Awesome
<h1 align='center'>torchcde</h1> <h2 align='center'>Differentiable GPU-capable solvers for CDEs</h2>Update: for any new projects, I would now recommend using Diffrax instead. This is much faster, and producion-quality. torchcde was its prototype as a research project!
This library provides differentiable GPU-capable solvers for controlled differential equations (CDEs). Backpropagation through the solver or via the adjoint method is supported; the latter allows for improved memory efficiency.
In particular this allows for building Neural Controlled Differential Equation models, which are state-of-the-art models for (arbitrarily irregular!) time series. Neural CDEs can be thought of as a "continuous time RNN".
<p align="center"> <img align="middle" src="./imgs/main.png" width="666" /> </p>
Installation
pip install torchcde
Requires PyTorch >=1.7.
Example
import torch
import torchcde
# Create some data
batch, length, input_channels = 1, 10, 2
hidden_channels = 3
t = torch.linspace(0, 1, length)
t_ = t.unsqueeze(0).unsqueeze(-1).expand(batch, length, 1)
x_ = torch.rand(batch, length, input_channels - 1)
x = torch.cat([t_, x_], dim=2) # include time as a channel
# Interpolate it
coeffs = torchcde.hermite_cubic_coefficients_with_backward_differences(x)
X = torchcde.CubicSpline(coeffs)
# Create the Neural CDE system
class F(torch.nn.Module):
def __init__(self):
super(F, self).__init__()
self.linear = torch.nn.Linear(hidden_channels,
hidden_channels * input_channels)
def forward(self, t, z):
return self.linear(z).view(batch, hidden_channels, input_channels)
func = F()
z0 = torch.rand(batch, hidden_channels)
# Integrate it
torchcde.cdeint(X=X, func=func, z0=z0, t=X.interval)
See time_series_classification.py, which demonstrates how to use the library to train a Neural CDE model to predict the chirality of a spiral.
Also see irregular_data.py, for demonstrations on how to handle variable-length inputs, irregular sampling, or missing data, all of which can be handled easily, without changing the model.
Citation
If you found use this library useful, please consider citing
@article{kidger2020neuralcde,
title={{N}eural {C}ontrolled {D}ifferential {E}quations for {I}rregular {T}ime {S}eries},
author={Kidger, Patrick and Morrill, James and Foster, James and Lyons, Terry},
journal={Advances in Neural Information Processing Systems},
year={2020}
}
Documentation
The library consists of two main components: (1) integrators for solving controlled differential equations, and (2) ways of constructing controls from data.
Integrators
The library provides the cdeint
function, which solves the system of controlled differential equations:
dz(t) = f(t, z(t))dX(t) z(t_0) = z0
The goal is to find the response z
driven by the control X
. This can be re-written as the following differential equation:
dz/dt(t) = f(t, z)dX/dt(t) z(t_0) = z0
where the right hand side describes a matrix-vector product between f(t, z)
and dX/dt(t)
.
This is solved by
cdeint(X, func, z0, t, adjoint, backend, **kwargs)
where letting ...
denote an arbitrary number of batch dimensions:
X
is atorch.nn.Module
with methodderivative
, such thatX.derivative(t)
is a Tensor of shape(..., input_channels)
,func
is atorch.nn.Module
, such thatfunc(t, z)
returns a Tensor of shape(..., hidden_channels, input_channels)
,z0
is a Tensor of shape(..., hidden_channels)
,t
is a one-dimensional Tensor of times to outputz
at.adjoint
is a boolean (defaulting toTrue
).backend
is a string (defaulting to"torchdiffeq"
).
Adjoint backpropagation (which is slower but more memory efficient) can be toggled with adjoint=True/False
.
The backend
should be either "torchdiffeq"
or "torchsde"
, corresponding to which underlying library to use for the solvers. If using torchsde then the stochastic term is zero -- so the CDE is still reduced to an ODE. This is useful if one library supports a feature that the other doesn't. (For example torchsde supports a reversible solver, the reversible Heun method; at time of writing torchdiffeq does not support any reversible solvers.)
Any additional **kwargs
are passed on to torchdiffeq.odeint[_adjoint]
or torchsde.sdeint[_adjoint]
, for example to specify the solver.
