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0032548153
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Geophysical investigations [L. Bréger and B. Romanowicz, Science 282, 718 (1998); D. V. Helmberger, L. Wen. X. Ding, Nature 396, 251 (1998); S. A. Russell, T. Lay, E. J. Garnero, Nature 396, 255 (1998); H. Bijwaard and W. Spakman, Earth Planet. Sci. Lett. 166, 121 (1999)] together with geochemical investigations [R. J. Walker, J. W. Morgan, M. F. Horan, Science 269, 819 (1995); E. Widom and S. B. Shirey, Earth Planet. Sci. Lett. 142, 451 (1996); R. J. Walker et al., Geochim. Cosmochim. Acta 61, 4799 (1997); A. D. Brandon, R. J. Walker, J. W. Morgan, M. D. Norman, H. M. Prichard, Science 280, 1570 (1998); J. E. Snow and G. Schmidt, Nature 391, 166 (1998); J. M. Bird, A. Meibom, R. Frei, T. F. Nägler, Earth Planet. Sci. Lett. 170, 83 (1999)] suggest that plumes emerge from the core-mantle boundary.
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Geophysical investigations [L. Bréger and B. Romanowicz, Science 282, 718 (1998); D. V. Helmberger, L. Wen. X. Ding, Nature 396, 251 (1998); S. A. Russell, T. Lay, E. J. Garnero, Nature 396, 255 (1998); H. Bijwaard and W. Spakman, Earth Planet. Sci. Lett. 166, 121 (1999)] together with geochemical investigations [R. J. Walker, J. W. Morgan, M. F. Horan, Science 269, 819 (1995); E. Widom and S. B. Shirey, Earth Planet. Sci. Lett. 142, 451 (1996); R. J. Walker et al., Geochim. Cosmochim. Acta 61, 4799 (1997); A. D. Brandon, R. J. Walker, J. W. Morgan, M. D. Norman, H. M. Prichard, Science 280, 1570 (1998); J. E. Snow and G. Schmidt, Nature 391, 166 (1998); J. M. Bird, A. Meibom, R. Frei, T. F. Nägler, Earth Planet. Sci. Lett. 170, 83 (1999)] suggest that plumes emerge from the core-mantle boundary.
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Geophysical investigations [L. Bréger and B. Romanowicz, Science 282, 718 (1998); D. V. Helmberger, L. Wen. X. Ding, Nature 396, 251 (1998); S. A. Russell, T. Lay, E. J. Garnero, Nature 396, 255 (1998); H. Bijwaard and W. Spakman, Earth Planet. Sci. Lett. 166, 121 (1999)] together with geochemical investigations [R. J. Walker, J. W. Morgan, M. F. Horan, Science 269, 819 (1995); E. Widom and S. B. Shirey, Earth Planet. Sci. Lett. 142, 451 (1996); R. J. Walker et al., Geochim. Cosmochim. Acta 61, 4799 (1997); A. D. Brandon, R. J. Walker, J. W. Morgan, M. D. Norman, H. M. Prichard, Science 280, 1570 (1998); J. E. Snow and G. Schmidt, Nature 391, 166 (1998); J. M. Bird, A. Meibom, R. Frei, T. F. Nägler, Earth Planet. Sci. Lett. 170, 83 (1999)] suggest that plumes emerge from the core-mantle boundary.
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0342421145
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36Ar was measured by ion counting after amplification by an electron multiplier.
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36
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0002438587
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22Ne ratio measured so far in mantle rocks [M. Ozima and S. Zashu, Geochim. Cosmochim. Acta 52, 19 (1988)] is dose to the solar ratio [J.-P. Benkert, H. Baur, P. Signer, R. Wieler, J. Geophys. Res. 98, 13147 (1993)] and is much higher than any other known component such as Ne-E [M. H. A. Jungck and P. Eberhardt, Meteoritics 14, 439 (1979)], cosmogenic Ne [E. Mazor, D. Heymann, E. Anders, Ceochim. Cosmochim. Acta 34, 781 (1970)]. Ne-A [M. Tang and E. Anders, Geochim. Cosmochim. Acta 52, 1245 (1988)], or Ne-Q [R. Wieler, E. Anders, H. Baur, R. S. Lewis, P. Signer, Ceochim. Cosmochim. Acta 56, 2907 (1992)].
