Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/26453
DC Field | Value | Language |
---|---|---|
dc.contributor.author | DE MARCO, Rossana | en_US |
dc.contributor.author | MARCUCCI, Maria Federica | en_US |
dc.contributor.author | BRUNO, Roberto | en_US |
dc.contributor.author | D'AMICIS, RAFFAELLA | en_US |
dc.contributor.author | Servidio, S. | en_US |
dc.contributor.author | Valentini, F. | en_US |
dc.contributor.author | Lavraud, B. | en_US |
dc.contributor.author | Louarn, P. | en_US |
dc.contributor.author | Salatti, M. | en_US |
dc.date.accessioned | 2020-07-14T15:34:45Z | - |
dc.date.available | 2020-07-14T15:34:45Z | - |
dc.date.issued | 2016 | en_US |
dc.identifier.issn | 1748-0221 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/26453 | - |
dc.description.abstract | We use a numerical code which reproduces the angular/energy response of a typical top-hat electrostatic analyser starting from solar wind proton velocity distribution functions (VDFs) generated by numerical simulations. The simulations are based on the Hybrid Vlasov-Maxwell numerical algorithm which integrates the Vlasov equation for the ion distribution function, while the electrons are treated as a fluid. A virtual satellite launched through the simulation box measures the particle VDFs. Such VDFs are moved from the simulation Cartesian grid to energy-angular coordinates to mimic the response of a real sensor in the solar wind. Different energy-angular resolutions of the analyser are investigated in order to understand the influence of the phase-space resolution in existing and upcoming space missions, with regards to determining the key parameters of plasma dynamics. | en_US |
dc.language.iso | eng | en_US |
dc.title | Importance of energy and angular resolutions in top-hat electrostatic analysers for solar wind proton measurements | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1088/1748-0221/11/08/C08010 | en_US |
dc.identifier.scopus | 2-s2.0-84985930988 | en_US |
dc.identifier.isi | 000387859900008 | en_US |
dc.identifier.url | http://iopscience.iop.org/article/10.1088/1748-0221/11/08/C08010/meta | en_US |
dc.relation.medium | ELETTRONICO | en_US |
dc.relation.volume | 11 | en_US |
dc.relation.issue | 8 | en_US |
dc.relation.firstpage | C08010 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.numberofauthors | 9 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | FRA | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | JOURNAL OF INSTRUMENTATION | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2016JInst..11C8010D | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.openairetype | Article | - |
item.languageiso639-1 | en | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | IAPS Roma | - |
crisitem.author.dept | IAPS Roma | - |
crisitem.author.dept | IAPS Roma | - |
crisitem.author.dept | IAPS Roma | - |
crisitem.author.orcid | 0000-0002-7426-7379 | - |
crisitem.author.orcid | 0000-0002-5002-6060 | - |
crisitem.author.orcid | 0000-0002-2152-0115 | - |
crisitem.author.orcid | 0000-0003-2647-117X | - |
crisitem.journal.journalissn | 1748-0221 | - |
crisitem.journal.ance | E190325 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
DeMarco_JINST_ICFDT4_revised.pdf | postprint | 1.21 MB | Adobe PDF | View/Open |
13_2016_TOPHAT_JINST.pdf | [Administrators only] | 1.24 MB | Adobe PDF |
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