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feat: add doks as a node module
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9
content/docs/examples/_index.md
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content/docs/examples/_index.md
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---
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title: "Examples"
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description: "Examples"
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lead: ""
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date: 2021-03-16T08:43:03+01:00
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lastmod: 2021-03-16T08:43:03+01:00
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draft: false
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images: []
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---
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79
content/docs/examples/code.md
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content/docs/examples/code.md
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---
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title: "Code"
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description: "Code highlighting examples."
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lead: "Code highlighting examples."
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date: 2021-03-16T08:43:34+01:00
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lastmod: 2021-03-16T08:43:34+01:00
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draft: false
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images: []
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menu:
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docs:
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parent: "examples"
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weight: 200
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toc: true
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---
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## JavaScript
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```js
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function $initHighlight(block, cls) {
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try {
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if (cls.search(/\bno\-highlight\b/) != -1)
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return process(block, true, 0x0F) +
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` class="${cls}"`;
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} catch (e) {
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/* handle exception */
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}
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for (var i = 0 / 2; i < classes.length; i++) {
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if (checkCondition(classes[i]) === undefined)
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console.log('undefined');
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}
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return (
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<div>
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<web-component>{block}</web-component>
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</div>
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)
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}
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export $initHighlight;
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```
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## JSON
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```json
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[
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{
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"title": "apples",
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"count": [12000, 20000],
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"description": {"text": "...", "sensitive": false}
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},
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{
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"title": "oranges",
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"count": [17500, null],
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"description": {"text": "...", "sensitive": false}
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}
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]
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```
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## Bash
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```bash
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#!/bin/bash
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###### CONFIG
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ACCEPTED_HOSTS="/root/.hag_accepted.conf"
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BE_VERBOSE=false
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if [ "$UID" -ne 0 ]
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then
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echo "Superuser rights required"
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exit 2
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fi
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genApacheConf(){
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echo -e "# Host ${HOME_DIR}$1/$2 :"
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}
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echo '"quoted"' | tr -d \" > text.txt
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```
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46
content/docs/examples/math.md
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content/docs/examples/math.md
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---
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title: "Math"
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description: "Math typesetting examples."
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lead: "Math typesetting examples."
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date: 2021-03-16T10:46:05+01:00
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lastmod: 2021-03-16T10:46:05+01:00
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draft: false
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images: []
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menu:
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docs:
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parent: "examples"
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weight: 210
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toc: true
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---
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[KaTeX](https://katex.org/) is switched off by default. Enable it by setting `kaTex = true` in the `[options]` section of `./config/_default/params.toml`.
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## Example 1
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_Excerpt taken from [Supernova Neutrinos](https://neutrino.leima.is/book/introduction/supernova-neutrinos/)_
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### Markdown
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```md
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The average energy of the neutrinos $\langle E \rangle$ emitted during a supernova explosion is of the order of 10MeV, and the neutrino luminosity at the early epoch of the explosion is approximately $10^{52}\mathrm{ergs\cdot s^{-1}}$.
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Therefore, the number density of the neutrinos at the radius $R$ is
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$$
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\begin{equation*}
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n \sim 10^{18} \mathrm{cm^{-3}} \left(\frac{100\mathrm{km}}{R}\right)^2 \left(\frac{10\mathrm{MeV}}{\langle E \rangle}\right).
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\end{equation*}
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$$
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```
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### HTML
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The average energy of the neutrinos $\langle E \rangle$ emitted during a supernova explosion is of the order of 10MeV, and the neutrino luminosity at the early epoch of the explosion is approximately $10^{52}\mathrm{ergs\cdot s^{-1}}$.
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Therefore, the number density of the neutrinos at the radius $R$ is
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$$
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\begin{equation*}
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n \sim 10^{18} \mathrm{cm^{-3}} \left(\frac{100\mathrm{km}}{R}\right)^2 \left(\frac{10\mathrm{MeV}}{\langle E \rangle}\right).
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\end{equation*}
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$$
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It turns out that the ambient dense neutrino medium has a significant impact on neutrino oscillations, which has been intensely investigated in the last decade.
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