FRONTIER RESEARCH ON EARTH EVOLUTION, VOL. 1 Quantitative analysis of rock-forming minerals and volcanic glasses by electron probe microanalyzer Hiroshi Shukuno Research Program for Geochemical Evolution, Institute for Frontier Research on Earth Evolution (IFREE) 2mm and an outer diameter of 3mm. Their standards are composed of natural minerals and synthetic compounds, and a set of standards can be selected for a given purpose by changing the combination used from those available. The JEOL standards have high quality and flexibility. At JAMSTEC, fiftytwo JEOL standards and one standard prepared at JAMSTEC are available, encompassing forty-three elements (B, C, F, Na, Mg, Al, Si, P, S, Cl, K, Ca, Ti, V, Cr, Mn, Fe, Co, Ni, Cu, Zn, Ga, Ge, Sr, Y, Zr, Nb, Ag, Cd, Sn, Sb, Te, Ba, Hf, W, Pt, Hg, Pb, Bi, La, Ce, Pr and Nd). A list of these standards and their chemical composition is given in Table 1. Carbon-coating was simultaneously applied to all the standard sets with a thickness of 20nm. Therefore, any systematic errors arising from differences in the thickness of the carbon-coating are minimized. Introduction An analysis of a small area on the surface of a solid specimen can be carried out with an electron probe microanalyzer (EPMA). An electron beam is focused on to the surface of the specimen and interacts with it, resulting in emission of backscattered primary electrons, low-energy photoelectrons, Auger electrons and characteristic X-rays. An X-ray detector, a wavelength- dispersive spectrometer (WDS) and/or an energy-dispersive spectrometer (EDS), records the X-ray spectrum emitted from the specimens in the EPMA. EPMA technology has been developed since 1960s, and EPMA chemical analyses for common rock-forming minerals have been technically achieved by petrologists and mineralogists. The methods of analysis by EPMA have been described by many researchers (e.g., Soejima, 1987). An EPMA can perform analyses of micron-scale areas, can qualitatively analyze elements from 5Be to 92U, and quantitatively detect amounts greater than 0.001wt.%. In JAMSTEC, two EPMAs have been installed for use by many researchers. One is a JEOL SUPERPROBE JXA-8900 equipped with five WDS-type detectors and an EDS-type detector. The other is a JEOL SUPERPROBE JXA-8800 equipped with four WDS-type detectors. Chemical analyses of rock-forming minerals and volcanic glasses have been carried out with the EPMAs in IFREE, in order to resolve the genesis and evolution of magmas from subduction zones and mantle plumes. In this paper, quantitative analyses for major and some minor components of rock-forming minerals and volcanic glasses using the EPMAs will be described. Analytical procedures The JXA-8900 and JXA-8800 microanalyzers at JAMSTEC are equipped with five and four WDS detectors, respectively. Each WDS detector contains two analyzing crystals (spectroscopic crystals), which have different crystal lattice planes for Bragg diffraction. These crystals can be adequately changed through the computer system, according to the elements analyzed. The EPMAs at JAMSTEC have LDE1, LDE2, TAP, PET and LiF analyzing crystals and cover a wide variation of elements for analyses (Table 2). The EPMAs have two types of X-ray detectors. The first type is a gas-flow counter, and the second is a gas-filled counter. The analyzing crystals with relatively wide distances between crystal lattice planes are combined with gas-flow type detectors, e.g., LDE1, LDE2, TAP and PET crystals. The gas-filled type detectors are combined with PET and LiF crystals. A list of the analyzing crystals and the X-ray detectors is given in Table 2. The conditions for analysis, which are composed of an accelerating voltage, probe current, probe diameter, count time, peak position and background position, are carefully chosen depending on target material and elements analyzed. Sample resistibility to the electron beam under analyzing conditions was verified empirically using the standards and the target materials. The conditions for analysing alkali elements, such as Na and K, were checked with particular caution, to prevent loss of X-ray intensity. Lower and upper background positions for the analyzed elements were determined by doing a peak scan near the peak for the element, both in the standards and in minerals similar in composition to the material analyzed. The peak count