<?xml version='1.0' encoding='utf-8'?>
<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>Joseph D. Devine III</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>Malcom J. Rutherford</dc:creator>
  <dc:date>2008</dc:date>
  <dc:description>The 2004-6 eruption of Mount St. Helens produced 
dacite that contains 40-50 volume percent phenocrysts of 
plagioclase, amphibole, low-Ca pyroxene, magnetite, and 
ilmenite in a groundmass that is nearly totally crystallized. 
Phenocrysts of amphibole and pyroxene range from 3 to 5 
mm long and are cyclically zoned, with one to three alternations of Fe- and Al-rich to Mg- and Si-rich layers showing 
little indication of phenocryst dissolution between zones. 
Similar-size plagioclase phenocrysts also contain several 
cyclic zones ranging between ~An&lt;sub&gt;68&lt;/sub&gt; and An&lt;sub&gt;45-35&lt;/sub&gt;. Textural evidence indicates that amphibole, pyroxene, and ilmenite began 
to crystallize before the most An-rich plagioclase. Magnetite 
and ilmenite phenocrysts are small (less than 100 &amp;mu;m), vary 
somewhat in composition from grain to grain, and are sporadically zoned. Magnetite-ilmenite pairs yield temperatures 
of equilibration ranging from 820&amp;deg;C to 890&amp;deg;C and f&lt;sub&gt;
O2&lt;/sub&gt;
 values 
of NNO +1 log unit. Magnetite compositions suggest that the 
2004-6 magma was formed by mingling of magmas less than 
5-8 weeks before eruption and that the magma last equilibrated within this temperature range. The amphibole phenocryst zoning involves approximately equal amounts of a 
pressure-sensitive Al-Tschermak molecular substitution and 
a temperature-sensitive edenite substitution in one cycle of 
growth. Hydrothermal experiments done on the natural dacite 
show that crystallization of the Fe- and Al-rich amphibole 
end member requires pressures of 200-300 MPa at temperatures of 900&amp;deg;C, conditions approaching the upper temperature limit of amphibole stability. The dacitic magma crystallizes the An&lt;sub&gt;68&lt;/sub&gt; plagioclase when the pressure drops to 200 
MPa at 900&amp;deg;C. The magma must cool at this depth to produce 
a complete An&lt;sub&gt;68&lt;/sub&gt;-An&lt;sub&gt;40&lt;/sub&gt; plagioclase zone and a Mg-rich layer on the amphiboles before the magma is cycled back to a high 
pressure, when a new layer of Fe-rich amphibole is acquired. 
The amphibole crystallizing in the dacite experiments at less 
than 200 MPa is lower in aluminum than any compositions 
in the natural cyclically zoned phenocrysts. The outer rim on 
some 2004-6 amphibole phenocrysts appears to have formed 
in the 100-200 MPa range, as do some phenocrysts in the 
May 1980 dacite pumice. Plagioclase rims of An&lt;sub&gt;35&lt;/sub&gt; in the 
2004-6 magmas indicate that phenocryst growth continued 
until the pressure decreased to 130 MPa and that ascent was 
slow until this depth. Magma then entered the conduit for a 
relatively rapid ascent to the surface as indicated by the very 
thin (less than 5 &amp;mu;m) decompression-induced rims on the 
amphibole phenocrysts.</dc:description>
  <dc:format>application/pdf</dc:format>
  <dc:identifier>10.3133/pp175031</dc:identifier>
  <dc:language>en</dc:language>
  <dc:publisher>U.S. Geological Survey</dc:publisher>
  <dc:title>Magmatic conditions and processes in the storage zone of the 2004-2006 Mount St. Helens dacite</dc:title>
  <dc:type>reports</dc:type>
</oai_dc:dc>