Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/27504
DC Field | Value | Language |
---|---|---|
dc.contributor.author | MIGLIORINI, Alessandra | en_US |
dc.contributor.author | Snels, M. | en_US |
dc.contributor.author | Gérard, J. -C. | en_US |
dc.contributor.author | Soret, L. | en_US |
dc.contributor.author | PICCIONI, GIUSEPPE | en_US |
dc.contributor.author | Drossart, P. | en_US |
dc.date.accessioned | 2020-09-29T07:14:06Z | - |
dc.date.available | 2020-09-29T07:14:06Z | - |
dc.date.issued | 2018 | en_US |
dc.identifier.issn | 0019-1035 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/27504 | - |
dc.description.abstract | The temperature of the night side of Venus at about 95 km has been determined by using spectral features of the hydroxyl airglow emission around 3 μm, recorded from July 2006 to July 2008 by VIRTIS onboard Venus Express. The retrieved temperatures vary from 145.5 to about 198.1 K with an average value of 176.3 ± 14.3 K and are in good agreement with previous ground-based and space observations. The variability with respect to latitude and local time has been studied, showing a minimum of temperature at equatorial latitudes, while temperature values increase toward mid latitudes with a local maximum at about 35°N. The present work provides an independent contribution to the temperature estimation in the transition region between the Venus upper mesosphere and the lower thermosphere, by using the OH emission as a thermometer, following the technique previously applied to the high-resolution O<SUB>2</SUB>(a<SUP>1</SUP>∆<SUB>g</SUB>) airglow emissions observed from ground. | en_US |
dc.language.iso | eng | en_US |
dc.title | Temperature estimation from hydroxyl airglow emission in the Venus night side mesosphere | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1016/j.icarus.2017.09.026 | en_US |
dc.identifier.scopus | 2-s2.0-85032636345 | en_US |
dc.identifier.isi | 000414507300027 | en_US |
dc.identifier.url | https://www.sciencedirect.com/science/article/pii/S0019103517303937?via%3Dihub | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 300 | en_US |
dc.relation.firstpage | 386 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | FRA | en_US |
dc.contributor.country | BEL | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | ICARUS | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2018Icar..300..386M | 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.dept | IAPS Roma | - |
crisitem.author.dept | IAPS Roma | - |
crisitem.author.orcid | 0000-0001-7386-9215 | - |
crisitem.author.orcid | 0000-0002-7893-6808 | - |
crisitem.journal.journalissn | 0019-1035 | - |
crisitem.journal.ance | E079353 | - |
Appears in Collections: | 1.01 Articoli in rivista |
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File | Description | Size | Format | Existing users please |
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1-s2.0-S0019103517303937-main.pdf | [Administrators only] | 1.19 MB | Adobe PDF |
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