time for each element was selected to obtain sufficient X-ray intensities for the analysis. The probe diameter must be selected, taking specimen damage, loss of X-ray intensity, and defocus of the spectrometer into consideration. It was checked that the probe diameter selected in the analyzing condition minimized specimen damage. Consequently, a phenocryst- Selection of standards EPMA analyses are relative analyses. Therefore, the selection of standard materials is very important. The requirements for standards for EPMA analysis are as follows: (1) accurately determined chemical composition, (2) micro-scale homogeneity and (3) stability under electron exposure during measurement. Many kinds of materials are prepared as standard materials, for example, pure metals, alloys, oxides and boron minerals. It is preferred that standards with pure chemical compositions or standards similar in composition to the material analyzed are selected for EPMA analyses, to minimize systematic errors from matrix corrections (Soejima, 1987; Scott et al., 1995). It is difficult to collect a large number of high quality standard materials for EPMA analyses, and to prepare them for each instrument. At present, several companies produce high quality standards available for electron microprobe analysis (e.g., Astimex Scientific Ltd. and JEOL DATUM Ltd., etc.). For example, the standards prepared by JEOL are mounted in pipes with a length of 10mm, an inner diameter of 129 FRONTIER RESEARCH ON EARTH EVOLUTION, VOL. 1 sized grain was analyzed with a probe diameter of 5µm, and a focused beam was used for a micro-grain, such as inclusions, at conditions of 15-20kV and 12-25nA. Volcanic glass sensitive to an electron beam, was analyzed with a probe diameter of 10µm at 15kV and 10nA. A matrix correction for all analyses was processed by the ZAF correction prepared by JEOL. The combinations of analyzing crystals and count times for some examples are shown in Table 2. The standard materials used are also summarized in Table 2. A summary of the conditions used for some analyses is as follows. Results and discussion Representative analyses are shown in Tables 3-5. Averages and standard deviations of more than ten analyses are also listed in Tables 3-5. Most of the analytical results satisfy the stoichiometry and the total amount of each mineral analyzed. The low standard deviations indicate that the analyzed minerals were homogeneous. The results between JXA-8900 and JXA8800 are almost identical (Tables 3-5), although there are some exceptions. The results of SiO2 and Al2O3 contents in enstatite indicate slightly different values between JXA-8900 and JXA-8800 (Table 3). This difference is probably due to heterogeneity within each enstatite grain analyzed. K2O content of K-bearing minerals such as K-feldspar and adularia, is also slightly different between JXA-8900 and JXA-8800 (Table 3). This difference is caused by the standard materials selected for K analysis. K-feldspar (K 2O=5.62wt.%) and potassium titanium phosphate (K2O=23.80wt.%), which are prepared by JEOL, are used in JXA-8900 and JXA-8800, respectively. The K2O content of the K-feldspar is too low as a standard for K-analysis. In addition, the true value may be slightly lower than the recommended value reported by JEOL. The analytical results of olivine by 20kV-25nA are listed in Table 4 with the recommended compositions. The analytical results, including minor components such as MnO, CaO and NiO, have good agreement with the recommended composition. The results between JXA-8900 and JXA-8800 are almost equivalent (Table 4). Table 5 shows analytical results of the submarine volcanic glass. The compositions determined by XRF in JAMSTEC are also shown in Table 5. There is good agreement in each element, although the SiO2 content and the total amount by EPMA are slightly higher and lower than those by XRF, respectively. Table 5 shows analytical results of three individual grains from the volcanic glass. These results are almost equivalent, indicating that the analyzed glass is almost homogeneous and a good reference sample. Most of the analytical results in this study are quantitatively and stoichiometricaly satisfactory for our purpose. Common rock-forming minerals The conditions for analysis of common rock-forming minerals are an accelerating voltage of 15kV, a beam current of 15nA on