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Author Correction: Evidence for auroral influence on Jupiter’s nitrogen and oxygen chemistry revealed by ALMA

hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
hal.structure.identifierLaboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics [LESIA]
dc.contributor.authorCAVALIÉ, T
hal.structure.identifierMax-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research [MPS]
dc.contributor.authorREZAC, L
hal.structure.identifierLaboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics [LESIA]
dc.contributor.authorMORENO, R
hal.structure.identifierLaboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics [LESIA]
dc.contributor.authorLELLOUCH, E
hal.structure.identifierPôle Planétologie du LESIA
hal.structure.identifierLaboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics [LESIA]
dc.contributor.authorFOUCHET, T
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
dc.contributor.authorBENMAHI, B
hal.structure.identifierSouthwest Research Institute [San Antonio] [SwRI]
dc.contributor.authorGREATHOUSE, T.
hal.structure.identifierJet Propulsion Laboratory [JPL]
dc.contributor.authorSINCLAIR, J
hal.structure.identifierSouthwest Research Institute [San Antonio] [SwRI]
dc.contributor.authorHUE, V
hal.structure.identifierMax-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research [MPS]
dc.contributor.authorHARTOGH, P
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
dc.contributor.authorDOBRIJEVIC, M
hal.structure.identifierPLANETO - LATMOS
dc.contributor.authorCARRASCO, Nathalie
hal.structure.identifierPLANETO - LATMOS
dc.contributor.authorPERRIN, Zoé
dc.date.issued2024-08-02
dc.description.abstractEn<div><p>In the version of the article originally published, all column density values were a factor of 10 too low. Consequently, "two orders" has been changed to "one order" in the abstract and the text, and the values have been corrected on the y axes of Fig. 3 and the color scales in Fig. 4. In addition, in the section "The spatial distribution of CO and HCN", the CO and HCN masses reported in the text were a factor of 10 too low and the loss factors for CO and HCN were a factor of 10 too high; they have been corrected accordingly. Specifically, CO is now shown to have a meridionally uniform column density of 1.86 ± 0.52 × 10 16 cm -2 and the total mass of SL9-derived CO is 5.47 ± 0.26 × 10 14 g. This corresponds to a loss factor of 0.9 ± 0.3 since 1995-1998. HCN has a uniform column density of 22.6 ± 5.7 × 10 13 cm -2 , which is one order of magnitude lower than that measured 6.5 years after the SL9 impacts. The total mass of HCN is 5.0 ± 0.1 × 10 12 g. This corresponds to a loss factor of 5.0 ± 3.0 when compared with the 1995-1998 period, or 12.0 ± 3.5 when compared with the value derived in 2000 from the Cassini flyby data. The conclusions of the paper remain unchanged.</p></div>
dc.language.isoen
dc.publisherNature Publishing Group
dc.titleAuthor Correction: Evidence for auroral influence on Jupiter’s nitrogen and oxygen chemistry revealed by ALMA
dc.typeArticle de revue
dc.identifier.doi10.1038/s41550-024-02348-y
dc.subject.halPlanète et Univers [physics]
bordeaux.journalNature Astronomy
bordeaux.page1206
bordeaux.volume8
bordeaux.peerReviewedoui
hal.identifierinsu-04764081
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//insu-04764081v1
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