Constructing controls
A very common scenario is to construct the continuous controlX
from discrete data (which may be irregularly sampled with missing values). To support this, we provide three main interpolation schemes:
- Hermite cubic splines with backwards differences
- Linear interpolation
- Rectilinear interpolation
Note that if for some reason you already have a continuous control X
then you won't need an interpolation scheme at all!
Hermite cubic splines are usually the best choice, if possible. Linear and rectilinear interpolations are particularly useful in causal settings -- when at inference time the data is arriving over time. We go into further details in the Further Documentation below.
Just demonstrating Hermite cubic splines for now:
coeffs = hermite_cubic_coefficients_with_backward_differences(x)
# coeffs is a torch.Tensor you can save, load,
# pass through Datasets and DataLoaders etc.
X = CubicSpline(coeffs)
where:
x
is a Tensor of shape(..., length, input_channels)
, where...
is some number of batch dimensions. Missing data should be represented as aNaN
.
The interface provided by CubicSpline
is:
.interval
, which gives the time interval the spline is defined over. (Often used as thet
argument incdeint
.) This is determined implicitly from the length of the data, and so does not in general correspond to the time your data was actually observed at. (See the Further Documentation note on reparameterisation invariance.).grid_points
is all of the knots in the spline, so that for exampleX.evaluate(X.grid_points)
will recover the original data..evaluate(t)
, wheret
is an any-dimensional Tensor, to evaluate the spline at any (collection of) time(s)..derivative(t)
, wheret
is an any-dimensional Tensor, to evaluate the derivative of the spline at any (collection of) time(s).
Usually hermite_cubic_coefficients_with_backward_differences
should be computed as a preprocessing step, whilst CubicSpline
should be called inside the forward pass of your model. See time_series_classification.py for a worked example.
Then call:
cdeint(X=X, func=... z0=..., t=X.interval)
Further documentation
The earlier documentation section should give everything you need to get up and running.
Here we discuss a few more advanced bits of functionality:
- The reparameterisation invariance property of CDEs.
- Other interpolation methods, and the differences between them.
- The use of fixed solvers. (They just work.)
- Stacking CDEs (i.e. controlling one by the output of another).
- Computing logsignatures for the log-ODE method.
Reparameterisation invariance
This is a classical fact about CDEs.
Let <img src="https://render.githubusercontent.com/render/math?math=%5Cpsi%20%5Ccolon%20%5Ba%2C%20b%5D%20%5Cto%20%5Bc%2C%20d%5D"> be differentiable and increasing, with <img src="https://render.githubusercontent.com/render/math?math=%5Cpsi(a)%20%3D%20c"> and <img src="https://render.githubusercontent.com/render/math?math=%5Cpsi(b)%20%3D%20d">. Let <img src="https://render.githubusercontent.com/render/math?math=T%20%5Cin%20%5Bc%2C%20d%5D">, let <img src="https://render.githubusercontent.com/render/math?math=%5Cwidetilde%7Bz%7D%20%3D%20z%20%5Ccirc%20%5Cpsi">, let <img src="https://render.githubusercontent.com/render/math?math=%5Cwidetilde%7BX%7D%20%3D%20X%20%5Ccirc%20%5Cpsi">, and let <img src="https://render.githubusercontent.com/render/math?math=%5Cmathcal%7BT%7D%20%3D%20%5Cpsi(T)">. Then substituting <img src="https://render.githubusercontent.com/render/math?math=t%20%3D%20%5Cpsi(%5Ctau)"> into a CDE (and just using the standard change of variables formula):
