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 --- .../concept/optical-wave-breaking/frequency-full.png | Bin 0 -> 66775 bytes .../concept/optical-wave-breaking/frequency-half.avif | Bin 0 -> 12506 bytes .../concept/optical-wave-breaking/frequency-half.jpg | Bin 0 -> 52244 bytes .../concept/optical-wave-breaking/frequency-half.png | Bin 0 -> 41824 bytes .../concept/optical-wave-breaking/frequency-half.webp | Bin 0 -> 27408 bytes source/know/concept/optical-wave-breaking/index.md | 12 +++--------- .../optical-wave-breaking/pheno-break-inst-small.jpg | Bin 38886 -> 0 bytes .../optical-wave-breaking/pheno-break-inst.jpg | Bin 107870 -> 0 bytes .../optical-wave-breaking/pheno-break-sgram-small.jpg | Bin 173644 -> 0 bytes .../optical-wave-breaking/pheno-break-sgram.jpg | Bin 518792 -> 0 bytes .../optical-wave-breaking/pheno-break-small.jpg | Bin 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0000000..26f4d94 Binary files /dev/null and b/source/know/concept/optical-wave-breaking/frequency-half.webp differ 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 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 deleted file mode 100644 index f7568e6..0000000 Binary files a/source/know/concept/optical-wave-breaking/pheno-break-inst-small.jpg and /dev/null differ diff --git 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