more doc updates

This commit is contained in:
Jan Petykiewicz 2020-02-19 18:42:06 -08:00
parent 7d8901539c
commit 6e3cc1c3bd
12 changed files with 774 additions and 154 deletions

3
.gitignore vendored
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@ -63,3 +63,6 @@ target/
.*.sw[op]
*.svg
*.html

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@ -1,3 +1,15 @@
#!/bin/bash
cd ~/projects/meanas
pdoc3 --html --force --template-dir pdoc_templates -o doc .
# Approach 1: pdf to html?
#pdoc3 --pdf --force --template-dir pdoc_templates -o doc . | \
# pandoc --metadata=title:"meanas" --toc --toc-depth=4 --from=markdown+abbreviations --to=html --output=doc.html --gladtex -s -
# Approach 2: pdf to html with gladtex
pdoc3 --pdf --force --template-dir pdoc_templates -o doc . > doc.md
pandoc --metadata=title:"meanas" --from=markdown+abbreviations --to=html --output=doc.html --gladtex -s --css pdoc_templates/pdoc.css doc.md
gladtex -a -n -d _doc_mathimg -c white doc.html
# Approach 3: html with gladtex
#pdoc3 --html --force --template-dir pdoc_templates -o doc .
#find doc -iname '*.html' -exec gladtex -a -n -d _mathimg -c white {} \;

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@ -14,7 +14,20 @@ Submodules:
- `waveguide_3d`: Functions for transforming `waveguide_2d` results into 3D.
===========
================================================================
From the "Frequency domain" section of `meanas.fdmath`, we have
$$
\\begin{aligned}
\\tilde{E}_{l, \\vec{r}} &= \\tilde{E}_{\\vec{r}} e^{-\\imath \\omega l \\Delta_t} \\\\
\\tilde{J}_{l, \\vec{r}} &= \\tilde{J}_{\\vec{r}} e^{-\\imath \\omega (l - \\frac{1}{2}) \\Delta_t} \\\\
\\hat{\\nabla} \\times (\\mu^{-1}_{\\vec{r} + \\frac{1}{2}} \\cdot \\tilde{\\nabla} \\times \\tilde{E}_{\\vec{r}})
-\\Omega^2 \\epsilon_{\\vec{r}} \\cdot \\tilde{E}_{\\vec{r}} &= \\imath \\Omega \\tilde{J}_{\\vec{r}} \\\\
\\Omega &= 2 \\sin(\\omega \\Delta_t / 2) / \\Delta_t
\\end{aligned}
$$
# TODO FDFD?
# TODO PML

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@ -185,8 +185,8 @@ def e_tfsf_source(TF_region: fdfield_t,
def poynting_e_cross_h(dxes: dx_lists_t) -> Callable[[fdfield_t, fdfield_t], fdfield_t]:
"""
Generates a function that takes the single-frequency `E` and `H` fields
and calculates the cross product `E` x `H` = \\( E \\times H \\) as required
for the Poynting vector, \\( S = E \\times H \\)
and calculates the cross product `E` x `H` = $E \\times H$ as required
for the Poynting vector, $S = E \\times H$
Note:
This function also shifts the input `E` field by one cell as required

