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Volumn 278, Issue 5337, 1997, Pages 434-436

Ferric iron content of mineral inclusions in diamonds from Sao Luiz: A view into the lower mantle

Author keywords

[No Author keywords available]

Indexed keywords

DIAMOND; FERRIC ION; MINERAL;

EID: 0030667978     PISSN: 00368075     EISSN: None     Source Type: Journal    
DOI: 10.1126/science.278.5337.434     Document Type: Review
Times cited : (116)

References (29)
  • 6
    • 0026187321 scopus 로고
    • 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)].
    • (1991) Meas. Sci. Technol. , vol.2 , pp. 657
    • McCammon, C.A.1    Chaskar, V.2    Richards, G.G.3
  • 7
    • 0000109947 scopus 로고
    • 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)].
    • (1994) Hyper. Int. , vol.92 , pp. 1235
    • McCammon, C.A.1
  • 8
    • 1842387634 scopus 로고    scopus 로고
    • note
    • 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.
  • 9
    • 1842273995 scopus 로고    scopus 로고
    • note
    • 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).
  • 11
    • 1842389548 scopus 로고    scopus 로고
    • note
    • 3+ absorption is constrained by the asymmetry of the main doublet, and is therefore relatively independant of the fitting model.
  • 16
    • 0008256390 scopus 로고    scopus 로고
    • C. A. McCammon, Phase Trans. 58, 1 (1996); G. M. Bancroft, A. G. Maddock, R. G. Burns, Geochim. Cosmochim. Acta 31, 2219 (1967).
    • (1996) Phase Trans. , vol.58 , pp. 1
    • McCammon, C.A.1
  • 25
    • 0026082414 scopus 로고
    • 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).
    • (1991) J. Geophys. Res. , vol.96 , pp. 2157
    • Fei, Y.1    Mao, H.K.2    Mysen, B.O.3
  • 26
    • 0027063865 scopus 로고
    • 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).
    • (1991) Earth Planet. Sci. Lett. , vol.111 , pp. 229
    • Kesson, S.E.1    Fitz Gerald, J.D.2
  • 29
    • 1842285750 scopus 로고    scopus 로고
    • note
    • 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.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.