Atmospheric erosion at Venus in the HYB simulation
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Summary
Escaping planetary atomic oxygen ions (O+) viewed by a virtual spacecraft orbiting around Venus in the HYB simulation. The colouring on two perpendicular planes and on a spherical shell just above the planet give the density of oxygen ions in a logarithmic scale (red: high density; dark blue: low de
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Details
- Source collection: Wikimedia Commons
- License: CC / Public Domain
- Category: Space