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<!DOCTYPE article SYSTEM "http://www.atmos-chem-phys-discuss.net/inc/acpd/copernicus.dtd">
<article language="en">
	<journal>
		<journal_title>Atmospheric Chemistry and Physics Discussions</journal_title>
		<journal_url>www.atmos-chem-phys-discuss.net</journal_url>
		<issn>1680-7367</issn>
		<eissn>1680-7375</eissn>
		<volume_number>3</volume_number>
		<issue_number>6</issue_number>
		<publication_year>2003</publication_year>
	</journal>
	<doi>10.5194/acpd-3-6721-2003</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/3/6721/2003/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/3/6721/2003/acpd-3-6721-2003.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/3/6721/2003/acpd-3-6721-2003.pdf</fulltext_pdf>
	<start_page>6721</start_page>
	<end_page>6732</end_page>
	<publication_date>2003-12-18</publication_date>
	<article_title content_type="html">Evaporation of high speed sporadic meteors</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>E. Murad</name>
		</author>
		<author numeration="2" affiliations="2">
			<name>C. Roth</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Air Force Research Laboratory, Space Vehicles Directorate, Hanscom AFB, MA 01731, USA</affiliation>
		<affiliation numeration="2" content_type="html">Radex, Inc., 3 Preston Court, Bedford, MA 01730, USA</affiliation>
	</affiliations>
	<abstract content_type="html">Recent measurements conducted at the Arecibo Observatory report high-speed sporadic meteors
      having velocities near 50 km/s.  The results seem to indicate a bimodal velocity distribution in
      the sporadic meteors (maxima at ~20 km/s and ~50 km/s).  The particles have a maximum mass
      of ~1 &amp;mu;g.   This paper will present an analysis of the ablation of
      1 &amp;mu;g meteoroids having velocities of 20, 30, 50, and
      70 km/s.  The calculations show that there is fractionation even for the fast meteoroids, the effect being particularly noticeable for the
      1 &amp;mu;g sporadic particles, and less so for the heavier particles.  The relevance of the calculations to the radar observations of the
      sporadic meteors will be discussed.</abstract>
	<references>
	</references>
</article>