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@ -12,82 +12,82 @@ As the z-dependence is known, all the functions in this file assume a 2D grid
Consider Maxwell's equations in continuous space, in the frequency domain. Assuming
a structure with some (x, y) cross-section extending uniformly into the z dimension,
with a diagonal \\( \\epsilon \\) tensor, we have
with a diagonal $\\epsilon$ tensor, we have
$$
\\begin{align*}
\\begin{aligned}
\\nabla \\times \\vec{E}(x, y, z) &= -\\imath \\omega \\mu \\vec{H} \\\\
\\nabla \\times \\vec{H}(x, y, z) &= \\imath \\omega \\epsilon \\vec{E} \\\\
\\vec{E}(x,y,z) = (\\vec{E}_t(x, y) + E_z(x, y)\\vec{z}) e^{-\\gamma z} \\\\
\\vec{H}(x,y,z) = (\\vec{H}_t(x, y) + H_z(x, y)\\vec{z}) e^{-\\gamma z} \\\\
\\end{align*}
\\end{aligned}
$$
Expanding the first two equations into vector components, we get
$$
\\begin{align*}
\\begin{aligned}
-\\imath \\omega \\mu_{xx} H_x &= \\partial_y E_z - \\partial_z E_y \\\\
-\\imath \\omega \\mu_{yy} H_y &= \\partial_z E_x - \\partial_x E_z \\\\
-\\imath \\omega \\mu_{zz} H_z &= \\partial_x E_y - \\partial_y E_x \\\\
\\imath \\omega \\epsilon_{xx} E_x &= \\partial_y H_z - \\partial_z H_y \\\\
\\imath \\omega \\epsilon_{yy} E_y &= \\partial_z H_x - \\partial_x H_z \\\\
\\imath \\omega \\epsilon_{zz} E_z &= \\partial_x H_y - \\partial_y H_x \\\\
\\end{align*}
\\end{aligned}
$$
Substituting in our expressions for \\( \\vec{E}, \\vec{H} \\) and discretizing:
Substituting in our expressions for $\\vec{E}$, $\\vec{H}$ and discretizing:
$$
\\begin{align*}
\\begin{aligned}
-\\imath \\omega \\mu_{xx} H_x &= \\tilde{\\partial}_y E_z + \\gamma E_y \\\\
-\\imath \\omega \\mu_{yy} H_y &= -\\gamma E_x - \\tilde{\\partial}_x E_z \\\\
-\\imath \\omega \\mu_{zz} H_z &= \\tilde{\\partial}_x E_y - \\tilde{\\partial}_y E_x \\\\
\\imath \\omega \\epsilon_{xx} E_x &= \\hat{\\partial}_y H_z + \\gamma H_y \\\\
\\imath \\omega \\epsilon_{yy} E_y &= -\\gamma H_x - \\hat{\\partial}_x H_z \\\\
\\imath \\omega \\epsilon_{zz} E_z &= \\hat{\\partial}_x H_y - \\hat{\\partial}_y H_x \\\\
\\end{align*}
\\end{aligned}
$$
Rewrite the last three equations as
$$
\\begin{align*}
\\begin{aligned}
\\gamma H_y &= \\imath \\omega \\epsilon_{xx} E_x - \\hat{\\partial}_y H_z \\\\
\\gamma H_x &= -\\imath \\omega \\epsilon_{yy} E_y - \\hat{\\partial}_x H_z \\\\
\\imath \\omega E_z &= \\frac{1}{\\epsilon_{zz}} \\hat{\\partial}_x H_y - \\frac{1}{\\epsilon_{zz}} \\hat{\\partial}_y H_x \\\\
\\end{align*}
\\end{aligned}
$$
Now apply \\( \\gamma \\tilde{\\partial}_x \\) to the last equation,
then substitute in for \\( \\gamma H_x \\) and \\( \\gamma H_y \\):
Now apply $\\gamma \\tilde{\\partial}_x$ to the last equation,
then substitute in for $\\gamma H_x$ and $\\gamma H_y$:
$$
\\begin{align*}
\\begin{aligned}
\\gamma \\tilde{\\partial}_x \\imath \\omega E_z &= \\gamma \\tilde{\\partial}_x \\frac{1}{\\epsilon_{zz}} \\hat{\\partial}_x H_y
- \\gamma \\tilde{\\partial}_x \\frac{1}{\\epsilon_{zz}} \\hat{\\partial}_y H_x \\\\
&= \\tilde{\\partial}_x \\frac{1}{\\epsilon_{zz}} \\hat{\\partial}_x ( \\imath \\omega \\epsilon{xx} E_x - \\hat{\\partial}_y H_z)
- \\tilde{\\partial}_x \\frac{1}{\\epsilon_{zz}} \\hat{\\partial}_y (-\\imath \\omega \\epsilon{yy} E_y - \\hat{\\partial}_x H_z) \\\\
&= \\tilde{\\partial}_x \\frac{1}{\\epsilon_{zz}} \\hat{\\partial}_x ( \\imath \\omega \\epsilon{xx} E_x)
- \\tilde{\\partial}_x \\frac{1}{\\epsilon_{zz}} \\hat{\\partial}_y (-\\imath \\omega \\epsilon{yy} E_y) \\\\
&= \\tilde{\\partial}_x \\frac{1}{\\epsilon_{zz}} \\hat{\\partial}_x ( \\imath \\omega \\epsilon_{xx} E_x - \\hat{\\partial}_y H_z)
- \\tilde{\\partial}_x \\frac{1}{\\epsilon_{zz}} \\hat{\\partial}_y (-\\imath \\omega \\epsilon_{yy} E_y - \\hat{\\partial}_x H_z) \\\\
&= \\tilde{\\partial}_x \\frac{1}{\\epsilon_{zz}} \\hat{\\partial}_x ( \\imath \\omega \\epsilon_{xx} E_x)
- \\tilde{\\partial}_x \\frac{1}{\\epsilon_{zz}} \\hat{\\partial}_y (-\\imath \\omega \\epsilon_{yy} E_y) \\\\
\\gamma \\tilde{\\partial}_x E_z &= \\tilde{\\partial}_x \\frac{1}{\\epsilon_zz} \\hat{\\partial}_x (\\epsilon_{xx} E_x)
\\tilde{\\partial}_x \\frac{1}{\\epsilon_zz} \\hat{\\partial}_y (\\epsilon_{yy} E_y) \\\\
\\end{align*}
\\end{aligned}
$$
With a similar approach (but using \\( \\gamma \\tilde{\\partial}_y \\) instead), we can get
With a similar approach (but using $\\gamma \\tilde{\\partial}_y$ instead), we can get
$$
\\begin{align*}
\\begin{aligned}
\\gamma \\tilde{\\partial}_y E_z &= \\tilde{\\partial}_y \\frac{1}{\\epsilon_zz} \\hat{\\partial}_x (\\epsilon_{xx} E_x)
\\tilde{\\partial}_y \\frac{1}{\\epsilon_zz} \\hat{\\partial}_y (\\epsilon_{yy} E_y) \\\\
\\end{align*}
\\end{aligned}
$$
We can combine this equation for \\( \\gamma \\tilde{\\partial}_y E_z \\) with
the unused \\( \\imath \\omega \\mu_{xx} H_z \\) and \\( \\imath \\omega \\mu_{yy} H_y \\) equations to get
We can combine this equation for $\\gamma \\tilde{\\partial}_y E_z$ with
the unused $\\imath \\omega \\mu_{xx} H_z$ and $\\imath \\omega \\mu_{yy} H_y$ equations to get
$$
\\begin{align*}
\\begin{aligned}
-\\imath \\omega \\mu_{xx} \\gamma H_x &= \\gamma^2 E_y + \\tilde{\\partial}_y (
\\tilde{\\partial}_x \\frac{1}{\\epsilon_zz} \\hat{\\partial}_x (\\epsilon_{xx} E_x)
+ \\tilde{\\partial}_x \\frac{1}{\\epsilon_zz} \\hat{\\partial}_y (\\epsilon_{yy} E_y)
@ -96,30 +96,30 @@ $$
\\tilde{\\partial}_y \\frac{1}{\\epsilon_zz} \\hat{\\partial}_x (\\epsilon_{xx} E_x)
+ \\tilde{\\partial}_y \\frac{1}{\\epsilon_zz} \\hat{\\partial}_y (\\epsilon_{yy} E_y)
)\\\\
\\end{align*}
\\end{aligned}
$$
However, based on our rewritten equation for \\( \\gamma H_x \\) and the so-far unused
equation for \\( \\imath \\omega \\mu_{zz} H_z \\) we can also write
However, based on our rewritten equation for $\\gamma H_x$ and the so-far unused
equation for $\\imath \\omega \\mu_{zz} H_z$ we can also write
$$
\\begin{align*}
\\begin{aligned}
-\\imath \\omega \\mu_{xx} (\\gamma H_x) &= -\\imath \\omega \\mu_{xx} (-\\imath \\omega \\epsilon_{yy} E_y - \\hat{\\partial}_x H_z) \\\\
&= -\\omega^2 \\mu_{xx} \\epsilon_{yy} E_y
-\\imath \\omega \\mu_{xx} \\hat{\\partial}_x (
\\frac{1}{-\\imath \\omega \\mu_{zz}} (\\tilde{\\partial}_x E_y - \\tilde{\\partial}_y E_x)) \\\\
&= -\\omega^2 \\mu_{xx} \\epsilon_{yy} E_y
+\\mu_{xx} \\hat{\\partial}_x \\frac{1}{\\mu_{zz}} (\\tilde{\\partial}_x E_y - \\tilde{\\partial}_y E_x) \\\\
\\end{align*}
\\end{aligned}
$$
and, similarly,
$$
\\begin{align*}
\\begin{aligned}
-\\imath \\omega \\mu_{yy} (\\gamma H_y) &= -\\omega^2 \\mu_{yy} \\epsilon_{xx} E_x
+\\mu_{yy} \\hat{\\partial}_y \\frac{1}{\\mu_{zz}} (\\tilde{\\partial}_x E_y - \\tilde{\\partial}_y E_x) \\\\
\\end{align*}
\\end{aligned}
$$
Using these, we can construct the eigenvalue problem
@ -137,9 +137,9 @@ $$ \\beta^2 \\begin{bmatrix} E_x \\\\
E_y \\end{bmatrix}
$$
An equivalent eigenvalue problem can be formed using the \\( H_x, H_y \\) fields, if those are more convenient.
An equivalent eigenvalue problem can be formed using the $H_x$ and $H_y$ fields, if those are more convenient.
Note that \\( E_z \\) was never discretized, so \\( \\gamma \\) and \\( \\beta \\) will need adjustment
Note that $E_z$ was never discretized, so $\\gamma$ and $\\beta$ will need adjustment
to account for numerical dispersion if the result is introduced into a space with a discretized z-axis.
@ -187,8 +187,8 @@ def operator_e(omega: complex,
\\begin{bmatrix} \\hat{\\partial}_x \\epsilon_{xx} & \\hat{\\partial}_y \\epsilon_{yy} \\end{bmatrix}
$$
\\( \\tilde{\\partial}_x \\) and \\( \\hat{\\partial}_x \\) are the forward and backward derivatives along x,
and each \\( \\epsilon_{xx}, \\mu_{yy}, \\) etc. is a diagonal matrix containing the vectorized material
$\\tilde{\\partial}_x$ and $\\hat{\\partial}_x$ are the forward and backward derivatives along x,
and each $\\epsilon_{xx}$, $\\mu_{yy}$, etc. is a diagonal matrix containing the vectorized material
property distribution.
This operator can be used to form an eigenvalue problem of the form
@ -253,8 +253,8 @@ def operator_h(omega: complex,
\\begin{bmatrix} \\tilde{\\partial}_x \\mu_{xx} & \\tilde{\\partial}_y \\mu_{yy} \\end{bmatrix}
$$
\\( \\tilde{\\partial}_x \\) and \\( \\hat{\\partial}_x \\) are the forward and backward derivatives along x,
and each \\( \\epsilon_{xx}, \\mu_{yy}, \\) etc. is a diagonal matrix containing the vectorized material
$\\tilde{\\partial}_x$ and $\\hat{\\partial}_x$ are the forward and backward derivatives along x,
and each $\\epsilon_{xx}$, $\\mu_{yy}$, etc. is a diagonal matrix containing the vectorized material
property distribution.
This operator can be used to form an eigenvalue problem of the form

