Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/26859
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Sindoni, G. | en_US |
dc.contributor.author | GRASSI, Davide | en_US |
dc.contributor.author | ADRIANI, Alberto | en_US |
dc.contributor.author | MURA, Alessandro | en_US |
dc.contributor.author | Moriconi, M. L. | en_US |
dc.contributor.author | Dinelli, B. M. | en_US |
dc.contributor.author | FILACCHIONE, GIANRICO | en_US |
dc.contributor.author | TOSI, Federico | en_US |
dc.contributor.author | PICCIONI, GIUSEPPE | en_US |
dc.contributor.author | MIGLIORINI, Alessandra | en_US |
dc.contributor.author | ALTIERI, FRANCESCA | en_US |
dc.contributor.author | Fabiano, F. | en_US |
dc.contributor.author | TURRINI, Diego | en_US |
dc.contributor.author | NOSCHESE, RAFFAELLA | en_US |
dc.contributor.author | CICCHETTI, ANDREA | en_US |
dc.contributor.author | STEFANI, STEFANIA | en_US |
dc.contributor.author | Bolton, S. J. | en_US |
dc.contributor.author | Connerney, J. E. P. | en_US |
dc.contributor.author | Atreya, S. K. | en_US |
dc.contributor.author | Bagenal, F. | en_US |
dc.contributor.author | Hansen, C. | en_US |
dc.contributor.author | Ingersoll, A. | en_US |
dc.contributor.author | Janssen, M. | en_US |
dc.contributor.author | Levin, S. M. | en_US |
dc.contributor.author | Lunine, J. I. | en_US |
dc.contributor.author | Orton, G. | en_US |
dc.contributor.author | Olivieri, A. | en_US |
dc.contributor.author | Amoroso, M. | en_US |
dc.date.accessioned | 2020-08-27T09:07:58Z | - |
dc.date.available | 2020-08-27T09:07:58Z | - |
dc.date.issued | 2017 | en_US |
dc.identifier.issn | 0094-8276 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/26859 | - |
dc.description.abstract | During the first perijove passage of the Juno mission, the Jovian InfraRed Auroral Mapper (JIRAM) observed a line of closely spaced oval features in Jupiter's southern hemisphere, between 30°S and 45°S. In this work, we focused on the longitudinal region covering the three ovals having higher contrast at 5 μm, i.e., between 120°W and 60°W in System III coordinates. We used the JIRAM's full spectral capability in the range 2.4-3 μm together with a Bayesian data inversion approach to retrieve maps of column densities and altitudes for an NH<SUB>3</SUB> cloud and an N<SUB>2</SUB>H<SUB>4</SUB> haze. The deep (under the saturation level) volume mixing ratio and the relative humidity for gaseous ammonia were also retrieved. Our results suggest different vortex activity for the three ovals. Updraft and downdraft together with considerations about the ammonia condensation could explain our maps providing evidences of cyclonic and anticyclonic structures. <P /> | en_US |
dc.language.iso | eng | en_US |
dc.title | Characterization of the white ovals on Jupiter's southern hemisphere using the first data by the Juno/JIRAM instrument | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1002/2017GL072940 | en_US |
dc.identifier.scopus | 2-s2.0-85019854814 | en_US |
dc.identifier.isi | 000404131900034 | en_US |
dc.identifier.url | https://agupubs.onlinelibrary.wiley.com/doi/full/10.1002/2017GL072940 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 44 | en_US |
dc.relation.issue | 10 | en_US |
dc.relation.firstpage | 4660 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | USA | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | GEOPHYSICAL RESEARCH LETTERS | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2017GeoRL..44.4660S | 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 | embargo_21200713 | - |
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.dept | IAPS Roma | - |
crisitem.author.dept | IAPS Roma | - |
crisitem.author.dept | IAPS Roma | - |
crisitem.author.dept | O.A. Torino | - |
crisitem.author.dept | IAPS Roma | - |
crisitem.author.dept | IAPS Roma | - |
crisitem.author.dept | IAPS Roma | - |
crisitem.author.orcid | 0000-0003-1653-3066 | - |
crisitem.author.orcid | 0000-0003-4998-8008 | - |
crisitem.author.orcid | 0000-0002-4552-4292 | - |
crisitem.author.orcid | 0000-0001-9567-0055 | - |
crisitem.author.orcid | 0000-0003-4002-2434 | - |
crisitem.author.orcid | 0000-0002-7893-6808 | - |
crisitem.author.orcid | 0000-0001-7386-9215 | - |
crisitem.author.orcid | 0000-0002-6338-8300 | - |
crisitem.author.orcid | 0000-0002-1923-7740 | - |
crisitem.author.orcid | 0000-0003-0502-0337 | - |
crisitem.author.orcid | 0000-0002-9588-6531 | - |
crisitem.author.orcid | 0000-0001-5762-4947 | - |
crisitem.journal.journalissn | 0094-8276 | - |
crisitem.journal.ance | E070238 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | Existing users please |
---|---|---|---|---|
Sindoni_et_al-2017-Geophysical_Research_Letters.pdf | Editorial PDF | 963.24 kB | Adobe PDF | Embargoed until July 13, 2120 |
804674_1_merged_1490802517_small.pdf | postprint | 1.56 MB | Adobe PDF | View/Open |
Page view(s)
105
checked on Apr 26, 2024
Download(s)
20
checked on Apr 26, 2024
Google ScholarTM
Check
Altmetric
Altmetric
Items in DSpace are published in Open Access, unless otherwise indicated.