# Computing Neural Network Gradients

Computing the neural network gradient requires very simple calculus, yet can be tedious.

## Affine Transformation (Fully Connected Layer) Gradients

For a simple fully connected layer with batch size $n$ with the feature dimension $d_i$ and output feature dimension is $d_o$ ($d_i$ neurons as an inputs and $d_o$ neurons as output), the layer has $W \in \mathbb{R}^{d_o \times d_i}$ and $b \in \mathbb{R}^{d_o}$ as parameters. The resulting response $Y \in \mathbb{R}^{d_o \times n}$ is $Y = AX + b$.

The summation is a broadcasting sum.

The gradient $\frac{\partial Y_{ij}}{\partial W_{pq}}$ can be computed as

\begin{align} \frac{\partial Y_{ij}}{\partial W_{pq}} & = \frac{\partial}{\partial W_{pq}}\left( \sum_l W_{il}X_{lj} + b_j\right) \\ & = X_{iq} \delta_{ip} \delta_{jq} \end{align}

Also the gradient for the scaler $b$ is

\begin{align} \frac{\partial Y_{ij}}{\partial b_{p}} & = \frac{\partial}{\partial b_{p}}\left( \sum_l W_{il}X_{lj} + b_j\right) \\ & = \delta_{jp} \end{align}

where $\delta_{ij}$ is a kronecker delta $\delta_{ij} = 1$ if $i = j$, otherwise $0$.

\begin{align} \frac{\partial Y_{ij}}{\partial X_{pq}} & = \frac{\partial}{\partial X_{pq}}\left( \sum_l W_{il}X_{lj} \right) \\ & = W_{iq} \delta_{ip} \delta_{jq} \end{align}

Let’s say that the gradient from the upper layer propagated gradient $\frac{\partial E}{\partial Y} \in \mathbb{R}^{n \times d_o}$ to the current layer. The resulting gradient for the weight $W$ is

\begin{align} \frac{\partial E}{\partial W} & = \frac{\partial E}{\partial Y} \frac{\partial Y}{\partial W} \\ & = \frac{\partial E}{\partial Y} X^T \end{align} \begin{align} \frac{\partial E}{\partial b} & = \frac{\partial E}{\partial Y} \frac{\partial Y}{\partial b} \\ & = \sum_i \frac{\partial E}{\partial Y_i} \end{align}

where $Y_i$ is the $i$ th datapoint in the batch. The gradient propagated back to the lower layer is

\begin{align} \frac{\partial E}{\partial X} & = \frac{\partial E}{\partial Y} \frac{\partial Y}{\partial X} \\ & = W^T \frac{\partial E}{\partial Y} \end{align}

The only thing that you have to be careful with is matching the dimension of the matrices. Everything will work out if you just match the dimensions of matrices that you multiply. For instance, the dimension of $W$ and TODO

The Rectified Linear Unit (ReLU) has been widely used for simplicity and faster convergence. The ReLU units allow stronger gradients to propagate back to the lower layers, unlike sigmoid units or hyperbolic tangent units. Since there is no weight to learn, we can just compute the gradients $\frac{\partial E}{\partial X}$, where $Y = f(X)$ and the $f(\cdot)$ is the element-wise ReLU.

\begin{align} \frac{\partial E}{\partial X} & = \frac{\partial E}{\partial Y} \frac{\partial Y}{\partial X}\\ & = \frac{\partial E}{\partial Y} \circ \Delta(X) \end{align}

where $\circ$ is the Hadammard product and $\Delta(X)$ has elements $\delta_{ij} = I\left(x_{ij} > 0 \right)$.

## Generalized Convolution Gradients

The convolution is a conventional signal filtering technique. In CNN terminology, you can also think of it as 2D or ND filter that extract edges, blobs, or high frequency changes. In this example, we follow the caffe Blob convention and compute 2D convolution.

Unlike traditional signal processing convolution, neural network convolution is a generalization of convolution $\ast$. For instance, there is the stride which controls the step size, and you can think of the standard convolution as a convolution with the stride 1. Also the output convolution size is not $n + k - 1$ where $n$ is the input signal size and $k$ is the kernel size. The neural network convolution kernel always fits within the input size. Thus the output size is $n - k + 1$.

I will use $\ast_s$ to denote the convolution with stride $s$. Suppose that the result after convolution is $Y = F \ast_s X + b$ where $Y \in \mathbb{R}^{n \times h_y \times \times w_y}$ and $F \in \mathbb{R}^{c \times h_f \times w_f}$ and $X \in \mathbb{R}^{c \times h_x \times w_x}$ and $b \in \mathbb{R}$.

The summation is a broadcasting sum that makes the summation consistent.

If we add paddings along width and height, the problem becomes simplified since we do not have to account the borderline cases where filter only sees not enough data.

\begin{align} \frac{\partial Y_{nhw}}{\partial X_{ncij}} & = \sum_{k\in \{i, i+s, i+2s, \dots, i+rs\}} \sum_{l\in \{j, j+s, j+2s, \dots, j+os\}} W_{ckl}\\ & = \sum_{k = 0}^{r-1} \sum_{l = 0}^{o-1} W_{c,(i + ks),(j + ls)} \end{align}

Where $s$ is the stride (this is not standard convolution parameter). In standard convolution, the stride is 1. $o$ and $r$ are the number of strides it can make to make the indexing plausible.

For parameters,

\begin{align} \frac{\partial Y_{nhw}}{\partial W_{cij}} & = X_{n,(h + i),(w + j)}\\ \frac{\partial Y_{nhw}}{\partial b} & = 1 \end{align}

Thus the gradient propagated through the network will be

\begin{align} \frac{\partial E}{\partial X_{ncij}} & = \sum_k \sum_l \frac{\partial E}{\partial Y_{nkl}} \frac{\partial Y_{nkl}}{\partial X_{ncij}}\\ & = \sum_k \sum_l \frac{\partial E}{\partial Y_{nkl}} \sum_{k = 0}^{r-1} \sum_{l = 0}^{o-1} W_{c,(i + ks),(j + ls)}\\ \end{align}

Also for the weight update,

\begin{align} \frac{\partial E}{\partial W_{cij}} & = \sum_p \sum_q \frac{\partial E}{\partial Y_{nij}} \frac{\partial Y_{nij}}{\partial W_{cij}}\\ & = \sum_p \sum_q \frac{\partial E}{\partial Y_{npq}} \sum_{k = 0}^{r-1} \sum_{l = 0}^{o-1} X_{c,(i + ks),(j + ls)}\\ \frac{\partial E}{\partial b} & = \sum_k \sum_l \frac{\partial E}{\partial Y_{nkl}} \frac{\partial Y_{nkl}}{\partial b}\\ & = \sum_k \sum_l \frac{\partial E}{\partial Y_{nkl}} \end{align}

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