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We describe the structure of bifurcations in the unbounded classicalDiamagnetic Kepler problem. We conjecture that this system does not have anystable orbits and that the non-wandering set is described by a complete trinarysymbolic dynamics for scaled energies larger then $\epsilon_c=0.328782\ldots$.Comment: 15 pages PostScript uuencoded with figure

Bifurcations and complete chaos for the diamagnetic Kepler problem