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author | Prefetch | 2021-03-01 11:45:21 +0100 |
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committer | Prefetch | 2021-03-01 11:45:21 +0100 |
commit | 20e7c96c35b922252e17fd5fc9ff0407d9bd30ca (patch) | |
tree | 540108e358c2b6906f405bf85022eab6573b5d91 /content/know/concept | |
parent | 8a72b73ec7ed7e95842cc783195004d08c541091 (diff) |
Optimize images
Diffstat (limited to 'content/know/concept')
-rw-r--r-- | content/know/concept/dispersive-broadening/index.pdc | 4 | ||||
-rw-r--r-- | content/know/concept/dispersive-broadening/pheno-disp-small.jpg | bin | 0 -> 95385 bytes | |||
-rw-r--r-- | content/know/concept/modulational-instability/index.pdc | 4 | ||||
-rw-r--r-- | content/know/concept/modulational-instability/pheno-mi-small.jpg | bin | 0 -> 72375 bytes | |||
-rw-r--r-- | content/know/concept/optical-wave-breaking/index.pdc | 12 | ||||
-rw-r--r-- | content/know/concept/optical-wave-breaking/pheno-break-inst-small.jpg | bin | 0 -> 38886 bytes | |||
-rw-r--r-- | content/know/concept/optical-wave-breaking/pheno-break-sgram-small.jpg | bin | 0 -> 173644 bytes | |||
-rw-r--r-- | content/know/concept/optical-wave-breaking/pheno-break-small.jpg | bin | 0 -> 71450 bytes | |||
-rw-r--r-- | content/know/concept/self-phase-modulation/index.pdc | 4 | ||||
-rw-r--r-- | content/know/concept/self-phase-modulation/pheno-spm-small.jpg | bin | 0 -> 121984 bytes | |||
-rw-r--r-- | content/know/concept/self-steepening/index.pdc | 4 | ||||
-rw-r--r-- | content/know/concept/self-steepening/pheno-steep-small.jpg | bin | 0 -> 91324 bytes |
12 files changed, 20 insertions, 8 deletions
diff --git a/content/know/concept/dispersive-broadening/index.pdc b/content/know/concept/dispersive-broadening/index.pdc index 7342295..f053eb6 100644 --- a/content/know/concept/dispersive-broadening/index.pdc +++ b/content/know/concept/dispersive-broadening/index.pdc @@ -64,7 +64,9 @@ This phenomenon is illustrated below for our example of a Gaussian pulse with parameter values $T_0 = 1\:\mathrm{ps}$, $P_0 = 1\:\mathrm{kW}$, $\beta_2 = -10 \:\mathrm{ps}^2/\mathrm{m}$ and $\gamma = 0$: -<img src="pheno-disp.jpg"> +<a href="pheno-disp.jpg"> +<img src="pheno-disp-small.jpg"> +</a> The **instantaneous frequency** $\omega_\mathrm{GVD}(z, t)$, which describes the dominant angular frequency at a given point in the time domain, diff --git a/content/know/concept/dispersive-broadening/pheno-disp-small.jpg b/content/know/concept/dispersive-broadening/pheno-disp-small.jpg Binary files differnew file mode 100644 index 0000000..8c70eac --- /dev/null +++ b/content/know/concept/dispersive-broadening/pheno-disp-small.jpg diff --git a/content/know/concept/modulational-instability/index.pdc b/content/know/concept/modulational-instability/index.pdc index d912c04..26d2552 100644 --- a/content/know/concept/modulational-instability/index.pdc +++ b/content/know/concept/modulational-instability/index.pdc @@ -177,7 +177,9 @@ $$\begin{aligned} = \sqrt{P_0} \sech\!\Big(\frac{t}{T_0}\Big) \end{aligned}$$ -<img src="pheno-mi.jpg"> +<a href="pheno-mi.jpg"> +<img src="pheno-mi-small.jpg"> +</a> Where $L_\mathrm{NL} = 1/(\gamma P_0)$ is the characteristic length of nonlinear effects. Note that no noise was added to the simulation; diff --git a/content/know/concept/modulational-instability/pheno-mi-small.jpg b/content/know/concept/modulational-instability/pheno-mi-small.jpg Binary files differnew file mode 100644 index 0000000..995ec81 --- /dev/null +++ b/content/know/concept/modulational-instability/pheno-mi-small.jpg diff --git a/content/know/concept/optical-wave-breaking/index.pdc b/content/know/concept/optical-wave-breaking/index.pdc index 3c509fe..757a633 100644 --- a/content/know/concept/optical-wave-breaking/index.pdc +++ b/content/know/concept/optical-wave-breaking/index.pdc @@ -39,7 +39,9 @@ Shortly before the slope would become infinite, small waves start "falling off" the edge of the pulse, hence the name *wave breaking*: -<img src="pheno-break-inst.jpg"> +<a href="pheno-break-inst.jpg"> +<img src="pheno-break-inst-small.jpg"> +</a> Several interesting things happen around this moment. To demonstrate this, spectrograms of the same simulation @@ -57,7 +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.jpg" style="width:80%;display:block;margin:auto;"> +<img src="pheno-break-sgram-small.jpg" style="width:80%;display:block;margin:auto;"> </a> We call the distance at which the wave breaks $L_\mathrm{WB}$, @@ -87,7 +89,7 @@ expression can be reduced to: $$\begin{aligned} \omega_i(z,t) \approx \frac{\beta_2 tz}{T_0^4} \bigg( 1 + 2\frac{\gamma P_0 T_0^2}{\beta_2} \exp\!