diff options
Diffstat (limited to 'content/know/concept/optical-wave-breaking/index.pdc')
| -rw-r--r-- | content/know/concept/optical-wave-breaking/index.pdc | 6 |
1 files changed, 3 insertions, 3 deletions
diff --git a/content/know/concept/optical-wave-breaking/index.pdc b/content/know/concept/optical-wave-breaking/index.pdc index 30305f5..ecd5a4f 100644 --- a/content/know/concept/optical-wave-breaking/index.pdc +++ b/content/know/concept/optical-wave-breaking/index.pdc @@ -40,7 +40,7 @@ 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"> +<img src="pheno-break-inst-small.jpg" style="width:100%"> </a> Several interesting things happen around this moment. @@ -59,7 +59,7 @@ 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%;display:block;margin:auto;"> +<img src="pheno-break-sgram-small.jpg" style="width:80%"> </a> We call the distance at which the wave breaks $L_\mathrm{WB}$, @@ -189,7 +189,7 @@ 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"> +<img src="pheno-break-small.jpg" style="width:100%"> </a> Because all spectral broadening up to $L_\mathrm{WB}$ is caused by SPM, |