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

Open Access

Fig. B.1

Sky maps of the modeled distances to the inner $(r_{inner}^{ℓ_{\max} = 6}, left)$ $\left( {r_{{\rm{inner}}}^{{\ell _{\max }} = 6},{\rm{left}}} \right)$ and outer $(r_{outer}^{ℓ_{max} = 6}, right)$ $\left( {r_{{\rm{outer}}}^{{\ell _{{\rm{max}}}} = 6},{\rm{right}}} \right)$ surfaces of the shell of the Local Bubble as measured from the Sun. Projection and conventions are the same as in Fig. 4.

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