<img src="https://render.githubusercontent.com/render/math?math=%5Cbegin%7Balign*%7D%0A%5Cwidetilde%7Bz%7D(%5Cmathcal%7BT%7D)%20%26%3D%20z(T)%5C%5C%0A%20%26%3D%20z(c)%20%2B%20%5Cint_c%5ET%20f(z(t))%5C%2C%5Cmathrm%7Bd%7DX(t)%5C%5C%0A%26%3D%20z(c)%20%2B%20%5Cint_c%5ET%20f(z(t))%5C%2C%5Cfrac%7B%5Cmathrm%7Bd%7DX%7D%7B%5Cmathrm%7Bd%7Dt%7D(t)%5C%2C%5Cmathrm%7Bd%7Dt%5C%5C%0A%20%26%3D%20z(%5Cpsi(a))%20%2B%20%5Cint_a%5E%7B%5Cpsi%5E%7B-1%7D(T)%7D%20f(z(%5Cpsi(%5Ctau)))%5C%2C%5Cfrac%7B%5Cmathrm%7Bd%7DX%7D%7B%5Cmathrm%7Bd%7Dt%7D(%5Cpsi(%5Ctau))%5C%2C%5Cfrac%7B%5Cmathrm%7Bd%7D%5Cpsi%7D%7B%5Cmathrm%7Bd%7D%5Ctau%7D(%5Ctau)%5C%2C%5Cmathrm%7Bd%7D%5Ctau%5C%5C%0A%20%26%3D%20(z%5Ccirc%5Cpsi)(a)%20%2B%20%5Cint_a%5E%7B%5Cpsi%5E%7B-1%7D(T)%7D%20f((z%5Ccirc%5Cpsi)(%5Ctau))%5C%2C%5Cfrac%7B%5Cmathrm%7Bd%7D(X%5Ccirc%20%5Cpsi)%7D%7B%5Cmathrm%7Bd%7D%5Ctau%7D(%5Ctau)%5C%2C%5Cmathrm%7Bd%7D%5Ctau%5C%5C%0A%20%26%3D%20(z%5Ccirc%5Cpsi)(a)%20%2B%20%5Cint_a%5E%7B%5Cpsi%5E%7B-1%7D(T)%7D%20f((z%5Ccirc%20%5Cpsi)(%5Ctau))%5C%2C%5Cmathrm%7Bd%7D(X%5Ccirc%20%5Cpsi)(%5Ctau)%5C%5C%0A%26%3D%20%5Cwidetilde%7Bz%7D(c)%20%2B%20%5Cint_c%5E%5Cmathcal%7BT%7D%20f(%5Cwidetilde%7Bz%7D(%5Ctau))%20%5C%2C%5Cmathrm%7Bd%7D%5Cwidetilde%7BX%7D(%5Ctau)%0A%5Cend%7Balign*%7D">We see that <img src="https://render.githubusercontent.com/render/math?math=%5Cwidetilde%7Bz%7D"> also satisfies the neural CDE equation, just with <img src="https://render.githubusercontent.com/render/math?math=%5Cwidetilde%7BX%7D"> as input instead of <img src="https://render.githubusercontent.com/render/math?math=X">. In other words, using <img src="https://render.githubusercontent.com/render/math?math=\psi"> changes the speed at which we traverse the input <img src="https://render.githubusercontent.com/render/math?math=X">, and correspondingly changes the speed at which we traverse the output <img src="https://render.githubusercontent.com/render/math?math=z"> -- and that's it! In particular the CDE itself doesn't need any adjusting.
This ends up being a really useful fact for writing neater software. We can handle things like messy data (e.g. variable length time series) just during data preprocessing, without it complicating the model code. In time_series_classification.py, the region we integrate over is given by X.interval
as a standardised region to integrate over. In the example irregular_data.py, we use this to handle variable-length data.
Different interpolation methods
For a full breakdown into the interpolation schemes, see Neural Controlled Differential Equations for Online Prediction Tasks where each interpolation scheme is scrutinised, and best practices are presented.
In brief:
- Will your data: (a) be arriving in an online fashion at inference time; and (b) be multivariate; and (c) potentially have missing values?
- Yes: rectilinear interpolation.
- No: Are you using an adaptive step size solver (e.g. the default
dopri5
)?- Yes: Hermite cubic splines with backwards differences.
- No: linear interpolation.
- Not sure / both: Hermite cubic splines with backwards differences.
In more detail:
- Linear interpolation: these are "kind-of" causal.
During inference we can simply wait at each time point for the next data point to arrive, and then interpolate towards the next data point when it arrives, and solve the CDE over that interval.
If there is missing data, however, then this isn't possible. (As some of the channels might not have observations you can interpolate to.) In this case use rectilinear interpolation, below.
Example:
coeffs = linear_interpolation_coeffs(x)
X = LinearInterpolation(coeffs)
cdeint(X=X, ...)
Linear interpolation has kinks. If using adaptive step size solvers then it should be told about the kinks. (Rather than expensively finding them for itself -- slowing down to resolve the kink, and then speeding up again afterwards.) This is done with the jump_t
option when using the torchdiffeq
backend:
cdeint(...,
backend='torchdiffeq',
method='dopri5',
options=dict(jump_t=X.grid_points))
Although adaptive step size solvers will probably find it easier to resolve Hermite cubic splines with backward differences, below.
