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<oai_dc:dc xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
  <dc:contributor>Michael Lisowski</dc:contributor>
  <dc:contributor>Michael P. Poland</dc:contributor>
  <dc:contributor>David R. Sherrod</dc:contributor>
  <dc:contributor>Richard G. LaHusen</dc:contributor>
  <dc:contributor>David R. Sherrod</dc:contributor>
  <dc:contributor>William E. Scott</dc:contributor>
  <dc:contributor>Peter H. Stauffer</dc:contributor>
  <dc:creator>Daniel Dzurisin</dc:creator>
  <dc:date>2008</dc:date>
  <dc:description>A prolonged period of dome growth at Mount St. Helens 
starting in September-October 2004 provides an opportunity 
to study how the volcano deforms before, during, and after an 
eruption by using modern instruments and techniques, such as 
global positioning system (GPS) receivers and interferometric 
synthetic aperture radar (InSAR), together with more traditional ones, including tiltmeters, triangulation, photogrammetry, and time-lapse photography. No precursory ground 
deformation was detected by campaign GPS measurements 
made in 2000 and 2003, nor by a continuous GPS station 
(JRO1) operating ~9 km to the north-northwest of the vent 
area since May 1997. However, JRO1 abruptly began moving downward and southward, toward a source centered about 
8 km beneath the volcano, concurrently with the start of a 
shallow earthquake swarm on September 23, 2004. The JRO1 
velocity slowed from ~0.5 millimeters per day (mm/d) in late 
September–early October 2004 until spring 2005. Thereafter, 
it was essentially constant at ~0.04 mm/d through December 
2005. In similar fashion, the growth rate of the welt on the 
south crater floor slowed from 8.9 m&lt;sup&gt;3&lt;/sup&gt;/s during October 4–11 
to 6.4 m&lt;sup&gt;3&lt;/sup&gt;/s during October 11-13, 2004; this trend continued 
after emergence of the first lava spine on October 11. The 
volumetric extrusion rate decreased from 5.9 m&lt;sup&gt;3&lt;/sup&gt;/s during 
October 13-November 4, 2004, to 2.5 m&lt;sup&gt;3&lt;/sup&gt;/s during December 
11, 2004-January 3, 2005, and for the remainder of 2005, it 
was in the range 2.0-0.7 m&lt;sup&gt;3&lt;/sup&gt;/s. Fifteen continuous GPS stations, installed soon after the eruption began, showed radially 
inward and downward ground motions through December 
2005. Likewise, InSAR observations spanning the first year of the eruption indicate broad subsidence centered near the vent. 
Model-derived estimates of source-volume decrease from 
September 23, 2004, to October 31, 2006, are 16-24×10&lt;sup&gt;6&lt;/sup&gt; m&lt;sup&gt;3&lt;/sup&gt;, 
substantially less than the volume erupted during the same 
period (87×10&lt;sup&gt;6&lt;/sup&gt; m&lt;sup&gt;3&lt;/sup&gt;
 through October 21, 2006). The discrepancy can be explained by a combination of magma expansion 
and recharge in the source region.
Lack of precursory deformation at JRO1 suggests that 
the conduit is poorly coupled to the rest of the edifice, so the 
rising magma column was able to push ahead older conduit material rather than intruding it. Constraints on conduit 
length and radius require that reservoir magma (as opposed 
to conduit-filling magma) reached the surface early during 
the eruption, probably soon after CO&lt;sub&gt;2&lt;/sub&gt;
 emission rates peaked 
in early October 2004. If rapid emergence of spine 3 (the first 
whaleback-shaped extrusion) in late October 2004 marked 
the arrival of reservoir magma, then the volume of conduit 
material flushed from the system was about 20×10&lt;sup&gt;6&lt;/sup&gt; m&lt;sup&gt;3&lt;/sup&gt;
--the 
volume of surface deformation plus spines on November 4, 
2004. The corresponding radius for a cylinder extending from 
the surface to depth d = 5 km is 35.7 m, or 28.2 m for d = 8 
km. The average ascent rate through the conduit, assuming 
reservoir magma began its rise on September 23, 2004, was 
120 m/d for d = 5 km, or 190 m/d for d = 8 km. Observed lineal extrusion rates were 2-10 m/d, so the conduit must widen 
considerably near the surface. Equating magma flux through 
the conduit to that at the surface, we obtain a vent radius of 
125 m and an extrusion rate of 5.7 m&lt;sup&gt;3&lt;/sup&gt;/s--both values representative of the early part of the eruption.
Lack of precursory inflation suggests that the volcano was poised to erupt magma already stored in a crustal 
reservoir when JRO1 was installed in 1997. Trilateration 
and campaign GPS data indicate surface dilatation, presumably caused by reservoir expansion between 1982 and 1991, 
but no measurable deformation between 1991 and 2003. We 
conclude that all three of the traditionally reliable eruption precursors (seismicity, ground deformation, and volcanic 
gas emission) failed to provide warning that an eruption was 
imminent until a few days before a visible welt appeared at 
the surface--a situation reminiscent of the 1980 north-flank 
bulge at Mount St. Helens.</dc:description>
  <dc:format>application/pdf</dc:format>
  <dc:identifier>10.3133/pp175014</dc:identifier>
  <dc:language>en</dc:language>
  <dc:publisher>U.S. Geological Survey</dc:publisher>
  <dc:title>Constraints and conundrums resulting from ground-deformation measurements made during the 2004-2005 dome-building eruption of Mount St. Helens, Washington</dc:title>
  <dc:type>reports</dc:type>
</oai_dc:dc>