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@ -43,11 +43,11 @@ Scalar derivatives and cell shifts
----------------------------------
Define the discrete forward derivative as
$$ [\\tilde{\\partial}_x f ]_{m + \\frac{1}{2}} = \\frac{1}{\\Delta_{x, m}} (f_{m + 1} - f_m) $$
where \\( f \\) is a function defined at discrete locations on the x-axis (labeled using \\( m \\)).
The value at \\( m \\) occupies a length \\( \\Delta_{x, m} \\) along the x-axis. Note that \\( m \\)
$$ [\\tilde{\\partial}_x f]_{m + \\frac{1}{2}} = \\frac{1}{\\Delta_{x, m}} (f_{m + 1} - f_m) $$
where $f$ is a function defined at discrete locations on the x-axis (labeled using $m$).
The value at $m$ occupies a length $\\Delta_{x, m}$ along the x-axis. Note that $m$
is an index along the x-axis, _not_ necessarily an x-coordinate, since each length
\\( \\Delta_{x, m}, \\Delta_{x, m+1}, ...\\) is independently chosen.
$\\Delta_{x, m}, \\Delta_{x, m+1}, ...$ is independently chosen.
If we treat `f` as a 1D array of values, with the `i`-th value `f[i]` taking up a length `dx[i]`
along the x-axis, the forward derivative is
@ -62,7 +62,7 @@ Likewise, discrete reverse derivative is
deriv_back(f)[i] = (f[i] - f[i - 1]) / dx[i]
The derivatives' values are shifted by a half-cell relative to the original function, and
will have different cell widths if all the `dx[i]` ( \\( \\Delta_{x, m} \\) ) are not
will have different cell widths if all the `dx[i]` ( $\\Delta_{x, m}$ ) are not
identical:
[figure: derivatives and cell sizes]
@ -87,19 +87,20 @@ identical:
Periodic boundaries are used here and elsewhere unless otherwise noted.
In the above figure,
`f0 =` \\(f_0\\), `f1 =` \\(f_1\\)
`Df0 =` \\([\\tilde{\\partial}f]_{0 + \\frac{1}{2}}\\)
`Df1 =` \\([\\tilde{\\partial}f]_{1 + \\frac{1}{2}}\\)
`df0 =` \\([\\hat{\\partial}f]_{0 - \\frac{1}{2}}\\)
`f0 =` $f_0$, `f1 =` $f_1$
`Df0 =` $[\\tilde{\\partial}f]_{0 + \\frac{1}{2}}$
`Df1 =` $[\\tilde{\\partial}f]_{1 + \\frac{1}{2}}$
`df0 =` $[\\hat{\\partial}f]_{0 - \\frac{1}{2}}$
etc.
The fractional subscript \\( m + \\frac{1}{2} \\) is used to indicate values defined
at shifted locations relative to the original \\( m \\), with corresponding lengths
The fractional subscript $m + \\frac{1}{2}$ is used to indicate values defined
at shifted locations relative to the original $m$, with corresponding lengths
$$ \\Delta_{x, m + \\frac{1}{2}} = \\frac{1}{2} * (\\Delta_{x, m} + \\Delta_{x, m + 1}) $$
Just as \\( m \\) is not itself an x-coordinate, neither is \\( m + \\frac{1}{2} \\);
Just as $m$ is not itself an x-coordinate, neither is $m + \\frac{1}{2}$;
carefully note the positions of the various cells in the above figure vs their labels.
If the positions labeled with \\( m \\) are considered the "base" or "original" grid,
the positions labeled with \\( m + \\frac{1}{2} \\) are said to lie on a "dual" or
If the positions labeled with $m$ are considered the "base" or "original" grid,
the positions labeled with $m + \\frac{1}{2}$ are said to lie on a "dual" or
"derived" grid.
For the remainder of the `Discrete calculus` section, all figures will show
@ -201,8 +202,8 @@ There are also two divergences,
where `g = [gx, gy, gz]` is a fore- or back-vector field.
Since we applied the forward divergence to the back-vector (and vice-versa), the resulting scalar value
is defined at the back-vector's (fore-vectors) location \\( (m,n,p) \\) and not at the locations of its components
\\( (m \\pm \\frac{1}{2},n,p) \\) etc.
is defined at the back-vector's (fore-vector's) location $(m,n,p)$ and not at the locations of its components
$(m \\pm \\frac{1}{2},n,p)$ etc.
[figure: divergence]
^^
@ -226,23 +227,23 @@ Curls
The two curls are then
$$ \\begin{align*}
$$ \\begin{aligned}
\\hat{h}_{m + \\frac{1}{2}, n + \\frac{1}{2}, p + \\frac{1}{2}} &= \\\\
[\\tilde{\\nabla} \\times \\tilde{g}]_{m + \\frac{1}{2}, n + \\frac{1}{2}, p + \\frac{1}{2}} &=
\\vec{x} (\\tilde{\\partial}_y g^z_{m,n,p + \\frac{1}{2}} - \\tilde{\\partial}_z g^y_{m,n + \\frac{1}{2},p}) \\\\
&+ \\vec{y} (\\tilde{\\partial}_z g^x_{m + \\frac{1}{2},n,p} - \\tilde{\\partial}_x g^z_{m,n,p + \\frac{1}{2}}) \\\\
&+ \\vec{z} (\\tilde{\\partial}_x g^y_{m,n + \\frac{1}{2},p} - \\tilde{\\partial}_y g^z_{m + \\frac{1}{2},n,p})
\\end{align*} $$
\\end{aligned} $$
and
$$ \\tilde{h}_{m - \\frac{1}{2}, n - \\frac{1}{2}, p - \\frac{1}{2}} =
[\\hat{\\nabla} \\times \\hat{g}]_{m - \\frac{1}{2}, n - \\frac{1}{2}, p - \\frac{1}{2}} $$
where \\( \\hat{g} \\) and \\( \\tilde{g} \\) are located at \\((m,n,p)\\)
with components at \\( (m \\pm \\frac{1}{2},n,p) \\) etc.,
while \\( \\hat{h} \\) and \\( \\tilde{h} \\) are located at \\((m \\pm \\frac{1}{2}, n \\pm \\frac{1}{2}, p \\pm \\frac{1}{2})\\)
with components at \\((m, n \\pm \\frac{1}{2}, p \\pm \\frac{1}{2})\\) etc.
where $\\hat{g}$ and $\\tilde{g}$ are located at $(m,n,p)$
with components at $(m \\pm \\frac{1}{2},n,p)$ etc.,
while $\\hat{h}$ and $\\tilde{h}$ are located at $(m \\pm \\frac{1}{2}, n \\pm \\frac{1}{2}, p \\pm \\frac{1}{2})$
with components at $(m, n \\pm \\frac{1}{2}, p \\pm \\frac{1}{2})$ etc.
[code: curls]
@ -286,27 +287,27 @@ Maxwell's Equations
If we discretize both space (m,n,p) and time (l), Maxwell's equations become