- Hermite cubic splines with backwards differences: these are "kind-of" causal in the same way as linear interpolation, but dont have kinks, which makes them faster with adaptive step size solvers. (But is simply an unnecessary overhead when working with fixed step size solvers, which is why we recommend linear interpolation is you know you're only going to be using fixed step size solvers.)
Example:
coeffs = hermite_cubic_coefficients_with_backward_differences(x)
X = CubicSpline(coeffs)
cdeint(X=X, ...)
- Rectilinear interpolation: This is appropriate if there is multivariate missing data, and you need causality.
What is done is to linearly interpolate forward in time (keeping the observations constant), and then linearly interpolate the values (keeping the time constant). This is possible because time is a channel (and doesn't need to line up with the "time" used in the differential equation solver, as per the reparameterisation invariance of the previous section).
This can be a bit unintuitive at first. We suggest firing up matplotlib and plotting things to get a feel for what's going on. As a fun sidenote, using rectilinear interpolation makes neural CDEs generalise ODE-RNNs.
Example:
# standard setup for a neural CDE: include time as a channel
t = torch.linspace(0, 1, 10)
x = torch.rand(2, 10, 3)
t_ = t.unsqueeze(0).unsqueeze(-1).expand(2, 10, 1)
x = torch.cat([t_, x], dim=-1)
del t, t_ # won't need these again!
# The `rectilinear` argument is the channel index corresponding to time
coeffs = linear_interpolation_coeffs(x, rectilinear=0)
X = LinearInterpolation(coeffs)
cdeint(X=X, ...)
As before, if using an adaptive step size solver, it should be informed about the kinks.
cdeint(...,
backend='torchdiffeq',
method='dopri5',
options=dict(jump_t=X.grid_points))
Fixed solvers
Solving CDEs (regardless of the choice of interpolation scheme in a Neural CDE) with fixed solvers like euler
, midpoint
, rk4
etc. is pretty much exactly the same as solving an ODE with a fixed solver. Just make sure to set the step_size
option to something sensible; for example the smallest gap between times:
X = LinearInterpolation(coeffs)
step_size = (X.grid_points[1:] - X.grid_points[:-1]).min()
cdeint(
X=X, t=X.interval, func=..., method='rk4',
options=dict(step_size=step_size)
)
Stacking CDEs
You may wish to use the output of one CDE to control another. That is, to solve the coupled CDEs:
du(t) = g(t, u(t))dz(t) u(t_0) = u0
dz(t) = f(t, z(t))dX(t) z(t_0) = z0
There are two ways to do this. The first way is to put everything inside a single cdeint
call, by solving the system
v = [u, z]
v0 = [u0, z0]
h(t, v) = [g(t, u)f(t, z), f(t, z)]
dv(t) = h(t, v(t))dX(t) v(t_0) = v0
and using cdeint
as normal. This is usually the best way to do it! It's simpler and usually faster. (But forces you to use the same solver for the whole system, for example.)
The second way is to have cdeint
output z(t)
at multiple times t
, interpolate the discrete output into a continuous path, and then call cdeint
again. This is probably less memory efficient, but allows for different choices of solver for each call to cdeint
.
For example, this could be used to create multi-layer Neural CDEs, just like multi-layer RNNs. Although as of writing this, no-one seems to have tried this yet!
The log-ODE method
This is a way of reducing the length of data by using extra channels. (For example, this may help train Neural CDE models faster, as the extra channels can be parallelised, but extra length cannot.)
This is done by splitting the control X
up into windows, and computing the logsignature of the control over each window. The logsignature is a transform known to extract the information that is most important to describing how X
controls a CDE.
This is supported by the logsig_windows
function, which takes in data, and produces a transformed path, that now exists in logsignature space:
batch, length, channels = 1, 100, 2
x = torch.rand(batch, length, channels)
depth, window = 3, 10.0
x = torchcde.logsig_windows(x, depth, window)
# use x as you would normally: interpolate, etc.
See the paper Neural Rough Differential Equations for Long Time Series for more information. See logsignature_example.py for a worked example.
Note that this requires installing the Signatory package.