Unveiling the Mysteries of Lightning: Exploring its fundamental Physical Processes with SKA-LOW

Lightning is a surprisingly poorly understood phenomena.

It consists of a wide variety of complex processes such as initiation, propagation, connection to ground, even emission of high-energy radiation.

However, due to the extreme challenges in observing lightning at fast time scales, small spatial scales, and behind obscuring clouds, these processes are not well understood.

In the past, interferometers such as the LOFAR radio telescope have provided unique insight and discoveries into the physics of lightning.

The new SKA-LOW being built in western Australia will provide unrivaled spectral bandwidth and sensitivity, which will be combined with high resolution resulting from large antenna baselines.

We will use SKA-LOW to observe lightning in order to explore its fundamental plasma physics, such as how it initiates and propagates.

SKA's high bandwidth will allow us to test how lightning emits VHF radiation, giving tremendous insight into precisely how the plasma behaves.

SKA's sensitivity will allow us to explore extremely faint lightning processes, such as the very first radio emission from a lightning flash.

Here, we detail the lightning physics that can be explored with SKA, as well as the observation strategy needed explore such physics.