<?xml version="1.0" encoding="utf-8" standalone="no"?>
<!DOCTYPE article SYSTEM "http://www.electronic-earth-discuss.net/inc/eed/copernicus.dtd">
<article language="en">
	<journal>
		<journal_title>eEarth Discussions</journal_title>
		<journal_url>www.electronic-earth-discuss.net</journal_url>
		<issn>1815-3836</issn>
		<eissn>1815-3844</eissn>
		<volume_number>1</volume_number>
		<issue_number>2</issue_number>
		<publication_year>2006</publication_year>
	</journal>
	<doi>10.5194/eed-1-97-2006</doi>
	<article_url>http://www.electronic-earth-discuss.net/1/97/2006/</article_url>
	<abstract_html>http://www.electronic-earth-discuss.net/1/97/2006/eed-1-97-2006.html</abstract_html>
	<fulltext_pdf>http://www.electronic-earth-discuss.net/1/97/2006/eed-1-97-2006.pdf</fulltext_pdf>
	<start_page>97</start_page>
	<end_page>121</end_page>
	<publication_date>2006-07-24</publication_date>
	<article_title content_type="html">Stimulated infrared emission from rocks: assessing a stress indicator</article_title>
	<authors>
		<author numeration="1" affiliations="1,2,3">
			<name>F. T. Freund</name>
		</author>
		<author numeration="2" affiliations="2,4">
			<name>A. Takeuchi</name>
		</author>
		<author numeration="3" affiliations="2">
			<name>B. W. S. Lau</name>
		</author>
		<author numeration="4" affiliations="5">
			<name>A. Al-Manaseer</name>
		</author>
		<author numeration="5" affiliations="6">
			<name>C. C. Fu</name>
		</author>
		<author numeration="6" affiliations="7">
			<name>N. A. Bryant</name>
		</author>
		<author numeration="7" affiliations="8">
			<name>D. Ouzounov</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Ecosystems Science and Technology Branch, Code SGE, NASA Ames Research Center, Moffett Field, 94035-1000, CA, USA</affiliation>
		<affiliation numeration="2" content_type="html">Department of Physics, San Jose State University, San Jose, 95192-0106 CA, USA</affiliation>
		<affiliation numeration="3" content_type="html">SETI Institute, Mountain View 94043, CA, USA</affiliation>
		<affiliation numeration="4" content_type="html">Department of Chemistry, Niigata University, Ikarashi-ninotyo, Niigata 950-2181, Japan</affiliation>
		<affiliation numeration="5" content_type="html">Department of Civil Engineering, San Jose State University, San Jose, 95192-008 CA, USA</affiliation>
		<affiliation numeration="6" content_type="html">Department of Civil Engineering, University of Maryland, College Park, 20742 MD, USA</affiliation>
		<affiliation numeration="7" content_type="html">Jet Propulsion Laboratory, Org. 3880, Pasadena, CA 91109-8099, USA</affiliation>
		<affiliation numeration="8" content_type="html">CEORS, George Mason University, Fairfax, VA 22030-4444, USA</affiliation>
	</affiliations>
	<abstract content_type="html">To study the effect of stress-activated positive hole (p-hole) charge
carriers on the infrared (IR) emission from rocks, we subjected a portion
(~10 vol.%) of a large (60&amp;times;30&amp;times;7.5 cm&lt;sup&gt;3&lt;/sup&gt;) block of
anorthosite, a nearly monomineralic (Ca-rich feldspar) igneous rock, to
uniaxial deviatory stress up to failure. We measured the IR emission from a
flat surface &amp;asymp;40 cm from the stressed rock volume over the 800&amp;ndash;1300 cm&lt;sup&gt;&amp;minus;1&lt;/sup&gt; (7.7&amp;ndash;12.5 &amp;mu;m) range.
Upon loading, the intensity and spectrum of the IR emission change. Narrow bands near instantly appear at 930 cm&lt;sup&gt;&amp;minus;1&lt;/sup&gt;
(10.75 &amp;mu;m), 880 cm&lt;sup&gt;&amp;minus;1&lt;/sup&gt; (11.36 &amp;mu;m), 820 cm&lt;sup&gt;&amp;minus;1&lt;/sup&gt; (12.4 &amp;mu;m)
plus additional bands in the 1000&amp;ndash;1300 cm&lt;sup&gt;&amp;minus;1&lt;/sup&gt; (10.0&amp;ndash;7.7 &amp;mu;m) range.
Upon further loading the bands broaden and shift. Their intensities increase
but also fluctuate. Near the emission maxima at 300 K, at 1150 cm&lt;sup&gt;&amp;minus;1&lt;/sup&gt; and
1030 cm&lt;sup&gt;&amp;minus;1&lt;/sup&gt; (8.7 and 9 &amp;mu;m), barely any intensity increase
occurs suggesting that the temperature of the surface does not actually
increase. We propose that the observed narrow IR emission bands arise from
vibrationally excited O-O stretching modes which form when p-hole charge
carriers (activated in the stressed rock) spread into the unstressed portion
of the rock to the surface, where they recombine and radiatively decay. The
effect, stimulated IR emission due to hole-hole recombination, may help
explain the enhanced IR emission seen in night-time satellite images of
the land surface before major earthquakes known as &quot;thermal anomalies&apos;&apos;.</abstract>
	<references>
	</references>
</article>

