Cascadia Initiative Workshop Update


Portland, Oregon, October 15-16, 2010

Jeff McGuire1, Doug Toomey2, Chris Goldfinger3, Susan Schwartz4, Richard Allen5

1WHOI; 2University of Oregon; 3Oregon State University; 4UC Santa Cruz; 5UC Berkeley

PBO GPS stations upgraded as part of the Cascadia Initiative (black triangles) and broadband seismometers (circles) expected to operate in the Cascadia Region in various time windows between 2011 and 2015. For a detailed discussion of the different seismometer experiments (color-coded) and the schedule of their deployments, please see the full workshop report.

PBO GPS stations upgraded as part of the Cascadia Initiative (black triangles) and broadband seismometers (circles) expected to operate in the Cascadia Region in various time windows between 2011 and 2015. For a detailed discussion of the different seismometer experiments (color-coded) and the schedule of their deployments, please see the full workshop report.

As part of the 2009 Stimulus or ARRA (American Recovery and Reinvestment Act) spending, NSF’s Earth Sciences (EAR) and Ocean Sciences (OCE) divisions each received $5M in facility-related investment. The funds were targeted toward the creation of an Amphibious Array Facility (AAF) to support EarthScope and MARGINS science objectives. The initial emphasis and deployment site was onshore/offshore studies of the Cascadia margin, with an expectation that the facility would later move to other locations. Thus, the Cascadia Initiative (CI) is an onshore/offshore seismic and geodetic experiment that takes advantage of the Amphibious Array to study questions ranging from megathrust earthquakes, to volcanic arc structure, to the formation, deformation and hydration of the Juan De Fuca and Gorda pPlates. The Initiative was featured in Vice President Biden’s list of “100 Recovery Act Projects that are Changing America” under the heading “Research to Avert Disaster: Understanding Earthquakes in the Pacific Northwest – Oregon, Washington, Northern California”. In October 2010, we convened an open community workshop that produced a series of recommendations to maximize the scientific return of the CI as well asand to develop deployment plans for the offshore component of the experiment. We summarize some of the main points of the full workshop report here.

The science objectives of the CI are wide-ranging. The new instrumentation will enable: real-time, high-rate GPS data to be used both for studying large earthquakes in the region and potentially for real-time seismic and volcanic hazard mitigation; continued monitoring of non-volcanic tremor along the entire subduction zone; imaging of the physical properties of the (offshore) megathrust properties; and studies of the formation, evolution, deformation and hydration of the incoming Juan de Fuca and Gorda plates as it they moves from ridge to trench. This diverse set of objectives are all components of understanding the overall subduction zone system and require an array that provides high quality data that crosses the shoreline and encompasses relevant plate boundaries.

The ARRA funded upgrades to 232 Cascadia GPS stations that are part of the Plate Boundary Observatory, that are being carried out by UNAVCO (Figure 1). The improvements include switching from daily downloads to continuous, real-time streaming of data from daily downloads, and increasing the rate of sampling from 30-second to 1-second epochs. The majority of these upgrades have already been completed;, the project is on schedule and on budget., and the remainder of the PBO stations will be completed by summer of 2011.

The onshore seismic component of the AAF consists of 27 EarthScope/USArray/Transportable Array station sites that have been deployed to complement the existing distribution of broadband stations in Cascadia, (Figure 1). Where possible and appropriate, some of the 27 sites are reoccupying the original sites of the Transportable Array in the region. In other cases, new sites were have been identified to complement existing stations and/or when if the original site was is not available. All 27 sites have a broadband velocity sensor and a strong-motion accelerometer and the deployments were completed in the summer of 2010 (Figure 2). All are operational with data streaming in near-real time to the IRIS Data Management Center (DMC), and will operate until at least September 2013. The data are archived at the IRIS Data Management CenterDMC. Stations report their data under the TA network code, and use the standard TA station naming convention. In addition, the Virtual Network Definition (VND) capability at the DMC provides a simple means to access these data. The virtual network “_CASCADIA” will provide access to the 27 TA stations plus 47 other broadband stations in the area, while the “_CASCADIA-TA” VND provides access to the 27 TA Cascadia stations.