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22Ne ratio measured so far in mantle rocks [M. Ozima and S. Zashu, Geochim. Cosmochim. Acta 52, 19 (1988)] is dose to the solar ratio [J.-P. Benkert, H. Baur, P. Signer, R. Wieler, J. Geophys. Res. 98, 13147 (1993)] and is much higher than any other known component such as Ne-E [M. H. A. Jungck and P. Eberhardt, Meteoritics 14, 439 (1979)], cosmogenic Ne [E. Mazor, D. Heymann, E. Anders, Ceochim. Cosmochim. Acta 34, 781 (1970)]. Ne-A [M. Tang and E. Anders, Geochim. Cosmochim. Acta 52, 1245 (1988)], or Ne-Q [R. Wieler, E. Anders, H. Baur, R. S. Lewis, P. Signer, Ceochim. Cosmochim. Acta 56, 2907 (1992)].
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0005000859
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22Ne ratio measured so far in mantle rocks [M. Ozima and S. Zashu, Geochim. Cosmochim. Acta 52, 19 (1988)] is dose to the solar ratio [J.-P. Benkert, H. Baur, P. Signer, R. Wieler, J. Geophys. Res. 98, 13147 (1993)] and is much higher than any other known component such as Ne-E [M. H. A. Jungck and P. Eberhardt, Meteoritics 14, 439 (1979)], cosmogenic Ne [E. Mazor, D. Heymann, E. Anders, Ceochim. Cosmochim. Acta 34, 781 (1970)]. Ne-A [M. Tang and E. Anders, Geochim. Cosmochim. Acta 52, 1245 (1988)], or Ne-Q [R. Wieler, E. Anders, H. Baur, R. S. Lewis, P. Signer, Ceochim. Cosmochim. Acta 56, 2907 (1992)].
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22Ne ratio measured so far in mantle rocks [M. Ozima and S. Zashu, Geochim. Cosmochim. Acta 52, 19 (1988)] is dose to the solar ratio [J.-P. Benkert, H. Baur, P. Signer, R. Wieler, J. Geophys. Res. 98, 13147 (1993)] and is much higher than any other known component such as Ne-E [M. H. A. Jungck and P. Eberhardt, Meteoritics 14, 439 (1979)], cosmogenic Ne [E. Mazor, D. Heymann, E. Anders, Ceochim. Cosmochim. Acta 34, 781 (1970)]. Ne-A [M. Tang and E. Anders, Geochim. Cosmochim. Acta 52, 1245 (1988)], or Ne-Q [R. Wieler, E. Anders, H. Baur, R. S. Lewis, P. Signer, Ceochim. Cosmochim. Acta 56, 2907 (1992)].
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22Ne ratio measured so far in mantle rocks [M. Ozima and S. Zashu, Geochim. Cosmochim. Acta 52, 19 (1988)] is dose to the solar ratio [J.-P. Benkert, H. Baur, P. Signer, R. Wieler, J. Geophys. Res. 98, 13147 (1993)] and is much higher than any other known component such as Ne-E [M. H. A. Jungck and P. Eberhardt, Meteoritics 14, 439 (1979)], cosmogenic Ne [E. Mazor, D. Heymann, E. Anders, Ceochim. Cosmochim. Acta 34, 781 (1970)]. Ne-A [M. Tang and E. Anders, Geochim. Cosmochim. Acta 52, 1245 (1988)], or Ne-Q [R. Wieler, E. Anders, H. Baur, R. S. Lewis, P. Signer, Ceochim. Cosmochim. Acta 56, 2907 (1992)].
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22Ne ratio measured so far in mantle rocks [M. Ozima and S. Zashu, Geochim. Cosmochim. Acta 52, 19 (1988)] is dose to the solar ratio [J.-P. Benkert, H. Baur, P. Signer, R. Wieler, J. Geophys. Res. 98, 13147 (1993)] and is much higher than any other known component such as Ne-E [M. H. A. Jungck and P. Eberhardt, Meteoritics 14, 439 (1979)], cosmogenic Ne [E. Mazor, D. Heymann, E. Anders, Ceochim. Cosmochim. Acta 34, 781 (1970)]. Ne-A [M. Tang and E. Anders, Geochim. Cosmochim. Acta 52, 1245 (1988)], or Ne-Q [R. Wieler, E. Anders, H. Baur, R. S. Lewis, P. Signer, Ceochim. Cosmochim. Acta 56, 2907 (1992)].
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2/Ar ratios in mantle vesicles do not correlate with any index of partial melting or degassing, which suggests a comparable behavior of Ar and N. Because Ar is incompatible, this element and by inference N are thoroughly extracted from the mantle during magma genesis and subsequent degassing (70, 13, 27).
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We thank I. N. Tolstikhin for providing us with these unique samples; K. Hashizume and S. R. Boyd for insightful discussions; and L. Zimmermann, P. Robert, and G. Sauder for help in keeping the mass spectrometer in fine shape. This is contribution 1434 of the Centre de Recherches Pétrographiques et Géochimiques.
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