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improved indentation and whitespace for markdown code blocks

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All code blocks in markdown have been intended by at least 4 spaces.

We add `--tab-stop=8` to all `pandoc(1)` executions in order to set
a better tab stop indentation, especially for tab intended code blocks.

Changed `bin/pandoc-wrapper.sh` VERSION from "1.5.3 2024-03-26"
to "1.6 2024-03-31".

Fixed `1991/brnstnd/sorta.README.md` so that the sorta code
is code blocks.

Removed unneeded paragraph group in copyright in `inc/footer.default.html`.

Fixed excess whitespace after list Author on entry `index.html` page.

Changed `bin/output-index-author.sh` VERSION from "1.5.2 2024-03-26"
to "1.6 2024-03-31".

Performed `make www` to perform the above and test under macOS.

TODO: Fix the problem of the initial line of code being extra intended.
TODO: Fix excess whitespace around code that is inline.
This commit is contained in:
Landon Curt Noll committed 2024-04-01 04:48:48 -07:00
1 parent b84c27ce02
commit a996f8d2b8
734 files changed
+16723 -16963
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2000/rince/README.md
+47 -47
View File
@@ -1,7 +1,7 @@
## To build:
```sh
make all
make all
```
@@ -10,7 +10,7 @@ make all
The current status of this entry is:
```
STATUS: INABIAF - please **DO NOT** fix
STATUS: INABIAF - please **DO NOT** fix
```
For more detailed information see [2000 rince bugs](../../bugs.html#2000_rince).
@@ -19,7 +19,7 @@ For more detailed information see [2000 rince bugs](../../bugs.html#2000_rince).
## To use:
```sh
./rince number number2
./rince number number2
```
If `DISPLAY` is not set the program will very likely crash or do something
@@ -29,7 +29,7 @@ different.
## Try:
```sh
./try.sh
./try.sh
```
This will run the program several times with different parameters to show
@@ -52,7 +52,7 @@ observation.
The simplest way to run it is with no arguments. Just type:
```sh
./rince
./rince
```
You will need to have access to X windows, although it doesn't require
@@ -66,7 +66,7 @@ which is used to ensure that we see the "live" pictures. Simply specify
the fraction of a day to skip forward for each screen refresh. I suggest:
```sh
./rince 0.01
./rince 0.01
```
To display the output (still guessing?) for a given date, specify two
@@ -74,8 +74,8 @@ arguments. The first argument is as before and the second argument is a
Julian day number (given as a fractional component). E.g.:
```sh
./rince 0 2441193.6
./rince 0.01 2441193.6
./rince 0 2441193.6
./rince 0.01 2441193.6
```
A Julian day is defined to be the number of days since January 1st in the year
@@ -98,10 +98,10 @@ The moons are labelled with Roman numerals from `I` to `IV`, `I` being the
closest to the planet and `IV` being the furthest. They are:
```
I Io
II Europa
III Ganymede
IV Callisto
I Io
II Europa
III Ganymede
IV Callisto
```
Amazingly, all it takes is a pair of binoculars to see the Galilean moons,
@@ -134,46 +134,46 @@ Galileo discovered the moons in January 1610.
states the following:
```
By early 1610, Galileo had further improved his telescope by
double its power, so it now enlarged objects a thousand
times. He began looking at the stars and couldn't believe how
many more he could now see! The number seemed infinite. He was
beginning to realize the fixed stars weren't a flat distant
wall on a globe, but a three-dimensional expanse bigger than
anyone had ever thought!
By early 1610, Galileo had further improved his telescope by
double its power, so it now enlarged objects a thousand
times. He began looking at the stars and couldn't believe how
many more he could now see! The number seemed infinite. He was
beginning to realize the fixed stars weren't a flat distant
wall on a globe, but a three-dimensional expanse bigger than
anyone had ever thought!
Then, on January 7, about an hour after sunset, Jupiter rose
in the east, and Galileo happened to turn his powerful scope
on its bright disk. It wasn't the first time he had looked at
