Juno observations of large‐scale compressions of Jupiter's dawnside magnetopause. Issue 15 (31st July 2017)

• Record Type: Journal Article
• Authors: Gershman, Daniel J.; DiBraccio, Gina A.; Connerney, John E. P.; Hospodarsky, George; Kurth, William S.; Ebert, Robert W.; Szalay, Jamey R.; Wilson, Robert J.; Allegrini, Frederic; Valek, Phil; McComas, David J.; Bagenal, Fran; Levin, Steve; Bolton, Scott J.
• Is Part Of: Geophysical research letters. Volume 44:Issue 15(2017)
• Page Start: 7559
• Page End: 7568
• Publication Date: 2017-07-31
• Subjects: Jupiter magnetosphere -- magnetosphere compression -- magnetopause -- magnetosonic wave -- magnetopause reconnection -- magnetopause boundary layer; Geophysics -- Periodicals; Planets -- Periodicals; Lunar geology -- Periodicals; 550
• DOI: 10.1002/2017GL073132
• Languages: English
• ISSNs: 0094-8276

Abstract

Abstract: We investigate the structure of Jupiter's dawnside magnetopause using observations obtained by particle and fields instrumentation on the Juno spacecraft. Characterization of Jupiter's magnetopause is critical for the understanding of mass and energy transport between the solar wind and the magnetosphere. We find an extended magnetopause boundary layer (MPBL) during a magnetopause crossing on 14 July 2016. This thick MPBL, in combination with a large magnetic field component normal to the magnetopause boundary, suggests that strong magnetospheric compression enhances mass transport across the magnetopause via magnetic reconnection. We further identify ~2 h increases in the total magnetospheric pressure adjacent to the magnetopause on 14 July 2016 and 1 August 2016. These large‐scale structures provide evidence of focused energy transport into the magnetosphere via magnetohydrodynamic structures. Key Points: Jupiter's dawnside magnetosphere is highly compressible and subject to strong Alfvén‐magnetosonic mode coupling Magnetospheric compressions may enhance reconnection rates and increase mass transport across the magnetopause Total pressure increases inside the magnetopause with durations of hours are indicative of strong solar wind‐magnetosphere energy transport