 
 
 EarthScope is 
  gearing up to outfit North America with a vast array of instruments designed 
  to help scientists determine the processes and pieces that make up a continent. 
  The endeavor aims to address the many persisting earth science puzzles that 
  conventional individual efforts have yet to solve  such as how earthquakes 
  start and how magma flows beneath active volcanoes. With access to data from 
  instrument networks across the country, scientists from multiple disciplines 
  will be able to collaborate. Now, after securing National Science Foundation 
  funding last September, the various EarthScope committees are moving beyond 
  the planning stage to implementation.
EarthScope is 
  gearing up to outfit North America with a vast array of instruments designed 
  to help scientists determine the processes and pieces that make up a continent. 
  The endeavor aims to address the many persisting earth science puzzles that 
  conventional individual efforts have yet to solve  such as how earthquakes 
  start and how magma flows beneath active volcanoes. With access to data from 
  instrument networks across the country, scientists from multiple disciplines 
  will be able to collaborate. Now, after securing National Science Foundation 
  funding last September, the various EarthScope committees are moving beyond 
  the planning stage to implementation. 
  
  Part of EarthScope, the San Andreas Fault Observatory at Depth will monitor 
  activity below an active fault. Researchers drilled a 2-kilometer-deep pilot 
  hole in 2003 and plan to begin drilling the main hole this spring. Courtesy 
  of EarthScope.
  
  The questions that the earth science community is asking now are big, 
  complicated questions. And they cant be answered with one simple discipline, 
  says geophysicist David Simpson, an EarthScope facility manager. Instead, he 
  says that a multi-scaled investigation is necessary, and EarthScope instruments 
  are designed for just that. Scientists awaiting EarthScope data come from research 
  institutions and universities all over the country, as well as government agencies, 
  such as state geologic surveys and the U.S. Geological Survey (USGS).
  
  EarthScope components are designed to reveal features of the North American 
  continent at different scales. At the finest scale, the San Andreas Fault Observatory 
  at Depth, or SAFOD, will zoom in on Californias infamous fault zone. It 
  will, in fact, go inside the fault zone to become the first observatory monitoring 
  an active fault from within, rather than from the surface. Scaling up, the Plate 
  Boundary Observatory (PBO) will examine the deforming U.S. West Coast and Alaska. 
  Zooming out again, the USArray will provide a 3-D view of the North American 
  continent from crust to core. And EarthScope hopes to add Interferometric Synthetic 
  Aperture Radar (InSAR) imagery to these three components, in order to measure 
  ground deformations from space. The individual EarthScope components are designed 
  to complement and enhance one another, so scientists will benefit from access 
  to several datasets teased from the four observatories. Theyd be 
  good by themselves, but theyre far better working together, says 
  Mark Zoback, geophysics professor at Stanford University and facility manager 
  for SAFOD (see comment). 
  