the Faraday cup, a peak count time of 20-30sec, and a probe diameter of 5µm for phenocryst-sized grains. A focused beam is used for analysis of small grains, such as inclusions. When using a focused beam, a beam current of 12nA and a peak count time of 10-20sec are used. 11 major elements (Si, Ti, Al, Cr, Fe, Mn, Mg, Ca, Na, K and Ni) are analyzed. Minor components for olivine Olivine is composed of cations of Mg, Fe and Si, and minor Mn, Ca and Ni. Minor components in mafic minerals give us information about magma generation. Consequently, they must be analyzed with high precision. A sufficient X-ray intensity for this analysis is not obtained with the conditions shown above. An incident electron energy at least 2 to 3 times of the critical excitation energy is required in order to obtain precise analyses. Although a high accelerating voltage can obtain a relatively high X-ray intensity, the following problems occur: (1) penetration of the beam into the specimen, (2) necessity of a large absorption correction, and (3) loss of spatial resolution. Suitable conditions for the analysis of minor components of olivine were obtained in this study: an accelerating voltage of 20kV, a beam current of 25nA and a probe diameter of 5µm. The peak count times are 10-30sec for major components (Si, Mg and Fe) and 100-200sec for minor components (Ca, Mn and Ni). A combination of high sensitive analyzing crystal (LiFH) and detector was used in the analyses for Mn and Ni. This combination can obtain about 3 times the X-ray intensity relative to the regular combination. Therefore, the total analyzing time was relatively decreased. Acknowledgements. I wish to thank N. Irino and K. Tani for XRF analysis of the volcanic glass. I am also greatly indebted to Y. Tamura, T. Tsujimori and T. Morishita for their suggestion. K. Uematsu assisted with operation of JXA-8900. References Scott, V. D., G. Love, and S. J. B. Reed, Quantitative electron-probe microanalysis, 311pp., Ellis Horwood Limited, 1995. Soejima, H., Electron probe microanalysis, 597pp., The Nikkan Kogyo Shinbun, LTD., 1987. Volcanic glass Glass is very sensitive to an electron beam. The analytical conditions must be carefully chosen. Fig. 1 shows the variations of X-ray intensity for Na-Kα with count time under some conditions. It indicates that a focused beam decreases the X-ray intensity of Na-Kα with time. The preferred analytical conditions are: 15kV, 10nA, and a probe diameter of 10µm. The peak count time is 10-30sec. Ten major elements (Si, Ti, Al, Fe, Mn, Mg, Ca, Na, K and P) can be analyzed. The total analyzing time for a point is less than 4 minutes. It was checked that the submarine volcanic glass as a reference sample could survive damage from electron exposure during analysis. 130 FRONTIER RESEARCH ON EARTH EVOLUTION, VOL. 1 Figure 1. Variations of X-ray intensity of Na-Kα to count time in the volcanic glass. (a) 15kV, 10nA and focused beam. (b) 15kV, 20nA and focused beam. (c) 15kV, 10nA and broad beam (10µm). The intensity of Na-Kα decreases with count time in the conditions using a focus beam (a and b). However, the intensity of Na-Kα is almost constant with count time in the condition using a broad beam (10µm). 131 FRONTIER RESEARCH ON EARTH EVOLUTION, VOL. 1 Table 1. Lists of standard materials and their compositions 132 FRONTIER RESEARCH ON EARTH EVOLUTION, VOL. 1 Table 2. Lists of analyzing crystals and analytical conditions. (a) Combinations of analyzing crystals and X-ray detectors. (b) Combinations of analyzing crystals and analyzing time. (c) Combinations of standard materials for each target material. 133 FRONTIER RESEARCH ON EARTH EVOLUTION, VOL. 1 Table 3. Analyses of silicate and oxide minerals in 15kV-15nA. Representative analyses, average and standard deviations (>15) are listed. 134 FRONTIER RESEARCH ON EARTH EVOLUTION, VOL. 1 Table 3. (Continued) 135 FRONTIER RESEARCH ON EARTH EVOLUTION, VOL. 1 Table 4. Analyses of olivine in 20kV-25nA. Recommended compositions, represent analyses, average and standard deviations (>20) are listed. Table 5. Analytical results of submarine volcanic glass by broad beam (10µm) in 15kV10nA. The compositions determined by XRF are also listed. The results of three individual grains are almost equivalent. It suggests that the analyzed glass is homogeneous. 136
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