FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2966091027> ?p ?o ?g. }

• W2966091027 endingPage "20180404" @default.
• W2966091027 startingPage "20180404" @default.
• W2966091027 abstract "Thirty years of observations of <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML overflow=scroll> <mml:msup> <mml:mrow> <mml:msub> <mml:mrow> <mml:mi mathvariant=normal>H</mml:mi> </mml:mrow> <mml:mn>3</mml:mn> </mml:msub> </mml:mrow> <mml:mo>+</mml:mo> </mml:msup> </mml:math> on Jupiter have addressed many complex questions about the physics of the ionospheres of the giant planets. Spectroscopy, imaging and imaging spectroscopy in the infrared have allowed investigators to retrieve fundamental parameters of the ionosphere, overcoming the inherent limitations and complexities in radiative transfer, and these results are now introduced as model constraints for upper atmospheric structure and dynamics. This paper will focus on the mid-latitude emissions, which are fainter and less well studied than the auroral regions. A new analysis of VLT/ISAAC spectral imaging observations of Jupiter obtained in 2000 at 3.5 µm is presented and discussed in comparison with previous observations to show the spatial distribution of <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML overflow=scroll> <mml:msup> <mml:mrow> <mml:msub> <mml:mrow> <mml:mi mathvariant=normal>H</mml:mi> </mml:mrow> <mml:mn>3</mml:mn> </mml:msub> </mml:mrow> <mml:mo>+</mml:mo> </mml:msup> </mml:math> emissions compared with other atmospheric structures. Cylindrical maps of Jupiter in three different selected wavelengths show the spatial variations at different altitudes in the atmosphere, from cloud level up to the ionosphere. Evidence for fluctuations in the <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML overflow=scroll> <mml:msup> <mml:mrow> <mml:msub> <mml:mrow> <mml:mi mathvariant=normal>H</mml:mi> </mml:mrow> <mml:mn>3</mml:mn> </mml:msub> </mml:mrow> <mml:mo>+</mml:mo> </mml:msup> </mml:math> emissions could be due to the presence of stationary or dynamic processes. If the exact origin of these phenomena remains unidentified, several plausible mechanisms are proposed to explain the observed energy deposition and variability: future observation campaigns should deepen the understanding of these complex phenomena, in order to prepare for the future ESA/JUICE mission. This article is part of a discussion meeting issue ‘Advances in hydrogen molecular ions: H 3 + , H 5 + and beyond’." @default.
• W2966091027 created "2019-08-13" @default.
• W2966091027 creator A5067157184 @default.
• W2966091027 date "2019-08-05" @default.
• W2966091027 modified "2023-10-01" @default.
• W2966091027 title "H ₃ ⁺ as an ionospheric sounder of Jupiter and giant planets: an observational perspective" @default.
• W2966091027 cites W1870603923 @default.
• W2966091027 cites W1897164622 @default.
• W2966091027 cites W1954826965 @default.
• W2966091027 cites W1965972466 @default.
• W2966091027 cites W1969259093 @default.
• W2966091027 cites W1977185101 @default.
• W2966091027 cites W1988055306 @default.
• W2966091027 cites W1990441425 @default.
• W2966091027 cites W2007247150 @default.
• W2966091027 cites W2009481673 @default.
• W2966091027 cites W2010469137 @default.
• W2966091027 cites W2029394232 @default.
• W2966091027 cites W2029965200 @default.
• W2966091027 cites W2030218971 @default.
• W2966091027 cites W2033705551 @default.
• W2966091027 cites W2051928257 @default.
• W2966091027 cites W2063071793 @default.
• W2966091027 cites W2072198384 @default.
• W2966091027 cites W2076086044 @default.
• W2966091027 cites W2076672119 @default.
• W2966091027 cites W2084945420 @default.
• W2966091027 cites W2105492798 @default.
• W2966091027 cites W2123610080 @default.
• W2966091027 cites W2124154663 @default.
• W2966091027 cites W2125980008 @default.
