TY - JOUR
T1 - Deep Mantle Influence on the Cameroon Volcanic Line
AU - Saeidi, Hesam
AU - Hansen, Samantha E.
AU - Nyblade, Andrew A.
N1 - Funding Information:
We thank Scott King and an anonymous reviewer for their thorough critiques of our manuscript. Much of the new seismic data used in this study were collected by projects supported by the National Science Foundation (Grants 0440032, 0530062, 0824781, 1128936, and 1634108).
Funding Information:
Data management handling was provided by the Incorporated Research Institutions for Seismology Data Management Center (IRIS DMC; http://ds.iris.edu/mda/ ), which is funded through the Seismological Facilities for the Advancement of Geoscience award of the NSF under cooperative support agreement EAR‐1851048. Some figures were generated with Generic Mapping Tools (Wessel et al., 2013 ).
Publisher Copyright:
© 2022 The Authors.
PY - 2023/1
Y1 - 2023/1
N2 - The origin of the Cameroon Volcanic Line (CVL), which is difficult to explain with traditional plate tectonics and mantle convection models because the volcanism does not display clear age progression, remains widely debated. Existing seismic tomography models show anomalously slow structure beneath the CVL, which some have interpreted to reflect upper mantle convective processes, possibly associated with edge-driven flow related to the neighboring Congo Craton. However, mid- and lower mantle depths are generally not well resolved in these models, making it difficult to determine the extent of the anomalous CVL structure. Here, we present a new P-wave velocity model for the African mantle, developed with the largest collection of travel-time residuals recorded across the continent to date and an adaptive model parameterization. Our extensive data set and inversion method yield high resolution images of the mantle structure beneath western Africa, particularly at the critical mid- and lower mantle depths needed to further evaluate processes associated with the formation of the CVL. Our new model provides strong evidence for a connection between the African Large Low Velocity Province, centered in the lower mantle beneath southern Africa, and the continental portion of the CVL. We suggest that seismically slow material generated near the core-mantle boundary beneath southern Africa moves northwestward under the Congo Craton. At the northern edge of the craton, the hot, buoyant material rises through the upper mantle, causing the CVL volcanism. Consequently, CVL magmatism can be linked to large-scale mantle processes rooted in the deep mantle.
AB - The origin of the Cameroon Volcanic Line (CVL), which is difficult to explain with traditional plate tectonics and mantle convection models because the volcanism does not display clear age progression, remains widely debated. Existing seismic tomography models show anomalously slow structure beneath the CVL, which some have interpreted to reflect upper mantle convective processes, possibly associated with edge-driven flow related to the neighboring Congo Craton. However, mid- and lower mantle depths are generally not well resolved in these models, making it difficult to determine the extent of the anomalous CVL structure. Here, we present a new P-wave velocity model for the African mantle, developed with the largest collection of travel-time residuals recorded across the continent to date and an adaptive model parameterization. Our extensive data set and inversion method yield high resolution images of the mantle structure beneath western Africa, particularly at the critical mid- and lower mantle depths needed to further evaluate processes associated with the formation of the CVL. Our new model provides strong evidence for a connection between the African Large Low Velocity Province, centered in the lower mantle beneath southern Africa, and the continental portion of the CVL. We suggest that seismically slow material generated near the core-mantle boundary beneath southern Africa moves northwestward under the Congo Craton. At the northern edge of the craton, the hot, buoyant material rises through the upper mantle, causing the CVL volcanism. Consequently, CVL magmatism can be linked to large-scale mantle processes rooted in the deep mantle.
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U2 - 10.1029/2022GC010621
DO - 10.1029/2022GC010621
M3 - Article
AN - SCOPUS:85147089954
SN - 1525-2027
VL - 24
JO - Geochemistry, Geophysics, Geosystems
JF - Geochemistry, Geophysics, Geosystems
IS - 1
M1 - e2022GC010621
ER -