Fatemi, ShahabPoppe, A.R.Vorburger, AudreyLindkvist, JesperHamrin, Maria
We study the dynamics of the thermal O+ and H+ ions at Ganymede's magnetopause when Ganymede is inside and outside of the Jovian plasma sheet using a three-dimensional hybrid model of plasma (kinetic ions, fluid electrons). We present the global structure of the electric fields and power density (E ⋅ J) in the magnetosphere of Ganymede and show tha...
This thesis deals with the development of the Jovian Neutrals Analyzer (JNA) for the Jupiter ICy moons Explorer (JUICE) mission to Jupiter, planned to launch in 2023. Jupiter, the largest planet in the Solar System, orbits the Sun at five times the distance from the Earth to the Sun, accompanied by dozens of moons, rings, and the largest object in ...
Vorburger, AudreyFatemi, ShahabGalli, AndréLiuzzo, LucasPoppe, Andrew R.Wurz, Peter
In this paper we present ab initio 3D Monte-Carlo simulations of Ganymede's surface sputtered and sublimated H2O exosphere. As inputs, we include surface water content maps and temperature distribution maps based on Galileo and Very Large Telescope (VLT) observations. For plasma precipitation, we use hybrid model results for thermal H+ and O+, ener...
Moirano, AlessandroMura, AlessandroAdriani, AlbertoDols, VincentBonfond, BertrandWaite, Jack H.Hue, VincentSzalay, Jamey R.Sulaiman, Ali H.Dinelli, Bianca M.
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Jupiter hosts intense auroral activity associated with charged particles precipitating into the planet's atmosphere. The Galilean moons orbiting within the magnetosphere are swept by the magnetic field: the resulting perturbation travels along field lines as Alfven waves, which are able to accelerate electrons toward the planet, producing satellite...
Soderlund, Krista M.Kalousová, KláraBuffo, Jacob J.Glein, Christopher R.Goodman, Jason C.Mitri, GiuseppePatterson, G. WesleyPostberg, FrankRovira-Navarro, MarcRückriemen, Tina
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A growing number of satellites in the outer solar system likely have global oceans beneath their outer icy shells. While the presence of liquid water makes these ocean worlds compelling astrobiological targets, the exchange of heat and materials between the deep interior and the surface also plays a critical role in promoting habitable environments...
Ganymede's surface is subject to constant bombardment by Jovian magnetospheric and Ganymede's ionospheric ions. These populations sputter the surface and contribute to the replenishment of the moon's exosphere.Thus far, estimates for sputtering on the moon's surface have included only the contribution from Jovian ions. In this work, we have used ou...
Soderlund, Krista M;Kalousova, Klara;Buffo, Jacob J;Glein, Christopher R;Goodman, Jason C;Mitri, Giuseppe;Patterson, G Wesley;Postberg, Frank;Rovira-Navarro, Marc;Rueckriemen, Tina;
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The JUICE (JUpiter ICy moons Explorer) mission by ESA aims to explore the emergence of habitable worlds around gas giants and the Jupiter system as an archetype for gas giants. MAJIS (Moons and Jupiter Imaging Spectrometer) is the visible to near-infrared imaging spectrometer onboard JUICE which will characterize the surfaces and exospheres of the ...