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<!DOCTYPE article SYSTEM "http://www.nonlin-processes-geophys.net/inc/npg/copernicus.dtd">
<article language="en">
	<journal>
		<journal_title>Nonlinear Processes  in Geophysics</journal_title>
		<journal_url>www.nonlin-processes-geophys.net</journal_url>
		<issn>1023-5809</issn>
		<eissn>1607-7946</eissn>
		<volume_number>9</volume_number>
		<issue_number>5/6</issue_number>
		<publication_year>2002</publication_year>
	</journal>
	<doi>10.5194/npg-9-425-2002</doi>
	<article_url>http://www.nonlin-processes-geophys.net/9/425/2002/</article_url>
	<abstract_html>http://www.nonlin-processes-geophys.net/9/425/2002/npg-9-425-2002.html</abstract_html>
	<fulltext_pdf>http://www.nonlin-processes-geophys.net/9/425/2002/npg-9-425-2002.pdf</fulltext_pdf>
	<start_page>425</start_page>
	<end_page>433</end_page>
	<publication_date>0000-00-00</publication_date>
	<article_title content_type="html">Neural network prediction of geomagnetic activity: a method using local Hölder exponents</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>Z. Vörös</name>
		</author>
		<author numeration="2" affiliations="1">
			<name>D. Jankovičová</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Geomagnetic Observatory Hurbanovo, Geophysical Institute SAS, Slovak Republic</affiliation>
	</affiliations>
	<abstract content_type="html">Local scaling and
      singularity properties of solar wind and geomagnetic time series were
      analysed using Hölder exponents . It was shown that in analysed cases due
      to the multifractality of fluctuations, α changes from point to point. We
      argued there exists a peculiar interplay between regularity/irregularity
      and amplitude characteristics of fluctuations which could be exploited for
      the improvement of predictions of geomagnetic activity. To this end, a
      layered back-propagation artificial neural network model with feedback
      connection was used for the study of the solar wind magnetosphere coupling
      and prediction of the geomagnetic D&lt;sub&gt;st&lt;/sub&gt; index. The solar wind
      input was taken from the principal component analysis of the
      interplanetary magnetic field, proton density and bulk velocity. Superior
      network performance was achieved in cases when the information on local
      Hölder exponents was added to the input layer.</abstract>
	<references>
	</references>
</article>

