FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2062761738> ?p ?o ?g. }

• W2062761738 endingPage "15366" @default.
• W2062761738 startingPage "15354" @default.
• W2062761738 abstract "Voyager 2 observations have shown that Uranus possesses a well‐developed bipolar magnetotail similar in certain characteristics to that of Earth, in spite of an anomalously large tilt of the planetary magnetic dipole to the rotation axis at Uranus. The intensity of the magnetic field in the tail lobes decreases with increasing distance down the tail from the planet as | x SM | −0.59±0.03 . This gradient is similar to that found in the Earth's tail but significantly less steep than that observed in the tails of Jupiter and Saturn. The thickness of the plasma sheet is a minimum (∼10 R U ) near the tail center, increasing toward the flanks as at Earth. Pressure balance within the plasma sheet is maintained predominantly by protons and electrons with energies 10 eV to 6 keV. Except in transient events, the contribution of ≥28‐keV protons to pressure balance in the sheet is <5%. This is in contrast to the dominant role played by more energetic plasma ions in the Jovian magnetotail. An average value of β ∼ 7 was found in the plasma sheet at Uranus and ∼0.1 in the lobe plasma. The Uranian magnetic tail was observed to rotate 360° about its longitudinal axis, a result of the approximately sunward pointing planetary rotation axis at the time of encounter. This, together with the large tilt (60°) of the magnetic dipole, results in a small but measurable twist in the tail's magnetic lines of force, with a derived helical pitch of 5.5° ± 3.0°. The B yz (SM) component of the tail field can be modeled as the sum of the twist component, a radial (diverging or converging from the x SM axis) component, and a component parallel to the z SM axis that closes through the neutral sheet and is strongest there. The cross‐tail current density at the neutral sheet is estimated to be ≃3 × 10 −11 A m −2 . Large temporal variations observed in magnetic fields and plasmas during the Voyager 2 traverse of the magnetotail may have been produced by substorm activity." @default.
• W2062761738 created "2016-06-24" @default.
• W2062761738 creator A5018300832 @default.
• W2062761738 creator A5023904336 @default.
• W2062761738 creator A5025300641 @default.
• W2062761738 creator A5031575654 @default.
• W2062761738 creator A5051204793 @default.
• W2062761738 creator A5086845934 @default.
• W2062761738 creator A5087110149 @default.
• W2062761738 date "1987-12-30" @default.
• W2062761738 modified "2023-10-08" @default.
• W2062761738 title "The magnetotail of Uranus" @default.
• W2062761738 cites W1963583238 @default.
• W2062761738 cites W1971856417 @default.
• W2062761738 cites W1974917692 @default.
• W2062761738 cites W1983190920 @default.
• W2062761738 cites W1986355244 @default.
• W2062761738 cites W1994867222 @default.
• W2062761738 cites W1995133541 @default.
• W2062761738 cites W1995333698 @default.
• W2062761738 cites W1995890907 @default.
• W2062761738 cites W1996254939 @default.
• W2062761738 cites W1996787265 @default.
• W2062761738 cites W1997956179 @default.
• W2062761738 cites W2001344513 @default.
• W2062761738 cites W2008889474 @default.
• W2062761738 cites W2009678820 @default.
• W2062761738 cites W2016912680 @default.
• W2062761738 cites W2017017453 @default.
• W2062761738 cites W2019810401 @default.
• W2062761738 cites W2020115368 @default.
• W2062761738 cites W2020824124 @default.
• W2062761738 cites W2025688824 @default.
• W2062761738 cites W2035104573 @default.
• W2062761738 cites W2039479649 @default.
• W2062761738 cites W2040891018 @default.
• W2062761738 cites W2043992583 @default.
• W2062761738 cites W2046685683 @default.
• W2062761738 cites W2056151613 @default.
• W2062761738 cites W2058749215 @default.
• W2062761738 cites W2067836186 @default.
• W2062761738 cites W2068126016 @default.
• W2062761738 cites W2071103779 @default.
• W2062761738 cites W2074671638 @default.
• W2062761738 cites W2075193088 @default.
• W2062761738 cites W2075217090 @default.
• W2062761738 cites W2083737230 @default.
• W2062761738 cites W2083813471 @default.
• W2062761738 cites W2084350572 @default.
• W2062761738 cites W2084385981 @default.
• W2062761738 cites W2092880483 @default.
• W2062761738 cites W2095191398 @default.
• W2062761738 cites W2101643504 @default.
• W2062761738 cites W2103041946 @default.
• W2062761738 cites W2109640488 @default.
• W2062761738 cites W2134887475 @default.
• W2062761738 cites W2166014791 @default.
• W2062761738 cites W2916048270 @default.
• W2062761738 cites W4229676538 @default.
• W2062761738 cites W4243072205 @default.
• W2062761738 doi "https://doi.org/10.1029/ja092ia13p15354" @default.
• W2062761738 hasPublicationYear "1987" @default.
• W2062761738 type Work @default.
• W2062761738 sameAs 2062761738 @default.
• W2062761738 citedByCount "35" @default.
• W2062761738 countsByYear W20627617382012 @default.
• W2062761738 countsByYear W20627617382013 @default.
• W2062761738 countsByYear W20627617382014 @default.
• W2062761738 countsByYear W20627617382015 @default.
• W2062761738 countsByYear W20627617382017 @default.
• W2062761738 countsByYear W20627617382018 @default.
• W2062761738 countsByYear W20627617382019 @default.
• W2062761738 countsByYear W20627617382020 @default.
• W2062761738 countsByYear W20627617382021 @default.
• W2062761738 crossrefType "journal-article" @default.
• W2062761738 hasAuthorship W2062761738A5018300832 @default.
• W2062761738 hasAuthorship W2062761738A5023904336 @default.
• W2062761738 hasAuthorship W2062761738A5025300641 @default.
• W2062761738 hasAuthorship W2062761738A5031575654 @default.
• W2062761738 hasAuthorship W2062761738A5051204793 @default.
• W2062761738 hasAuthorship W2062761738A5086845934 @default.
• W2062761738 hasAuthorship W2062761738A5087110149 @default.
• W2062761738 hasConcept C106125477 @default.
• W2062761738 hasConcept C115260700 @default.
• W2062761738 hasConcept C118873486 @default.
• W2062761738 hasConcept C121332964 @default.
• W2062761738 hasConcept C1276947 @default.
• W2062761738 hasConcept C130443932 @default.
• W2062761738 hasConcept C134581325 @default.
• W2062761738 hasConcept C13966519 @default.
• W2062761738 hasConcept C150846664 @default.
• W2062761738 hasConcept C169852918 @default.
• W2062761738 hasConcept C173523689 @default.
• W2062761738 hasConcept C185544564 @default.
• W2062761738 hasConcept C22268893 @default.
• W2062761738 hasConcept C2780114079 @default.
• W2062761738 hasConcept C31532427 @default.
• W2062761738 hasConcept C44870925 @default.

• next