Matches in SemOpenAlex for { <https://semopenalex.org/work/W2898039892> ?p ?o ?g. }
Showing items 1 to 84 of
84
with 100 items per page.
- W2898039892 endingPage "249" @default.
- W2898039892 startingPage "244" @default.
- W2898039892 abstract "Abstract With the arrival of the Juno spacecraft at Jupiter, assumptions regarding the tidal response of Jupiter's atmosphere need to be carefully reconsidered. This is motivated both by surprising new observations as well as the fact that Juno studies have so far been conducted largely in the absence of a tidal model or assumptions that are consistent with classical tidal theory. Estimation of fully consistent tidal response solutions is somewhat tedious and for many planetary applications simplifying assumptions regarding reduced dynamics or a quasi-static balance are justified. But Jupiter's atmosphere should not be expected to be one of these simple cases because its equatorial rotation speed of ∼12 km/s near the surface exceeds most plausible internal wave speeds (including acoustic) and predicts a dynamic tidal response out of equilibrium. The goal of this study is narrowly focused on the fundamental question—does Jupiter's atmosphere contain resonantly forced tidal states? The tidal response controls the efficiency at which spin/orbit energy is deposited in the interior. The associated power levels can be enhanced by many orders of magnitude in resonantly forced states. Here classical tidal theory and Juno observations are combined and an effort is made to separate robust conclusions from ones that depend sensitively on internal-parameter assumptions. It is shown that one should expect that there are resonantly forced tides in Jupiter, and that these amplified tides may explain the observed net energy emitted from Jupiter, astrometric observations of Io's orbit implicating high tidal dissipation, and the observed banding with a dynamical boundary near ± 50 degrees latitude." @default.
- W2898039892 created "2018-10-26" @default.
- W2898039892 creator A5040082446 @default.
- W2898039892 date "2019-01-01" @default.
- W2898039892 modified "2023-09-24" @default.
- W2898039892 title "Tidal power and banding in Jupiter" @default.
- W2898039892 cites W1982028541 @default.
- W2898039892 cites W2013043332 @default.
- W2898039892 cites W2040341447 @default.
- W2898039892 cites W2071990736 @default.
- W2898039892 cites W2089177308 @default.
- W2898039892 cites W2124785356 @default.
- W2898039892 cites W2620099545 @default.
- W2898039892 cites W2789293361 @default.
- W2898039892 cites W2791926639 @default.
- W2898039892 cites W2794048965 @default.
- W2898039892 cites W2794138887 @default.
- W2898039892 cites W2794194779 @default.
- W2898039892 doi "https://doi.org/10.1016/j.pss.2018.10.002" @default.
- W2898039892 hasPublicationYear "2019" @default.
- W2898039892 type Work @default.
- W2898039892 sameAs 2898039892 @default.
- W2898039892 citedByCount "3" @default.
- W2898039892 countsByYear W28980398922021 @default.
- W2898039892 countsByYear W28980398922022 @default.
- W2898039892 crossrefType "journal-article" @default.
- W2898039892 hasAuthorship W2898039892A5040082446 @default.
- W2898039892 hasConcept C118873486 @default.
- W2898039892 hasConcept C119599485 @default.
- W2898039892 hasConcept C121332964 @default.
- W2898039892 hasConcept C127313418 @default.
- W2898039892 hasConcept C127413603 @default.
- W2898039892 hasConcept C1276947 @default.
- W2898039892 hasConcept C163258240 @default.
- W2898039892 hasConcept C177871831 @default.
- W2898039892 hasConcept C22268893 @default.
- W2898039892 hasConcept C29829512 @default.
- W2898039892 hasConcept C39432304 @default.
- W2898039892 hasConcept C40018170 @default.
- W2898039892 hasConcept C511503438 @default.
- W2898039892 hasConcept C51244244 @default.
- W2898039892 hasConcept C8058405 @default.
- W2898039892 hasConcept C87355193 @default.
- W2898039892 hasConcept C91586092 @default.
- W2898039892 hasConcept C97355855 @default.
- W2898039892 hasConceptScore W2898039892C118873486 @default.
- W2898039892 hasConceptScore W2898039892C119599485 @default.
- W2898039892 hasConceptScore W2898039892C121332964 @default.
- W2898039892 hasConceptScore W2898039892C127313418 @default.
- W2898039892 hasConceptScore W2898039892C127413603 @default.
- W2898039892 hasConceptScore W2898039892C1276947 @default.
- W2898039892 hasConceptScore W2898039892C163258240 @default.
- W2898039892 hasConceptScore W2898039892C177871831 @default.
- W2898039892 hasConceptScore W2898039892C22268893 @default.
- W2898039892 hasConceptScore W2898039892C29829512 @default.
- W2898039892 hasConceptScore W2898039892C39432304 @default.
- W2898039892 hasConceptScore W2898039892C40018170 @default.
- W2898039892 hasConceptScore W2898039892C511503438 @default.
- W2898039892 hasConceptScore W2898039892C51244244 @default.
- W2898039892 hasConceptScore W2898039892C8058405 @default.
- W2898039892 hasConceptScore W2898039892C87355193 @default.
- W2898039892 hasConceptScore W2898039892C91586092 @default.
- W2898039892 hasConceptScore W2898039892C97355855 @default.
- W2898039892 hasFunder F4320306101 @default.
- W2898039892 hasLocation W28980398921 @default.
- W2898039892 hasOpenAccess W2898039892 @default.
- W2898039892 hasPrimaryLocation W28980398921 @default.
- W2898039892 hasRelatedWork W1619685438 @default.
- W2898039892 hasRelatedWork W1640579312 @default.
- W2898039892 hasRelatedWork W1983025269 @default.
- W2898039892 hasRelatedWork W2080878819 @default.
- W2898039892 hasRelatedWork W3014253202 @default.
- W2898039892 hasRelatedWork W3015653336 @default.
- W2898039892 hasRelatedWork W3165490869 @default.
- W2898039892 hasRelatedWork W3176769230 @default.
- W2898039892 hasRelatedWork W4210284476 @default.
- W2898039892 hasRelatedWork W4244443368 @default.
- W2898039892 hasVolume "165" @default.
- W2898039892 isParatext "false" @default.
- W2898039892 isRetracted "false" @default.
- W2898039892 magId "2898039892" @default.
- W2898039892 workType "article" @default.