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tex2html_wrap_inline3922   Strongly polarised, up to 100%
tex2html_wrap_inline3922   Both circular and linear

Figure 57: Polarisation of pulsars

tex2html_wrap_inline3922   Smooth S-shape position angle swing
tex2html_wrap_inline3922   Not frequency dependant!
tex2html_wrap_inline3922   Independant of the number of components
tex2html_wrap_inline3922   Poln parallel to curvature of field
tex2html_wrap_inline3922   Evidence for conal curvature radiation

Figure 58:

Jon Bell
Thu Dec 19 15:15:11 GMT 1996