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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>David J. Schneider</dc:contributor>
  <dc:contributor>Steve P. Schilling</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>James W. Vallance</dc:creator>
  <dc:date>2008</dc:date>
  <dc:description>The eruption of Mount St. Helens from 2004 to 2006 
has comprised extrusion of solid lava spines whose growth 
patterns were shaped by a large space south of the 1980-86 
dome that was occupied by the unique combination of glacial 
ice, concealed subglacial slopes, the crater walls, and relics 
of previous spines. The eruption beginning September 2004 
can be divided (as of April 2006) into five phases: (1) predome deformation and phreatic activity, (2) initial extrusion 
of spines, (3) recumbent spine growth and repeated breakup, 
(4) southward extrusion across previous dome debris, and (5) 
normal faulting of the phase 4 dome to form a depression, a 
shift to westward extrusion and overthrusting of earlier phase 
5 products. Overall, steady spine extrusion gradually slowed 
from 6 m&lt;sup&gt;3&lt;/sup&gt;/s in November 2004 to 0.6 m&lt;sup&gt;3&lt;/sup&gt;/s in February 2006.
Thermal camera data show that phase 1 activity included 
low-temperature thermal features, such as fumaroles, fractures, and ground warming related to rapid uplift, as well as 
deformation in the south moat of the crater. The relatively cold 
(&lt;160&amp;deg;C) phreatic eruptions of early October heralded activity 
at a subglacial vent situated along the south-sloping margin of 
the 1980–86 dome. Thermal infrared imagery, documenting 
increased heat flow, presaged phase 2 extrusion of the October 
11–15, 2004, lava spine. The thermal images of the extruding 
spine revealed a hot basal margin and highest temperatures of 
600–730&amp;deg;C. 
During phase 3, a recumbent whaleback-shaped spine 
with a low-temperature shroud of fault gouge and a hot, 
U-shaped basal margin extruded. This spine pushed southward 
along the bed of the glacier until it encountered the south wall 
of the 1980 crater, whereupon it broke up, decoupled, and 
regrew. Continued southward growth of the recumbent spine pushed cold deformed rock, hot dome rubble, and glacier 
ice eastward at a rate of 2 m/d. In April 2005, breakup of the 
whaleback and growth of a lava spine across previous dome 
rubble heralded phase 4 spine thrusting over previous spine 
remnants. During phase 4, the active spine pushed southward with an increasingly vertical component and increasing 
incidence of large rockfalls. In late July, the spine decoupled 
from its source, the vent reorganized, and a new spine began 
to grow westward at right angles to the previous growth direction, defining phase 5. Dome migration again plowed glacier 
ice out of the way at a rate of about 2 m/d, this time westward. In early October, the spine buckled near the vent and 
thrust over the previous one. A massive spine monolith had 
been constructed by December 2005, and growth of spines 
with increasingly steep slopes characterized activity through 
April 2006.
The chief near-surface controls on spine extrusion during 
2004-6 have been vent location, relict topographic surfaces 
from the 1980s, and spine remnants emplaced previously 
during the present eruption. In contrast, glacier ice has had 
minimal influence on spine growth. Ice as thick as 150 m has 
prevented formation of marginal angle-of-repose talus fans 
but has not provided sufficient resistance to stop spine growth 
or slow it appreciably. Spines initially emerged along a relict 
south-facing slope as steep as 40&amp;deg; on the 1980s dome. The 
open space of the moat between that dome and the crater walls 
permitted initial southward migration of recumbent spines. 
An initial spine impinged on the opposing slopes of the crater 
and stopped; in contrast, recumbent whaleback spines of phase 
3 impinged on opposing walls of the crater at oblique angles 
and rotated eastward before breaking up. Once spine remnants 
occupied all available open space to the south, spines thrust 
over previous remnants. Finally, with south and east portions of the moat filled, spine growth proceeded westward. 
Although Crater Glacier had only a small influence on the 
growing spines, spine growth affected the glacier dramatically, 
initially dividing it into two arms and then bulldozing it hundreds of meters, first east and then west, and heaping it more 
than 100 m higher than its original altitude.</dc:description>
  <dc:format>application/pdf</dc:format>
  <dc:identifier>10.3133/pp17509</dc:identifier>
  <dc:language>en</dc:language>
  <dc:publisher>U.S. Geological Survey</dc:publisher>
  <dc:title>Growth of the 2004-2006 lava-dome complex at Mount St. Helens, Washington</dc:title>
  <dc:type>reports</dc:type>
</oai_dc:dc>