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\@writefile{lof}{\contentsline {figure}{\numberline {2}{\ignorespaces The two portions of the back projection operator. $\bf  T_{z,ray}$ is the pair of rays through $\bf  s_{0}$ from the source to the receiver that obey Snell's law at the reflector. $\bf  T_{z,ref}$ is the raypath from this reflection point to the surface.}}{4}}
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\@writefile{lof}{\contentsline {figure}{\numberline {5}{\ignorespaces Left panel is the same model as in Figure\nobreakspace  {}\G@refundefinedtrue {\unhbox \voidb@x \hbox {\normalfont  \bfseries  ??}}\GenericWarning  {               }{LaTeX Warning: Reference `fig:depth-initial' on page 6 undefined} in tau, the right is our initial guess in tau. Note how our reflectors positions are much more accurate in the tau case compared to the depth case.}}{6}}
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\@writefile{lof}{\contentsline {figure}{\numberline {12}{\ignorespaces The difference between the operators calculated from the correct and our initial guess at velocity, for depth (left) and tau (right. Note the significant spikes at the reflector and at the lower layer boundary in the depth case.}}{12}}
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