FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W1485017209> ?p ?o ?g. }

• W1485017209 endingPage "n/a" @default.
• W1485017209 startingPage "n/a" @default.
• W1485017209 abstract "[1] Initial Cassini magnetometer observations in the E-ring plasma torus reveal the presence of previously unreported diamagnetic decreases in the magnetic field. The decrease in magnetic pressure on these flux tubes implies the presence of additional plasma energy densities up to 1 keV/cm3. They are less stretched than surrounding flux tubes suggesting the centrifugal force acting on them is less, possibly because they have a lower mass content or lower azimuthal velocity than their neighbors. Outward from these isolated tubes, at about 6 Saturn radii, an irregular transition from predominantly cool to predominantly warm flux tubes is observed. A similar boundary is observed in the jovian magnetosphere at the outer edge of the Io torus. Both the saturnian and jovian boundaries are candidates for the interchange instability but other processes may also be acting. ULF waves are associated with some, but not all, of these flux tubes." @default.
• W1485017209 created "2016-06-24" @default.
• W1485017209 creator A5011650421 @default.
• W1485017209 creator A5030474716 @default.
• W1485017209 creator A5033225529 @default.
• W1485017209 creator A5076274178 @default.
• W1485017209 creator A5082957105 @default.
• W1485017209 date "2005-06-16" @default.
• W1485017209 modified "2023-10-12" @default.
• W1485017209 title "Warm flux tubes in the E-ring plasma torus: Initial Cassini magnetometer observations" @default.
• W1485017209 cites W1525087382 @default.
• W1485017209 cites W1559078273 @default.
• W1485017209 cites W1618633739 @default.
• W1485017209 cites W1967552633 @default.
• W1485017209 cites W1972209947 @default.
• W1485017209 cites W1980519402 @default.
• W1485017209 cites W1997728670 @default.
• W1485017209 cites W2019084785 @default.
• W1485017209 cites W2042011111 @default.
• W1485017209 cites W2042516193 @default.
• W1485017209 cites W2047324657 @default.
• W1485017209 cites W2049577632 @default.
• W1485017209 cites W2050173557 @default.
• W1485017209 cites W2083116850 @default.
• W1485017209 cites W2101174378 @default.
• W1485017209 cites W2116858201 @default.
• W1485017209 cites W2130690556 @default.
• W1485017209 cites W2155804188 @default.
• W1485017209 cites W2165476196 @default.
• W1485017209 doi "https://doi.org/10.1029/2005gl022652" @default.
• W1485017209 hasPublicationYear "2005" @default.
• W1485017209 type Work @default.
• W1485017209 sameAs 1485017209 @default.
• W1485017209 citedByCount "33" @default.
• W1485017209 countsByYear W14850172092012 @default.
• W1485017209 countsByYear W14850172092013 @default.
• W1485017209 countsByYear W14850172092014 @default.
• W1485017209 countsByYear W14850172092015 @default.
• W1485017209 countsByYear W14850172092016 @default.
• W1485017209 countsByYear W14850172092017 @default.
• W1485017209 countsByYear W14850172092018 @default.
• W1485017209 countsByYear W14850172092020 @default.
• W1485017209 countsByYear W14850172092022 @default.
• W1485017209 countsByYear W14850172092023 @default.
• W1485017209 crossrefType "journal-article" @default.
• W1485017209 hasAuthorship W1485017209A5011650421 @default.
• W1485017209 hasAuthorship W1485017209A5030474716 @default.
• W1485017209 hasAuthorship W1485017209A5033225529 @default.
• W1485017209 hasAuthorship W1485017209A5076274178 @default.
• W1485017209 hasAuthorship W1485017209A5082957105 @default.
• W1485017209 hasBestOaLocation W14850172091 @default.
• W1485017209 hasConcept C106125477 @default.
• W1485017209 hasConcept C115260700 @default.
• W1485017209 hasConcept C118873486 @default.
• W1485017209 hasConcept C121332964 @default.
• W1485017209 hasConcept C1276947 @default.
• W1485017209 hasConcept C130443932 @default.
• W1485017209 hasConcept C134581325 @default.
• W1485017209 hasConcept C140161248 @default.
• W1485017209 hasConcept C153946474 @default.
• W1485017209 hasConcept C154959693 @default.
• W1485017209 hasConcept C157479481 @default.
• W1485017209 hasConcept C191897082 @default.
• W1485017209 hasConcept C192562407 @default.
• W1485017209 hasConcept C22268893 @default.
• W1485017209 hasConcept C2524010 @default.
• W1485017209 hasConcept C33923547 @default.
• W1485017209 hasConcept C44870925 @default.
• W1485017209 hasConcept C511503438 @default.
• W1485017209 hasConcept C51244244 @default.
• W1485017209 hasConcept C62520636 @default.
• W1485017209 hasConcept C68709404 @default.
• W1485017209 hasConcept C8058405 @default.
• W1485017209 hasConcept C82706917 @default.
• W1485017209 hasConcept C96026104 @default.
• W1485017209 hasConcept C9767117 @default.
• W1485017209 hasConceptScore W1485017209C106125477 @default.
• W1485017209 hasConceptScore W1485017209C115260700 @default.
• W1485017209 hasConceptScore W1485017209C118873486 @default.
• W1485017209 hasConceptScore W1485017209C121332964 @default.
• W1485017209 hasConceptScore W1485017209C1276947 @default.
• W1485017209 hasConceptScore W1485017209C130443932 @default.
• W1485017209 hasConceptScore W1485017209C134581325 @default.
• W1485017209 hasConceptScore W1485017209C140161248 @default.
• W1485017209 hasConceptScore W1485017209C153946474 @default.
• W1485017209 hasConceptScore W1485017209C154959693 @default.
• W1485017209 hasConceptScore W1485017209C157479481 @default.
• W1485017209 hasConceptScore W1485017209C191897082 @default.
• W1485017209 hasConceptScore W1485017209C192562407 @default.
• W1485017209 hasConceptScore W1485017209C22268893 @default.
• W1485017209 hasConceptScore W1485017209C2524010 @default.
• W1485017209 hasConceptScore W1485017209C33923547 @default.
• W1485017209 hasConceptScore W1485017209C44870925 @default.
• W1485017209 hasConceptScore W1485017209C511503438 @default.
• W1485017209 hasConceptScore W1485017209C51244244 @default.
• W1485017209 hasConceptScore W1485017209C62520636 @default.
• W1485017209 hasConceptScore W1485017209C68709404 @default.
• W1485017209 hasConceptScore W1485017209C8058405 @default.

• next