Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/26954
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | Bagnulo, S. | en_US |
dc.contributor.author | Belskaya, I. | en_US |
dc.contributor.author | CELLINO, Alberto | en_US |
dc.contributor.author | Kolokolova, L. | en_US |
dc.date.accessioned | 2020-08-28T12:41:58Z | - |
dc.date.available | 2020-08-28T12:41:58Z | - |
dc.date.issued | 2017 | en_US |
dc.identifier.issn | 2190-5444 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/26954 | - |
dc.description.abstract | The large majority of astronomical observations are based on intensity measurements as a function of either wavelength or time, or both. Polarimetry, a technique which measures the way in which the electromagnetic field associated to the radiation oscillates, does provide further information about the objects that have emitted or scattered the observed radiation. For instance, polarimetric measurements can provide important constraints to the characterisation of cosmic dust (be it of interstellar or cometary origin), of the surfaces of the atmosphereless bodies and of planetary atmospheres. This property has been exploited in solar system science to study asteroids, comets, rocky and giant gaseous planets, and their satellites. In this paper we present a review of the polarimetric studies of the small bodies of the Solar System. | en_US |
dc.language.iso | eng | en_US |
dc.title | Polarimetry of small bodies and satellites of our Solar System | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1140/epjp/i2017-11690-6 | en_US |
dc.identifier.scopus | 2-s2.0-85030096129 | en_US |
dc.identifier.isi | 000412067200002 | en_US |
dc.identifier.url | https://link.springer.com/article/10.1140%2Fepjp%2Fi2017-11690-6 | en_US |
dc.relation.medium | ELETTRONICO | en_US |
dc.relation.volume | 132 | en_US |
dc.relation.issue | 9 | en_US |
dc.relation.firstpage | 405 | en_US |
dc.relation.numberofpages | 20 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.numberofauthors | 4 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | USA | en_US |
dc.contributor.country | GBR | en_US |
dc.contributor.country | UKR | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | THE EUROPEAN PHYSICAL JOURNAL PLUS | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2017EPJP..132..405B | 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::PE9_2 Planetary systems sciences | 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 | reserved | - |
item.fulltext | With Fulltext | - |
crisitem.author.orcid | 0000-0002-6645-334X | - |
crisitem.journal.journalissn | 2190-5444 | - |
crisitem.journal.ance | E204598 | - |
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