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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>11</volume_number>
		<issue_number>4</issue_number>
		<publication_year>2004</publication_year>
	</journal>
	<doi>10.5194/npg-11-441-2004</doi>
	<article_url>http://www.nonlin-processes-geophys.net/11/441/2004/</article_url>
	<abstract_html>http://www.nonlin-processes-geophys.net/11/441/2004/npg-11-441-2004.html</abstract_html>
	<fulltext_pdf>http://www.nonlin-processes-geophys.net/11/441/2004/npg-11-441-2004.pdf</fulltext_pdf>
	<start_page>441</start_page>
	<end_page>445</end_page>
	<publication_date>2004-09-28</publication_date>
	<article_title content_type="html">Multifractal structure of the large-scale heliospheric magnetic field strength fluctuations near 85AU</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>L. F. Burlaga</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">NASA-Goddard Space Flight Center, Laboratory for Extraterrestrial Physics, Code 692, Greenbelt, Maryland 20771, USA</affiliation>
	</affiliations>
	<abstract content_type="html">During 2002, the Voyager 1 spacecraft was in the heliosphere
between 83.4 and 85.9AU (1AU is the mean distance from the
Sun to Earth) at 34&amp;deg; N heliographic latitude. The
magnetic field strength profile observed in this region had a
multifractal structure in the range of scales from 2 to 16 days.
The multifractal spectrum observed near 85AU is similar to
that observed near 40AU, indicating relatively little evolution
of the multifractal structure of the magnetic field with
increasing distance in the distant heliosphere in the epoch
near solar maximum.</abstract>
	<references>
	</references>
</article>

