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This work is licensed under a Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND).
We use co-located CTD/transmissometry casts and multichannel seismic reﬂection surveys conducted at the Costa Rica Rift (CRR) to provide a better understanding of magma-hydrothermal processes occurring at an intermediate-rate spreading center. Water column observations reveal an ∼200 m thick plume head ∼650 m above the seaﬂoor, which corresponds to a hydrothermal heat output of ∼200 ± 100 MW at the ridge axis. Assuming a hydrothermal vent temperature of 350◦C and a discharge area between 104and 105 m2, this heat output implies a mean crustal permeability within the discharge zone of between 2 × 10−14 and 6 × 10−13 m2, and a conductive thermal boundary layer thickness of ∼20 m. The volume of magma required to maintain the current hydrothermal heat output over the past two decades should result in an across-axis axial magma lens (AML) width between 270 and 1300 m, depending on the amount of cooling and crystallization. However, seismic reﬂection images, acquired in 1994 and 2015, while showing an apparent along-axis growth of the AML from 2.4 to 6.0 km between surveys, also suggest that, as of 2015, the AML has an apparent across-axis width of no more than 300 m, and that magma delivery at the intermediate spreading rate CRR may be episodic on time scales of tens of years. The data on magma-hydrothermal interactions at the CRR collected in 1994 and 2015 suggest that the hydrothermal system may have signiﬁcantly cooled and crystallized the AML, primarily in the across-axis direction, and that this hydrothermal system may also episodically turn on and off. The current pattern of microseismicity supports this conclusion, with events not only mirroring the AML depth and location beneath the ridge axis, but also having a temporally varying focus.
Author(s): Lowell RP, Zhang L, Morales Maqueda MA, Banyte D, Tong VCH, Jhonston RER, Harris RN, Hobbs RW, Peirce C, Robinson AH, Kolandaivelu K
Publication type: Article
Publication status: Published
Journal: Earth and Planetary Science Letters
Online publication date: 06/12/2019
Acceptance date: 27/11/2019
Date deposited: 10/12/2019
ISSN (print): 0012-821X
ISSN (electronic): 1385-013X
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