FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2904308259> ?p ?o ?g. }

• W2904308259 endingPage "563" @default.
• W2904308259 startingPage "550" @default.
• W2904308259 abstract "Recent analysis of Gemini-North/NIFS H-band (1.45–1.8 µm) observations of Uranus, recorded in 2010, with recently updated line data has revealed the spectral signature of hydrogen sulphide (H2S) in Uranus’s atmosphere (Irwin et al., 2018). Here, we extend this analysis to Gemini-North/NIFS observations of Neptune recorded in 2009 and find a similar detection of H2S spectral absorption features in the 1.57–1.58 µm range, albeit slightly less evident, and retrieve a mole fraction of ∼1−3 ppm at the cloud tops. We find a much clearer detection (and much higher retrieved column abundance above the clouds) at southern polar latitudes compared with equatorial latitudes, which suggests a higher relative humidity of H2S here. We find our retrieved H2S abundances are most consistent with atmospheric models that have reduced methane abundance near Neptune’s south pole, consistent with HST/STIS determinations (Karkoschka and Tomasko, 2011). We also conducted a Principal Component Analysis (PCA) of the Neptune and Uranus data and found that in the 1.57–1.60 µm range, some of the Empirical Orthogonal Functions (EOFs) mapped closely to physically significant quantities, with one being strongly correlated with the modelled H2S signal and clearly mapping the spatial dependence of its spectral detectability. Just as for Uranus, the detection of H2S at the cloud tops constrains the deep bulk sulphur/nitrogen abundance to exceed unity (i.e. >4.4−5.0 times the solar value) in Neptune’s bulk atmosphere, provided that ammonia is not sequestered at great depths, and places a lower limit on its mole fraction below the observed cloud of (0.4–1.3) ×10−5. The detection of gaseous H2S at these pressure levels adds to the weight of evidence that the principal constituent of the 2.5–3.5 bar cloud is likely to be H2S ice." @default.
• W2904308259 created "2018-12-22" @default.
• W2904308259 creator A5012555749 @default.
• W2904308259 creator A5042720670 @default.
• W2904308259 creator A5043417117 @default.
• W2904308259 creator A5046845566 @default.
• W2904308259 creator A5050530413 @default.
• W2904308259 creator A5058653937 @default.
• W2904308259 creator A5081508890 @default.
• W2904308259 date "2019-03-01" @default.
• W2904308259 modified "2023-09-30" @default.
• W2904308259 title "Probable detection of hydrogen sulphide (H2S) in Neptune’s atmosphere" @default.
• W2904308259 cites W1490136218 @default.
• W2904308259 cites W1674795780 @default.
• W2904308259 cites W1964772605 @default.
• W2904308259 cites W1964787845 @default.
• W2904308259 cites W1966730814 @default.
• W2904308259 cites W1988708372 @default.
• W2904308259 cites W1996277899 @default.
• W2904308259 cites W2001982438 @default.
• W2904308259 cites W2005007711 @default.
• W2904308259 cites W2008126355 @default.
• W2904308259 cites W2011951131 @default.
• W2904308259 cites W2014572895 @default.
• W2904308259 cites W2016151600 @default.
• W2904308259 cites W2025427999 @default.
• W2904308259 cites W2035203343 @default.
• W2904308259 cites W2045570539 @default.
• W2904308259 cites W2053656335 @default.
• W2904308259 cites W2059756096 @default.
• W2904308259 cites W2059897684 @default.
• W2904308259 cites W2062625349 @default.
• W2904308259 cites W2069582232 @default.
• W2904308259 cites W2090068249 @default.
• W2904308259 cites W2092028504 @default.
• W2904308259 cites W2112399522 @default.
• W2904308259 cites W2127992393 @default.
• W2904308259 cites W2165030930 @default.
• W2904308259 cites W2268685673 @default.
• W2904308259 cites W2343092005 @default.
• W2904308259 cites W2799823195 @default.
• W2904308259 cites W4206050372 @default.
• W2904308259 cites W4235319851 @default.
• W2904308259 doi "https://doi.org/10.1016/j.icarus.2018.12.014" @default.
• W2904308259 hasPublicationYear "2019" @default.
• W2904308259 type Work @default.
• W2904308259 sameAs 2904308259 @default.
• W2904308259 citedByCount "44" @default.
• W2904308259 countsByYear W29043082592019 @default.
• W2904308259 countsByYear W29043082592020 @default.
• W2904308259 countsByYear W29043082592021 @default.
• W2904308259 countsByYear W29043082592022 @default.
• W2904308259 countsByYear W29043082592023 @default.
• W2904308259 crossrefType "journal-article" @default.
• W2904308259 hasAuthorship W2904308259A5012555749 @default.
• W2904308259 hasAuthorship W2904308259A5042720670 @default.
• W2904308259 hasAuthorship W2904308259A5043417117 @default.
• W2904308259 hasAuthorship W2904308259A5046845566 @default.
• W2904308259 hasAuthorship W2904308259A5050530413 @default.
• W2904308259 hasAuthorship W2904308259A5058653937 @default.
• W2904308259 hasAuthorship W2904308259A5081508890 @default.
• W2904308259 hasBestOaLocation W29043082594 @default.
• W2904308259 hasConcept C121332964 @default.
• W2904308259 hasConcept C122523270 @default.
• W2904308259 hasConcept C1276947 @default.
• W2904308259 hasConcept C153294291 @default.
• W2904308259 hasConcept C2780114079 @default.
• W2904308259 hasConcept C39432304 @default.
• W2904308259 hasConcept C44870925 @default.
• W2904308259 hasConcept C51244244 @default.
• W2904308259 hasConcept C525488444 @default.
• W2904308259 hasConcept C65440619 @default.
• W2904308259 hasConcept C91586092 @default.
• W2904308259 hasConceptScore W2904308259C121332964 @default.
• W2904308259 hasConceptScore W2904308259C122523270 @default.
• W2904308259 hasConceptScore W2904308259C1276947 @default.
• W2904308259 hasConceptScore W2904308259C153294291 @default.
• W2904308259 hasConceptScore W2904308259C2780114079 @default.
• W2904308259 hasConceptScore W2904308259C39432304 @default.
• W2904308259 hasConceptScore W2904308259C44870925 @default.
• W2904308259 hasConceptScore W2904308259C51244244 @default.
• W2904308259 hasConceptScore W2904308259C525488444 @default.
• W2904308259 hasConceptScore W2904308259C65440619 @default.
• W2904308259 hasConceptScore W2904308259C91586092 @default.
• W2904308259 hasFunder F4320335254 @default.
• W2904308259 hasLocation W29043082591 @default.
• W2904308259 hasLocation W29043082592 @default.
• W2904308259 hasLocation W29043082593 @default.
• W2904308259 hasLocation W29043082594 @default.
• W2904308259 hasLocation W29043082595 @default.
• W2904308259 hasLocation W29043082596 @default.
• W2904308259 hasLocation W29043082597 @default.
• W2904308259 hasLocation W29043082598 @default.
• W2904308259 hasLocation W29043082599 @default.
• W2904308259 hasOpenAccess W2904308259 @default.
• W2904308259 hasPrimaryLocation W29043082591 @default.
• W2904308259 hasRelatedWork W1499149823 @default.
• W2904308259 hasRelatedWork W186254715 @default.

• next