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J. W. Harris, M. T. Hutchison, M. Hursthouse, M. Light, B. Harte, Nature 387, 486 (1997).
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Nature
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Harris, J.W.1
Hutchison, M.T.2
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Light, M.4
Harte, B.5
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5
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0005197513
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abstr.
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M. T. Hutchison, B. Harte, J. W. Harris, I. Fitzsimons, 6th Int. Kimberlite Conf. (abstr.) (1995), p. 242.
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Hutchison, M.T.1
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6
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0026187321
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2). The gamma rays are collimated to the selected sample diameter using a Pb shield, and the source-sample distance is reduced to <5 mm. The latter results in a solid angle similar to conventional experiments, and hence a similar count rate. Because the signal quality depends on absorber density (measured in milligrams of Fe per square centimeter) and not the total amount of iron in the sample, the reduction in sample size has no effect on the effective thickness of the absorber. When electronic absorption due to heavier elements is low and the point source is relatively new (<1 year old), high-quality Mössbauer spectra (comparable to conventional measurements) can be recorded on samples with diameters as small as 100 μm. For further information see C. A. McCammon, V. Chaskar, and G. G. Richards [Meas. Sci. Technol. 2, 657 (1991)] and C. A. McCammon [Hyper. Int. 92, 1235 (1994)].
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McCammon, C.A.1
Chaskar, V.2
Richards, G.G.3
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7
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0000109947
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2). The gamma rays are collimated to the selected sample diameter using a Pb shield, and the source-sample distance is reduced to <5 mm. The latter results in a solid angle similar to conventional experiments, and hence a similar count rate. Because the signal quality depends on absorber density (measured in milligrams of Fe per square centimeter) and not the total amount of iron in the sample, the reduction in sample size has no effect on the effective thickness of the absorber. When electronic absorption due to heavier elements is low and the point source is relatively new (<1 year old), high-quality Mössbauer spectra (comparable to conventional measurements) can be recorded on samples with diameters as small as 100 μm. For further information see C. A. McCammon, V. Chaskar, and G. G. Richards [Meas. Sci. Technol. 2, 657 (1991)] and C. A. McCammon [Hyper. Int. 92, 1235 (1994)].
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McCammon, C.A.1
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8
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1842387634
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note
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Compositions were determined using a Cameca Camebax electron microprobe at the University of Edinburgh, Department of Geology and Geophysics, operating at 20 kV with a beam current of 20 nA.
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9
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1842273995
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note
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2) in a 12-μm Rh matrix. The velocity scale was calibrated relative to 25-μm α-Fe foil using the positions certified for National Bureau of Standards standard reference material no. 1541; line widths of 0.42 mm/s for the outer lines of α-Fe were obtained at room temperature. The spectra were fitted to Lorentzian and Voigt line shapes using the commercially available fitting program NORMOS written by R.A. Brand (distributed by Wissenschaftliche Elektronik GmbH, Germany).
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11
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1842389548
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note
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3+ absorption is constrained by the asymmetry of the main doublet, and is therefore relatively independant of the fitting model.
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12
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0344744335
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Plume 2, D. L. Anderson, S. R. Hart, A. W. Hofmann, Eds.
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C. A. McCammon, J. W. Harris, B. Harte, M. T. Hutchison, in Plume 2, D. L. Anderson, S. R. Hart, A. W. Hofmann, Eds. [Terra Nostra 3, 91 (1995)].
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Terra Nostra
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McCammon, C.A.1
Harris, J.W.2
Harte, B.3
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0019927296
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F. Seifert, B. O. Mysen, D. Virgo, E.-R. Neumann, Annu. Rep. Carneg. Inst. Wash. Geophys. Lab. 81, 355 (1982).
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Y. B. Wang, F. Guyot, R. C. Liebermann, J. Geophys. Res. 97, 12, 327 (1992).
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Liebermann, R.C.3
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0008256390
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C. A. McCammon, Phase Trans. 58, 1 (1996); G. M. Bancroft, A. G. Maddock, R. G. Burns, Geochim. Cosmochim. Acta 31, 2219 (1967).
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Phase Trans.
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McCammon, C.A.1
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C. A. McCammon, Phase Trans. 58, 1 (1996); G. M. Bancroft, A. G. Maddock, R. G. Burns, Geochim. Cosmochim. Acta 31, 2219 (1967).
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R. O. Moore, M. L. Otter, R. S. Rickard, J. W. Harris, J. J. Gurney, Geol. Soc. Aust. Abstr. 16, 409 (1986).
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Moore, R.O.1
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0024193953
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F. Guyot, M. Madon, J. Peyronneau, J. P. Poirier, Earth Planet. Sci. Lett. 90, 52 (1988); Y. Fei, H. K. Mao, B. O. Mysen, J. Geophys. Res. 96, 2157 (1991); S. E. Kesson and J. D. Fitz Gerald, Earth Planet. Sci. Lett. 111, 229 (1991).
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Guyot, F.1
Madon, M.2
Peyronneau, J.3
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0026082414
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F. Guyot, M. Madon, J. Peyronneau, J. P. Poirier, Earth Planet. Sci. Lett. 90, 52 (1988); Y. Fei, H. K. Mao, B. O. Mysen, J. Geophys. Res. 96, 2157 (1991); S. E. Kesson and J. D. Fitz Gerald, Earth Planet. Sci. Lett. 111, 229 (1991).
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Fei, Y.1
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0027063865
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F. Guyot, M. Madon, J. Peyronneau, J. P. Poirier, Earth Planet. Sci. Lett. 90, 52 (1988); Y. Fei, H. K. Mao, B. O. Mysen, J. Geophys. Res. 96, 2157 (1991); S. E. Kesson and J. D. Fitz Gerald, Earth Planet. Sci. Lett. 111, 229 (1991).
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1842355826
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Cologne, Germany, 15 to 19 September
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S. Lauterbach, C. A. McCammon, F. Seifert, paper presented at the 75th annual meeting of the German Mineralogical Society, Cologne, Germany, 15 to 19 September 1997.
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(1997)
75th Annual Meeting of the German Mineralogical Society
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Lauterbach, S.1
McCammon, C.A.2
Seifert, F.3
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29
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1842285750
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note
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The mineral inclusions were supplied by B. Harte, and the electron microprobe analyses for samples BZ66, BZ67, BZ73, and BZ210B were performed by M. Wilding and B. Harte. The manuscript was improved through discussions with B. Harte and S. Kesson.
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