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EarthScope

Earth science program exploring the structure of the North American continent

  • 19 min read
  • 5 chapters

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Through North America, Volcano and Tectonics

Observatories

There were three EarthScope project observatories:

  • The San Andreas Fault Observatory at Depth (SAFOD)
  • The Plate Boundary Observatory (PBO)
  • The Seismic and Magnetotelluric Observatory (USArray)

These observatories consisted of boreholes into an active fault zone, global positioning system (GPS) receivers, tiltmeters, long-baseline laser strainmeters, borehole strainmeters, permanent and portable seismometers, and magnetotelluric stations. The various EarthScope components provided integrated and highly accessible data on geochronology and thermochronology, petrology and geochemistry, structure and tectonics, surficial processes and geomorphology, geodynamic modeling, rock physics, and hydrogeology.

Seismic and Magnetotelluric Observatory (USArray)

USArray, managed by IRIS, was a 15-year program to place a dense network of permanent and portable seismographs across the continental United States. These seismographs recorded the seismic waves released by earthquakes that occur around the world. Seismic waves are indicators of energy disbursement within the earth. By analyzing the records of earthquakes obtained from this dense grid of seismometers, scientists could learn about Earth structure and dynamics and the physical processes controlling earthquakes and volcanoes. The goal of USArray was primarily to gain a better understanding of the structure and evolution of the continental crust, lithosphere, and mantle underneath North America.

The USArray was composed of four facilities: a Transportable Array, a Flexible Array, a Reference Network, and a Magnetotelluric Facility.

Transportable Array

The Transportable Array was composed of 400 seismometers that were deployed in a rolling grid across the United States over a period of 10 years. The stations were placed 70 km apart, and could map the upper 70 km of the Earth. After approximately two years, stations were moved east to the next site on the grid – unless adopted by an organization and made a permanent installation. Once the sweep across the United States was completed, over 2000 locations had been occupied. The Array Network Facility was responsible for data collection from the Transportable Array stations.

Flexible Array

The Flexible Array was composed of 291 broadband stations, 120 short period stations, and 1700 active source stations. The Flexible Array allowed sites to be targeted in a more focused manner than the broad Transportable Array. Natural or artificially created seismic waves could be used to map structures in the Earth.

Reference Network

The Reference Network was composed of permanent seismic stations spaced about 300 km apart. The Reference Network provided a baseline for the Transportable Array and Flexible Array. EarthScope added and upgraded 39 stations to the already existing Advanced National Seismic System, which was part of the Reference Network.

Magnetotelluric Facility

The Magnetotelluric Facility was composed of seven permanent and 20 portable sensors that recorded electromagnetic fields. It is the electromagnetic equivalent of the seismic arrays. The portable sensors were moved in a rolling grid similar to the Transportable Array grid, but were only in place about a month before they were moved to the next location. A magnetotelluric station consists of a magnetometer, four electrodes, and a data recording unit that are buried in shallow holes. The electrodes are oriented north-south and east-west and are saturated in a salt solution to improve conductivity with the ground.

Plate Boundary Observatory (PBO)

The Plate Boundary Observatory PBO consisted of a series of geodetic instruments, Global Positioning System (GPS) receivers and borehole strainmeters, that were installed to help understand the boundary between the North American Plate and Pacific Plate. The PBO network included several major observatory components: a network of 1100 permanent, continuously operating Global Positioning System (GPS) stations, many of which provide data at high-rate and in real-time, 78 borehole seismometers, 74 borehole strainmeters, 26 shallow borehole tiltmeters, and six long baseline laser strainmeters. These instruments were complemented by InSAR (interferometric synthetic aperture radar) and LiDAR (light detection and ranging) imagery and geochronology acquired as part of the GeoEarthScope initiative. PBO also included comprehensive data products, data management and education and outreach efforts. These permanent networks were supplemented by a pool of portable GPS receivers that could be deployed for temporary networks to researchers, to measure the crustal motion at a specific target or in response to a geologic event. The Plate Boundary Observatory portion of EarthScope was operated by UNAVCO.

San Andreas Fault Observatory at Depth (SAFOD)

The San Andreas Fault Observatory at Depth (SAFOD) consisted of a main borehole that cut across the active San Andreas Fault at a depth of approximately 3 km and a pilot hole about 2 km southwest of San Andreas Fault. Data from the instruments installed in the holes, which consisted of geophone sensors, data acquisition systems, and GPS clocks, as well as samples collected during drilling, helped to better understand the processes that control the behavior of the San Andreas Fault.

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