Hydrogen-neon mixtures phase-separate at substantially lower pressures than hydrogen-helium mixtures, with neon strongly stabilizing H2 molecules and suppressing electrical conductivity at planetary interior conditions.
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The spokes are modeled as a two-component system of persistent diamagnetic pyrolytic carbon and transient diamagnetic ice grains whose visibility and dynamics are controlled by electromagnetic interactions with Saturn's magnetosphere and solar elevation.
citing papers explorer
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Miscibility and Transport Properties in Hydrogen-Neon Mixtures
Hydrogen-neon mixtures phase-separate at substantially lower pressures than hydrogen-helium mixtures, with neon strongly stabilizing H2 molecules and suppressing electrical conductivity at planetary interior conditions.
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The Two-component Model of the 'spokes' in Saturn's Rings
The spokes are modeled as a two-component system of persistent diamagnetic pyrolytic carbon and transient diamagnetic ice grains whose visibility and dynamics are controlled by electromagnetic interactions with Saturn's magnetosphere and solar elevation.