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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>Andrew J. L. Harris</dc:contributor>
  <dc:contributor>Maurizio Ripepe</dc:contributor>
  <dc:contributor>Jonathan Dehn</dc:contributor>
  <dc:contributor>David A. Rothery</dc:contributor>
  <dc:contributor>Sonia Calvari</dc:contributor>
  <dc:creator>Matthew R. Patrick</dc:creator>
  <dc:date>2007</dc:date>
  <dc:description>&lt;p&gt;Forward Looking Infrared Radiometer (FLIR) cameras offer a unique view of explosive volcanism by providing an image of calibrated temperatures. In this study, 344 eruptive events at Stromboli volcano, Italy, were imaged in 2001&amp;ndash;2004 with a FLIR camera operating at up to 30 Hz. The FLIR was effective at revealing both ash plumes and coarse ballistic scoria, and a wide range of eruption styles was recorded. Eruptions at Stromboli can generally be classified into two groups: Type 1 eruptions, which are dominated by coarse ballistic particles, and Type 2 eruptions, which consist of an optically-thick, ash-rich plume, with (Type 2a) or without (Type 2b) large numbers of ballistic particles. Furthermore, Type 2a plumes exhibited gas thrust velocities (&amp;gt;15 m s&lt;sup&gt;&amp;minus;1&lt;/sup&gt; ) while Type 2b plumes were limited to buoyant velocities (&amp;lt;15 m s&amp;minus;1 ) above the crater rim. A given vent would normally maintain a particular gross eruption style (Type 1 vs. 2) for days to weeks, indicating stability of the uppermost conduit on these timescales. Velocities at the crater rim had a range of 3&amp;ndash;101 m s&amp;minus;1 , with an overall mean value of 24 m s&lt;sup&gt;&amp;minus;1&lt;/sup&gt;. Mean crater rim velocities by eruption style were: Type 1= 34 m s&lt;sup&gt;&amp;minus;1&lt;/sup&gt; , Type 2a=31 m s&lt;sup&gt;&amp;minus;1&lt;/sup&gt; , Type 2b=7 m s&lt;sup&gt;&amp;minus;1&lt;/sup&gt; . Eruption durations had a range of 6&amp;ndash;41 s, with a mean of 15 s, similar among eruption styles. The ash in Type 2 eruptions originates from either backfilled material (crater wall slumping or ejecta rollback) or rheological changes in the uppermost magma column. Type 2a and 2b behaviors are shown to be a function of the overpressure of the bursting slug. In general, our imaging data support a broadening of the current paradigm for strombolian behavior, incorporating an uppermost conduit that can be more variable than is commonly considered.&lt;/p&gt;</dc:description>
  <dc:format>application/pdf</dc:format>
  <dc:identifier>10.1007/s00445-006-0107-0</dc:identifier>
  <dc:language>en</dc:language>
  <dc:publisher>Springer-Verlag</dc:publisher>
  <dc:title>Strombolian explosive styles and source conditions</dc:title>
  <dc:type>article</dc:type>
</oai_dc:dc>