$$ \\begin{align*}
$$ \\begin{aligned}
\\tilde{\\nabla} \\times \\tilde{E}_{l,\\vec{r}} &= -\\tilde{\\partial}_t \\hat{B}_{l-\\frac{1}{2}, \\vec{r} + \\frac{1}{2}}
- \\hat{M}_{l, \\vec{r} + \\frac{1}{2}} \\\\
\\hat{\\nabla} \\times \\hat{H}_{l-\\frac{1}{2},\\vec{r} + \\frac{1}{2}} &= \\hat{\\partial}_t \\tilde{D}_{l, \\vec{r}}
+ \\tilde{J}_{l-\\frac{1}{2},\\vec{r}} \\\\
\\tilde{\\nabla} \\cdot \\hat{B}_{l-\\frac{1}{2}, \\vec{r} + \\frac{1}{2}} &= 0 \\\\
\\hat{\\nabla} \\cdot \\tilde{D}_{l,\\vec{r}} &= \\rho_{l,\\vec{r}}
\\end{align*} $$
\\end{aligned} $$
with
$$ \\begin{align*}
\\hat{B}_\\vec{r} &= \\mu_{\\vec{r} + \\frac{1}{2}} \\cdot \\hat{H}_{\\vec{r} + \\frac{1}{2}} \\\\
\\tilde{D}_\\vec{r} &= \\epsilon_\\vec{r} \\cdot \\tilde{E}_\\vec{r}
\\end{align*} $$
$$ \\begin{aligned}
\\hat{B}_{\\vec{r}} &= \\mu_{\\vec{r} + \\frac{1}{2}} \\cdot \\hat{H}_{\\vec{r} + \\frac{1}{2}} \\\\
\\tilde{D}_{\\vec{r}} &= \\epsilon_{\\vec{r}} \\cdot \\tilde{E}_{\\vec{r}}
\\end{aligned} $$
where the spatial subscripts are abbreviated as \\( \\vec{r} = (m, n, p) \\) and
\\( \\vec{r} + \\frac{1}{2} = (m + \\frac{1}{2}, n + \\frac{1}{2}, p + \\frac{1}{2}) \\),
\\( \\tilde{E} \\) and \\( \\hat{H} \\) are the electric and magnetic fields,
\\( \\tilde{J} \\) and \\( \\hat{M} \\) are the electric and magnetic current distributions,
and \\( \\epsilon \\) and \\( \\mu \\) are the dielectric permittivity and magnetic permeability.
where the spatial subscripts are abbreviated as $\\vec{r} = (m, n, p)$ and
$\\vec{r} + \\frac{1}{2} = (m + \\frac{1}{2}, n + \\frac{1}{2}, p + \\frac{1}{2})$,
$\\tilde{E}$ and $\\hat{H}$ are the electric and magnetic fields,
$\\tilde{J}$ and $\\hat{M}$ are the electric and magnetic current distributions,
and $\\epsilon$ and $\\mu$ are the dielectric permittivity and magnetic permeability.
The above is Yee's algorithm, written in a form analogous to Maxwell's equations.
The time derivatives can be expanded to form the update equations:
@ -375,12 +376,12 @@ and combining them with charge continuity,
Wave equation
-------------
Taking the backward curl of the \\( \\tilde{\\nabla} \\times \\tilde{E} \\) equation and
replacing the resulting \\( \\hat{\\nabla} \\times \\hat{H} \\) term using its respective equation,
and setting \\( \\hat{M} \\) to zero, we can form the discrete wave equation:
Taking the backward curl of the $\\tilde{\\nabla} \\times \\tilde{E}$ equation and
replacing the resulting $\\hat{\\nabla} \\times \\hat{H}$ term using its respective equation,
and setting $\\hat{M}$ to zero, we can form the discrete wave equation:
$$
\\begin{align*}
\\begin{aligned}
\\tilde{\\nabla} \\times \\tilde{E}_{l,\\vec{r}} &=
-\\tilde{\\partial}_t \\hat{B}_{l-\\frac{1}{2}, \\vec{r} + \\frac{1}{2}}
- \\hat{M}_{l-1, \\vec{r} + \\frac{1}{2}} \\\\
@ -391,11 +392,11 @@ $$
\\hat{\\nabla} \\times (\\mu^{-1}_{\\vec{r} + \\frac{1}{2}} \\cdot \\tilde{\\nabla} \\times \\tilde{E}_{l,\\vec{r}}) &=
-\\tilde{\\partial}_t \\hat{\\nabla} \\times \\hat{H}_{l-\\frac{1}{2}, \\vec{r} + \\frac{1}{2}} \\\\
\\hat{\\nabla} \\times (\\mu^{-1}_{\\vec{r} + \\frac{1}{2}} \\cdot \\tilde{\\nabla} \\times \\tilde{E}_{l,\\vec{r}}) &=
-\\tilde{\\partial}_t \\hat{\\partial}_t \\epsilon_\\vec{r} \\tilde{E}_{l, \\vec{r}} + \\hat{\\partial}_t \\tilde{J}_{l-\\frac{1}{2},\\vec{r}} \\\\
-\\tilde{\\partial}_t \\hat{\\partial}_t \\epsilon_{\\vec{r}} \\tilde{E}_{l, \\vec{r}} + \\hat{\\partial}_t \\tilde{J}_{l-\\frac{1}{2},\\vec{r}} \\\\
\\hat{\\nabla} \\times (\\mu^{-1}_{\\vec{r} + \\frac{1}{2}} \\cdot \\tilde{\\nabla} \\times \\tilde{E}_{l,\\vec{r}})
+ \\tilde{\\partial}_t \\hat{\\partial}_t \\epsilon_\\vec{r} \\cdot \\tilde{E}_{l, \\vec{r}}
+ \\tilde{\\partial}_t \\hat{\\partial}_t \\epsilon_{\\vec{r}} \\cdot \\tilde{E}_{l, \\vec{r}}
&= \\tilde{\\partial}_t \\tilde{J}_{l - \\frac{1}{2}, \\vec{r}}
\\end{align*}
\\end{aligned}
$$
@ -405,27 +406,27 @@ Frequency domain
We can substitute in a time-harmonic fields
$$
\\begin{align*}
\\tilde{E}_\\vec{r} &= \\tilde{E}_\\vec{r} e^{-\\imath \\omega l \\Delta_t} \\\\
\\tilde{J}_\\vec{r} &= \\tilde{J}_\\vec{r} e^{-\\imath \\omega (l - \\frac{1}{2}) \\Delta_t}
\\end{align*}
\\begin{aligned}
\\tilde{E}_{l, \\vec{r}} &= \\tilde{E}_{\\vec{r}} e^{-\\imath \\omega l \\Delta_t} \\\\
\\tilde{J}_{l, \\vec{r}} &= \\tilde{J}_{\\vec{r}} e^{-\\imath \\omega (l - \\frac{1}{2}) \\Delta_t}
\\end{aligned}
$$
resulting in
$$
\\begin{align*}
\\begin{aligned}
\\tilde{\\partial}_t &\\Rightarrow (e^{ \\imath \\omega \\Delta_t} - 1) / \\Delta_t = \\frac{-2 \\imath}{\\Delta_t} \\sin(\\omega \\Delta_t / 2) e^{-\\imath \\omega \\Delta_t / 2} = -\\imath \\Omega e^{-\\imath \\omega \\Delta_t / 2}\\\\
\\hat{\\partial}_t &\\Rightarrow (1 - e^{-\\imath \\omega \\Delta_t}) / \\Delta_t = \\frac{-2 \\imath}{\\Delta_t} \\sin(\\omega \\Delta_t / 2) e^{ \\imath \\omega \\Delta_t / 2} = -\\imath \\Omega e^{ \\imath \\omega \\Delta_t / 2}\\\\
\\Omega &= 2 \\sin(\\omega \\Delta_t / 2) / \\Delta_t
\\end{align*}
\\end{aligned}
$$
This gives the frequency-domain wave equation,
$$
\\hat{\\nabla} \\times (\\mu^{-1}_{\\vec{r} + \\frac{1}{2}} \\cdot \\tilde{\\nabla} \\times \\tilde{E}_\\vec{r})
-\\Omega^2 \\epsilon_\\vec{r} \\cdot \\tilde{E}_\\vec{r} = \\imath \\Omega \\tilde{J}_\\vec{r}
