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Shallowness of circulation in hot Jupiters: Advancing the Ohmic dissipation model
H. Knierim
, K. Batygin
,
B. Bitsch
Max Planck Institute for Astronomy
California Institute of Technology
Research output
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peer-review
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Engineering
Dissipation Rate
100%
Energy Dissipation
66%
Promising Candidate
33%
Penetration Depth
33%
Magnetic Field
33%
Magnetic Field Strength
33%
Scaling Law
33%
Layer Depth
33%
Equilibrium Temperature
33%
Atmospheric Flow
33%
Physics
Hot Jupiters
100%
Magnetic Field
40%
Atmospherics
40%
Field Strength
20%
Extrasolar Planet
20%
Wind Velocity
20%
Physical Process
20%
Chemical Engineering
Joule Heating
100%
Scaling Law
100%
Chemistry
Magnetic Field
100%
Scaling Law
50%
Material Science
Joule Heating
100%