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- W2172171429 abstract "Studies of the petrology, mineral chemistry, and rock magnetic properties of nine pyroxenite xenoliths from Hannuoba basalts, northern North China Craton, have been made to determine the magnetization signature of the continental lower crust. These pyroxenites are weakly magnetic with low average susceptibility (χ) and saturation isothermal remanent magnetization (Mrs) of 39.59 × 10−8 m3 kg−1 and 12.05 × 10−3 Am2 kg−1, respectively. The magnetic minerals are mainly magnetite, pyrrhotite, and Fe-rich spinel, which significantly contribute to χ and natural remanent magnetization. Magnetite occurs as interstitial microcrystals together with zeolite aggregates, indicating a secondary origin in a supergene environment. In contrast, pyrrhotite and Fe-rich spinel were formed prior to the xenoliths' ascent to the surface, as evidenced by their dominant occurrence as tiny inclusions and thin exsolution lamellae in pyroxene. The Fe-rich spinel has ~ 50% mole fraction of Fe3O4 and corresponds to the strongest magnetization, and its coexistence with Mg-rich spinel implies a reheating event due to the underplating of basaltic magma. Besides, armalcolite and ilmenite were found in the reaction rims between xenoliths and the basalt, but they contribute little to the whole rock magnetization. However, these pyroxenite xenoliths would be nonmagnetic at in situ depths, as well as peridotite and mafic granulite xenoliths derived from the crust-mantle transition zone (~ 32–42 km). Therefore, we suggest the limiting depth of magnetization at the boundary between weakly magnetic deep-seated (lower crust and upper mantle) xenoliths and strongly magnetic Archean granulite facies rocks (~ 32 km) in Hannuoba, northern North China Craton." @default.
- W2172171429 created "2016-06-24" @default.
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- W2172171429 date "2014-02-01" @default.
- W2172171429 modified "2023-10-16" @default.
- W2172171429 title "Magnetic mineralogy of pyroxenite xenoliths from Hannuoba basalts, northern North China Craton: Implications for magnetism in the continental lower crust" @default.
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- W2172171429 cites W1510196279 @default.
- W2172171429 cites W1544856261 @default.
- W2172171429 cites W1546413955 @default.
- W2172171429 cites W1587624588 @default.
- W2172171429 cites W1591480399 @default.
- W2172171429 cites W1860192746 @default.
- W2172171429 cites W1972174623 @default.
- W2172171429 cites W1973820924 @default.
- W2172171429 cites W1977431633 @default.
- W2172171429 cites W1981334834 @default.
- W2172171429 cites W1990130984 @default.
- W2172171429 cites W1992587453 @default.
- W2172171429 cites W1995941045 @default.
- W2172171429 cites W2000253240 @default.
- W2172171429 cites W2002499021 @default.
- W2172171429 cites W2002847449 @default.
- W2172171429 cites W2003678036 @default.
- W2172171429 cites W2007192582 @default.
- W2172171429 cites W2007301182 @default.
- W2172171429 cites W2007770378 @default.
- W2172171429 cites W2011138323 @default.
- W2172171429 cites W2011938120 @default.
- W2172171429 cites W2011971340 @default.
- W2172171429 cites W2014665449 @default.
- W2172171429 cites W2014757385 @default.
- W2172171429 cites W2016959530 @default.
- W2172171429 cites W2018264648 @default.
- W2172171429 cites W2019475090 @default.
- W2172171429 cites W2021290249 @default.
- W2172171429 cites W2022650564 @default.
- W2172171429 cites W2022854579 @default.
- W2172171429 cites W2024674080 @default.
- W2172171429 cites W2026133956 @default.
- W2172171429 cites W2027025610 @default.
- W2172171429 cites W2033354344 @default.
- W2172171429 cites W2035686077 @default.
- W2172171429 cites W2035751343 @default.
- W2172171429 cites W2036883149 @default.
- W2172171429 cites W2045752704 @default.
- W2172171429 cites W2046141409 @default.
- W2172171429 cites W2052128667 @default.
- W2172171429 cites W2054360327 @default.
- W2172171429 cites W2056098342 @default.
- W2172171429 cites W2058977872 @default.
- W2172171429 cites W2061417166 @default.
- W2172171429 cites W2064616831 @default.
- W2172171429 cites W2067711104 @default.
- W2172171429 cites W2069778669 @default.
- W2172171429 cites W2077080626 @default.
- W2172171429 cites W2077085454 @default.
- W2172171429 cites W2078204936 @default.
- W2172171429 cites W2083656706 @default.
- W2172171429 cites W2084892663 @default.
- W2172171429 cites W2085002667 @default.
- W2172171429 cites W2087690822 @default.
- W2172171429 cites W2088114914 @default.
- W2172171429 cites W2088850138 @default.
- W2172171429 cites W2089122977 @default.
- W2172171429 cites W2090189534 @default.
- W2172171429 cites W2092678398 @default.
- W2172171429 cites W2093599524 @default.
- W2172171429 cites W2103490462 @default.
- W2172171429 cites W2122467685 @default.
- W2172171429 cites W2129225116 @default.
- W2172171429 cites W2133042542 @default.
- W2172171429 cites W2138035397 @default.
- W2172171429 cites W2152135643 @default.
- W2172171429 cites W2166901676 @default.
- W2172171429 cites W2167856052 @default.
- W2172171429 cites W2169997237 @default.
- W2172171429 cites W2202998678 @default.
- W2172171429 cites W2312965665 @default.
- W2172171429 cites W2345027921 @default.
- W2172171429 cites W2470900732 @default.
- W2172171429 doi "https://doi.org/10.1002/2013jb010599" @default.
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