Jupiter, but before it was with one of his lesser-powered
telescopes. This time, though, he noticed three small but
bright stars near the planet, two to one side and one to the
other. He wondered at how bright the small stars were and how
they were arranged in what seemed like a straight line. The
next night he decided to look at Jupiter again, and to his
surprise, the stars had moved. But not in such a way as he
would expect. If Jupiter was moving as it normally should, the
stars would be east of Jupiter. But all three were to the
west! The next night was cloudy, but on January 10, Galileo
was able to observe the planet again. One of the stars was
gone, and the other two were now on the east side. As the
stars moved around Jupiter on each succeeding night, and were
finally joined by a fourth star, it dawned on Galileo that
what he had found were moons orbiting Jupiter! Almost at once
he realized that this was proof that not all objects orbited
the Earth. Here were four bodies that were orbiting
Jupiter. One argument against the sun-centered theory was, if
the Earth orbited the sun, wouldn't the moon get left behind?
Here he could see for himself that somehow, a planet could
orbit the sun, and not leave a moon behind!
Then, on January 7, about an hour after sunset, Jupiter rose
in the east, and Galileo happened to turn his powerful scope
on its bright disk. It wasn't the first time he had looked at
Jupiter, but before it was with one of his lesser-powered
telescopes. This time, though, he noticed three small but
bright stars near the planet, two to one side and one to the
other. He wondered at how bright the small stars were and how
they were arranged in what seemed like a straight line. The
next night he decided to look at Jupiter again, and to his
surprise, the stars had moved. But not in such a way as he
would expect. If Jupiter was moving as it normally should, the
stars would be east of Jupiter. But all three were to the
west! The next night was cloudy, but on January 10, Galileo
was able to observe the planet again. One of the stars was
gone, and the other two were now on the east side. As the
stars moved around Jupiter on each succeeding night, and were
finally joined by a fourth star, it dawned on Galileo that
what he had found were moons orbiting Jupiter! Almost at once
he realized that this was proof that not all objects orbited
the Earth. Here were four bodies that were orbiting
Jupiter. One argument against the sun-centered theory was, if
the Earth orbited the sun, wouldn't the moon get left behind?
Here he could see for himself that somehow, a planet could
orbit the sun, and not leave a moon behind!
```
Thus we can plot Galileo's discoveries using the following three plots:
```sh
./rince 0 $(./dmy2jd 7.8 1 1610)
./rince 0 $(./dmy2jd 8.8 1 1610)
./rince 0 $(./dmy2jd 10.8 1 1610)
./rince 0 $(./dmy2jd 7.8 1 1610)
./rince 0 $(./dmy2jd 8.8 1 1610)
./rince 0 $(./dmy2jd 10.8 1 1610)
```
However we can go one better by seeing what Galileo would have seen if it
@@ -181,7 +181,7 @@ wasn't cloudy on the 9th. Try:
```sh
./rince 0 $(./dmy2jd 9.85 1 1610)
./rince 0 $(./dmy2jd 9.85 1 1610)
```
to see what he was missing out on. I wonder what he'd have made of that!
2000/rince/index.html
+48 -49
View File
@@ -132,8 +132,7 @@
<h2 id="author"><a name="author"></a>Author:</h2>
<ul>
<li>Name: <a href="../../authors.html#James_Bonfield">James Bonfield</a><br>
Location: <a href="../../location.html#GB">GB</a> - <em>United Kingdom of Great Britain and Northern Ireland</em> (<em>United Kingdom</em>)
<br><br></li>
Location: <a href="../../location.html#GB">GB</a> - <em>United Kingdom of Great Britain and Northern Ireland</em> (<em>United Kingdom</em>)</li>
</ul>
<!-- END: next line ends content generated by: bin/output-index-author.sh -->
@@ -142,17 +141,17 @@ Location: <a href="../../location.html#GB">GB</a> - <em>United Kingdom of Great
<!-- START: this line starts content for HTML phase 21 by: bin/pandoc-wrapper.sh via bin/md2html.sh -->
<h2 id="to-build">To build:</h2>
