FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W1516670254> ?p ?o ?g. }

• W1516670254 endingPage "5442" @default.
• W1516670254 startingPage "5432" @default.
• W1516670254 abstract "Abstract Observations of Mercury's local plasma environment by MErcury Surface, Space ENvironment, GEochemistry, and Ranging have revealed that the planet hosts a strongly asymmetric magnetosphere as a result of an off‐axis dipolar or quadrupolar internal field and significant finite Larmor radius effects at the boundary layer between magnetospheric and solar wind plasma environments. One important asymmetry appears in the growth and evolution of Kelvin‐Helmholtz (K‐H) waves at the dawn and dusk flanks of the magnetopause. Linear analysis and global hybrid simulations support a dusk‐dawn asymmetry in the growth rate caused by finite Larmor radius effects, and indeed, K‐H waves have been almost exclusively observed at the dusk magnetopause during northward interplanetary magnetic field. Observations of these K‐H waves at sodium gyroscales invite investigation into the impact of the hot planetary sodium ion population, itself distributed preferentially on the dusk flank, on the growth of the K‐H instability and associated plasma transport. We present local two‐dimensional hybrid simulations of the dusk and dawn boundary layers, with varying magnetospheric sodium ion number density, and examine the associated changes in the growth rates of the K‐H instability, K‐H wave spectra, and cross‐boundary particle transport. We show that gyroresonance between growing K‐H vortices and sodium ion gyration introduces a strong spectral peak at sodium gyroscales at the dusk magnetopause, that an increase in sodium ion number density increases dawn‐dusk asymmetry of K‐H growth rates, and that cross‐boundary particle transport decreases with sodium number density at the dawn flank." @default.
• W1516670254 created "2016-06-24" @default.
• W1516670254 creator A5030726035 @default.
• W1516670254 creator A5061122430 @default.
• W1516670254 creator A5062739432 @default.
• W1516670254 date "2015-07-01" @default.
• W1516670254 modified "2023-10-16" @default.
• W1516670254 title "The impact of a hot sodium ion population on the growth of the Kelvin‐Helmholtz instability in Mercury's magnetotail" @default.
• W1516670254 cites W1580553785 @default.
• W1516670254 cites W1638181329 @default.
• W1516670254 cites W1686505431 @default.
• W1516670254 cites W1880663918 @default.
• W1516670254 cites W1965489224 @default.
• W1516670254 cites W1968282221 @default.
• W1516670254 cites W1982984662 @default.
• W1516670254 cites W1988970979 @default.
• W1516670254 cites W1990386529 @default.
• W1516670254 cites W1991760079 @default.
• W1516670254 cites W1992823225 @default.
• W1516670254 cites W1993648813 @default.
• W1516670254 cites W2016559669 @default.
• W1516670254 cites W2017397770 @default.
• W1516670254 cites W2018481961 @default.
• W1516670254 cites W2022328357 @default.
• W1516670254 cites W2023919031 @default.
• W1516670254 cites W2032357757 @default.
• W1516670254 cites W2033866694 @default.
• W1516670254 cites W2038136343 @default.
• W1516670254 cites W2040269907 @default.
• W1516670254 cites W2041318119 @default.
• W1516670254 cites W2041551771 @default.
• W1516670254 cites W2042954659 @default.
• W1516670254 cites W2045388333 @default.
• W1516670254 cites W2065379860 @default.
• W1516670254 cites W2065700915 @default.
• W1516670254 cites W2070444152 @default.
• W1516670254 cites W2071385422 @default.
• W1516670254 cites W2074670978 @default.
• W1516670254 cites W2085960116 @default.
• W1516670254 cites W2087102345 @default.
• W1516670254 cites W2089527981 @default.
• W1516670254 cites W2096969439 @default.
• W1516670254 cites W2153790431 @default.
• W1516670254 cites W2164639749 @default.
• W1516670254 cites W4236162395 @default.
• W1516670254 doi "https://doi.org/10.1002/2015ja021433" @default.
• W1516670254 hasPublicationYear "2015" @default.
• W1516670254 type Work @default.
• W1516670254 sameAs 1516670254 @default.
• W1516670254 citedByCount "6" @default.
• W1516670254 countsByYear W15166702542015 @default.
• W1516670254 countsByYear W15166702542017 @default.
• W1516670254 countsByYear W15166702542018 @default.
• W1516670254 countsByYear W15166702542019 @default.
• W1516670254 countsByYear W15166702542020 @default.
• W1516670254 crossrefType "journal-article" @default.
• W1516670254 hasAuthorship W1516670254A5030726035 @default.
• W1516670254 hasAuthorship W1516670254A5061122430 @default.
• W1516670254 hasAuthorship W1516670254A5062739432 @default.
• W1516670254 hasBestOaLocation W15166702541 @default.
• W1516670254 hasConcept C108411613 @default.
• W1516670254 hasConcept C115260700 @default.
• W1516670254 hasConcept C121332964 @default.
• W1516670254 hasConcept C130443932 @default.
• W1516670254 hasConcept C134581325 @default.
• W1516670254 hasConcept C140161248 @default.
• W1516670254 hasConcept C144024400 @default.
• W1516670254 hasConcept C149923435 @default.
• W1516670254 hasConcept C154959693 @default.
• W1516670254 hasConcept C184779094 @default.
• W1516670254 hasConcept C207821765 @default.
• W1516670254 hasConcept C2908647359 @default.
• W1516670254 hasConcept C30475298 @default.
• W1516670254 hasConcept C57879066 @default.
• W1516670254 hasConcept C61922881 @default.
• W1516670254 hasConcept C62520636 @default.
• W1516670254 hasConcept C8058405 @default.
• W1516670254 hasConcept C91571402 @default.
• W1516670254 hasConceptScore W1516670254C108411613 @default.
• W1516670254 hasConceptScore W1516670254C115260700 @default.
• W1516670254 hasConceptScore W1516670254C121332964 @default.
• W1516670254 hasConceptScore W1516670254C130443932 @default.
• W1516670254 hasConceptScore W1516670254C134581325 @default.
• W1516670254 hasConceptScore W1516670254C140161248 @default.
• W1516670254 hasConceptScore W1516670254C144024400 @default.
• W1516670254 hasConceptScore W1516670254C149923435 @default.
• W1516670254 hasConceptScore W1516670254C154959693 @default.
• W1516670254 hasConceptScore W1516670254C184779094 @default.
• W1516670254 hasConceptScore W1516670254C207821765 @default.
• W1516670254 hasConceptScore W1516670254C2908647359 @default.
• W1516670254 hasConceptScore W1516670254C30475298 @default.
• W1516670254 hasConceptScore W1516670254C57879066 @default.
• W1516670254 hasConceptScore W1516670254C61922881 @default.
• W1516670254 hasConceptScore W1516670254C62520636 @default.
• W1516670254 hasConceptScore W1516670254C8058405 @default.
• W1516670254 hasConceptScore W1516670254C91571402 @default.
• W1516670254 hasFunder F4320334632 @default.
• W1516670254 hasIssue "7" @default.

• next