  The challenge of EarthScope lies in erecting the whole system. Because this 
  is an endeavor more than 10 years in the making, the technology behind the individual 
  instruments in the project were conceived of long ago. Only recently, however, 
  has communications technology ripened to the point where EarthScope can employ 
  a global communications system for transferring all its data to central archives 
  and providing access to that data to anyone, anytime. For the first time 
  we can talk about gathering data from anywhere in the United States and making 
  it available in real time. That certainly could not have been done 10 years 
  ago, Simpson says.
Observing a fault
SAFOD scientists are already monitoring a 2-kilometer-deep pilot hole drilled 
  adjacent to the San Andreas Fault at Parkfield, Calif., in 2002. When spring 
  rains subside in May 2004, the company Therma-Source of Santa Rosa, Calif., 
  will begin drilling the main hole. Although researchers will not puncture the 
  heart of the fault zone this summer, they will case the hole in steel, monitor 
  it, and finally traverse the fault zone in the summer of 2005. Eventually, SAFOD 
  drillers will angle the borehole to cross from the Pacific plate eastward to 
  the North American plate, and will then core four side holes to extract and 
  test materials within the active fault zone. Once the hole is finished, a steel 
  pipe cemented into the rock will provide a channel for the placement of sensitive 
  instruments within the fault zone to monitor the precise locations of fault 
  movement and the physical processes controlling earthquake generation. The instruments 
  will stand at the ready, awaiting the next big quake, Zoback says. A year 
  and a day after we finish, itll be time for the earthquake, he says 
  jokingly.
  According to Stephen Hickman, a USGS geophysicist and facility manager for SAFOD, 
  the borehole monitoring instruments employ state-of-the-art technology that 
  will be tested in the pilot hole and constantly updated. The drilling team is 
  adapting techniques used by the oil industry, such as advanced directional drilling 
  methods, to target small, seismically active portions of the fault (see page 
  18). At various stages, a gyroscopic device lowered into the hole will provide 
  a 3-D view of the drill path. When the hole is complete, a seismic recording 
  system and sensors measuring strain, fluid pressure and temperature will locate 
  earthquakes with extreme precision, and monitor the behavior and physical properties 
  of fault zones through multiple earthquake cycles. 
  Well set the thing up as a long-term observatory, as a sort of soda 
  straw into the fault zone, Hickman says. No one has ever drilled 
  through the San Andreas Fault Zone before. It will bring lots of surprises, 
  but that is what makes this project really exciting.
Measuring movement
Drilling into a fault zone is an exhausting scientific endeavor on its own. 
  But if EarthScope hopes to achieve one of its loftier goals  to help predict 
  potentially damaging earthquakes  it must place the SAFOD findings in 
  a wider context. That is where PBO comes in. The western third of the United 
  States absorbs the strain imposed as the Pacific plate grinds slowly past the 
  North American plate. These awesome forces created the San Andreas Fault system, 
  and understanding them is crucial to earthquake hazard assessment. 
  Through PBO, EarthScope will permanently install 875 GPS receivers, 175 borehole 
  strainmeters and five laser strainmeters, and will provide 100 portable GPS 
  systems to scientists for targeted studies. These instruments will measure every 
  ground movement from the Rocky Mountains westward. 
  The borehole strainmeters are so precise, says PBO Director Mike Jackson, that 
  they record deformation exerted against Earth by the revolution of the moon 
  around it. In addition to monitoring motions associated with building stress 
  before an earthquake, PBO instruments will record ground-level adjustments caused 
  by shifting magma levels in volcanoes. 
  And, says Nancy King, a geophysicist with USGS, PBO is likely to reveal unexpected 
  movements. Before joining the PBO team, King oversaw the day-to-day running 
  of the 250-station Southern California Integrated GPS Network (SCIGN). She says 
  that the SCIGN data surprised scientists by revealing deformation caused by 
  water pumping and withdrawal.
  Kings experience with the logistics of setting up SCIGN will likely prove 
  useful as PBO launches into action. The first step is to convince landowners 
  to host the instruments. We were very naïve about how long it was 
  going to take to get some of these permits [for SCIGN], King says. I 
  think the scientific goals are great. But its easy to underestimate the 
  logistical difficulties. We did. 
  In addition to permitting, PBO planning demands flexibility in outfitting each 
  specific site. 
  Researchers will anchor GPS antennas on 30- to 40-foot-deep drilled monuments. 
  The instruments run off power from solar panels, but sites in the cloudy Pacific 
  Northwest may need auxiliary power. Transferring data from most sites via satellites, 
  wireless internet or radio modem is run of the mill these days; but getting 
  data from remote sites like the Alaskan interior will require some ingenuity. 
  Still, Jackson says he isnt worried. Were ready to hit the 
  ground running, he says. He has obtained permits for almost half of the 
  50 PBO sites scheduled for this year and hopes data will begin flowing from 
  those sites by December.
Seeing the continent
Just as PBO seeks permission to begin installing sites, USArray faces similar 
  challenges at a larger scale. Its aim is to create a 3-D picture of the underpinnings 
  of the North American continent by recording vibrations transmitted through 
  the United States from earthquakes around the world. By monitoring the arrival 
  times of ground vibrations, scientists can differentiate old, cold pieces of 
  the crust and underlying mantle from young, hot pieces. USArray data will also 
  help scientists explore Earths core and magnetic structure. Scientists 
  hope the seismic data will provide insight into how faults start and grow and 
  eventually link together. 
  The backbone of the USArray network consists of 40 reference stations that will 
  be added to the existing Advanced National Seismic System run by USGS (Geotimes, 
  October 2003). These permanent stations will be augmented with observations 
  from 400 portable seismometers, which will cover the United States one swath 
  at a time, recording in a location for up to two years before moving to the 
  next. In effect, 400 roving instruments will accrue the equivalent data of 2,000 
  stations over the next 10 years. This array will provide good resolution from 
  the deep crust to the core. The task of filling in the blanks near Earths 
  surface then lies with the flexible array, a pool of 2,400 portable instruments 
  for high-density, shorter-term observations. By the end of 2004, USArray should 
  have its first group of instruments assembled, and deployment will begin on 
  the West Coast.
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