2018
DOI: 10.5194/bg-2018-167
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Faunal carbon flows in the abyssal plain food web of the Peru Basin have not recovered during 26 years from an experimental sediment disturbance

Abstract: <p><strong>Abstract.</strong> Future deep-sea mining for polymetallic nodules in abyssal plains will impact the benthic ecosystem, but it is largely unclear whether this ecosystem will be able to recover from mining disturbance and if so, at what time scale and to which extent. In 1989, during the "DISturbance and reCOLonization" (DISCOL) experiment, a total of 22 % of the surface within a 10.8 km<sup>… Show more

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Cited by 2 publications
(2 citation statements)
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“…One reason that Kaikoūra Canyon megafauna do not fit the previous slow recovery paradigm may be because they are in the head of a physically active canyon in the bathyal zone (905-1190 m) rather than deeper abyssal, submarine fan environments (between 2900-5050 m) which have been the focus of previous studies on ancient turbidity flows. With increasing depth there is a decrease in abundance and size of organisms due to decreased nutrient availability and slower growth rates compared to shallower waters (Thiel, 1992;Rex et al, 2006), and it is therefore probable that communities in abyssal environments may be more susceptible to impact from large-scale disturbances (Radziejewska and Stoyanova, 2000;Stratmann et al, 2018). In addition, submarine canyons are high energy environments that are frequently disturbed by strong bottom currents, internal tidal mixing, and mass wasting events of various sizes (Fernandez-Arcaya et al, 2017), such that communities in these environments are expected to be resilient to physical disturbances on a range of temporal scales (Rowe, 1971).…”
Section: Time To Recovery Of the Megafauna Communitymentioning
confidence: 99%
“…One reason that Kaikoūra Canyon megafauna do not fit the previous slow recovery paradigm may be because they are in the head of a physically active canyon in the bathyal zone (905-1190 m) rather than deeper abyssal, submarine fan environments (between 2900-5050 m) which have been the focus of previous studies on ancient turbidity flows. With increasing depth there is a decrease in abundance and size of organisms due to decreased nutrient availability and slower growth rates compared to shallower waters (Thiel, 1992;Rex et al, 2006), and it is therefore probable that communities in abyssal environments may be more susceptible to impact from large-scale disturbances (Radziejewska and Stoyanova, 2000;Stratmann et al, 2018). In addition, submarine canyons are high energy environments that are frequently disturbed by strong bottom currents, internal tidal mixing, and mass wasting events of various sizes (Fernandez-Arcaya et al, 2017), such that communities in these environments are expected to be resilient to physical disturbances on a range of temporal scales (Rowe, 1971).…”
Section: Time To Recovery Of the Megafauna Communitymentioning
confidence: 99%
“…These carbon-based food web models are based on the principle of mass conservation and combine physiological parameters (e.g., assimilation and growth efficiency, secondary production, mortality, respiration), with site-specific flux constraints on carbon influx and loss, and biomasses of individual food-web compartments to calculate the carbon flows between compartments in the pre-defined topological food-web (Soetaert and van Oevelen, 2009;van Oevelen et al, 2010). They have been used previously to assess the potential recovery from a small-scale sediment disturbance in the SE Pacific (Stratmann et al, 2018a;de Jonge et al, 2020) and here, they will be applied to estimate changes in carbon flows depending on the presence and absence of noduledependent fauna at two sites of the GSR exploration license area in the CCZ.…”
Section: Introductionmentioning
confidence: 99%