ИСТИНА

AKR-like emissions are phenomena similar to the typical Auroral Kilometric Radiation (AKR)events, but observed by satellites at lower altitudes, as well as by the ground-based instruments.The typical Auroral Kilometric Radiation (AKR) consists of intense electromagnetic emissions generated by energetic electron beams in the Electron Cyclotron Maser process at heights over 2000 km in the auroral region, whereas the exact nature of AKR-like emissions observed in the ionosphere as well as on the ground is still not well understood. In this work, we selected observations of AKR-like emissions from the RELEC (Relativistic Electron) mission, in the time period from August to December 2014. The statistical analysis of AKR-like events observed for different invariant latitudes, magnetic local times and altitudes (in the range of 600-850 km, well below AKR sources lower height limit) will be presented. The selected events have also been divided due to the observed features that might shed light on the physical processes responsible for their origin.