Pulsar glitch substructure and pulsar interiors

University of Tasmania, AustraliaPulsar timing at the Mt Pleasant observatory focused on Vela, which could be tracked for 18hours of the day. These nearly continuous timing records extend over 24 years allowing a greatinsight into details of timing noise, micro glitchesand other more exotic effects. It has been foundthat the spin upfor the Velapulsar occurs instantaneously to within the uncertainties of the data.The potential for new, higher resolution data, to unveil insights of the Neutron Star interiors isdiscussed.Bursts, Pulses and Flickering:Wide-field monitoring of thedynamic radio sky June 12-15 2007Kerastari, Tripolis, Greece