\\hat{\\nabla} \\times (\\mu^{-1}_{\\vec{r} + \\frac{1}{2}} \\cdot \\tilde{\\nabla} \\times \\tilde{E}_{\\vec{r}})
-\\Omega^2 \\epsilon_{\\vec{r}} \\cdot \\tilde{E}_{\\vec{r}} = \\imath \\Omega \\tilde{J}_{\\vec{r}}
$$
@ -435,69 +436,69 @@ Plane waves and Dispersion relation
With uniform material distribution and no sources
$$
\\begin{align*}
\\begin{aligned}
\\mu_{\\vec{r} + \\frac{1}{2}} &= \\mu \\\\
\\epsilon_\\vec{r} &= \\epsilon \\\\
\\tilde{J}_\\vec{r} &= 0 \\\\
\\end{align*}
\\epsilon_{\\vec{r}} &= \\epsilon \\\\
\\tilde{J}_{\\vec{r}} &= 0 \\\\
\\end{aligned}
$$
the frequency domain wave equation simplifies to
$$ \\hat{\\nabla} \\times \\tilde{\\nabla} \\times \\tilde{E}_\\vec{r} - \\Omega^2 \\epsilon \\mu \\tilde{E}_\\vec{r} = 0 $$
$$ \\hat{\\nabla} \\times \\tilde{\\nabla} \\times \\tilde{E}_{\\vec{r}} - \\Omega^2 \\epsilon \\mu \\tilde{E}_{\\vec{r}} = 0 $$
Since \\( \\hat{\\nabla} \\cdot \\tilde{E}_\\vec{r} = 0 \\), we can simplify
Since $\\hat{\\nabla} \\cdot \\tilde{E}_{\\vec{r}} = 0$, we can simplify
$$
\\begin{align*}
\\hat{\\nabla} \\times \\tilde{\\nabla} \\times \\tilde{E}_\\vec{r}
&= \\tilde{\\nabla}(\\hat{\\nabla} \\cdot \\tilde{E}_\\vec{r}) - \\hat{\\nabla} \\cdot \\tilde{\\nabla} \\tilde{E}_\\vec{r} \\\\
&= - \\hat{\\nabla} \\cdot \\tilde{\\nabla} \\tilde{E}_\\vec{r} \\\\
&= - \\tilde{\\nabla}^2 \\tilde{E}_\\vec{r}
\\end{align*}
\\begin{aligned}
\\hat{\\nabla} \\times \\tilde{\\nabla} \\times \\tilde{E}_{\\vec{r}}
&= \\tilde{\\nabla}(\\hat{\\nabla} \\cdot \\tilde{E}_{\\vec{r}}) - \\hat{\\nabla} \\cdot \\tilde{\\nabla} \\tilde{E}_{\\vec{r}} \\\\
&= - \\hat{\\nabla} \\cdot \\tilde{\\nabla} \\tilde{E}_{\\vec{r}} \\\\
&= - \\tilde{\\nabla}^2 \\tilde{E}_{\\vec{r}}
\\end{aligned}
$$
and we get
$$ \\tilde{\\nabla}^2 \\tilde{E}_\\vec{r} + \\Omega^2 \\epsilon \\mu \\tilde{E}_\\vec{r} = 0 $$
$$ \\tilde{\\nabla}^2 \\tilde{E}_{\\vec{r}} + \\Omega^2 \\epsilon \\mu \\tilde{E}_{\\vec{r}} = 0 $$
We can convert this to three scalar-wave equations of the form
$$ (\\tilde{\\nabla}^2 + K^2) \\phi_\\vec{r} = 0 $$
$$ (\\tilde{\\nabla}^2 + K^2) \\phi_{\\vec{r}} = 0 $$
with \\( K^2 = \\Omega^2 \\mu \\epsilon \\). Now we let
with $K^2 = \\Omega^2 \\mu \\epsilon$. Now we let
$$ \\phi_\\vec{r} = A e^{\\imath (k_x m \\Delta_x + k_y n \\Delta_y + k_z p \\Delta_z)} $$
$$ \\phi_{\\vec{r}} = A e^{\\imath (k_x m \\Delta_x + k_y n \\Delta_y + k_z p \\Delta_z)} $$
resulting in
$$
\\begin{align*}
\\begin{aligned}
\\tilde{\\partial}_x &\\Rightarrow (e^{ \\imath k_x \\Delta_x} - 1) / \\Delta_t = \\frac{-2 \\imath}{\\Delta_x} \\sin(k_x \\Delta_x / 2) e^{ \\imath k_x \\Delta_x / 2} = \\imath K_x e^{ \\imath k_x \\Delta_x / 2}\\\\
\\hat{\\partial}_x &\\Rightarrow (1 - e^{-\\imath k_x \\Delta_x}) / \\Delta_t = \\frac{-2 \\imath}{\\Delta_x} \\sin(k_x \\Delta_x / 2) e^{-\\imath k_x \\Delta_x / 2} = \\imath K_x e^{-\\imath k_x \\Delta_x / 2}\\\\
K_x &= 2 \\sin(k_x \\Delta_x / 2) / \\Delta_x \\\\
\\end{align*}
\\end{aligned}
$$
with similar expressions for the y and z dimnsions (and \\( K_y, K_z \\)).
with similar expressions for the y and z dimnsions (and $K_y, K_z$).
This implies
$$
\\tilde{\\nabla}^2 = -(K_x^2 + K_y^2 + K_z^2) \\phi_\\vec{r} \\\\
\\tilde{\\nabla}^2 = -(K_x^2 + K_y^2 + K_z^2) \\phi_{\\vec{r}} \\\\
K_x^2 + K_y^2 + K_z^2 = \\Omega^2 \\mu \\epsilon = \\Omega^2 / c^2
$$
where \\( c = \\sqrt{\\mu \\epsilon} \\).
where $c = \\sqrt{\\mu \\epsilon}$.
Assuming real \\( (k_x, k_y, k_z), \\omega \\) will be real only if
Assuming real $(k_x, k_y, k_z), \\omega$ will be real only if
$$ c^2 \\Delta_t^2 = \\frac{\\Delta_t^2}{\\mu \\epsilon} < 1/(\\frac{1}{\\Delta_x^2} + \\frac{1}{\\Delta_y^2} + \\frac{1}{\\Delta_z^2}) $$
If \\( \\Delta_x = \\Delta_y = \\Delta_z \\), this simplifies to \\( c \\Delta_t < \\Delta_x / \\sqrt{3} \\).
If $\\Delta_x = \\Delta_y = \\Delta_z$, this simplifies to $c \\Delta_t < \\Delta_x / \\sqrt{3}$.
This last form can be interpreted as enforcing causality; the distance that light
travels in one timestep (i.e., \\( c \\Delta_t \\)) must be less than the diagonal
of the smallest cell ( \\( \\Delta_x / \\sqrt{3} \\) when on a uniform cubic grid).
travels in one timestep (i.e., $c \\Delta_t$) must be less than the diagonal
of the smallest cell ( $\\Delta_x / \\sqrt{3}$ when on a uniform cubic grid).
Grid description
@ -513,9 +514,9 @@ To get a better sense of how this works, let's start by drawing a grid with unif
to make the illustration simpler; we need at least two cells in the x dimension to
demonstrate how nonuniform `dx` affects the various components.
Place the E fore-vectors at integer indices \\( r = (m, n, p) \\) and the H back-vectors
at fractional indices \\( r + \\frac{1}{2} = (m + \\frac{1}{2}, n + \\frac{1}{2},
p + \\frac{1}{2}) \\). Remember that these are indices and not coordinates; they can
Place the E fore-vectors at integer indices $r = (m, n, p)$ and the H back-vectors
at fractional indices $r + \\frac{1}{2} = (m + \\frac{1}{2}, n + \\frac{1}{2},
p + \\frac{1}{2})$. Remember that these are indices and not coordinates; they can
correspond to arbitrary (monotonically increasing) coordinates depending on the cell widths.
Draw lines to denote the planes on which the H components and back-vectors are defined.