\Big(\!-\!\frac{t^2}{T_0^2}\Big) \bigg) - = \frac{\beta_2 t z}{T_0^4} \bigg( 1 \pm 2 N_\mathrm{sol}^2 \exp\!\Big(\!-\!\frac{t^2}{T_0^2}\Big) \bigg) + = \frac{\beta_2 t z}{T_0^4} \bigg( 1 + 2 N_\mathrm{sol}^2 \exp\!\Big(\!-\!\frac{t^2}{T_0^2}\Big) \bigg) \end{aligned}$$ Where we have assumed $\beta_2 > 0$, @@ -183,7 +185,9 @@ $$\begin{aligned} This prediction for $L_\mathrm{WB}$ appears to agree well with the OWB observed in the simulation: -<img src="pheno-break.jpg"> +<a href="pheno-break.jpg"> +<img src="pheno-break-small.jpg"> +</a> Because all spectral broadening up to $L_\mathrm{WB}$ is caused by SPM, whose frequency behaviour is known, it is in fact possible to draw diff --git a/content/know/concept/optical-wave-breaking/pheno-break-inst-small.jpg b/content/know/concept/optical-wave-breaking/pheno-break-inst-small.jpg Binary files differnew file mode 100644 index 0000000..f7568e6 --- /dev/null +++ b/content/know/concept/optical-wave-breaking/pheno-break-inst-small.jpg diff --git a/content/know/concept/optical-wave-breaking/pheno-break-sgram-small.jpg b/content/know/concept/optical-wave-breaking/pheno-break-sgram-small.jpg Binary files differnew file mode 100644 index 0000000..3c493f2 --- /dev/null +++ b/content/know/concept/optical-wave-breaking/pheno-break-sgram-small.jpg diff --git a/content/know/concept/optical-wave-breaking/pheno-break-small.jpg b/content/know/concept/optical-wave-breaking/pheno-break-small.jpg Binary files differnew file mode 100644 index 0000000..f29a32a --- /dev/null +++ b/content/know/concept/optical-wave-breaking/pheno-break-small.jpg diff --git a/content/know/concept/self-phase-modulation/index.pdc b/content/know/concept/self-phase-modulation/index.pdc index 868fd68..1ec3fdd 100644 --- a/content/know/concept/self-phase-modulation/index.pdc +++ b/content/know/concept/self-phase-modulation/index.pdc @@ -71,7 +71,9 @@ $$\begin{aligned} A(z, t) = \sqrt{P_0} \exp\!\Big(\!-\!\frac{t^2}{2 T_0^2}\Big) \exp\!\bigg( i \gamma z P_0 \exp\!\Big(\!-\!\frac{t^2}{T_0^2}\Big) \bigg) \end{aligned}$$ -<img src="pheno-spm.jpg"> +<a href="pheno-spm.jpg"> +<img src="pheno-spm-small.jpg"> +</a> The **instantaneous frequency** $\omega_\mathrm{SPM}(z, t)$, which describes the dominant angular frequency at a given point in the time domain, diff --git a/content/know/concept/self-phase-modulation/pheno-spm-small.jpg b/content/know/concept/self-phase-modulation/pheno-spm-small.jpg Binary files differnew file mode 100644 index 0000000..6f041ec --- /dev/null +++ b/content/know/concept/self-phase-modulation/pheno-spm-small.jpg diff --git a/content/know/concept/self-steepening/index.pdc b/content/know/concept/self-steepening/index.pdc index efbdfe4..97999b7 100644 --- a/content/know/concept/self-steepening/index.pdc +++ b/content/know/concept/self-steepening/index.pdc @@ -118,7 +118,9 @@ $L_\mathrm{shock} = 0.847\,\mathrm{m}$, which turns out to be accurate, although the simulation breaks down due to insufficient resolution: -<img src="pheno-steep.jpg"> +<a href="pheno-steep.jpg"> +<img src="pheno-steep-small.jpg"> +</a> Unfortunately, self-steepening cannot be simulated perfectly: as the pulse approaches $L_\mathrm{shock}$, its spectrum broadens to infinite diff --git a/content/know/concept/self-steepening/pheno-steep-small.jpg b/content/know/concept/self-steepening/pheno-steep-small.jpg Binary files differnew file mode 100644 index 0000000..bb2a158 --- /dev/null +++ b/content/know/concept/self-steepening/pheno-steep-small.jpg |