Please use this identifier to cite or link to this item:
http://hdl.handle.net/2122/5031
DC Field | Value | Language |
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dc.contributor.authorall | Consolini, G.; INAF-Istituto di Fisica dello Spazio Interplanetario, 00133 Roma, Italy | en |
dc.contributor.authorall | Bavassano, B.; INAF-Istituto di Fisica dello Spazio Interplanetario, 00133 Roma, Italy | en |
dc.contributor.authorall | De Michelis, P.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia | en |
dc.date.accessioned | 2009-04-21T08:47:26Z | en |
dc.date.available | 2009-04-21T08:47:26Z | en |
dc.date.issued | 2009-04-07 | en |
dc.identifier.uri | http://hdl.handle.net/2122/5031 | en |
dc.description.abstract | Since 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.iso | English | en |
dc.publisher.name | EGU/AGU - Copernicus Publications | en |
dc.relation.ispartof | Nonlinear Processes in Geophysics | en |
dc.relation.ispartofseries | / 16 (2009) | en |
dc.subject | fluctuations in space plasmas | en |
dc.subject | heterogeneity | en |
dc.subject | statistical features | en |
dc.subject | solar wind | en |
dc.title | A probabilistic approach to heterogeneity in space plasmas: the case of magnetic field intensity in solar wind | en |
dc.type | article | en |
dc.description.status | Published | en |
dc.type.QualityControl | Peer-reviewed | en |
dc.description.pagenumber | 265-273 | en |
dc.identifier.URL | http://www.nonlin-processes-geophys.net/16/265/2009/ | en |
dc.subject.INGV | 01. Atmosphere::01.03. Magnetosphere::01.03.01. Interplanetary physics | en |
dc.subject.INGV | 01. Atmosphere::01.03. Magnetosphere::01.03.05. Solar variability and solar wind | en |
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dc.description.obiettivoSpecifico | 3.9. Fisica della magnetosfera, ionosfera e meteorologia spaziale | en |
dc.description.journalType | JCR Journal | en |
dc.description.fulltext | open | en |
dc.contributor.author | Consolini, G. | en |
dc.contributor.author | Bavassano, B. | en |
dc.contributor.author | De Michelis, P. | en |
dc.contributor.department | INAF-Istituto di Fisica dello Spazio Interplanetario, 00133 Roma, Italy | en |
dc.contributor.department | Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia | en |
item.openairetype | article | - |
item.cerifentitytype | Publications | - |
item.languageiso639-1 | en | - |
item.grantfulltext | open | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | INAF – Istituto di Astrofisica e Planetologia Spaziali, 00133 Roma, Italy | - |
crisitem.author.dept | INAF-Istituto di Fisica dello Spazio Interplanetario, 00133 Roma, Italy | - |
crisitem.author.dept | Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia | - |
crisitem.author.orcid | 0000-0002-3403-647X | - |
crisitem.author.orcid | 0000-0002-2708-0739 | - |
crisitem.author.parentorg | Istituto Nazionale di Geofisica e Vulcanologia | - |
crisitem.classification.parent | 01. Atmosphere | - |
crisitem.classification.parent | 01. Atmosphere | - |
crisitem.department.parentorg | Istituto Nazionale di Geofisica e Vulcanologia | - |
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