Underground explosives will be used in research about Mount St. Helens
Sarah Phillips, of the Johnston Ridge Observatory at Mount St. Helen's, educates the public about the explosive eruptive past and the eruptive future of Washington's most famous volcano, May 13, 2014. (Dean J. Koepfler/Tacoma News Tribune/MCT)
Dean J. Koepfler / Tacoma News Tribune
Crowds enjoy the view at the Johnston Ridge Observatory at Mount St. Helens on May 13.
A seismic monitor measures the vertical and horizontal movement of the ground surrounding a prototype “passive seismic” sensor that will be arrayed around Mount St. Helens as part of a battery of multidisciplinary imaging experiments collectively called iMUSH, for Imaging Magma Under St. Helens.
Dean J. Koepfler / Tacoma News Tribune
Seismic specialist and UW professor emeritus Steve Malone (from left), UW graduate student Carl Ulberg and Victor Kress, of the Pacific Northwest Seismic Network, assembled and tested a passive seismic station design in the back yard of Kress’ Lake Forest Park home Monday.
Dean J. Koepfler / Tacoma News Tribune
The panoramic and breathtaking view of the south rim of Mount St. Helens, looking past a still venting lava dome north toward Spirit Lake and Mount Rainier, is awe-inspiring but scientists are focused on a repressurizing of the magma chamber below the volcano.
This summer, the scientists will be the ones setting off the explosions.
Using techniques developed by the oil industry, researchers are preparing to set off explosive charges buried in two dozen 80-foot-deep wells drilled around the mountain. They'll record the seismic energy of the explosions on thousands of portable seismometers placed by an army of volunteers traveling by car, on foot and on horseback.
Their goal is to see with greater clarity the details of how molten rock, or magma, makes its way to St. Helens' crater from the area where tectonic plates collide and the magma is created, some 60 miles beneath the surface.
“We've been looking at what's beneath the volcano through very fuzzy glasses,” said Seth Moran, a seismicity expert with the U.S. Geological Survey's Cascade Volcano Observatory in Vancouver, Washington. “This still won't give us anything like 20/20 vision, but it should make things quite a bit clearer.”
The explosive experiments, or “active imaging events,” scheduled for this summer are one part of a battery of multidisciplinary imaging experiments collectively called iMUSH for “Imaging Magma Under St. Helens.” Together, they constitute what researchers say is the one of the most complete and ambitious series of imaging experiments ever conducted on any volcano in the world.
The $3 million project, funded mostly by the National Science Foundation, is headed by Kenneth Creager, a University of Washington professor of earth and space sciences.
The explosive research, which will use about $1 million of the total, is being conducted by a research team from Rice University, headed by earth science professor Alan Levander.
Along with UW, Rice and the USGS, participants include teams of researchers at Oregon State University in Corvallis, the Lamont-Doherty Earth Observatory at Columbia University in New York and Eidgenoessische Technische Hochschule of Zurich.
In addition to the explosive testing, specialists in other disciplines are preparing for experiments using enhanced receptors for naturally occurring seismic activity. They'll also examine the magnetic and electrical properties of rock deep beneath the volcano, which scientists say is a useful guide to identifying magma.
The goal is to “see” deep below St. Helens to the area where the Juan de Fuca tectonic plate from the Pacific is forced under the North America plate. This Cascade “subduction zone” also is the area that can produce magnitude-9 earthquakes when the plates slip or break.
Magma from this zone makes its way to the surface in Northwest volcanoes, but exactly how that happens remains a mystery despite more than three decades of research.
Scientists have a good sense of what's beneath the volcano down to a depth of about 6 miles, Moran said. There are many theories about what's going on in deeper reaches, but nobody has been able to prove one.
Does the magma pool in a reservoir at the crust? Does it make its way upward in a single, narrow pipelike conduit? Or does it collect in one or more underground ponds along the way?
Finding answers is important, scientists say, because it will enable them to better interpret the volcano's signals when magma is on the move. That knowledge, they say, will help them predict eruptions not only at St. Helens but also at other volcanoes in the Cascade Range and around the world — and possibly save many thousands of lives.
“It's long been looked at by individual disciplines,” Moran said. “All of them have their own resolution issues and error issues, plus they're all measuring different kinds of things.”
By combining the strengths of the various imaging methods, he said, individual weaknesses will be filtered out.
“By throwing multiple things at this, we'll have a better sense of the whole,” he said.
Moran and other USGS analysts confirmed last month that St. Helens remains active. While an eruption is not impending, the analysis showed a new supply of magma is slowly repressurizing the magma chamber beneath the mountain.
Steve Malone, now a UW professor emeritus, but a seismicity superstar when St. Helens erupted 34 years ago, is an active participant in the iMush studies.
Scientists did not foresee St. Helens' unusual sideways blast May 18, 1980, but thanks to Malone and others, they were able to roughly predict when the eruption would occur and thereby saved many lives.
Fifty-seven people died in the eruption, which devastated 150 square miles of southwestern Washington and sent up an eruption cloud that reached the stratosphere.
Malone and his colleagues are meeting to design 70 enhanced seismic stations that will be installed up to 30 miles from the mountain for “passive” tests that will measure natural seismicity.
“It's pretty much good to go, but there's still some paperwork left,” Malone said this month. “We're hoping to start putting instruments out in June and by the end of June to get to all of the sites.”
Obtaining the necessary permits to install instruments has been a logistical challenge, Malone said, because of multiple landowners, including state and federal government agencies, Weyerhaeuser and other timber companies and private landowners. All have their own legal requirements and concerns.
Snow is still keeping teams out of areas in the Cascades, and the window of opportunity for testing will end when the high-risk fire season starts in late summer.
The thousands of smaller seismometers that will be used in the explosive testing are easily portable, Moran said. They're slightly smaller than a can of tennis balls, and run off two D-cell batteries.
“You can put 15 of them in a backpack,” he said.
Even so, installing 2,600 seismometers in the rugged and roadless areas closest to the volcano and within the Mount St. Helens National Monument, as the plan calls for, will be extremely labor intensive. In their proposal, Rice scientists predicted that installing the instruments in that inner ring will be a “vexing deployment.”
“Something of that scale wouldn't be possible without an army of volunteers,” said Carolyn Driedger, a USGS hydrologist and public outreach coordinator at the Cascades Volcano Observatory.
The public's involvement in the iMUSH project has value of its own, independent of the scientific goals, Driedger said.
“It's good because it involves people in studying the world in which they live,” she said. “Here in the Pacific Northwest we are literally living on the edge. It's not a stable place.”
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