View File

@ -63,7 +63,7 @@ def curl_forward(dx_e: List[numpy.ndarray] = None) -> fdfield_updater_t:
Returns:
Function `f` for taking the discrete forward curl of a field,
`f(E)` -> curlE \\( = \\nabla_f \\times E \\)
`f(E)` -> curlE $= \\nabla_f \\times E$
"""
Dx, Dy, Dz = deriv_forward(dx_e)
@ -90,7 +90,7 @@ def curl_back(dx_h: List[numpy.ndarray] = None) -> fdfield_updater_t:
Returns:
Function `f` for taking the discrete backward curl of a field,
`f(H)` -> curlH \\( = \\nabla_b \\times H \\)
`f(H)` -> curlH $= \\nabla_b \\times H$
"""
Dx, Dy, Dz = deriv_back(dx_h)

View File

@ -13,7 +13,7 @@ we have
$$ c^2 \\Delta_t^2 = \\frac{\\Delta_t^2}{\\mu \\epsilon} < 1/(\\frac{1}{\\Delta_x^2} + \\frac{1}{\\Delta_y^2} + \\frac{1}{\\Delta_z^2}) $$
or, if \\( \\Delta_x = \\Delta_y = \\Delta_z \\), then \\( c \\Delta_t < \\frac{\\Delta_x}{\\sqrt{3}} \\).
or, if $\\Delta_x = \\Delta_y = \\Delta_z$, then $c \\Delta_t < \\frac{\\Delta_x}{\\sqrt{3}}$.
Based on this, we can set
@ -27,21 +27,21 @@ Poynting Vector and Energy Conservation
Let
$$ \\begin{align*}
$$ \\begin{aligned}
\\tilde{S}_{l, l', \\vec{r}} &=& &\\tilde{E}_{l, \\vec{r}} \\otimes \\hat{H}_{l', \\vec{r} + \\frac{1}{2}} \\\\
&=& &\\vec{x} (\\tilde{E}^y_{l,m+1,n,p} \\hat{H}^z_{l',\\vec{r} + \\frac{1}{2}} - \\tilde{E}^z_{l,m+1,n,p} \\hat{H}^y_{l', \\vec{r} + \\frac{1}{2}}) \\\\
& &+ &\\vec{y} (\\tilde{E}^z_{l,m,n+1,p} \\hat{H}^x_{l',\\vec{r} + \\frac{1}{2}} - \\tilde{E}^x_{l,m,n+1,p} \\hat{H}^z_{l', \\vec{r} + \\frac{1}{2}}) \\\\
& &+ &\\vec{z} (\\tilde{E}^x_{l,m,n,p+1} \\hat{H}^y_{l',\\vec{r} + \\frac{1}{2}} - \\tilde{E}^y_{l,m,n,p+1} \\hat{H}^z_{l', \\vec{r} + \\frac{1}{2}})
\\end{align*}
\\end{aligned}
$$
where \\( \\vec{r} = (m, n, p) \\) and \\( \\otimes \\) is a modified cross product
in which the \\( \\tilde{E} \\) terms are shifted as indicated.
where $\\vec{r} = (m, n, p)$ and $\\otimes$ is a modified cross product
in which the $\\tilde{E}$ terms are shifted as indicated.
By taking the divergence and rearranging terms, we can show that
$$
\\begin{align*}
\\begin{aligned}
\\hat{\\nabla} \\cdot \\tilde{S}_{l, l', \\vec{r}}
&= \\hat{\\nabla} \\cdot (\\tilde{E}_{l, \\vec{r}} \\otimes \\hat{H}_{l', \\vec{r} + \\frac{1}{2}}) \\\\
&= \\hat{H}_{l', \\vec{r} + \\frac{1}{2}} \\cdot \\tilde{\\nabla} \\times \\tilde{E}_{l, \\vec{r}} -
@ -49,30 +49,30 @@ $$
&= \\hat{H}_{l', \\vec{r} + \\frac{1}{2}} \\cdot
(-\\tilde{\\partial}_t \\mu_{\\vec{r} + \\frac{1}{2}} \\hat{H}_{l - \\frac{1}{2}, \\vec{r} + \\frac{1}{2}} -
\\hat{M}_{l-1, \\vec{r} + \\frac{1}{2}}) -
\\tilde{E}_{l, \\vec{r}} \\cdot (\\hat{\\partial}_t \\tilde{\\epsilon}_\\vec{r} \\tilde{E}_{l'+\\frac{1}{2}, \\vec{r}} +
\\tilde{E}_{l, \\vec{r}} \\cdot (\\hat{\\partial}_t \\tilde{\\epsilon}_{\\vec{r}} \\tilde{E}_{l'+\\frac{1}{2}, \\vec{r}} +
\\tilde{J}_{l', \\vec{r}}) \\\\
&= \\hat{H}_{l'} \\cdot (-\\mu / \\Delta_t)(\\hat{H}_{l + \\frac{1}{2}} - \\hat{H}_{l - \\frac{1}{2}}) -
\\tilde{E}_l \\cdot (\\epsilon / \\Delta_t )(\\tilde{E}_{l'+\\frac{1}{2}} - \\tilde{E}_{l'-\\frac{1}{2}})
- \\hat{H}_{l'} \\cdot \\hat{M}_{l-1} - \\tilde{E}_l \\cdot \\tilde{J}_{l'} \\\\
\\end{align*}
\\end{aligned}
$$
where in the last line the spatial subscripts have been dropped to emphasize
the time subscripts \\( l, l' \\), i.e.
the time subscripts $l, l'$, i.e.
$$
\\begin{align*}
\\begin{aligned}
\\tilde{E}_l &= \\tilde{E}_{l, \\vec{r}} \\\\
\\hat{H}_l &= \\tilde{H}_{l, \\vec{r} + \\frac{1}{2}} \\\\
\\tilde{\\epsilon} &= \\tilde{\\epsilon}_\\vec{r} \\\\
\\end{align*}
\\tilde{\\epsilon} &= \\tilde{\\epsilon}_{\\vec{r}} \\\\
\\end{aligned}
$$
etc.
For \\( l' = l + \\frac{1}{2} \\) we get
For $l' = l + \\frac{1}{2}$ we get
$$
\\begin{align*}
\\begin{aligned}
\\hat{\\nabla} \\cdot \\tilde{S}_{l, l + \\frac{1}{2}}
&= \\hat{H}_{l + \\frac{1}{2}} \\cdot
(-\\mu / \\Delta_t)(\\hat{H}_{l + \\frac{1}{2}} - \\hat{H}_{l - \\frac{1}{2}}) -
@ -87,13 +87,13 @@ $$
+\\epsilon \\tilde{E}^2_l) / \\Delta_t \\ \\
- \\hat{H}_{l+\\frac{1}{2}} \\cdot \\hat{M}_l \\ \\
- \\tilde{E}_l \\cdot \\tilde{J}_{l+\\frac{1}{2}} \\\\
\\end{align*}
\\end{aligned}
$$
and for \\( l' = l - \\frac{1}{2} \\),
and for $l' = l - \\frac{1}{2}$,
$$
\\begin{align*}
\\begin{aligned}
\\hat{\\nabla} \\cdot \\tilde{S}_{l, l - \\frac{1}{2}}
&= (\\mu \\hat{H}^2_{l - \\frac{1}{2}}
+\\epsilon \\tilde{E}_{l-1} \\cdot \\tilde{E}_l) / \\Delta_t \\ \\
@ -101,7 +101,7 @@ $$
+\\epsilon \\tilde{E}^2_l) / \\Delta_t \\ \\
- \\hat{H}_{l-\\frac{1}{2}} \\cdot \\hat{M}_l \\ \\
- \\tilde{E}_l \\cdot \\tilde{J}_{l-\\frac{1}{2}} \\\\
\\end{align*}
\\end{aligned}
$$
These two results form the discrete time-domain analogue to Poynting's theorem.
