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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!