<div class="sourceCode" id="cb1"><pre class="sourceCode sh"><code class="sourceCode bash"><span id="cb1-1"><a href="#cb1-1" aria-hidden="true" tabindex="-1"></a><span class="fu">make</span> all</span></code></pre></div>
<div class="sourceCode" id="cb1"><pre class="sourceCode sh"><code class="sourceCode bash"><span id="cb1-1"><a href="#cb1-1" aria-hidden="true" tabindex="-1"></a> <span class="fu">make</span> all</span></code></pre></div>
<h3 id="bugs-and-misfeatures">Bugs and (Mis)features:</h3>
<p>The current status of this entry is:</p>
<pre><code>STATUS: INABIAF - please **DO NOT** fix</code></pre>
<pre><code> STATUS: INABIAF - please **DO NOT** fix</code></pre>
<p>For more detailed information see <a href="../../bugs.html#2000_rince">2000 rince bugs</a>.</p>
<h2 id="to-use">To use:</h2>
<div class="sourceCode" id="cb3"><pre class="sourceCode sh"><code class="sourceCode bash"><span id="cb3-1"><a href="#cb3-1" aria-hidden="true" tabindex="-1"></a><span class="ex">./rince</span> number number2</span></code></pre></div>
<div class="sourceCode" id="cb3"><pre class="sourceCode sh"><code class="sourceCode bash"><span id="cb3-1"><a href="#cb3-1" aria-hidden="true" tabindex="-1"></a> <span class="ex">./rince</span> number number2</span></code></pre></div>
<p>If <code>DISPLAY</code> is not set the program will very likely crash or do something
different.</p>
<h2 id="try">Try:</h2>
<div class="sourceCode" id="cb4"><pre class="sourceCode sh"><code class="sourceCode bash"><span id="cb4-1"><a href="#cb4-1" aria-hidden="true" tabindex="-1"></a><span class="ex">./try.sh</span></span></code></pre></div>
<div class="sourceCode" id="cb4"><pre class="sourceCode sh"><code class="sourceCode bash"><span id="cb4-1"><a href="#cb4-1" aria-hidden="true" tabindex="-1"></a> <span class="ex">./try.sh</span></span></code></pre></div>
<p>This will run the program several times with different parameters to show
different types of things. See the author’s remarks for more details.</p>
<h2 id="judges-remarks">Judges’ remarks:</h2>
@@ -163,7 +162,7 @@ observation.</p>
<h2 id="authors-remarks">Author’s remarks:</h2>
<h3 id="how-to-use-it">How to use it</h3>
<p>The simplest way to run it is with no arguments. Just type:</p>
<div class="sourceCode" id="cb5"><pre class="sourceCode sh"><code class="sourceCode bash"><span id="cb5-1"><a href="#cb5-1" aria-hidden="true" tabindex="-1"></a><span class="ex">./rince</span></span></code></pre></div>
<div class="sourceCode" id="cb5"><pre class="sourceCode sh"><code class="sourceCode bash"><span id="cb5-1"><a href="#cb5-1" aria-hidden="true" tabindex="-1"></a> <span class="ex">./rince</span></span></code></pre></div>
<p>You will need to have access to X windows, although it doesn’t require
desperately high resolution and there are no known limitations on colour
depth.</p>
@@ -172,12 +171,12 @@ or more to be visible. For those that cannot wait that long the program
has a built in time machine. Indeed the program knows the speed of light,
which is used to ensure that we see the “live” pictures. Simply specify
the fraction of a day to skip forward for each screen refresh. I suggest:</p>
<div class="sourceCode" id="cb6"><pre class="sourceCode sh"><code class="sourceCode bash"><span id="cb6-1"><a href="#cb6-1" aria-hidden="true" tabindex="-1"></a><span class="ex">./rince</span> 0.01</span></code></pre></div>
<div class="sourceCode" id="cb6"><pre class="sourceCode sh"><code class="sourceCode bash"><span id="cb6-1"><a href="#cb6-1" aria-hidden="true" tabindex="-1"></a> <span class="ex">./rince</span> 0.01</span></code></pre></div>
<p>To display the output (still guessing?) for a given date, specify two
arguments. The first argument is as before and the second argument is a
Julian day number (given as a fractional component). E.g.:</p>
<div class="sourceCode" id="cb7"><pre class="sourceCode sh"><code class="sourceCode bash"><span id="cb7-1"><a href="#cb7-1" aria-hidden="true" tabindex="-1"></a><span class="ex">./rince</span> 0 2441193.6</span>
<span id="cb7-2"><a href="#cb7-2" aria-hidden="true" tabindex="-1"></a><span class="ex">./rince</span> 0.01 2441193.6</span></code></pre></div>
