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<!DOCTYPE article SYSTEM "http://www.adv-radio-sci.net/inc/ars/copernicus.dtd">
<article language="en">
	<journal>
		<journal_title>Advances in Radio Science</journal_title>
		<journal_url>www.adv-radio-sci.net</journal_url>
		<issn>1684-9965</issn>
		<eissn>1684-9973</eissn>
		<volume_number>3</volume_number>
		<volume_title>Kleinheubacher Berichte 2004</volume_title>
		<publication_year>2005</publication_year>
	</journal>
	<doi>10.5194/ars-3-441-2005</doi>
	<article_url>http://www.adv-radio-sci.net/3/441/2005/</article_url>
	<abstract_html>http://www.adv-radio-sci.net/3/441/2005/ars-3-441-2005.html</abstract_html>
	<fulltext_pdf>http://www.adv-radio-sci.net/3/441/2005/ars-3-441-2005.pdf</fulltext_pdf>
	<start_page>441</start_page>
	<end_page>447</end_page>
	<publication_date>2005-05-13</publication_date>
	<article_title content_type="html">Model modulation to add smaller scale structures to large scale electron density models</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>R. Leitinger</name>
		</author>
		<author numeration="2" affiliations="1">
			<name>E. Feichter</name>
		</author>
		<author numeration="3" affiliations="1">
			<name>M. Rieger</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Institut für Geophysik, Astrophysik und Meteorologie, Universität Graz, Austria</affiliation>
	</affiliations>
	<abstract content_type="html">Usually regional and global electron density models provide large scale spatial structures only
and smooth out the smaller scale features of the electron density distribution.
We present a method to modulate existing electron density models by multiplication:
&lt;i&gt;M&lt;/i&gt;(&lt;i&gt;h, &amp;#x03C6;, &amp;#x03BB;, t&lt;/i&gt;) = &lt;i&gt;L&lt;/i&gt;(&lt;i&gt;h, &amp;#x03C6;, &amp;#x03BB;, t&lt;/i&gt;) &amp;#x00D7; &lt;i&gt;S&lt;sub&gt;1&lt;/sub&gt;&lt;/i&gt;(&lt;i&gt;h, &amp;#x03C6;, &amp;#x03BB;, t&lt;/i&gt;) &amp;#x00D7; &lt;i&gt;S&lt;sub&gt;2&lt;/sub&gt;&lt;/i&gt;(&lt;i&gt;h, &amp;#x03C6;, &amp;#x03BB;, t&lt;/i&gt;) &amp;#x00D7; ... &lt;i&gt;S&lt;sub&gt;n&lt;/sub&gt;&lt;/i&gt;(&lt;i&gt;h, &amp;#x03C6;, &amp;#x03BB;, t&lt;/i&gt;)
&lt;br&gt;
&lt;i&gt;M&lt;/i&gt;: resulting electron density distribution, &lt;i&gt;L&lt;/i&gt;: large scale model,
&lt;i&gt;S&lt;sub&gt;1&lt;/sub&gt;...S&lt;sub&gt;n&lt;/sub&gt;&lt;/i&gt;: modulating models for              n
the smaller scale structures; &lt;i&gt;h&lt;/i&gt;: height; &lt;i&gt;φ, λ&lt;/i&gt;:
geographic coordinates, &lt;i&gt;t&lt;/i&gt;: Universal Time.
There are no restrictions to the nature of the large scale model provided it
takes height and
horizontal coordinates as input. Examples are models of the &quot;profiler&quot; type
which use large scale
&quot;maps&quot; for profile anchor points (e.g., E, F1, F2 peak properties) like
the International Reference Ionosphere (IRI). Typical examples for smaller
scale structures are
ridges, troughs and wavelike disturbances.
The advantage of modulation by multiplication is that there is no danger
to get zero or negative
values of electron density as long as the background and modulations are

&amp;gt;0 everywhere.  For
each modulation model, unity means &quot;undisturbed&quot;.</abstract>
	<references>
	</references>
</article>

