Dynamical constraints on the vertical structure of Jupiter's polar cyclones.

Summary: Jupiter has giant, swirling storms called cyclones at its north and south poles. These storms slowly move in a circle over time. Scientists wanted to know how deep these storms go into the planet. Surprisingly, they found that shallower storms move slower than deeper ones! By studying how fast the storms move, scientists figured out a clever way to measure their depth. This new discovery will help us understand the amazing data coming from the Juno spacecraft and solve the mystery of how these giant storms form.