Stunning progress has been made in low frequency radio astronomy (<300 MHz) in recent years, with the Low Frequency Array (LOFAR) leading the way. Thanks to major advances in calibration techniques and software development, LOFAR is now capable of achieving sub arc second resolution and high dynamic range, revealing unprecedented detail of the low frequency sky.
This session will present recent results from a vast range of astronomy topics such as pulsars and transients, cosmic rays, extragalactic surveys, Epoch of Reionisation, solar and cosmic magnetism.