FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2893447549> ?p ?o ?g. }

• W2893447549 abstract "The magnetosphere−ionosphere system is recognized as a complex and active element affected by space weather and as a region where important scientific questions related to space weather impacts need to be answered. In this framework, there is a high priority on the un− derstanding of how local, regional, and global−scale phenomena couple to produce observed responses across various scales. Turbulence provides one pathway by which energy cascades across scales from large to small ones where energy can be dissipated in the form of heat− ing. The Swarm mission, that is a true multi−point and multi−purpose constellation, represents a unique opportunity to address some of these scientific questions. In detail, it gives us a chance of investigating the nature and the scaling features of magnetic field fluctuations for different geomagnetic activity levels, and unveiling the role played by turbulence of ionospheric plasma medium on the magnetic field fluctuations. Recently, using Swarm magnetic field data at high−latitude in the Northern Hemisphere, the local scaling indices of the 1st and 2nd order structure functions of the magnetic field fluctuations have been evaluated, showing their capability both to give new in− sights about the ionosphere−magnetosphere coupling and to provide information on the ionospheric turbulence. Here, we improve and ex− tend the analysis by investigating the scaling features of the geomagnetic field fluctuations of external origin, recorded by Swarm A satellite during a period of 2 years (April 2014 – March 2016). Maps of the local Hurst exponent values, which allow us to study scaling properties of the geomagnetic field’s spatial fluctuations are shown, both at high−latitudes (in the Northern and Southern Hemisphere) and at low− and mid−latitudes (±60°) according to two different geomagnetic activity conditions. The aim is to capture the essential features of the spatial fluctuations of the geomagnetic field and understand their origins." @default.
• W2893447549 created "2018-10-05" @default.
• W2893447549 creator A5012433558 @default.
• W2893447549 creator A5016158869 @default.
• W2893447549 creator A5035685017 @default.
• W2893447549 creator A5048398644 @default.
• W2893447549 creator A5058012017 @default.
• W2893447549 creator A5089593436 @default.
• W2893447549 date "2018-09-25" @default.
• W2893447549 modified "2023-10-01" @default.
• W2893447549 title "Features of Magnetic Field Fluctuations in the Ionosphere at Swarm altitude" @default.
• W2893447549 cites W1969479973 @default.
• W2893447549 cites W1971713959 @default.
• W2893447549 cites W1985781151 @default.
• W2893447549 cites W1992625621 @default.
• W2893447549 cites W2012106254 @default.
• W2893447549 cites W2012502319 @default.
• W2893447549 cites W2015714729 @default.
• W2893447549 cites W2016386969 @default.
• W2893447549 cites W2020865574 @default.
• W2893447549 cites W2035642048 @default.
• W2893447549 cites W2042766907 @default.
• W2893447549 cites W2051623371 @default.
• W2893447549 cites W2062479631 @default.
• W2893447549 cites W2063841808 @default.
• W2893447549 cites W2074513525 @default.
• W2893447549 cites W2074845482 @default.
• W2893447549 cites W2085959206 @default.
• W2893447549 cites W2090100313 @default.
• W2893447549 cites W2090805550 @default.
• W2893447549 cites W2093587072 @default.
• W2893447549 cites W2096398879 @default.
• W2893447549 cites W2103547601 @default.
• W2893447549 cites W2112217963 @default.
• W2893447549 cites W2126251407 @default.
• W2893447549 cites W2126786514 @default.
• W2893447549 cites W2128858114 @default.
• W2893447549 cites W2142300149 @default.
• W2893447549 cites W2150067632 @default.
• W2893447549 cites W2160225847 @default.
• W2893447549 cites W2167411386 @default.
• W2893447549 cites W2525531047 @default.
• W2893447549 doi "https://doi.org/10.4401/ag-7789" @default.
• W2893447549 hasPublicationYear "2018" @default.
• W2893447549 type Work @default.
• W2893447549 sameAs 2893447549 @default.
• W2893447549 citedByCount "3" @default.
• W2893447549 countsByYear W28934475492020 @default.
• W2893447549 countsByYear W28934475492021 @default.
• W2893447549 countsByYear W28934475492022 @default.
• W2893447549 crossrefType "journal-article" @default.
• W2893447549 hasAuthorship W2893447549A5012433558 @default.
• W2893447549 hasAuthorship W2893447549A5016158869 @default.
• W2893447549 hasAuthorship W2893447549A5035685017 @default.
• W2893447549 hasAuthorship W2893447549A5048398644 @default.
• W2893447549 hasAuthorship W2893447549A5058012017 @default.
• W2893447549 hasAuthorship W2893447549A5089593436 @default.
• W2893447549 hasBestOaLocation W28934475491 @default.
• W2893447549 hasConcept C115260700 @default.
• W2893447549 hasConcept C116403925 @default.
• W2893447549 hasConcept C121332964 @default.
• W2893447549 hasConcept C121864883 @default.
• W2893447549 hasConcept C130443932 @default.
• W2893447549 hasConcept C135736735 @default.
• W2893447549 hasConcept C151325931 @default.
• W2893447549 hasConcept C154945302 @default.
• W2893447549 hasConcept C181335050 @default.
• W2893447549 hasConcept C199635899 @default.
• W2893447549 hasConcept C2524010 @default.
• W2893447549 hasConcept C33923547 @default.
• W2893447549 hasConcept C41008148 @default.
• W2893447549 hasConcept C62520636 @default.
• W2893447549 hasConcept C8058405 @default.
• W2893447549 hasConcept C99844830 @default.
• W2893447549 hasConceptScore W2893447549C115260700 @default.
• W2893447549 hasConceptScore W2893447549C116403925 @default.
• W2893447549 hasConceptScore W2893447549C121332964 @default.
• W2893447549 hasConceptScore W2893447549C121864883 @default.
• W2893447549 hasConceptScore W2893447549C130443932 @default.
• W2893447549 hasConceptScore W2893447549C135736735 @default.
• W2893447549 hasConceptScore W2893447549C151325931 @default.
• W2893447549 hasConceptScore W2893447549C154945302 @default.
• W2893447549 hasConceptScore W2893447549C181335050 @default.
• W2893447549 hasConceptScore W2893447549C199635899 @default.
• W2893447549 hasConceptScore W2893447549C2524010 @default.
• W2893447549 hasConceptScore W2893447549C33923547 @default.
• W2893447549 hasConceptScore W2893447549C41008148 @default.
• W2893447549 hasConceptScore W2893447549C62520636 @default.
• W2893447549 hasConceptScore W2893447549C8058405 @default.
• W2893447549 hasConceptScore W2893447549C99844830 @default.
• W2893447549 hasIssue "Vol 61 (2018)" @default.
• W2893447549 hasLocation W28934475491 @default.
• W2893447549 hasOpenAccess W2893447549 @default.
• W2893447549 hasPrimaryLocation W28934475491 @default.
• W2893447549 hasRelatedWork W1433270626 @default.
• W2893447549 hasRelatedWork W2012418971 @default.
• W2893447549 hasRelatedWork W2085417922 @default.
• W2893447549 hasRelatedWork W2291234652 @default.
• W2893447549 hasRelatedWork W2626925519 @default.
• W2893447549 hasRelatedWork W28702998 @default.

• next