An analytical model for the magnetic field in the thick shell of Galactic bubbles with uniform initial conditions

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Table 3

Reduced χ² for the six scenarios.

	SCO	SCA	DCO	DCA	DDO	DDA
$χ_{R M}^{2} / ndf$ $\chi _{RM}^2/{\rm{ndf}}$	0.79	0.92	1.0	0.96	0.9	0.91
$χ_{Q}^{2} / ndf$ $\chi _Q^2/{\rm{ndf}}$	1.26	1.15	1.38	2.44	1.25	1.46
$χ_{U}^{2} / ndf$ $\chi _U^2/{\rm{ndf}}$	0.85	0.78	1.04	1.75	0.75	0.86
$χ_{tot}^{2} / ndf$ $\chi _{{\rm{tot }}}^2/{\rm{ndf}}$	0.96	0.95	1.14	1.7	0.97	1.07

Notes. Values for the reduced χ² corresponding to the three maps and for the six scenarios. $χ_{tot}^{2} / ndf$ $\chi _{{\rm{tot }}}^2/{\rm{ndf}}$ results from the combination of the three maps.

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