New Results From Galileo's First Flyby of Ganymede: Reconnection‐Driven Flows at the Low‐Latitude Magnetopause Boundary, Crossing the Cusp, and Icy Ionospheric Escape. Issue 8 (30th April 2018)

• Record Type: Journal Article
• Authors: Collinson, Glyn; Paterson, William R.; Bard, Christopher; Dorelli, John; Glocer, Alex; Sarantos, Menelaos; Wilson, Rob
• Is Part Of: Geophysical research letters. Volume 45:Issue 8(2018)
• Page Start: 3382
• Page End: 3392
• Publication Date: 2018-04-30
• Subjects: Ganymede -- Galileo -- plasma -- magnetosphere -- current sheet -- plasma sheet; Geophysics -- Periodicals; Planets -- Periodicals; Lunar geology -- Periodicals; 550
• DOI: 10.1002/2017GL075487
• Languages: English
• ISSNs: 0094-8276

Abstract

Abstract: On 27 June 1996, the NASA Galileo spacecraft made humanity's first flyby of Jupiter's largest moon, Ganymede, discovering that it is the only moon known to possess an internally generated magnetic field. Resurrecting the original Galileo Plasma Subsystem (PLS) data analysis software, we processed the raw PLS data from G01 and for the first time present the properties of plasmas encountered. Entry into the magnetosphere of Ganymede occurred near the confluence of the magnetopause and plasma sheet. Reconnection‐driven plasma flows were observed (consistent with an Earth‐like Dungey cycle), which may be a result of reconnection in the plasma sheet, magnetopause, or might be Ganymede's equivalent of a Low‐Latitude Boundary Layer. Dropouts in plasma density combined with velocity perturbations afterward suggest that Galileo briefly crossed the cusps into closed magnetic field lines. Galileo then crossed the cusps, where field‐aligned precipitating ions were observed flowing down into the surface, at a location consistent with observations by the Hubble Space Telescope. The density of plasma outflowing from Ganymede jumped an order of magnitude around closest approach over the north polar cap. The abrupt increase may be a result of crossing the cusp or may represent an altitude‐dependent boundary such as an ionopause. More diffuse, warmer field‐aligned outflows were observed in the lobes. Fluxes of particles near the moon on the nightside were significantly lower than on the dayside, possibly resulting from a diurnal cycle of the ionosphere and/or neutral atmosphere. Plain Language Summary: NASA's Galileo spacecraft made the first ever flyby of Jupiter's largest moon, Ganymede, on 27 June 1996, discovering that it is the only moon known to generate a magnetic field. As at Earth, Ganymede's magnetic field projects a magnetic bubble around it called a magnetosphere. Galileo carried a package called the Plasma Subsystem (PLS) that was designed to measure charged particles. Although PLS collected data during this first flyby, the results were never published. Resurrecting the original flight software, we processed these data and present them here for the first time, permitting us to go back with a fine detail brush and fill in some of the structure of this complex and exotic magnetosphere. Charged water‐based particles were observed escaping from the moon, having been blasted off the icy surface by an energetic rain of particles from Jupiter. We also find that Galileo flew just above Ganymede's auroral zones, at the precise location where they have been observed by the Hubble Space Telescope. We also observe evidence for the acceleration of plasmas by magnetic reconnection, wherein magnetic energy is converted into kinetic and thermal energy in space plasmas. Key Points: We present the first in situ observations of plasmas in Ganymede's cusp/auroral zones and low‐latitude magnetopause boundary We observe unambiguous evidence for magnetic reconnection near the intersection between Ganymede's magnetopause and tail plasma sheet Field‐aligned downflows of ions were observed in the cusp, in a location consistent with auroral observations by the Hubble Space Telescope