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The phenomenology of accretion disc, coronnae and jets in X-ray binaries israther well established. However the structure of the accretion flow in thevarious spectral states is still debated and the connection between the hotflow and compact jet is far from being understood. Simbol-X should addressthese two important questions in several ways. First, it will provide us withthe capability of producing high sensivity, broad band spectra and thereforeconstrain simultaneously the shape and luminosity of all spectral components(iron line, reflection bump, thermal disc and comptonised emission) which inturn provides information on the geometry of the accretion flow. It will alsodetermine the exact contribution of jets to the X-ray band both in bright andquiescent states. Finally it will shed new lights on the underlying mechanismstriggering spectral state transitions by allowing us to follow in exquisitedetails the rapid spectral evolution and its correlation with the radio jetemission during those transitions.

Accretion discs, coronae and jets in black hole binaries: prospects for Simbol-X