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Scattering and apparent diameter


tex2html_wrap_inline3922   Greater path lengths for scattered photons
tex2html_wrap_inline3922   Smearing of pulses by
tex2html_wrap_inline3922   Loosely correlated with DM
tex2html_wrap_inline3922   Scattering angles are sufficient to make the apparent angular size observable - diam tex2html_wrap_inline15170
tex2html_wrap_inline3922   0.1 arcseconds at 100MHz for the Crab pulsar

Figure 14: Scattering of the Vela pulsar. From Lyne & Graham-Smith 1990 [23]

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