. Assume astronomers discover a new planet with a characteristic horizontal velocity scale (at middle latitudes), and a rotation rate equal to Earth's. How small would a planet have to be in order that the effect of curvature term on the flow would be comparable to the Coriolis force?
. Assume astronomers discover a new planet with a characteristic horizontal velocity scale (at middle latitudes), and a rotation rate equal to Earth's. How small would a planet have to be in order that the effect of curvature term on the flow would be comparable to the Coriolis force?
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![3.11. Assume astronomers discover a new planet with a characteristic horizontal velocity scale
(at middle latitudes), and a rotation rate equal to Earth's. How small would a planet
have to be in order that the effect of curvature term on the flow would be comparable
to the Coriolis force?
The book claims the answer
is:
a = 10° m](/v2/_next/image?url=https%3A%2F%2Fcontent.bartleby.com%2Fqna-images%2Fquestion%2F335a8df7-2845-4cd4-b53b-dca022bd0cf8%2F38c0d1ba-c482-484f-86b3-56e92688739e%2Fcun42n_processed.jpeg&w=3840&q=75)
Transcribed Image Text:3.11. Assume astronomers discover a new planet with a characteristic horizontal velocity scale
(at middle latitudes), and a rotation rate equal to Earth's. How small would a planet
have to be in order that the effect of curvature term on the flow would be comparable
to the Coriolis force?
The book claims the answer
is:
a = 10° m
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