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<article language="en">
	<journal>
		<journal_title>Astrophysics and Space Sciences Transactions</journal_title>
		<journal_url>www.astrophys-space-sci-trans.net</journal_url>
		<issn>1810-6528</issn>
		<eissn>1810-6536</eissn>
		<volume_number>2</volume_number>
		<issue_number>2</issue_number>
		<publication_year>2006</publication_year>
	</journal>
	<doi>10.5194/astra-2-53-2006</doi>
	<article_url>http://www.astrophys-space-sci-trans.net/2/53/2006/</article_url>
	<abstract_html>http://www.astrophys-space-sci-trans.net/2/53/2006/astra-2-53-2006.html</abstract_html>
	<fulltext_pdf>http://www.astrophys-space-sci-trans.net/2/53/2006/astra-2-53-2006.pdf</fulltext_pdf>
	<start_page>53</start_page>
	<end_page>61</end_page>
	<publication_date>2006-08-08</publication_date>
	<article_title content_type="html">The Sun&apos;s journey through the local interstellar medium: the paleoLISM and paleoheliosphere</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>P. C. Frisch</name>
		</author>
		<author numeration="2" affiliations="2">
			<name>J. D. Slavin</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">University of Chicago, Department of Astronomy and Astrophysics, 5640 S. Ellis Ave., Chicago, IL  60637, USA</affiliation>
		<affiliation numeration="2" content_type="html">Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA</affiliation>
	</affiliations>
	<abstract content_type="html">Over the recent past, the galactic environment of the Sun has differed
substantially from today.  Sometime within the past ~130 000
years, and possibly as recent as ~56 000 years ago, the Sun
entered the tenuous tepid partially ionized interstellar material now flowing
past the Sun.  Prior to that, the Sun was in the low density interior
of the Local Bubble.  As the Sun entered the local ISM flow, we passed
briefly through an interface region of some type.  The low column
densities of the cloud now surrounding the solar system indicate that
heliosphere boundary conditions will vary from opacity considerations
alone as the Sun moves through the cloud. These variations in the
interstellar material surrounding the Sun affected the
paleoheliosphere.</abstract>
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