Parkes observations for project P1031 semester 2019OCTS_01

We propose to study the pulsar emission mechanism using novel statistical methods that enable us to study the dynamics of the radio pulsar signal on short time scales (e.g. quasi-periodic sub-pulse structure, transitions between orthogonally polarized modes of emission, nulling, etc.) without needing to detect individual pulses. This pilot study will pave the way for a large-scale survey of dynamic/transient emission properties over a broad range of the pulsar population.