The CI funded the construction of a total of 60 Ocean Bottom Seismometers (OBSs) by the three Institutional Instrument Contributors (IICs) of the National Ocean Bottom Seismometer Instrumentation Pool (OBSIP). The IICS group at Lamont-Doherty Earth Observatory (LDEO) will build 30 OBSs, while the groups at the Scripps Institute of Oceanography (SIO) and the Woods Hole Oceanographic Institution (WHOI) will build 15 each. All 60 OBSs will be equipped with Nanometrics Trillium Compact seismometers. In addition to the seismometers, the SIO and WHOI OBSs will be equipped with Differential Pressure Gauges (DPGs) while the LDEO OBSs will carry Absolute Pressure Gauges (APGs). Twenty of the LDEO OBSs will be installed in trawl-resistant enclosures and will be available for deployments in water depths extending from the shelf down to 1,000 m. These 20 OBSs will be deployed via the ship’s wire and recovered using a Remotely-Operated Vehicle (ROV). These instruments will not be deployable in water depths greater than 1,000 m. The fifteen SIO OBSs will also be installed in trawl-resistant enclosures, and are deployable at depths extending from the shelf down to 6,000 m. The WHOI OBSs will not be deployable in depths shallower than 1000 m. All 60 instruments will be equipped with 12-month battery packs.

The OBSs will be utilized in four one-year long deployments. These experiments will provide an offshore extension of the EarthSscope Transportable Array (≈70 km spacing) as well as 3 dense experiments focused on either imaging various properties of the thrust interface and forearc or recording local seismicity (Figure 1). The OBS deployment geometry complements the cabled observatories of NEPTUNE Canada and the Regional Scale Nodes of the Ocean Observatory Initiative as well as funded, PI-driven OBS experiments designed to study deformation near the Blanco Transform and within the Gorda Plate. The proposed deployment plans are described in detail in the workshop report.

Figure 2. Installation of station N02D at Trinity Center in northern California in the fall of 2009

Figure 2. Installation of station N02D at Trinity Center in northern California in the fall of 2009

A team of PIs will lead expeditions to deploy and recover CI OBSs and to develop Education and Outreach modules. The team is being organized by Doug Toomey and includes Richard Allen, John Collins, Bob Dziak, Emilie Hooft, Dean Livelybrooks, Jeff McGuire, Susan Schwartz, Maya Tolstoy, Anne Trehu and William Wilcock. The PI team is knowledgeable about the science and operational objectives of the CI, includes individuals with chief scientist experience, as well as onessome who have not yet been to sea, and comprises representatives from both the EAR and OCE communities. It is anticipated that there will be berths for students, post-docs and other scientists to participate in either deployment or recovery legs, thus providing the seismological community with opportunities to gain valuable experience in planning and carrying out an OBS experiment. Funding and ship time for the deployments and recoveries of OBS will be supported primarily by the Ocean Sciences Division of NSF.

The CI has a finite duration with the intention that both the onshore and offshore components of the AAF will move to other locations following the completion of the CI. The community plan that resultinged from the October workshop requiresa four 4-years of onshore/offshore deployments in Cascadia, which will begin in the summer of 2011. The four4 one-year OBS deployments in the region would last until the summer/fall 2015 at which point the AAF could move to a new location, or could remain in Cascadia. The October workshop recommended that during the deploymentfour years, smaller workshops should be held to evaluate data quality, present results from initial analyses, and make adjustments to the deployment plan if necessary. A process is also needed to decide where the AAF should be deployed following the initial 4-year deployment in Cascadia. In the context of the ongoing EarthScope initiative, possible locations include the East Coast, the Gulf of Mexico, and Alaska. However, the AAF could also move to other locations, and could also or remain in Cascadia. A community workshop in 2014 was therefore proposed as a venue to decide on the next deployment of the AAF.

 Reference information
Cascadia Initiative Workshop Update, McGuire J. et al;

GeoPRISMS Newsletter, Issue No. 26, Spring 2011. Retrieved from http://geoprisms.org

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