Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/5031
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dc.contributor.authorallConsolini, G.; INAF-Istituto di Fisica dello Spazio Interplanetario, 00133 Roma, Italyen
dc.contributor.authorallBavassano, B.; INAF-Istituto di Fisica dello Spazio Interplanetario, 00133 Roma, Italyen
dc.contributor.authorallDe Michelis, P.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.date.accessioned2009-04-21T08:47:26Zen
dc.date.available2009-04-21T08:47:26Zen
dc.date.issued2009-04-07en
dc.identifier.urihttp://hdl.handle.net/2122/5031en
dc.description.abstractSince the early 90s it was shown that Probability Distribution Functions (PDFs) of small scale differences (fluctuations) of several quantities in space plasmas display significant departures from Gaussianity. The non-Gaussian shape of PDFs was ascribed to intermittency and discussed in the framework of intermittent MHD turbulence. Here, we put the attention to the PDF of magnetic field intensity instead of its differences showing how the PDF of such quantity in a quiet solar wind can be related with the occurrence of heterogeneity. In detail, we derive the shape of the PDFs by simple statistical considerations based on the concept of subordination in probability theory. An interpretation and a discussion in terms of existing coherent magnetic structures in a mechanical near-equilibrium state are also presented.en
dc.language.isoEnglishen
dc.publisher.nameEGU/AGU - Copernicus Publicationsen
dc.relation.ispartofNonlinear Processes in Geophysicsen
dc.relation.ispartofseries/ 16 (2009)en
dc.subjectfluctuations in space plasmasen
dc.subjectheterogeneityen
dc.subjectstatistical featuresen
dc.subjectsolar winden
dc.titleA probabilistic approach to heterogeneity in space plasmas: the case of magnetic field intensity in solar winden
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber265-273en
dc.identifier.URLhttp://www.nonlin-processes-geophys.net/16/265/2009/en
dc.subject.INGV01. Atmosphere::01.03. Magnetosphere::01.03.01. Interplanetary physicsen
dc.subject.INGV01. Atmosphere::01.03. Magnetosphere::01.03.05. Solar variability and solar winden
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dc.description.obiettivoSpecifico3.9. Fisica della magnetosfera, ionosfera e meteorologia spazialeen
dc.description.journalTypeJCR Journalen
dc.description.fulltextopenen
dc.contributor.authorConsolini, G.en
dc.contributor.authorBavassano, B.en
dc.contributor.authorDe Michelis, P.en
dc.contributor.departmentINAF-Istituto di Fisica dello Spazio Interplanetario, 00133 Roma, Italyen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextopen-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptINAF – Istituto di Astrofisica e Planetologia Spaziali, 00133 Roma, Italy-
crisitem.author.deptINAF-Istituto di Fisica dello Spazio Interplanetario, 00133 Roma, Italy-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia-
crisitem.author.orcid0000-0002-3403-647X-
crisitem.author.orcid0000-0002-2708-0739-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.classification.parent01. Atmosphere-
crisitem.classification.parent01. Atmosphere-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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