Results 71 to 80 of about 6,080 (232)
Astrometric observations of outer Jovian satellites with the `Saturn' telescope. First results [PDF]
M. Yu. Khovritchev +11 more
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Evidence for low density holes in Jupiter’s ionosphere
Intense electromagnetic impulses induced by Jupiter’s lightning can produce both low-frequency dispersed whistler emissions and non-dispersed radio pulses. Here, the authors show Jupiter dispersed pulses associated with Jovian lightning that are evidence
Masafumi Imai +9 more
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A translation of a section from the 1665 Astronomia Reformata of G. B. Riccioli discussing the appearance of the disk of Jupiter during the years 1630-1664; changes in the Jovian cloud belts as recorded by a variety of observers are a major feature of ...
Graney Christopher M.
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On the Origin and Dynamical Evolution of Jupiter’s Moon Amalthea
Interior to the orbits of Jupiter’s iconic Galilean moons are four small satellites with individual mean radii R ≲ 84 km. Multiple lines of evidence suggest that these bodies formed at a more distant location in Jupiter’s circumplanetary disk before ...
Ian R. Brunton, Konstantin Batygin
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Auroral radio emission from ultracool dwarfs: a Jovian model [PDF]
Sam Turnpenney +3 more
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A Search for Jovian Planets around Hot White Dwarfs [PDF]
You-Hua Chu +3 more
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Implications of Jovian X‐ray emission for magnetosphere‐ionosphere coupling [PDF]
T. E. Cravens +6 more
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In Situ Analysis of Jupiter's Broadband Kilometric Auroral Radio Emissions With Juno
Among the zoo of Jovian auroral radio emissions, the broadband kilometric (bKOM) component has been the least studied. Taking advantage of Juno in situ measurements within the auroral regions, we surveyed the Juno/Waves radio observations over the 60 ...
B. Collet +4 more
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Modeling the transport of low-energy (1−10 MeV) cosmic-ray electrons can lead to valuable insights as to the behavior of the heliospheric magnetic field (HMF), due to the fact that the mean free path (MFP) of these particles parallel to the HMF is ...
N. E. Engelbrecht
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We follow the orbital evolution of small dust particles generated from the break up of comet Shoemaker‐Levy 9. In addition to the usual perturbations, we also consider electrostatic charging and the consequent magnetospheric effects. We show, that in about ten years following the break up, a small fraction of the dust will settle into orbits well ...
openaire +1 more source

