Recent Observations

At Black Cat we currently only have 1 camera set up to feed into the UKMON and GMN networks. We operate under Rhos_a UK001M. The camera is posistioned in a…

Meteors that enter the atmosphere have ionisation trails of excited molecules that we observe as bright streaks. Those ionised areas are more reflective to radio waves and it is this characteristic…

Introduction Radio meteor detection relies on the ionized trails left by meteors as they enter the atmosphere. These trails reflect radio waves, allowing us to detect meteors at any time…