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...

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Detalles Bibliográficos
Autores principales:	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
Formato:	Journal article
Lenguaje:	English
Publicado:	2008

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

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