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# Licensed to the Apache Software Foundation (ASF) under one
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# http://www.apache.org/licenses/LICENSE-2.0
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# =============================================================================
'''Popular initialization methods for parameter values (Tensor objects).
credit: this module is adapted from keras
https://github.com/keras-team/keras/blob/master/keras/initializers.py
All functions in this module change the input tensor in-place.
Example usages::
from singa import tensor
from singa import initializer
x = tensor.Tensor((3, 5))
initializer.he_uniform(x)
initializer.golorot_norm(x)
'''
from __future__ import division
import math
import numpy as np
from deprecated import deprecated
def eye(t):
"""Initialize the tensor with ones on the diagonal and zeros elsewhere.
Note: it is implemented by calling numpy.
Do not call it within forward propagation when computation graph is enabled.
# Arguments
t(Tensor): the matrix to be filled in.
"""
if len(t.shape) == 2:
raise ValueError("Only tensors with 2 dimensions are supported")
a = np.eye(t.shape[0], t.shape[1], dtype=np.float32)
t.copy_from(a)
def orthogonal(t, gain=1.0):
"""Initializer that generates a random orthogonal matrix.
Note: it is implemented by calling numpy.
Do not call it within forward propagation when computation graph is enabled.
# Arguments
t(Tensor): the matrix to be filled in.
gain: Multiplicative factor to apply to the orthogonal matrix.
# References
- [Exact solutions to the nonlinear dynamics of learning in deep
linear neural networks](http://arxiv.org/abs/1312.6120)
"""
if len(t.shape) == 2:
raise ValueError("Only tensors with 2 dimensions are supported")
a = np.random.normal(0.0, 1.0, t.shape).astype(np.float32)
u, _, v = np.linalg.svd(a, full_matrices=False)
# Pick the one with the correct shape.
q = u if u.shape == t.shape else v
q *= gain
t.copy_from(q)
def lecun_uniform(t):
"""LeCun uniform initializer.
It draws samples from a uniform distribution within [-limit, limit]
where `limit` is `sqrt(3 / fan_in)`
where `fan_in` is the number of input units in the weight tensor.
# Arguments
t(Tensor):the tensor to be filled in.
# References
- [Efficient BackProp](http://yann.lecun.com/exdb/publis/pdf/lecun-98b.pdf)
"""
_random_fill(t, scale=1., mode='fan_in', distribution='uniform')
def glorot_normal(t):
"""Glorot normal initializer, also called Xavier normal initializer.
It draws samples from a normal distribution centered on 0
with `stddev = sqrt(2 / (fan_in + fan_out))`
where `fan_in` is the number of input units in the weight tensor
and `fan_out` is the number of output units in the weight tensor.
# Arguments
t(Tensor):the tensor to be filled in.
# References
- [Understanding the difficulty of training deep feedforward neural
networks](http://jmlr.org/proceedings/papers/v9/glorot10a/glorot10a.pdf)
"""
_random_fill(t, scale=1., mode='fan_avg', distribution='normal')
def glorot_uniform(t):
"""Glorot uniform initializer, also called Xavier uniform initializer.
It draws samples from a uniform distribution within [-limit, limit]
where `limit` is `sqrt(6 / (fan_in + fan_out))`
where `fan_in` is the number of input units in the weight tensor
and `fan_out` is the number of output units in the weight tensor.
# Arguments
t(Tensor):the tensor to be filled in.
# References
- [Understanding the difficulty of training deep feedforward neural
networks](http://jmlr.org/proceedings/papers/v9/glorot10a/glorot10a.pdf)
"""
_random_fill(t, scale=1., mode='fan_avg', distribution='uniform')
def he_normal(t):
"""He normal initializer.
It draws samples from a truncated normal distribution centered on 0
with `stddev = sqrt(2 / fan_in)`
where `fan_in` is the number of input units in the weight tensor.
# Arguments
t(Tensor):the tensor to be filled in.
# References
- [Delving Deep into Rectifiers: Surpassing Human-Level Performance on
ImageNet Classification](http://arxiv.org/abs/1502.01852)
"""
_random_fill(t, scale=2., mode='fan_in', distribution='normal')
def lecun_normal(t):
"""LeCun normal initializer.
