance ratio can be determined to 6%, a factor of 2
more precise than the solar spectroscopic ratio.