Parkes observations for project P842 semester 2013APRS

We propose to exploit the advanced pulsar instrumentation at the Parkes Observatory and employ novel methods of polarimetric calibration and statistical analysis to provide new insights into the rich variety of phenomena displayed by the Crab Nebula pulsar. Specifically, we will undertake baseband observations using the CASPSR system at 20 cm and 10 cm bands for the scientific objectives of (i) investigating the microstructure, and (ii) high time resolution polarimetry. With the ultra-high time resolution (2.5 ns) capabilities of CASPSR and its ability to sustain continuous recording for up to 4 hr, these observations will yield data of unprecedented quality, which will facilitate an in-depth, unbiased and accurate characterisation of giant pulses and microbursts. This will place novel constraints on pulsar emission mechanism.