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authorPrefetch2022-10-23 22:18:11 +0200
committerPrefetch2022-10-23 22:18:11 +0200
commitbcae81336764eb6c4cdf0f91e2fe632b625dd8b2 (patch)
treebf353d26203b6792bb2ab5d7bbb5c65819c9e0a0 /source/know/concept/optical-wave-breaking
parent16555851b6514a736c5c9d8e73de7da7fc9b6288 (diff)
Optimize and improve naming of all images in knowledge base
Diffstat (limited to 'source/know/concept/optical-wave-breaking')
-rw-r--r--source/know/concept/optical-wave-breaking/frequency-full.pngbin0 -> 66775 bytes
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-rw-r--r--source/know/concept/optical-wave-breaking/index.md12
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-rw-r--r--source/know/concept/optical-wave-breaking/simulation-full.pngbin0 -> 918927 bytes
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-rw-r--r--source/know/concept/optical-wave-breaking/spectrograms-full.pngbin0 -> 1037864 bytes
-rw-r--r--source/know/concept/optical-wave-breaking/spectrograms-half.avifbin0 -> 63914 bytes
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diff --git a/source/know/concept/optical-wave-breaking/frequency-full.png b/source/know/concept/optical-wave-breaking/frequency-full.png
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diff --git a/source/know/concept/optical-wave-breaking/index.md b/source/know/concept/optical-wave-breaking/index.md
index 42064ff..882749f 100644
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+++ 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*:
-<a href="pheno-break-inst.jpg">
-<img src="pheno-break-inst-small.jpg" style="width:100%">
-</a>
+{% 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:
-<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
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