Nonradial and nonpolytropic astrophysical outflows - X. Relativistic MHD rotating spine jets in Kerr metric

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Table 1

Set of parameters used for the four selected solutions in the Kerr metric.

	λ	κ	δ	ν	μ	l
K1	1.0	0.2	2.3	0.9	0.1	0.05

K2	1.0	0.2	1.35	0.46223	0.1	0.05

K3	1.2	0.005	2.3	0.42	0.08	0.024

K4	0.0143	1.451	3.14	0.8	0.41	0.15

Notes. K1 is the solution displayed in Figs. 4–6 (blue line). Solution K2 is displayed in Figs. 6 (red line) and 7, while solution K3 is displayed in Figs. 12 and 13. Finally, solution K4 is shown in Figs. 14 and 15.

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