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

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