  Based on a dynamical model describing how stationary, powerful and
self-collimated jets are being launched from a magnetized disk, we build a
consistent disk+jet microquasar picture. Our disk is a new type of disk
solution called the Jet Emitting Disk (JED), and whose characteristics are
directly constrained by the presence of a jet. We assume a one-temperature
plasma with thermal particles only. By solving the radiative equilibrium of the
disk, we obtain three branches of solutions, a hot and a cold ones (both
thermally stable), and an intermediate one, thermally unstable. The hot
solution possess the global observed characteristics of what has been often
called a "corona" located above the inner disk region. We present this new disk
solution, and how the radiative equilibrium is computed. We discuss the
richness of the solution, and show the ability of the model to reproduce an
observed spectral energy distribution of XTE J1118+480 with reasonable
parameters. We finally outline some perspectives of the model.
