Understanding pulsar magnetospheres with the SKA

A. Karastergiou∗1, S. Johnston2, N. Andersson3, R. Breton4, P. Brook1, C. Gwinn5, N. Lewandowska6, E. Keane7, M. Kramer8, J.-P. Macquart9, M. Serylak10, R. Shannon2, B. Stappers11, J. van Leeuwen12, J. P. W. Verbiest13, P. Weltevrede11, G. Wright14,11 1 Oxford Astrophysics, Oxford, UK. E-mail: aris@astro.ox.ac.uk; 2 CSIRO Astronomy & Space Science, Australia Telescope National Facility; 3 University of Southampton, UK; 4 University of Southampton, UK; 5 University of California, Santa Barbara, USA; 6 University of Wurzburg, Germany; 7 Swinburne University of Technology, Australia; 8 Max-Planck-Institut fuer Radioastronomie, Germany.; 9 ICRAR/Curtin Institute of Radio Astronomy, Australia; 10 University of the Western Cape, South Africa; 11 University of Manchester, UK; 12 ASTRON, The Netherlands; 13 Universitaet Bielefeld Germany; 14 University of Sussex, UK