Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/26467
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Podolak, Morris | en_US |
dc.contributor.author | Flandes, Alberto | en_US |
dc.contributor.author | DELLA CORTE, VINCENZO | en_US |
dc.contributor.author | Krüger, Harald | en_US |
dc.date.accessioned | 2020-07-16T10:22:31Z | - |
dc.date.available | 2020-07-16T10:22:31Z | - |
dc.date.issued | 2016 | en_US |
dc.identifier.issn | 0032-0633 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/26467 | - |
dc.description.abstract | We present a simple model for gas and dust flow from 67P/Churyumov-Gerasimenko that can be used to understand the grain impact observed by the DIM instrument on Philae (Krüger et al., 2015). We show how model results when applied to the GIADA measurements (Rotundi et al., 2015; Della Corte et al., 2015) can be used, in conjunction with the results found by the MIRO (Schloerb et al., 2015) and VIRTIS (De Sanctis et al., 2015) instruments to infer surface properties such as surface temperature and surface ice fraction. | en_US |
dc.language.iso | eng | en_US |
dc.title | A simple model for understanding the DIM dust measurement at comet 67P/Churyumov-Gerasimenko | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1016/j.pss.2016.04.006 | en_US |
dc.identifier.scopus | 2-s2.0-84964915956 | en_US |
dc.identifier.isi | 000389284800011 | en_US |
dc.identifier.url | https://www.sciencedirect.com/science/article/pii/S0032063315301057?via%3Dihub | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 133 | en_US |
dc.relation.firstpage | 85 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | DEU | en_US |
dc.contributor.country | ISR | en_US |
dc.contributor.country | MEX | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | PLANETARY AND SPACE SCIENCE | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2016P&SS..133...85P | en_US |
dc.relation.ercsector | ERC sectors::Physical Sciences and Engineering::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation | 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 | O.A. Capodimonte | - |
crisitem.author.orcid | 0000-0001-6461-5803 | - |
crisitem.journal.journalissn | 0032-0633 | - |
crisitem.journal.ance | E132431 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
dustcode2.pdf | preprint | 372.12 kB | Adobe PDF | View/Open |
PSS-main.pdf | [Administrators only] | 415.72 kB | Adobe PDF |
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Items in DSpace are published in Open Access, unless otherwise indicated.