Fig. 3
Simulated deterministic CMB temperature contributions in Bianchi VIIh cosmologies for varying x and Ωtot (left-to-right Ωtot ∈ { 0.10,0.50,0.95 }; top-to-bottom x ∈ { 0.1,0.3,0.7,1.5,6.0 }). In these maps the swirl pattern typical of Bianchi-induced temperature fluctuations is rotated from the South pole to the Galactic centre for illustrational purposes.
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