FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2141481397> ?p ?o ?g. }

• W2141481397 endingPage "638" @default.
• W2141481397 startingPage "632" @default.
• W2141481397 abstract "The Mariner 10 observations established the presence of a magnetosphere at Mercury with general characteristics similar to that of the Earth despite a much smaller size (i.e., magnetic dipole strength) and the absence of an atmosphere–ionosphere. Observationally, a mapping between the terrestrial and hermean magnetospheric regions has been made which entails increasing the size of the planet by a factor of 8. Recently, we have used the results of global hybrid (kinetic ions, fluid electrons) simulations of solar wind interaction with magnetic dipoles of varying strength to show the existence of a spectrum of magnetospheric structures whose size and level of complexity increases with the dipole moment. A physical parameter which helps characterize these magnetospheres is Dp, the distance ahead of the dipole where the magnetic field pressure balances the solar wind dynamic pressure. Expressed in units of ion skin depth, when Dp ∼ > 20 the interaction results in the formation of an earthlike magnetosphere. Thus, the magnetosphere of Mercury with Dp ∼ 65 should resemble that of the Earth. However, not all magnetospheric processes in Dp > 20 magnetospheres are guaranteed to be alike and possess the same spatial and temporal scales. In this paper, we use the results of global hybrid simulations, corresponding to Dp = 64, to examine the nature of the boundaries and discontinuities at the hermean magnetosphere and how they compare with the corresponding regions at the Earth." @default.
• W2141481397 created "2016-06-24" @default.
• W2141481397 creator A5005826888 @default.
• W2141481397 creator A5011650421 @default.
• W2141481397 creator A5033240665 @default.
• W2141481397 creator A5068397336 @default.
• W2141481397 date "2006-01-01" @default.
• W2141481397 modified "2023-10-16" @default.
• W2141481397 title "Global hybrid simulations of solar wind interaction with Mercury: Magnetosperic boundaries" @default.
• W2141481397 cites W1963815219 @default.
• W2141481397 cites W1972773689 @default.
• W2141481397 cites W1977232747 @default.
• W2141481397 cites W1985323234 @default.
• W2141481397 cites W1994032628 @default.
• W2141481397 cites W1996799499 @default.
• W2141481397 cites W2002359795 @default.
• W2141481397 cites W2029446784 @default.
• W2141481397 cites W2030324490 @default.
• W2141481397 cites W2034686001 @default.
• W2141481397 cites W2047239219 @default.
• W2141481397 cites W2051145965 @default.
• W2141481397 cites W2057642100 @default.
• W2141481397 cites W2061321567 @default.
• W2141481397 cites W2070804593 @default.
• W2141481397 cites W2074666301 @default.
• W2141481397 cites W2078257974 @default.
• W2141481397 cites W2081391399 @default.
• W2141481397 cites W2169863169 @default.
• W2141481397 doi "https://doi.org/10.1016/j.asr.2005.11.019" @default.
• W2141481397 hasPublicationYear "2006" @default.
• W2141481397 type Work @default.
• W2141481397 sameAs 2141481397 @default.
• W2141481397 citedByCount "21" @default.
• W2141481397 countsByYear W21414813972012 @default.
• W2141481397 countsByYear W21414813972013 @default.
• W2141481397 countsByYear W21414813972014 @default.
• W2141481397 countsByYear W21414813972015 @default.
• W2141481397 countsByYear W21414813972016 @default.
• W2141481397 countsByYear W21414813972017 @default.
• W2141481397 countsByYear W21414813972019 @default.
• W2141481397 countsByYear W21414813972022 @default.
• W2141481397 crossrefType "journal-article" @default.
• W2141481397 hasAuthorship W2141481397A5005826888 @default.
• W2141481397 hasAuthorship W2141481397A5011650421 @default.
• W2141481397 hasAuthorship W2141481397A5033240665 @default.
• W2141481397 hasAuthorship W2141481397A5068397336 @default.
• W2141481397 hasConcept C102988692 @default.
• W2141481397 hasConcept C108411613 @default.
• W2141481397 hasConcept C115260700 @default.
• W2141481397 hasConcept C116403925 @default.
• W2141481397 hasConcept C121332964 @default.
• W2141481397 hasConcept C130443932 @default.
• W2141481397 hasConcept C134306372 @default.
• W2141481397 hasConcept C140161248 @default.
• W2141481397 hasConcept C15627037 @default.
• W2141481397 hasConcept C169852918 @default.
• W2141481397 hasConcept C173523689 @default.
• W2141481397 hasConcept C175482610 @default.
• W2141481397 hasConcept C30475298 @default.
• W2141481397 hasConcept C33923547 @default.
• W2141481397 hasConcept C46567642 @default.
• W2141481397 hasConcept C62520636 @default.
• W2141481397 hasConcept C8058405 @default.
• W2141481397 hasConcept C91586092 @default.
• W2141481397 hasConceptScore W2141481397C102988692 @default.
• W2141481397 hasConceptScore W2141481397C108411613 @default.
• W2141481397 hasConceptScore W2141481397C115260700 @default.
• W2141481397 hasConceptScore W2141481397C116403925 @default.
• W2141481397 hasConceptScore W2141481397C121332964 @default.
• W2141481397 hasConceptScore W2141481397C130443932 @default.
• W2141481397 hasConceptScore W2141481397C134306372 @default.
• W2141481397 hasConceptScore W2141481397C140161248 @default.
• W2141481397 hasConceptScore W2141481397C15627037 @default.
• W2141481397 hasConceptScore W2141481397C169852918 @default.
• W2141481397 hasConceptScore W2141481397C173523689 @default.
• W2141481397 hasConceptScore W2141481397C175482610 @default.
• W2141481397 hasConceptScore W2141481397C30475298 @default.
• W2141481397 hasConceptScore W2141481397C33923547 @default.
• W2141481397 hasConceptScore W2141481397C46567642 @default.
• W2141481397 hasConceptScore W2141481397C62520636 @default.
• W2141481397 hasConceptScore W2141481397C8058405 @default.
• W2141481397 hasConceptScore W2141481397C91586092 @default.
• W2141481397 hasIssue "4" @default.
• W2141481397 hasLocation W21414813971 @default.
• W2141481397 hasOpenAccess W2141481397 @default.
• W2141481397 hasPrimaryLocation W21414813971 @default.
• W2141481397 hasRelatedWork W1590033903 @default.
• W2141481397 hasRelatedWork W1967118022 @default.
• W2141481397 hasRelatedWork W1968282221 @default.
• W2141481397 hasRelatedWork W2015414622 @default.
• W2141481397 hasRelatedWork W2067550403 @default.
• W2141481397 hasRelatedWork W2069979540 @default.
• W2141481397 hasRelatedWork W2114973195 @default.
• W2141481397 hasRelatedWork W2130284361 @default.
• W2141481397 hasRelatedWork W3162398580 @default.
• W2141481397 hasRelatedWork W994179962 @default.
• W2141481397 hasVolume "38" @default.
• W2141481397 isParatext "false" @default.

• next