• W2966091027 cites W2132561589 @default.
• W2966091027 cites W2136557798 @default.
• W2966091027 cites W2144681641 @default.
• W2966091027 cites W2164928505 @default.
• W2966091027 cites W2166261872 @default.
• W2966091027 cites W2170406859 @default.
• W2966091027 cites W2187387147 @default.
• W2966091027 cites W2476409102 @default.
• W2966091027 cites W2555801519 @default.
• W2966091027 cites W2619064320 @default.
• W2966091027 cites W2619827786 @default.
• W2966091027 cites W2836358272 @default.
• W2966091027 cites W2884502082 @default.
• W2966091027 cites W2892338809 @default.
• W2966091027 cites W2965754498 @default.
• W2966091027 cites W2966167257 @default.
• W2966091027 cites W2966875035 @default.
• W2966091027 cites W3100758839 @default.
• W2966091027 doi "https://doi.org/10.1098/rsta.2018.0404" @default.
• W2966091027 hasPubMedCentralId "https://www.ncbi.nlm.nih.gov/pmc/articles/6710887" @default.
• W2966091027 hasPubMedId "https://pubmed.ncbi.nlm.nih.gov/31378186" @default.
• W2966091027 hasPublicationYear "2019" @default.
• W2966091027 type Work @default.
• W2966091027 sameAs 2966091027 @default.
• W2966091027 citedByCount "4" @default.
• W2966091027 countsByYear W29660910272019 @default.
• W2966091027 countsByYear W29660910272020 @default.
• W2966091027 countsByYear W29660910272022 @default.
• W2966091027 crossrefType "journal-article" @default.
• W2966091027 hasAuthorship W2966091027A5067157184 @default.
• W2966091027 hasBestOaLocation W29660910271 @default.
• W2966091027 hasConcept C106125477 @default.
• W2966091027 hasConcept C11413529 @default.
• W2966091027 hasConcept C121332964 @default.
• W2966091027 hasConcept C127313418 @default.
• W2966091027 hasConcept C1276947 @default.
• W2966091027 hasConcept C22268893 @default.
• W2966091027 hasConcept C41008148 @default.
• W2966091027 hasConceptScore W2966091027C106125477 @default.
• W2966091027 hasConceptScore W2966091027C11413529 @default.
• W2966091027 hasConceptScore W2966091027C121332964 @default.
• W2966091027 hasConceptScore W2966091027C127313418 @default.
• W2966091027 hasConceptScore W2966091027C1276947 @default.
• W2966091027 hasConceptScore W2966091027C22268893 @default.
• W2966091027 hasConceptScore W2966091027C41008148 @default.
• W2966091027 hasIssue "2154" @default.
• W2966091027 hasLocation W29660910271 @default.
• W2966091027 hasLocation W296609102710 @default.
• W2966091027 hasLocation W29660910272 @default.
• W2966091027 hasLocation W29660910273 @default.
• W2966091027 hasLocation W29660910274 @default.
• W2966091027 hasLocation W29660910275 @default.
• W2966091027 hasLocation W29660910276 @default.
• W2966091027 hasLocation W29660910277 @default.
• W2966091027 hasLocation W29660910278 @default.
• W2966091027 hasLocation W29660910279 @default.
• W2966091027 hasOpenAccess W2966091027 @default.
• W2966091027 hasPrimaryLocation W29660910271 @default.
• W2966091027 hasRelatedWork W2271181815 @default.
• W2966091027 hasRelatedWork W2902782467 @default.
• W2966091027 hasRelatedWork W2935759653 @default.
• W2966091027 hasRelatedWork W3105167352 @default.
• W2966091027 hasRelatedWork W3148032049 @default.
• W2966091027 hasRelatedWork W54078636 @default.
• W2966091027 hasRelatedWork W1501425562 @default.
• W2966091027 hasRelatedWork W2298861036 @default.
• W2966091027 hasRelatedWork W2954470139 @default.

• next