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To demonstrate this, spectrograms of the same simulation @@ -53,9 +51,7 @@ After OWB, a train of small waves falls off the edges, which eventually melt together, leading to a trapezoid shape in the $$t$$-domain. Dispersive broadening then continues normally: -<a href="pheno-break-sgram.jpg"> -<img src="pheno-break-sgram-small.jpg" style="width:80%"> -</a> +{% include image.html file="spectrograms-full.png" width="100%" alt="Spectrograms of pulse shape evolution" %} We call the distance at which the wave breaks $$L_\mathrm{WB}$$, and would like to analytically predict it. @@ -183,9 +179,7 @@ $$\begin{aligned} This prediction for $$L_\mathrm{WB}$$ appears to agree well with the OWB observed in the simulation: -<a href="pheno-break.jpg"> -<img src="pheno-break-small.jpg" style="width:100%"> -</a> +{% include image.html file="simulation-full.png" width="100%" alt="Optical wave breaking simulation results" %} Because all spectral broadening up to $$L_\mathrm{WB}$$ is caused by SPM, whose frequency behaviour is known, it is in fact possible to draw diff --git a/source/know/concept/optical-wave-breaking/pheno-break-inst-small.jpg b/source/know/concept/optical-wave-breaking/pheno-break-inst-small.jpg 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