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Time variations of the heliospheric termination shock radius

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dc.contributor.author Exarhos, G en
dc.contributor.author Moussas, X en
dc.date.accessioned 2014-03-01T01:49:05Z
dc.date.available 2014-03-01T01:49:05Z
dc.date.issued 1999 en
dc.identifier.issn 0038-0938 en
dc.identifier.uri https://dspace.lib.ntua.gr/xmlui/handle/123456789/25664
dc.subject.classification Astronomy & Astrophysics en
dc.subject.other LOCAL INTERSTELLAR-MEDIUM en
dc.subject.other SOLAR-CYCLE VARIATIONS en
dc.subject.other COSMIC-RAY GRADIENTS en
dc.subject.other OUTER HELIOSPHERE en
dc.subject.other FLOW DOWNSTREAM en
dc.subject.other WIND PLASMA en
dc.subject.other HELIOPAUSE en
dc.subject.other BOUNDARY en
dc.subject.other ASYMMETRY en
dc.subject.other DISTANCE en
dc.title Time variations of the heliospheric termination shock radius en
heal.type journalArticle en
heal.language English en
heal.publicationDate 1999 en
heal.abstract In this work we study the temporal variation of the heliospheric termination shock radius using in-ecliptic combined measurements from different spacecraft at 1 AU near the Earth. The results show that the radius of the heliospheric termination shock varies in time with a period of 11 years. During some 11-year time periods the shock radius anti-correlates with the solar cycle activity, specifically with the sunspot number. The average radius is approximately 115 AU with minimum value similar to 80 AU and maximum value similar to 150 AU. These values are the upper limits since we do not take into account the charge exchange effects of solar wind with the interstellar neutrals. We also compare the results with those from other spacecraft (Helios 1 and Voyager 2). We find that Helios 1 measurements give almost the same result as the one obtained from measurements at 1 AU while Voyager 2 measurements give a heliospheric termination shock radius approximately 15 AU lower. en
heal.publisher KLUWER ACADEMIC PUBL en
heal.journalName SOLAR PHYSICS en
dc.identifier.isi ISI:000082534900011 en
dc.identifier.volume 187 en
dc.identifier.issue 1 en
dc.identifier.spage 145 en
dc.identifier.epage 155 en


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