@article{838957aca1594d0f8963cdec3d786059,
title = "Survey of Jupiter's Dawn Magnetosheath Using Juno",
abstract = "The Juno spacecraft crossed Jupiter's bow shock and into the magnetosheath on 24 June 2016. It then went into 53-day polar orbits with its apojoves at 113 Jovian radii on Jupiter's dawn side. These orbits have given us a unique opportunity to survey Jupiter's dawn magnetosheath. Using data from the Jovian Auroral Distributions Experiment, the Magnetic Field Investigation, and the Waves Investigation, we have identified 91 magnetosheath crossings for a total of 48.2 days of data. We present the statistical properties of the magnetosheath plasma, including density, velocity, magnetic field strength, temperature, plasma beta, pressures, and Mach numbers. We then show correlations between these various parameters. We confirm the rotation of the magnetic field to align with Jupiter's spin axis and find that this rotation correlates with several of the plasma properties, including magnetic field strength and plasma flow velocity. Finally, we discuss how these results can affect magnetic reconnection and the Kelvin-Helmholtz instability at Jupiter's dawn magnetopause boundary.",
keywords = "Juno, Jupiter, magnetosheath",
author = "Ranquist, {D. A.} and F. Bagenal and Wilson, {R. J.} and G. Hospodarsky and Ebert, {R. W.} and F. Allegrini and P. Valek and McComas, {D. J.} and Connerney, {J. E.P.} and Kurth, {W. S.} and Bolton, {S. J.}",
note = "Funding Information: JNO‐E_J_SS‐WAV‐3‐CDR‐SRVFULL‐V1.0 This work was supported at the University of Colorado as a part NASA's Juno mission supported by NASA through contract 699050X with the Southwest Research Institute. The Jet Propulsion Laboratory manages the Juno mission for the principal investigator, Scott Bolton, of Southwest Research Institute (SwRI). The Juno mission is funded by NASA and is part of the New Frontiers Program managed at NASA's Marshall Space Flight Center in Huntsville, Alabama. Work at SwRI is funded by NASA under contract number NNM06AA75C. This work was supported as a part of the work on the Jovian Auroral Distributions Experiment (JADE) on NASA's Juno mission. The research at the University of Iowa is supported by NASA through contract 699041X with SWRI. J. E. P. Connerney is supported by NASA contract J99042CP with SWRI. The JADE‐I ion species data are part of the JNO‐J/SW‐JAD‐3‐CALIBRATED‐V1.0 data set and may be obtained from the Planetary Data System (PDS) at https://pds.nasa.gov/ . The JADE background data were taken from the Version 01 electron files and ion logical files in the JNO‐J/SW‐JAD‐2‐UNCALIBRATED‐V1.0 data set from PDS. The MAG data may be obtained from the PDS, data set JNO‐J‐3‐FGM‐CAL‐V1.0. The Waves data can also be obtained from the PDS, data set . We wish to also acknowledge the helpful conversations with Adam Masters, Peter Delamere, Ali Sulaiman, Dan Gershman, and Michelle Thomsen. Publisher Copyright: {\textcopyright}2019. American Geophysical Union. All Rights Reserved.",
year = "2019",
month = nov,
day = "1",
doi = "10.1029/2019JA027382",
language = "English (US)",
volume = "124",
pages = "9106--9123",
journal = "Journal of Geophysical Research: Space Physics",
issn = "2169-9402",
number = "11",
}