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ReportsEnergetic Particles in the Jovian Magnetotail
When the solar wind hits Jupiter's magnetic field, it creates a long magnetotail trailing behind the planet that channels material out of the Jupiter system. The New Horizons spacecraft traversed the length of the jovian magnetotail to >2500 jovian radii (RJ; 1 RJ
1 Applied Physics Laboratory, Johns Hopkins University, Laurel, MD 20723, USA. 71,400 kilometers), observing a high-temperature, multispecies population of energetic particles. Velocity dispersions, anisotropies, and compositional variation seen in the deep-tail ( 500 RJ) with a 3-day periodicity are similar to variations seen closer to Jupiter in Galileo data. The signatures suggest plasma streaming away from the planet and injection sites in the near-tail region ( 200 to 400 RJ) that could be related to magnetic reconnection events. The tail structure remains coherent at least until it reaches the magnetosheath at 1655 RJ.
2 Academy of Athens, 28 Panapistimiou, 10679 Athens, Greece. 3 Southwest Research Institute, San Antonio, TX 78228, USA. 4 Laboratory of Atmospheric and Space Physics, University of Colorado, Boulder, CO 80309–0392, USA. 5 NASA Headquarters, Washington, DC 20546–0001, USA. 6 Southwest Research Institute, Boulder, CO 80302, USA. 7 NASA Ames Research Center, Moffett Field, CA 94035, USA. * To whom correspondence should be addressed. E-mail: ralph.mcnutt{at}jhuapl.edu
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Science. ISSN 0036-8075 (print), 1095-9203 (online)