From bcae81336764eb6c4cdf0f91e2fe632b625dd8b2 Mon Sep 17 00:00:00 2001
From: Prefetch
Date: Sun, 23 Oct 2022 22:18:11 +0200
Subject: Optimize and improve naming of all images in knowledge base
---
source/know/concept/optical-wave-breaking/index.md | 12 +++---------
1 file changed, 3 insertions(+), 9 deletions(-)
(limited to 'source/know/concept/optical-wave-breaking/index.md')
diff --git a/source/know/concept/optical-wave-breaking/index.md b/source/know/concept/optical-wave-breaking/index.md
index 42064ff..882749f 100644
--- a/source/know/concept/optical-wave-breaking/index.md
+++ b/source/know/concept/optical-wave-breaking/index.md
@@ -34,9 +34,7 @@ Shortly before the slope would become infinite,
small waves start "falling off" the edge of the pulse,
hence the name *wave breaking*:
-
-
-
+{% include image.html file="frequency-full.png" width="100%" alt="Instantaneous frequency profile evolution" %}
Several interesting things happen around this moment.
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:
-
-
-
+{% 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}$$ appears to agree well
with the OWB observed in the simulation:
-
-
-
+{% include image.html file="simulation-full.png" width="100%" alt="Optical wave breaking simulation results" %}
Because all spectral broadening up to $$L_\mathrm{WB}$$ is caused by SPM,
whose frequency behaviour is known, it is in fact possible to draw
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