Speaker
Prof.
A. Rozanska
Description
Content: the lecture will discuss timescales that are an outcome of multi-phase modelling of an inner accretion flow. In the model we consider the division of a total accretion energy is dissipated partially in an accretion disk, a warm corona responsible for soft X-ray excess and a hot corona where most hard X-ray radiation is emitted in radio quiet AGN. It will overview those timescales and put predictions on the multiwavelength observations of AGN variability.
