Each of the outer three Galilean satellites Europa, Ganymede, and Callisto have surficial ice and atmospheric water group species (H, H 2 , O, OH, H 2 O, and O 2 ). These species are abundant to varying degrees due to differing surface compositions and atmospheric source/loss processes (e.g.

Most space plasmas are weakly collisional. Due to the low collision rate, the plasmas are routinely out of local thermal equilibrium and often exhibit non‐Maxwellian velocity distributions. The charged particles typically exhibit anisotropy in temperature measurements, that is, distinct temperatures are observed perpendicular and parallel (T⊥i and T||i) to the local magnetic field. Numerous prior studies have shown that for increasing values of parallel ion beta (β||i), the range of ion temperature anisotropy (Ri = T⊥i/T||i) values becomes narrower. Conventionally, this behavior has been attributed to the actions of kinetic microinstabilities. This study is the first to explore such β||i‐dependent limits on ion temperature anisotropy in Jupiter's magnetosheath. We use linear Vlasov theory to compute contours of constant growth rate for different instability thresholds, which closely align with the limits of the data distribution, supporting that these instabilities are acting to limit extremes of ion temperature anisotropy in the Jovian magnetosheath.

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