@ -109,16 +109,16 @@ They hint at the expressions for the energy, which can be calculated at the same
time-index as either the E or H field:
$$
\\begin{align*}
\\begin{aligned}
U_l &= \\epsilon \\tilde{E}^2_l + \\mu \\hat{H}_{l + \\frac{1}{2}} \\cdot \\hat{H}_{l - \\frac{1}{2}} \\\\
U_{l + \\frac{1}{2}} &= \\epsilon \\tilde{E}_l \\cdot \\tilde{E}_{l + 1} + \\mu \\hat{H}^2_{l + \\frac{1}{2}} \\\\
\\end{align*}
\\end{aligned}
$$
Rewriting the Poynting theorem in terms of the energy expressions,
$$
\\begin{align*}
\\begin{aligned}
(U_{l+\\frac{1}{2}} - U_l) / \\Delta_t
&= -\\hat{\\nabla} \\cdot \\tilde{S}_{l, l + \\frac{1}{2}} \\ \\
- \\hat{H}_{l+\\frac{1}{2}} \\cdot \\hat{M}_l \\ \\
@ -127,14 +127,14 @@ $$
&= -\\hat{\\nabla} \\cdot \\tilde{S}_{l, l - \\frac{1}{2}} \\ \\
- \\hat{H}_{l-\\frac{1}{2}} \\cdot \\hat{M}_l \\ \\
- \\tilde{E}_l \\cdot \\tilde{J}_{l-\\frac{1}{2}} \\\\
\\end{align*}
\\end{aligned}
$$
This result is exact an should practically hold to within numerical precision. No time-
or spatial-averaging is necessary.
Note that each value of \\( J \\) contributes to the energy twice (i.e. once per field update)
despite only causing the value of \\( E \\) to change once (same for \\( M \\) and \\( H \\)).
Note that each value of $J$ contributes to the energy twice (i.e. once per field update)
despite only causing the value of $E$ to change once (same for $M$ and $H$).
Sources
@ -149,8 +149,8 @@ shape. It can be written
$$ f_r(t) = (1 - \\frac{1}{2} (\\omega (t - \\tau))^2) e^{-(\\frac{\\omega (t - \\tau)}{2})^2} $$
with \\( \\tau > \\frac{2 * \\pi}{\\omega} \\) as a minimum delay to avoid a discontinuity at
t=0 (assuming the source is off for t<0 this gives \\( \\sim 10^{-3} \\) error at t=0).
with $\\tau > \\frac{2 * \\pi}{\\omega}$ as a minimum delay to avoid a discontinuity at
t=0 (assuming the source is off for t<0 this gives $\\sim 10^{-3}$ error at t=0).

View File

@ -18,8 +18,9 @@
#git_link_template = 'https://github.com/USER/PROJECT/blob/{commit}/{path}#L{start_line}-L{end_line}'
#git_link_template = 'https://gitlab.com/USER/PROJECT/blob/{commit}/{path}#L{start_line}-L{end_line}'
#git_link_template = 'https://bitbucket.org/USER/PROJECT/src/{commit}/{path}#lines-{start_line}:{end_line}'
#git_link_template = 'https://CGIT_HOSTNAME/PROJECT/tree/{path}?id={commit}#n{start-line}'
git_link_template = None
#git_link_template = 'https://CGIT_HOSTNAME/PROJECT/tree/{path}?id={commit}#n{start_line}'
#git_link_template = None
git_link_template = 'https://mpxd.net/code/jan/fdfd_tools/src/commit/{commit}/{path}#L{start_line}-L{end_line}'
# A prefix to use for every HTML hyperlink in the generated documentation.
# No prefix results in all links being relative.

View File

@ -2,7 +2,10 @@
import os
import pdoc
from pdoc.html_helpers import extract_toc, glimpse, to_html as _to_html, format_git_link
from pdoc.html_helpers import extract_toc, glimpse, to_html as _to_html, format_git_link, _md, to_markdown
from markdown.inlinepatterns import InlineProcessor
from markdown.util import AtomicString, etree
def link(d, name=None, fmt='{}'):
@ -14,8 +17,33 @@
return '<a title="{}" href="{}">{}</a>'.format(d.refname, url, name)
def to_html(text):
return _to_html(text, module=module, link=link, latex_math=latex_math)
# Altered latex delimeters (allow inline $...$, wrap in <eq></eq>)
class _MathPattern(InlineProcessor):
NAME = 'pdoc-math'
PATTERN = r'(?<!\S|\\)(?:\\\((.+?)\\\)|\\\[(.+?)\\\]|\$\$(.+?)\$\$|\$(\S.*?)\$)'
PRIORITY = 181 # Larger than that of 'escape' pattern
def handleMatch(self, m, data):
for value, is_block in zip(m.groups(), (False, True, True, False)):
if value:
break
wrapper = etree.Element('eq')
wrapper.text = AtomicString(value)
return wrapper, m.start(0), m.end(0)
def to_html(text: str):
if not latex_math and _MathPattern.NAME in _md.inlinePatterns:
_md.inlinePatterns.deregister(_MathPattern.NAME)
elif latex_math and _MathPattern.NAME not in _md.inlinePatterns:
_md.inlinePatterns.register(_MathPattern(_MathPattern.PATTERN),
_MathPattern.NAME,
_MathPattern.PRIORITY)
md = to_markdown(text, docformat='numpy,google', module=module, link=link)
return _md.reset().convert(md)
# def to_html(text):
# return _to_html(text, module=module, link=link, latex_math=latex_math)
%>
<%def name="ident(name)"><span class="ident">${name}</span></%def>
@ -377,10 +405,6 @@
</script><script async src='https://www.google-analytics.com/analytics.js'></script>
% endif
% if latex_math:
<script async src='https://mpxd.net/scripts/MathJax/MathJax.js?config=TeX-AMS_CHTML'></script>
% endif
<%include file="head.mako"/>
</head>
<body>

