Marine magnetic anomalies as recorders of geomagnetic intensity variations
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Cited by (35)
Ridge propagation, oceanic core complexes, and ultramafic-hosted hydrothermalism at Rainbow (MAR 36°N): Insights from a multi-scale magnetic exploration
2018, Earth and Planetary Science LettersCitation Excerpt :The shape of this anomaly displays the characteristic three lobes of the axial anomaly at slow spreading rates (e.g., Gee et al., 1996) in the South Amar segment and the southern part of Amar Minor South segment (south of 36°10′N), as well as in the Amar segment. The central lobe marks the position of the active spreading center, where fresh basalt bears a stronger magnetization (Central Anomaly Magnetic High or CAMH of Klitgord, 1976), and the two secondary lobes correspond to the stronger intensity of the geomagnetic field that prevailed after the Brunhes–Matuyama reversal (Gee et al., 1996). These secondary lobes are not observed in the northern Amar Minor South segment and the whole Amar Minor North segment.
Dyking at EPR 16°N hypermagmatic ridge segment: Insights from near-seafloor magnetics
2016, Earth and Planetary Science LettersSource of Oceanic Magnetic Anomalies and the Geomagnetic Polarity Timescale
2015, Treatise on Geophysics: Second EditionThe Stardalur magnetic anomaly revisited-New insights into a complex cooling and alteration history
2007, Physics of the Earth and Planetary InteriorsSource of Oceanic Magnetic Anomalies and the Geomagnetic Polarity Timescale
2007, Treatise on Geophysics5.12 - Source of Oceanic Magnetic Anomalies and the Geomagnetic Polarity Timescale
2007, Treatise on Geophysics: Volume 1-10
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