FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W1970125218> ?p ?o ?g. }

• W1970125218 endingPage "722" @default.
• W1970125218 startingPage "717" @default.
• W1970125218 abstract "Abstract. Localised depressions in the magnetic field magnitude, or magnetic holes, are common features in many regions of solar system plasma. Two distinct mechanisms for their generation have been proposed. The first proposed that the structures are generated locally, close to the point of observation. The alternative has been proposed by Russell et al. (2008), who suggest that the observed magnetic holes represent nonlinear mirror structures that can be carried by the solar wind over vast distances of mirror stable plasma. According to Russell et al. (2008), magnetic holes are created in the vicinity of the sun and are convected by the solar wind outward. Periods of Cluster 1 and VEX data when both spacecraft were connected by the solar wind flow have been considered in this study, in order to determine the evolution of the magnetic holes occurrence rate. The comparison of the magnetic holes occurrence near the Venus and the Earth supports the Russell et al. (2008) premise that they are generated closer to the Sun most likely somewhere within the orbit of Mercury." @default.
• W1970125218 created "2016-06-24" @default.
• W1970125218 creator A5007766940 @default.
• W1970125218 creator A5084287970 @default.
• W1970125218 creator A5091142659 @default.
• W1970125218 date "2011-05-02" @default.
• W1970125218 modified "2023-10-02" @default.
• W1970125218 title "Occurrence rate of magnetic holes between 0.72 and 1 AU: comparative study of Cluster and VEX data" @default.
• W1970125218 cites W1636787526 @default.
• W1970125218 cites W1682136037 @default.
• W1970125218 cites W1907765294 @default.
• W1970125218 cites W1983258245 @default.
• W1970125218 cites W1995864778 @default.
• W1970125218 cites W2004744308 @default.
• W1970125218 cites W2005521083 @default.
• W1970125218 cites W2010969992 @default.
• W1970125218 cites W2011478304 @default.
• W1970125218 cites W2014986885 @default.
• W1970125218 cites W2035360268 @default.
• W1970125218 cites W2037478942 @default.
• W1970125218 cites W2050067775 @default.
• W1970125218 cites W2052332447 @default.
• W1970125218 cites W2060869189 @default.
• W1970125218 cites W2063233600 @default.
• W1970125218 cites W2064220123 @default.
• W1970125218 cites W2065609609 @default.
• W1970125218 cites W2065646850 @default.
• W1970125218 cites W2077461433 @default.
• W1970125218 cites W2084383883 @default.
• W1970125218 cites W2085570343 @default.
• W1970125218 cites W2091835117 @default.
• W1970125218 cites W2115671777 @default.
• W1970125218 cites W2143067656 @default.
• W1970125218 cites W2151289656 @default.
• W1970125218 cites W2160089112 @default.
• W1970125218 cites W4244429515 @default.
• W1970125218 doi "https://doi.org/10.5194/angeo-29-717-2011" @default.
• W1970125218 hasPublicationYear "2011" @default.
• W1970125218 type Work @default.
• W1970125218 sameAs 1970125218 @default.
• W1970125218 citedByCount "10" @default.
• W1970125218 countsByYear W19701252182012 @default.
• W1970125218 countsByYear W19701252182014 @default.
• W1970125218 countsByYear W19701252182016 @default.
• W1970125218 countsByYear W19701252182018 @default.
• W1970125218 countsByYear W19701252182020 @default.
• W1970125218 countsByYear W19701252182021 @default.
• W1970125218 countsByYear W19701252182022 @default.
• W1970125218 crossrefType "journal-article" @default.
• W1970125218 hasAuthorship W1970125218A5007766940 @default.
• W1970125218 hasAuthorship W1970125218A5084287970 @default.
• W1970125218 hasAuthorship W1970125218A5091142659 @default.
• W1970125218 hasBestOaLocation W19701252181 @default.
• W1970125218 hasConcept C102988692 @default.
• W1970125218 hasConcept C108411613 @default.
• W1970125218 hasConcept C115260700 @default.
• W1970125218 hasConcept C121332964 @default.
• W1970125218 hasConcept C128277356 @default.
• W1970125218 hasConcept C140161248 @default.
• W1970125218 hasConcept C188841122 @default.
• W1970125218 hasConcept C30475298 @default.
• W1970125218 hasConcept C44870925 @default.
• W1970125218 hasConcept C46567642 @default.
• W1970125218 hasConcept C62520636 @default.
• W1970125218 hasConcept C72886185 @default.
• W1970125218 hasConcept C8058405 @default.
• W1970125218 hasConcept C82706917 @default.
• W1970125218 hasConceptScore W1970125218C102988692 @default.
• W1970125218 hasConceptScore W1970125218C108411613 @default.
• W1970125218 hasConceptScore W1970125218C115260700 @default.
• W1970125218 hasConceptScore W1970125218C121332964 @default.
• W1970125218 hasConceptScore W1970125218C128277356 @default.
• W1970125218 hasConceptScore W1970125218C140161248 @default.
• W1970125218 hasConceptScore W1970125218C188841122 @default.
• W1970125218 hasConceptScore W1970125218C30475298 @default.
• W1970125218 hasConceptScore W1970125218C44870925 @default.
• W1970125218 hasConceptScore W1970125218C46567642 @default.
• W1970125218 hasConceptScore W1970125218C62520636 @default.
• W1970125218 hasConceptScore W1970125218C72886185 @default.
• W1970125218 hasConceptScore W1970125218C8058405 @default.
• W1970125218 hasConceptScore W1970125218C82706917 @default.
• W1970125218 hasIssue "5" @default.
• W1970125218 hasLocation W19701252181 @default.
• W1970125218 hasOpenAccess W1970125218 @default.
• W1970125218 hasPrimaryLocation W19701252181 @default.
• W1970125218 hasRelatedWork W140706210 @default.
• W1970125218 hasRelatedWork W2015414622 @default.
• W1970125218 hasRelatedWork W2043501188 @default.
• W1970125218 hasRelatedWork W2050119689 @default.
• W1970125218 hasRelatedWork W2093194265 @default.
• W1970125218 hasRelatedWork W2991816610 @default.
• W1970125218 hasRelatedWork W3159482817 @default.
• W1970125218 hasRelatedWork W3206208120 @default.
• W1970125218 hasRelatedWork W4234553788 @default.
• W1970125218 hasRelatedWork W4366452640 @default.
• W1970125218 hasVolume "29" @default.
• W1970125218 isParatext "false" @default.
• W1970125218 isRetracted "false" @default.

• next