185
pdoc_templates/pdf.mako Normal file
View File

@ -0,0 +1,185 @@
<%!
import re
import pdoc
from pdoc.html_helpers import to_markdown, format_git_link
def link(d, fmt='{}'):
name = fmt.format(d.qualname + ('()' if isinstance(d, pdoc.Function) else ''))
if isinstance(d, pdoc.External):
return name
return '[{}](#{})'.format(name, d.refname)
def _to_md(text, module):
text = to_markdown(text, module=module, link=link)
# Setext H2 headings to atx H2 headings
text = re.sub(r'\n(.+)\n-{3,}\n', r'\n## \1\n\n', text)
# Convert admonitions into simpler paragraphs, dedent contents
text = re.sub(r'^(?P<indent>( *))!!! \w+ \"([^\"]*)\"(.*(?:\n(?P=indent) +.*)*)',
lambda m: '{}**{}:** {}'.format(m.group(2), m.group(3),
re.sub('\n {,4}', '\n', m.group(4))),
text, flags=re.MULTILINE)
return text
def subh(text, level=2):
# Deepen heading levels so H2 becomes H4 etc.
return re.sub(r'\n(#+) +(.+)\n', r'\n%s\1 \2\n' % ('#' * level), text)
%>
<%def name="title(level, string, id=None)">
<% id = ' {#%s}' % id if id is not None else '' %>
${('#' * level) + ' ' + string + id}
</%def>
<%def name="funcdef(f)">
<%
returns = show_type_annotations and f.return_annotation() or ''
if returns:
returns = ' -> ' + returns
%>
> `${f.funcdef()} ${f.name}(${', '.join(f.params(annotate=show_type_annotations))})${returns}`
</%def>
<%def name="classdef(c)">
> `class ${c.name}(${', '.join(c.params(annotate=show_type_annotations))})`
</%def>
<%def name="show_source(d)">
% if (show_source_code or git_link_template) and d.source and d.obj is not getattr(d.inherits, 'obj', None):
<% git_link = format_git_link(git_link_template, d) %>
[[view code]](${git_link})
%endif
</%def>
---
description: |
API documentation for modules: ${', '.join(m.name for m in modules)}.
lang: en
classoption: oneside
geometry: margin=1in
papersize: a4
linkcolor: blue
links-as-notes: true
...
% for module in modules:
<%
submodules = module.submodules()
variables = module.variables()
functions = module.functions()
classes = module.classes()
def to_md(text):
return _to_md(text, module)
%>
-------------------------------------------
${title(1, ('Namespace' if module.is_namespace else 'Module') + ' `%s`' % module.name, module.refname)}
${module.docstring | to_md}
% if submodules:
${title(2, 'Sub-modules')}
% for m in submodules:
* [${m.name}](#${m.refname})
% endfor
% endif
% if variables:
${title(2, 'Variables')}
% for v in variables:
${title(3, 'Variable `%s`' % v.name, v.refname)}
${show_source(v)}
${v.docstring | to_md, subh, subh}
% endfor
% endif
% if functions:
${title(2, 'Functions')}
% for f in functions:
${title(3, 'Function `%s`' % f.name, f.refname)}
${show_source(f)}
${funcdef(f)}
${f.docstring | to_md, subh, subh}
% endfor
% endif
% if classes:
${title(2, 'Classes')}
% for cls in classes:
${title(3, 'Class `%s`' % cls.name, cls.refname)}
${show_source(cls)}
${classdef(cls)}
${cls.docstring | to_md, subh}
<%
class_vars = cls.class_variables(show_inherited_members, sort=sort_identifiers)
static_methods = cls.functions(show_inherited_members, sort=sort_identifiers)
inst_vars = cls.instance_variables(show_inherited_members, sort=sort_identifiers)
methods = cls.methods(show_inherited_members, sort=sort_identifiers)
mro = cls.mro()
subclasses = cls.subclasses()
%>
% if mro:
${title(4, 'Ancestors (in MRO)')}
% for c in mro:
* [${c.refname}](#${c.refname})
% endfor
% endif
% if subclasses:
${title(4, 'Descendants')}
% for c in subclasses:
* [${c.refname}](#${c.refname})
% endfor
% endif
% if class_vars:
${title(4, 'Class variables')}
% for v in class_vars:
${title(5, 'Variable `%s`' % v.name, v.refname)}
${v.docstring | to_md, subh, subh}
% endfor
% endif
% if inst_vars:
${title(4, 'Instance variables')}
% for v in inst_vars:
${title(5, 'Variable `%s`' % v.name, v.refname)}
${v.docstring | to_md, subh, subh}
% endfor
% endif
% if static_methods:
${title(4, 'Static methods')}
% for f in static_methods:
${title(5, '`Method %s`' % f.name, f.refname)}
${funcdef(f)}
${f.docstring | to_md, subh, subh}
% endfor
% endif
% if methods:
${title(4, 'Methods')}
% for f in methods:
${title(5, 'Method `%s`' % f.name, f.refname)}
${funcdef(f)}
${f.docstring | to_md, subh, subh}
% endfor
% endif
% endfor
% endif
##\## for module in modules:
% endfor
-----
Generated by *pdoc* ${pdoc.__version__} (<https://pdoc3.github.io>).

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.flex {
display: flex !important;
}
body {
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}
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#http-server-module-list div {
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.toc ul,
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#index h3 {
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#index h4 {
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#index h4 + ul {
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Assuming ~20-character identifiers and ~30% wide sidebar. */
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@media (min-width: 300ex) { #index .two-column { column-count: 3 } }
dl {
margin-bottom: 2em;
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dl dl:last-child {
margin-bottom: 4em;
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dd {
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#header-classes + dl > dd {
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dd dd {
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.admonition.tip,
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@media screen and (min-width: 700px) {
#sidebar {
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#content {
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pre code {
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.item .name {
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main {
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flex-direction: row-reverse;
justify-content: flex-end;
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.toc ul ul,
#index ul {
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.toc > ul > li {
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}
@media print {
#sidebar h1 {
page-break-before: always;
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.source {
display: none;
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}
@media print {
* {
background: transparent !important;
color: #000 !important; /* Black prints faster: h5bp.com/s */
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a[href]:after {
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font-size: 90%;
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/* Internal, documentation links, recognized by having a title,
don't need the URL explicity stated. */
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}
abbr[title]:after {
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/*
* Don't show links for images, or javascript/internal links
*/
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pre,
blockquote {
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thead {
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img {
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@page {
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p,
h2,
h3 {
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h1,
h2,
h3,
h4,
h5,
h6 {
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}