Recurrent Models
Recurrent cells
To introduce Flux's recurrence functionalities, we will consider the following vanilla recurrent neural network structure:
In the above, we have a sequence of length 3, where x1
to x3
represent the input at each step (could be a timestamp or a word in a sentence), and y1
to y3
are their respective outputs.
An aspect to recognize is that in such model, the recurrent cells A
all refer to the same structure. What distinguishes it from a simple dense layer is that the cell A
is fed, in addition to an input x
, with information from the previous state of the model (hidden state denoted as h1
& h2
in the diagram).
In the most basic RNN case, cell A could be defined by the following:
Wxh = randn(5, 2)
Whh = randn(5, 5)
b = randn(5)
function rnn(h, x)
h = tanh.(Wxh * x .+ Whh * h .+ b)
return h, h
end
x = rand(2) # dummy data
h = rand(5) # initial hidden state
h, y = rnn(h, x)
Notice how the above is essentially a Dense
layer that acts on two inputs, h
and x
.
If you run the last line a few times, you'll notice the output y
changing slightly even though the input x
is the same.
There are various recurrent cells available in Flux, notably RNNCell
, LSTMCell
and GRUCell
, which are documented in the layer reference. The hand-written example above can be replaced with:
using Flux
rnn = Flux.RNNCell(2, 5)
x = rand(Float32, 2) # dummy data
h = rand(Float32, 5) # initial hidden state
h, y = rnn(h, x)
Stateful Models
For the most part, we don't want to manage hidden states ourselves, but to treat our models as being stateful. Flux provides the Recur
wrapper to do this.
x = rand(Float32, 2)
h = rand(Float32, 5)
m = Flux.Recur(rnn, h)
y = m(x)
The Recur
wrapper stores the state between runs in the m.state
field.
If we use the RNN(2, 5)
constructor – as opposed to RNNCell
– you'll see that it's simply a wrapped cell.
julia> RNN(2, 5)
Recur(RNNCell(2, 5, tanh))
Equivalent to the RNN
stateful constructor, LSTM
and GRU
are also available.
Using these tools, we can now build the model shown in the above diagram with:
m = Chain(RNN(2, 5), Dense(5, 1), x -> reshape(x, :))
Working with sequences
Using the previously defined m
recurrent model, we can now apply it to a single step from our sequence:
x = rand(Float32, 2)
julia> m(x)
1-element Array{Float32,1}:
0.028398542
The m(x)
operation would be represented by x1 -> A -> y1
in our diagram. If we perform this operation a second time, it will be equivalent to x2 -> A -> y2
since the model m
has stored the state resulting from the x1
step:
x = rand(Float32, 2)
julia> m(x)
1-element Array{Float32,1}:
0.07381232
Now, instead of computing a single step at a time, we can get the full y1
to y3
sequence in a single pass by broadcasting the model on a sequence of data.
To do so, we'll need to structure the input data as a Vector
of observations at each time step. This Vector
will therefore be of length = seq_length
and each of its elements will represent the input features for a given step. In our example, this translates into a Vector
of length 3, where each element is a Matrix
of size (features, batch_size)
, or just a Vector
of length features
if dealing with a single observation.
x = [rand(Float32, 2) for i = 1:3]
julia> m.(x)
3-element Array{Array{Float32,1},1}:
[-0.17945863]
[-0.20863166]
[-0.20693761]
If for some reason one wants to exclude the first step of the RNN chain for the computation of the loss, that can be handled with:
function loss(x, y)
sum((Flux.stack(m.(x)[2:end],1) .- y) .^ 2)
end
y = rand(Float32, 2)
julia> loss(x, y)
1.7021208968648693
In such model, only y2
and y3
are used to compute the loss, hence the target y
being of length 2. This is a strategy that can be used to easily handle a seq-to-one
kind of structure, compared to the seq-to-seq
assumed so far.
Alternatively, if one wants to perform some warmup of the sequence, it could be performed once, followed with a regular training where all the steps of the sequence would be considered for the gradient update:
function loss(x, y)
sum((Flux.stack(m.(x),1) .- y) .^ 2)
end
seq_init = [rand(Float32, 2) for i = 1:1]
seq_1 = [rand(Float32, 2) for i = 1:3]
seq_2 = [rand(Float32, 2) for i = 1:3]
y1 = rand(Float32, 3)
y2 = rand(Float32, 3)
X = [seq_1, seq_2]
Y = [y1, y2]
data = zip(X,Y)
Flux.reset!(m)
m.(seq_init)
ps = params(m)
opt= ADAM(1e-3)
Flux.train!(loss, ps, data, opt)
In this previous example, model's state is first reset with Flux.reset!
. Then, there's a warmup that is performed over a sequence of length 1 by feeding it with seq_init
, resulting in a warmup state. The model can then be trained for 1 epoch, where 2 batches are provided (seq_1
and seq_2
) and all the timesteps outputs are considered for the loss (we no longer use a subset of m.(x)
in the loss function).
In this scenario, it is important to note that a single continuous sequence is considered. Since the model state is not reset between the 2 batches, the state of the model flows through the batches, which only makes sense in the context where seq_1
is the continuation of seq_init
and so on.
Batch size would be 1 here as there's only a single sequence within each batch. If the model was to be trained on multiple independent sequences, then these sequences could be added to the input data as a second dimension. For example, in a language model, each batch would contain multiple independent sentences. In such scenario, if we set the batch size to 4, a single batch would be of the shape:
batch = [rand(Float32, 2, 4) for i = 1:3]
That would mean that we have 4 sentences (or samples), each with 2 features (let's say a very small embedding!) and each with a length of 3 (3 words per sentence). Computing m(batch[1])
, would still represent x1 -> y1
in our diagram and returns the first word output, but now for each of the 4 independent sentences (second dimension of the input matrix).
In many situations, such as when dealing with a language model, each batch typically contains independent sentences, so we cannot handle the model as if each batch was the direct continuation of the previous one. To handle such situation, we need to reset the state of the model between each batch, which can be conveniently performed within the loss function:
function loss(x, y)
Flux.reset!(m)
sum((Flux.stack(m.(x),1) .- y) .^ 2)
end
A potential source of ambiguity with RNN in Flux can come from the different data layout compared to some common frameworks where data is typically a 3 dimensional array: (features, seq length, samples)
. In Flux, those 3 dimensions are provided through a vector of seq length containing a matrix (features, samples)
.