<div class="sourceCode" id="cb7"><pre class="sourceCode sh"><code class="sourceCode bash"><span id="cb7-1"><a href="#cb7-1" aria-hidden="true" tabindex="-1"></a> <span class="ex">./rince</span> 0 2441193.6</span>
<span id="cb7-2"><a href="#cb7-2" aria-hidden="true" tabindex="-1"></a> <span class="ex">./rince</span> 0.01 2441193.6</span></code></pre></div>
<p>A Julian day is defined to be the number of days since January 1st in the year
<code>-4712 (4713BC)</code>, starting at 12 noon GMT.<a href="#fn1" class="footnote-ref" id="fnref1" role="doc-noteref"><sup>1</sup></a><a href="#fn2" class="footnote-ref" id="fnref2" role="doc-noteref"><sup>2</sup></a> To aid conversion from our time
(GMT) to Julian day there is a supplementary program named:
@@ -192,10 +191,10 @@ location on Earth, but I assure you that the
<a href="https://en.wikipedia.org/wiki/Parallax#Astronomy">parallax</a> is minimal!</p>
<p>The moons are labelled with Roman numerals from <code>I</code> to <code>IV</code>, <code>I</code> being the
closest to the planet and <code>IV</code> being the furthest. They are:</p>
<pre><code>I Io
II Europa
III Ganymede
IV Callisto</code></pre>
<pre><code> I Io
II Europa
III Ganymede
IV Callisto</code></pre>
<p>Amazingly, all it takes is a pair of binoculars to see the Galilean moons,
so the results can be experimentally checked. (Note that at present, the
best views of Jupiter are over the autumn/winter.)</p>
@@ -216,45 +215,45 @@ confusion, please consult the following chart (*):</p>
<p>Galileo discovered the moons in January 1610.
<a href="https://web.archive.org/web/20001204212000/http://www-isds.jpl.nasa.gov/cwo/cwo_54ga/html/cd/galileo.htm" class="uri">https://web.archive.org/web/20001204212000/http://www-isds.jpl.nasa.gov/cwo/cwo_54ga/html/cd/galileo.htm</a>
states the following:</p>
<pre><code>By early 1610, Galileo had further improved his telescope by
double its power, so it now enlarged objects a thousand
times. He began looking at the stars and couldn&#39;t believe how
many more he could now see! The number seemed infinite. He was
beginning to realize the fixed stars weren&#39;t a flat distant
wall on a globe, but a three-dimensional expanse bigger than
anyone had ever thought!
<pre><code> By early 1610, Galileo had further improved his telescope by
double its power, so it now enlarged objects a thousand
times. He began looking at the stars and couldn&#39;t believe how
many more he could now see! The number seemed infinite. He was
beginning to realize the fixed stars weren&#39;t a flat distant
wall on a globe, but a three-dimensional expanse bigger than
anyone had ever thought!
Then, on January 7, about an hour after sunset, Jupiter rose
in the east, and Galileo happened to turn his powerful scope
on its bright disk. It wasn&#39;t the first time he had looked at
Jupiter, but before it was with one of his lesser-powered
telescopes. This time, though, he noticed three small but
bright stars near the planet, two to one side and one to the
other. He wondered at how bright the small stars were and how
they were arranged in what seemed like a straight line. The
next night he decided to look at Jupiter again, and to his
surprise, the stars had moved. But not in such a way as he
would expect. If Jupiter was moving as it normally should, the
stars would be east of Jupiter. But all three were to the
west! The next night was cloudy, but on January 10, Galileo
was able to observe the planet again. One of the stars was
gone, and the other two were now on the east side. As the
stars moved around Jupiter on each succeeding night, and were
finally joined by a fourth star, it dawned on Galileo that
what he had found were moons orbiting Jupiter! Almost at once
he realized that this was proof that not all objects orbited
the Earth. Here were four bodies that were orbiting
Jupiter. One argument against the sun-centered theory was, if
the Earth orbited the sun, wouldn&#39;t the moon get left behind?
