Depth of a strong jovian jet from a planetary-scale disturbance driven by storms.

Depth of a strong jovian jet from a planetary-scale disturbance driven by storms.

The atmospheres of the gas giant planets (Jupiter and Saturn) contain jets that dominate the circulation at visible levels. The power source for these jets (solar radiation, internal heat, or both) and their vertical structure below the upper cloud are major open questions in the atmospheric circula...

Bibliografski detalji
Glavni autori:	Sánchez-Lavega, A, Orton, G, Hueso, R, García-Melendo, E, Pérez-Hoyos, S, Simon-Miller, A, Rojas, J, Gómez, J, Yanamandra-Fisher, P, Fletcher, L, Joels, J, Kemerer, J, Hora, J, Karkoschka, E, de Pater, I, Wong, M, Marcus, P, Pinilla-Alonso, N, Carvalho, F, Go, C, Parker, D, Salway, M, Valimberti, M, Wesley, A, Pujic, Z
Format:	Journal article
Jezik:	English
Izdano:	2008

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