<?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>Donald A. Swanson</dc:contributor>
  <dc:contributor>Sebastien Biass</dc:contributor>
  <dc:contributor>Sarah A. Fagents</dc:contributor>
  <dc:contributor>Tim R. Orr</dc:contributor>
  <dc:creator>Bruce F. Houghton</dc:creator>
  <dc:date>2017</dc:date>
  <dc:description>&lt;p&gt;&lt;span&gt;We describe the discrete ballistic and wind-advected products of a small, but exceptionally well-characterized, explosive eruption of wall-rock-derived pyroclasts from Kīlauea volcano on 19 March 2008 and, for the first time, integrate the size distribution of the two subpopulations to reconstruct the true size distribution of a population of pyroclasts as it exited from the vent. Based on thinning and fining relationships, the wind-advected fraction had a mass of 6.1&amp;nbsp;×&amp;nbsp;10&lt;/span&gt;&lt;sup&gt;5&lt;/sup&gt;&lt;span&gt;&amp;nbsp;kg and a thickness half distance of 110&amp;nbsp;m, placing it at the bottom end of the magnitude and intensity spectra of pyroclastic falls. The ballistic population was mapped, in the field and by using structure-from-motion techniques, to a diameter of &amp;gt;&amp;nbsp;10–20&amp;nbsp;cm over an area of ~0.1&amp;nbsp;km&lt;/span&gt;&lt;sup&gt;2&lt;/sup&gt;&lt;span&gt;, with an estimated mass of 1&amp;nbsp;×&amp;nbsp;10&lt;/span&gt;&lt;sup&gt;5&lt;/sup&gt;&lt;span&gt;&amp;nbsp;kg. Initial ejection velocities of 50–80&amp;nbsp;m/s were estimated from inversion of isopleths. The total grain size distribution was estimated by using a mass partitioning of 98% of wind-advected material and 2% of ballistics, resulting in median and sorting values of −1.7&lt;/span&gt;&lt;i&gt;ϕ&lt;/i&gt;&lt;span&gt;&amp;nbsp;and 3.1&lt;/span&gt;&lt;i&gt;ϕ&lt;/i&gt;&lt;span&gt;. It is markedly broader than those calculated for the products of magmatic explosive eruptions, because the grain size of 19 March 2008 clast population is unrelated to a volcanic fragmentation event and instead was “inherited” from a population of talus clasts that temporary blocked the vent prior to the eruption. Despite a conspicuous near-field presence, the ballistic subpopulation has only a minor influence on the grain size distribution because of its rapid thinning and fining away from source.&lt;/span&gt;&lt;/p&gt;</dc:description>
  <dc:format>application/pdf</dc:format>
  <dc:identifier>10.1002/2017JB014040</dc:identifier>
  <dc:language>en</dc:language>
  <dc:publisher>American Geophysical Union</dc:publisher>
  <dc:title>Partitioning of pyroclasts between ballistic transport and a convective plume: Kīlauea volcano, 19 March 2008</dc:title>
  <dc:type>article</dc:type>
</oai_dc:dc>