Matches in SemOpenAlex for { <https://semopenalex.org/work/W2892336616> ?p ?o ?g. }
- W2892336616 endingPage "6222" @default.
- W2892336616 startingPage "6207" @default.
- W2892336616 abstract "The moon Io is the dominant plasma source for the Jupiter magnetosphere. The plasma is distributed into a torus of material around Jupiter, called the Io plasma torus. The Juno spacecraft performed its first perijove on 27 August 2016. During this time the spacecraft's X and Ka-band radio signals passed through the Io plasma torus. From the differential Doppler shift of the X and Ka-band frequencies we are able to determine the Io plasma torus total electron content. From the total electron content, we determine that the electron densities are larger than predicted from Voyager-based models by around 35 ± 14% in the cold torus and 38 ± 14% in the torus beyond 5.5 RJ. The ion temperatures were greater than predicted from the models by 44 ± 15% in the cold torus but consistent with models in the torus beyond 5.5 RJ. From the time of maximum total electron content, which is sensitive to the torus location, we also find the Io plasma torus equatorial plane appears to be tilted by about 1.5° more than the nominal centrifugal equator tilt based on the tilt of a dipole magnetic field approximation. Different tilts were found for the cold torus and torus beyond 5.5 RJ." @default.
- W2892336616 created "2018-09-27" @default.
- W2892336616 creator A5039841213 @default.
- W2892336616 creator A5045281373 @default.
- W2892336616 creator A5050645585 @default.
- W2892336616 creator A5070195319 @default.
- W2892336616 date "2018-08-01" @default.
- W2892336616 modified "2023-10-01" @default.
- W2892336616 title "Distribution of Plasma in the Io Plasma Torus as Seen by Radio Occultation During<i>Juno</i>Perijove 1" @default.
- W2892336616 cites W1599740112 @default.
- W2892336616 cites W1666064188 @default.
- W2892336616 cites W1668807532 @default.
- W2892336616 cites W1902882157 @default.
- W2892336616 cites W1967144177 @default.
- W2892336616 cites W1992341358 @default.
- W2892336616 cites W1993632200 @default.
- W2892336616 cites W2019349812 @default.
- W2892336616 cites W2022198791 @default.
- W2892336616 cites W2022599588 @default.
- W2892336616 cites W2026347813 @default.
- W2892336616 cites W2038063515 @default.
- W2892336616 cites W2056374285 @default.
- W2892336616 cites W2060746844 @default.
- W2892336616 cites W2063973453 @default.
- W2892336616 cites W2068170646 @default.
- W2892336616 cites W2073736682 @default.
- W2892336616 cites W2082723618 @default.
- W2892336616 cites W2083499611 @default.
- W2892336616 cites W2084945420 @default.
- W2892336616 cites W2085090241 @default.
- W2892336616 cites W2104208550 @default.
- W2892336616 cites W2106923334 @default.
- W2892336616 cites W2110659732 @default.
- W2892336616 cites W2115311464 @default.
- W2892336616 cites W2132889322 @default.
- W2892336616 cites W2172474649 @default.
- W2892336616 cites W2240716019 @default.
- W2892336616 cites W2571311412 @default.
- W2892336616 cites W2580849679 @default.
- W2892336616 cites W2596261392 @default.
- W2892336616 cites W2620302159 @default.
- W2892336616 cites W2727729278 @default.
- W2892336616 cites W2766680863 @default.
- W2892336616 cites W3102014803 @default.
- W2892336616 doi "https://doi.org/10.1029/2017ja025113" @default.
- W2892336616 hasPublicationYear "2018" @default.
- W2892336616 type Work @default.
- W2892336616 sameAs 2892336616 @default.
- W2892336616 citedByCount "17" @default.
- W2892336616 countsByYear W28923366162019 @default.
- W2892336616 countsByYear W28923366162020 @default.
- W2892336616 countsByYear W28923366162021 @default.
- W2892336616 countsByYear W28923366162022 @default.
- W2892336616 countsByYear W28923366162023 @default.
- W2892336616 crossrefType "journal-article" @default.
- W2892336616 hasAuthorship W2892336616A5039841213 @default.
- W2892336616 hasAuthorship W2892336616A5045281373 @default.
- W2892336616 hasAuthorship W2892336616A5050645585 @default.
- W2892336616 hasAuthorship W2892336616A5070195319 @default.
- W2892336616 hasConcept C121332964 @default.
- W2892336616 hasConcept C1276947 @default.
- W2892336616 hasConcept C130443932 @default.
- W2892336616 hasConcept C22268893 @default.
- W2892336616 hasConcept C2524010 @default.
- W2892336616 hasConcept C29829512 @default.
- W2892336616 hasConcept C33923547 @default.
- W2892336616 hasConcept C44870925 @default.
- W2892336616 hasConcept C62520636 @default.
- W2892336616 hasConcept C82706917 @default.
- W2892336616 hasConcept C9767117 @default.
- W2892336616 hasConceptScore W2892336616C121332964 @default.
- W2892336616 hasConceptScore W2892336616C1276947 @default.
- W2892336616 hasConceptScore W2892336616C130443932 @default.
- W2892336616 hasConceptScore W2892336616C22268893 @default.
- W2892336616 hasConceptScore W2892336616C2524010 @default.
- W2892336616 hasConceptScore W2892336616C29829512 @default.
- W2892336616 hasConceptScore W2892336616C33923547 @default.
- W2892336616 hasConceptScore W2892336616C44870925 @default.
- W2892336616 hasConceptScore W2892336616C62520636 @default.
- W2892336616 hasConceptScore W2892336616C82706917 @default.
- W2892336616 hasConceptScore W2892336616C9767117 @default.
- W2892336616 hasIssue "8" @default.
- W2892336616 hasLocation W28923366161 @default.
- W2892336616 hasOpenAccess W2892336616 @default.
- W2892336616 hasPrimaryLocation W28923366161 @default.
- W2892336616 hasRelatedWork W2150688528 @default.
- W2892336616 hasRelatedWork W2164194373 @default.
- W2892336616 hasRelatedWork W2580849679 @default.
- W2892336616 hasRelatedWork W2586892223 @default.
- W2892336616 hasRelatedWork W2805158686 @default.
- W2892336616 hasRelatedWork W2999974266 @default.
- W2892336616 hasRelatedWork W3027759835 @default.
- W2892336616 hasRelatedWork W3070256043 @default.
- W2892336616 hasRelatedWork W3158932059 @default.
- W2892336616 hasRelatedWork W4200226658 @default.
- W2892336616 hasVolume "123" @default.
- W2892336616 isParatext "false" @default.
- W2892336616 isRetracted "false" @default.