We study the relations between all the vacua of Lorentzian and Euclidean d=4,5,6 SUGRAs with 8 supercharges, finding a new limiting procedure that takes us from the over-rotating near-horizon BMPV black hole to the Gödel spacetime. The timelike compactification of the maximally supersymmetric Gödel solution of N=1, d=5 SUGRA gives a maximally supersymmetric solution of pure Euclidean N=2, d=4 with flat space but non-trivial anti-selfdual vector field flux ( flacuum) that, on the one hand, can be interpreted as an U(1) instanton on T 4 and that, on the other hand, coincides with the graviphoton background shown by Berkovits and Seiberg to produce the C-deformation introduced recently by Ooguri and Vafa. We construct flacuum solutions in other theories such as Euclidean type IIA supergravity.