RUSSIAN JOURNAL OF EARTH SCIENCES, VOL. 15, ES1004, doi:10.2205/2015ES000550, 2015
Component | 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 | 10 | 11 | 12 | 13 |
$\mathrm{SiO_2}$ | 38.46 | 39.92 | 40.10 | 38.65 | 42.57 | 39.85 | 41.15 | 40.89 | 42.21 | 42.92 | 43.90 | 43.76 | 39.77 |
$\mathrm{TiO_2}$ | 4.58 | 3.78 | 4.33 | 2.97 | 4.79 | 7.35 | 4.14 | 5.64 | 1.02 | 2.62 | 3.52 | 2.97 | 5.67 |
$\mathrm{Al_2O_3}$ | 13.50 | 14.54 | 13.03 | 16.61 | 11.05 | 12.69 | 14.61 | 14.25 | 15.15 | 14.56 | 13.63 | 14.05 | 14.06 |
FeO* | 16.29 | 13.99 | 14.08 | 13.08 | 10.38 | 9.50 | 8.05 | 6.23 | 4.33 | 3.40 | 3.81 | 4.02 | 11.25 |
MnO | 0.35 | 0.00 | 0.00 | 0.07 | 0.45 | 0.43 | 0.05 | 0.09 | 0.07 | 0.04 | 0.05 | 0.07 | 0.12 |
MgO | 9.66 | 10.47 | 11.65 | 13.65 | 10.66 | 10.27 | 14.46 | 14.97 | 17.34 | 17.04 | 16.85 | 16.79 | 11.47 |
CaO | 10.76 | 11.87 | 10.71 | 11.05 | 12.63 | 13.03 | 11.42 | 11.35 | 11.62 | 10.96 | 10.82 | 10.56 | 10.64 |
$\mathrm{Na_2O}$ | 3.17 | 3.15 | 2.92 | 2.44 | 2.97 | 2.63 | 2.36 | 2.15 | 3.32 | 3.31 | 3.85 | 3.49 | 2.74 |
$\mathrm{K_2O}$ | 1.32 | 0.32 | 1.08 | 1.26 | 0.84 | 0.83 | 2.17 | 2.13 | 0.06 | 1.63 | 0.67 | 1.35 | 1.40 |
$\mathrm{Cr_2O_3}$ | - | 0.26 | - | - | - | - | 0.17 | 0.89 | 0.82 | 1.06 | 0.86 | 0.18 | - |
N | 6 | 6 | 5 | 1 | 1 | 1 | 3 | 2 | 3 | 1 | 1 | 1 | 2 |
Note: the Roca Negra: 1 – sample RC1/10, 2 – sample RC1/5, 3 – sample RC10/3 (this publication), 4 – amphibole [Tournon, 1968], 5, 6 – sample 15126: 5 – grain core, 6 – grain margin [Sanchez, 1983], 7–9 – central Spain: 7 – K–Ti pargasite in glimmerite, 8 – K-kaersutite in micaceous lherzolite, 9 – pargasite in spinel lherzolite [Ancochea and Nixon, 1987], 10–11 – spinel lherzolite xenoliths [Ionov et al., 1984], 12 – pargasite in lherzolite xenolith [Dawson and Smith, 1977], 13 – kaersutite in xenoliths in basalts from the Tien Shan [Dobretsov and Dobretsova, 1975]. |
Citation: Grachev A. F. (2015), Pyroxenite xenoliths in basalts of the Roca Negra volcano, Catalonia, Russ. J. Earth Sci., 15, ES1004, doi:10.2205/2015ES000550.
Copyright 2015 by the Geophysical Center RAS.