4.7 Article

Formation of the Igneous Logi Ridge, NE Atlantic

期刊

出版社

AMER GEOPHYSICAL UNION
DOI: 10.1029/2021JB023891

关键词

gravity modeling; intraplate volcanism; magmatic production rate; Logi Ridge; seamount crustal structure

资金

  1. Scientific Research Fund of the Second Institute of Oceanography, MNR [HYGG2001]
  2. Natural Science Foundation of China [42006072]
  3. Innovation Group Project of Southern Marine Science and Engineering Guangdong Laboratory (Zhuhai) [311020018]
  4. Qianjiang talent [QJD2002033]
  5. Research Council of Norway [223272]

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This study investigates the geological features and volcanic activity of the Logi Ridge, finding that the ridge has a thick crust and the melting process is mainly influenced by enriched mantle rather than high mantle temperature.
The igneous Logi Ridge is located in the NE Atlantic north of the West Jan Mayen Fracture Zone on oceanic crust. The origin of the ridge may relate to the increased influence of the Iceland plume in the Oligocene though the exact mechanism is uncertain. We estimate the igneous volume and magma production rate of the ridge from 10 transects, comprising a refraction profile, six reflection profiles, and three bathymetric profiles. The refraction profile shows up to 12 km crustal thickness of the ridge, and the forward gravity modeling and/or isostatic balancing shows that this is characteristic for most of the ridges. A 3D volume model was created by interpolating between profiles and subtracted the similarly made regional crustal thickness (5-7 km), which gives an excess magma volume of (1.7 +/- 0.6) x 10(13) m(3). The admittance function between bathymetry and gravity indicates an elastic plate thickness of 3-5 km during the main ridge formation. This is consistent with the ridge being built on oceanic crust from Oligocene to earliest Miocene, indicating a main magmatic phase of similar to 5 Ma duration, which gives a magma production rate of 0.07-0.15 m(3)/s, comparable to the Louisville Seamount Chain (LSC). However, the lower crustal velocities of the refraction profile differ from that of the Louisville Guyot in the LSC, suggesting that the melting event was not mainly caused by high mantle temperature, instead it may have been caused in part by the enriched mantle presently seen at the northern end of the Kolbeinsey Ridge to the south.

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