The role of disturbance in deep-sea benthic ecosystems
Paul Snelgrove & Anna Metaxas
Phillippe Archambault, Brian Bornhold, Grant Ferris, Alex Hay, Kim Juniper, Verena Tunnicliffe
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Deep-sea ecosystems are the largest and among the most species-rich habitats on Earth, but are also among the least sampled. Studies to date suggest that environmental disturbances in the deep sea contribute significantly to habitat heterogeneity and recruitment variability on and above the sea floor. However, these studies have limited by a dependence on ship-based sampling. NEPTUNE observing system will provide us with unprecedented quality and volumes to information on the deep ocean. Using monitoring and responsive sampling with NEPTUNE, we can address for the first time how deep-sea faunal response is influenced by input of organic and inorganic material on temporal scales from days to decades. In particular, we will investigate the relative impacts on the deep-sea benthos of material flux from the overlying water column and from the nearby continental shelf and via a submarine canyon. These data will significantly advance our understanding of deep-sea ecosystems.
Sites at Barkley Shelf, Barkley Canyon & Axis comprise the main core of our research program and encompass a transect from shelf to abyssal depths. We hope to include targeted sampling at opportunistic intervals to better resolve the spatial component of the biology present in the region.
Our team consists of scientists from multiple disciplines and institutions, and we believe it includes most of the deep-sea benthic expertise in Canada. Although most investigators are primarily biologists, marine geologists and physicists are key members of our project. Moreover, most of the biologists are trained as interdisciplinary oceanographers with expertise in areas such as boundary layer flow and biological- physical coupling. We include investigators from 6 academic institutions (Memorial, Dalhousie, UQ Rimouski, UQAM, UBC andUVic) and the federal government (Fisheries and Oceans Canada). Many of us have collaborated on successful NSERC and/or CFI proposals and/or cruises in the past (e.g. Deibel & Snelgrove; Metaxas & Snelgrove; Metaxas, Tunnicliffe & Juniper; Metaxas, Deibel & Desrosiers, Deibel & Archambault; Deibel & Juniper; Metaxas, Hay & Hill; Juniper & Ferris). Many collaborations are long- standing (5-20 yrs), and extremely productive. Formal partnerships in marine sciences have already been established among academic institutions (e.g. through NEPTUNE). The proposed research will expand and strengthen these collaborations.
Most of the PIs collaborate with other Canadian scientists both within and outside their own institutions, and many maintain strong links and active collaboration with scientists in the United States with assistance from US funding programs (e.g. NOAA Ocean Exploration & NURP, ONR, NSF). Early success at NEPTUNE will attract these scientists to our program, since many share common interests and have been active in US NEPTUNE. Given these links, we believe we are an a unique position to integrate with US and other international scientists into NEPTUNE.
Our project is strongly integrated with the Water Column Processes Group. We have maintained active communication and will share some data sets, and write collaborative manuscripts. The cameras and SONAR which central to our work, will provide spectacular images to enhance NEPTUNE's outreach potential.