Here he could see for himself that somehow, a planet could
orbit the sun, and not leave a moon behind!</code></pre>
Then, on January 7, about an hour after sunset, Jupiter rose
in the east, and Galileo happened to turn his powerful scope
on its bright disk. It wasn&#39;t the first time he had looked at
Jupiter, but before it was with one of his lesser-powered
telescopes. This time, though, he noticed three small but
bright stars near the planet, two to one side and one to the
other. He wondered at how bright the small stars were and how
they were arranged in what seemed like a straight line. The
next night he decided to look at Jupiter again, and to his
surprise, the stars had moved. But not in such a way as he
would expect. If Jupiter was moving as it normally should, the
stars would be east of Jupiter. But all three were to the
west! The next night was cloudy, but on January 10, Galileo
was able to observe the planet again. One of the stars was
gone, and the other two were now on the east side. As the
stars moved around Jupiter on each succeeding night, and were
finally joined by a fourth star, it dawned on Galileo that
what he had found were moons orbiting Jupiter! Almost at once
he realized that this was proof that not all objects orbited
the Earth. Here were four bodies that were orbiting
Jupiter. One argument against the sun-centered theory was, if
the Earth orbited the sun, wouldn&#39;t the moon get left behind?
Here he could see for himself that somehow, a planet could
orbit the sun, and not leave a moon behind!</code></pre>
<p>Thus we can plot Galileo’s discoveries using the following three plots:</p>
<div class="sourceCode" id="cb11"><pre class="sourceCode sh"><code class="sourceCode bash"><span id="cb11-1"><a href="#cb11-1" aria-hidden="true" tabindex="-1"></a><span class="ex">./rince</span> 0 <span class="va">$(</span><span class="ex">./dmy2jd</span> 7.8 1 1610<span class="va">)</span></span>
<span id="cb11-2"><a href="#cb11-2" aria-hidden="true" tabindex="-1"></a><span class="ex">./rince</span> 0 <span class="va">$(</span><span class="ex">./dmy2jd</span> 8.8 1 1610<span class="va">)</span></span>
<span id="cb11-3"><a href="#cb11-3" aria-hidden="true" tabindex="-1"></a><span class="ex">./rince</span> 0 <span class="va">$(</span><span class="ex">./dmy2jd</span> 10.8 1 1610<span class="va">)</span></span></code></pre></div>
<div class="sourceCode" id="cb11"><pre class="sourceCode sh"><code class="sourceCode bash"><span id="cb11-1"><a href="#cb11-1" aria-hidden="true" tabindex="-1"></a> <span class="ex">./rince</span> 0 <span class="va">$(</span><span class="ex">./dmy2jd</span> 7.8 1 1610<span class="va">)</span></span>
<span id="cb11-2"><a href="#cb11-2" aria-hidden="true" tabindex="-1"></a> <span class="ex">./rince</span> 0 <span class="va">$(</span><span class="ex">./dmy2jd</span> 8.8 1 1610<span class="va">)</span></span>
<span id="cb11-3"><a href="#cb11-3" aria-hidden="true" tabindex="-1"></a> <span class="ex">./rince</span> 0 <span class="va">$(</span><span class="ex">./dmy2jd</span> 10.8 1 1610<span class="va">)</span></span></code></pre></div>
<p>However we can go one better by seeing what Galileo would have seen if it
wasn’t cloudy on the 9th. Try:</p>
<div class="sourceCode" id="cb12"><pre class="sourceCode sh"><code class="sourceCode bash"><span id="cb12-1"><a href="#cb12-1" aria-hidden="true" tabindex="-1"></a><span class="ex">./rince</span> 0 <span class="va">$(</span><span class="ex">./dmy2jd</span> 9.85 1 1610<span class="va">)</span></span></code></pre></div>
<div class="sourceCode" id="cb12"><pre class="sourceCode sh"><code class="sourceCode bash"><span id="cb12-1"><a href="#cb12-1" aria-hidden="true" tabindex="-1"></a> <span class="ex">./rince</span> 0 <span class="va">$(</span><span class="ex">./dmy2jd</span> 9.85 1 1610<span class="va">)</span></span></code></pre></div>
<p>to see what he was missing out on. I wonder what he’d have made of that!</p>
<p>Galileo discovered the fourth moon a few days later.</p>
<p>I’ve tried typing these dates into two Java based Jovian moon plotters,