Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/26465
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Hornung, Klaus | en_US |
dc.contributor.author | Merouane, Sihane | en_US |
dc.contributor.author | Hilchenbach, Martin | en_US |
dc.contributor.author | Langevin, Yves | en_US |
dc.contributor.author | Mellado, Eva Maria | en_US |
dc.contributor.author | DELLA CORTE, VINCENZO | en_US |
dc.contributor.author | Kissel, Jochen | en_US |
dc.contributor.author | Engrand, Cecile | en_US |
dc.contributor.author | Schulz, Rita | en_US |
dc.contributor.author | Ryno, Jouni | en_US |
dc.contributor.author | Silen, Johan | en_US |
dc.contributor.author | COSIMA Team | en_US |
dc.date.accessioned | 2020-07-16T10:00:10Z | - |
dc.date.available | 2020-07-16T10:00:10Z | - |
dc.date.issued | 2016 | en_US |
dc.identifier.issn | 0032-0633 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/26465 | - |
dc.description.abstract | Soon after the arrival of the ROSETTA spacecraft at Comet 67/P Churyumov-Gerasimenko the onboard instrument COSIMA ("Cometary Secondary Ion Mass Analyzer") collected a large number of cometary dust particles on targets from gold black of thickness between 10 and 30 μm. Inspection by its camera subsystem revealed that many of them consist of smaller units of typically some tens of micrometers in size. The collection process left the smaller dust particles in an essentially unaltered state whereas most particles larger than about 100 μm got fragmented into smaller pieces. Using the observed fragment size distributions, the present paper includes a first assessment of the strength for those dust particles that were disrupted upon impact. | en_US |
dc.language.iso | eng | en_US |
dc.title | A first assessment of the strength of cometary particles collected in-situ by the COSIMA instrument onboard ROSETTA | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1016/j.pss.2016.07.003 | en_US |
dc.identifier.scopus | 2-s2.0-84997530148 | en_US |
dc.identifier.isi | 000389284800009 | en_US |
dc.identifier.url | https://www.sciencedirect.com/science/article/pii/S0032063315300957?via%3Dihub | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 133 | en_US |
dc.relation.firstpage | 63 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.numberofauthors | 12 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | FRA | en_US |
dc.contributor.country | DEU | 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...63H | 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.fulltext | With Fulltext | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
crisitem.journal.journalissn | 0032-0633 | - |
crisitem.journal.ance | E132431 | - |
crisitem.author.dept | O.A. Capodimonte | - |
crisitem.author.orcid | 0000-0001-6461-5803 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
PSS_2015_99_Original_V0.pdf | preprint | 1.11 MB | Adobe PDF | View/Open |
Planetary SS-main.pdf | [Administrators only] | 1.74 MB | Adobe PDF |
Page view(s)
60
checked on Aug 7, 2024
Download(s)
41
checked on Aug 7, 2024
Google ScholarTM
Check
Altmetric
Altmetric
Items in DSpace are published in Open Access, unless otherwise indicated.