Revealing the intensity of turbulent energy transfer in planetary atmospheres
Images of the giant planets Jupiter and Saturn show highly turbulent storms and swirling clouds that reflect the intensity of turbulence in their atmospheres. Quantifying planetary turbulence is inaccessible to conventional tools, however, since they require large quantities of spatially and tempora...
Hauptverfasser: | Cabanes, S, Espa, S, Galperin, B, Young, RMB, Read, PL |
---|---|
Format: | Journal article |
Sprache: | English |
Veröffentlicht: |
Wiley
2020
|
Ähnliche Einträge
-
Predictability of a laboratory analogue for planetary atmospheres
von: Young, RMB
Veröffentlicht: (2009) -
The turbulent dynamics of Jupiter’s and Saturn’s weather layers: order out of chaos?
von: Read, PL, et al.
Veröffentlicht: (2020) -
The dynamics of planetary atmospheres
von: Taylor, F, et al.
Veröffentlicht: (1988) -
THE DYNAMICS OF PLANETARY-ATMOSPHERES
von: Taylor, F, et al.
Veröffentlicht: (1988) -
Assimilation of both column‐ and layer‐integrated dust opacity observations in the Martian atmosphere
von: Ruan, T, et al.
Veröffentlicht: (2021)