Dynamo action of the zonal winds in Jupiter | Astronomy & Astrophysics (A&A)

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Table 2

Definition of the models (first two columns) and different radii: radius r₁ where Rm⁽¹⁾ = 1, r₁₀ where Rm⁽¹⁾ = 10, r_Φ where Φ_O = Φ_T, and r_Θ where Θ_O = Θ_T (Cols. 3–6).

Conduct.	Flow
σ_F	U_G	0.967	0.960	0.961	0.955	2.8 × 10⁻³	1.2 × 10⁻¹	2.3 × 10⁻²

	U_Z	0.965	0.957	0.956	0.948	2.2 × 10⁻³	8.0 × 10⁻²	1.5 × 10⁻²

	U_K	0.963	0.954	0.946	0.929	3.0 × 10⁻³	4.8 × 10⁻²	9.0 × 10⁻³

σ_Z	U_G	0.960	0.956	0.956	0.953	1.8 × 10⁻³	1.5 × 10⁻¹	2.5 × 10⁻²

	U_Z	0.958	0.954	0.953	0.949	1.6 × 10⁻³	8.9 × 10⁻²	1.5 × 10⁻²

	U_K	0.957	0.952	0.948	0.942	1.7 × 10⁻³	2.9 × 10⁻²	4.9 × 10⁻³

Notes. Column 7 provides the ratio of rms radial LIF to rms radial background field at r₁. Columns 8 and 9 give ratios Φ_O∕Φ_T and Θ_O ∕Θ_T at r₁, respectively. Current density estimates j^(O) have been used.

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