A model for falling tone chorus in the Earth's magnetosphere

Motivated by the fact that geomagnetic field inhomogeneity is weak close to the chorus generation region and the observational evidence that falling-tone chorus tend to have large oblique angles of propagation, we present a new model for falling-tone chorus in which we propose that they start as a marginally unstable mode. The marginally unstable mode requires the presence of a relatively large damping, which has its origins in the Landau damping of oblique waves in this collision-less environment. A marginally unstable mode produces phase-space structures that release energy changing its frequency content. We show that the present model produces results in reasonable agreement with observations.