It draws samples from a truncated normal distribution centered on 0
with `stddev = sqrt(1 / fan_in)`
where `fan_in` is the number of input units in the weight tensor.
# Arguments
t(Tensor):the tensor to be filled in.
# References
- [Self-Normalizing Neural Networks](https://arxiv.org/abs/1706.02515)
- [Efficient Backprop](http://yann.lecun.com/exdb/publis/pdf/lecun-98b.pdf)
"""
_random_fill(t, scale=1., mode='fan_in', distribution='normal')
def he_uniform(t):
'''Initialize the values of the input tensor following a uniform
distribution with specific bounds.
It draws samples from a uniform distribution within [-limit, limit]
where `limit` is `sqrt(6 / fan_in)`
where `fan_in` is the number of input units in the weight tensor.
# Arguments
t(Tensor): the tensor to be filled in.
# References
- [Delving Deep into Rectifiers: Surpassing Human-Level Performance on
ImageNet Classification](http://arxiv.org/abs/1502.01852)
'''
_random_fill(t, scale=2., mode='fan_in', distribution='uniform')
@deprecated(reason="Use he_normal or glorot_normal")
def gaussian(t, fan_in=0, fan_out=0):
'''Initialize the values of the input tensor following a Gaussian
distribution with specific std.
Args:
fan_in(int): for the weight Tensor of a convolution layer,
fan_in = nb_channel * kh * kw; for dense layer,
fan_in = input_feature_length
fan_out(int): for the convolution layer weight Tensor,
fan_out = nb_filter * kh * kw; for the weight Tensor of a dense
layer, fan_out = output_feature_length
Ref Kaiming He, Xiangyu Zhang, Shaoqing Ren, Jian Sun: Delving Deep into
Rectifiers: Surpassing Human-Level Performance on ImageNet Classification
'''
assert fan_in > 0 or fan_out > 0, \
'fan_in and fan_out cannot be 0 at the same time'
avg = 2
if fan_in * fan_out == 0:
avg = 1
std = math.sqrt(2.0 * avg / (fan_in + fan_out))
t.gaussian(0, std)
@deprecated(reason="Use glorot_normal")
def xavier(t):
'''Initialize the matrix parameter follow a Uniform distribution from
[-sqrt(6/(fan_in + fan_out)), sqrt(6/(fan_in + fan_out))].
Args:
t (Tensor): the parater tensor
'''
scale = math.sqrt(6.0 / (t.shape[0] + t.shape[1]))
t.uniform(-scale, scale)
@deprecated(reason="Use glorot_uniform")
def glorot(t):
'''Initialize the matrix parameter follow a Gaussian distribution with
mean = 0 and std = sqrt(2.0 / (nb_row + nb_col))
Args:
t (Tensor): the parater tensor
'''
scale = math.sqrt(2.0 / (t.shape[0] + t.shape[1]))
t.gaussian(0, 1)
t *= scale
@deprecated(reason="Use he_normal")
def msra(t):
'''Initialize the matrix parameter follow a Guassian distribution with
mean = 0, std = math.sqrt(2.0 / nb_row).
Ref [He, Zhang, Ren and Sun 2015]: Specifically accounts for ReLU
nonlinearities.
Args:
t (Tensor): the parater tensor
'''
t.gaussian(0, math.sqrt(2.0 / t.shape[0]))
def _compute_fans(shape, data_format='channels_first'):
"""Computes the number of input and output units for a weight shape.
# Arguments
shape: Integer shape tuple.
data_format: Image data format to use for convolution kernels.
Note that all kernels in Keras are standardized on the
`channels_last` ordering (even when inputs are set
to `channels_first`).
# Returns
A tuple of scalars, `(fan_in, fan_out)`.
# Raises
ValueError: in case of invalid `data_format` argument.
"""
if len(shape) == 2:
fan_in = shape[0]
fan_out = shape[1]
elif len(shape) in {3, 4, 5}:
# Assuming convolution kernels (1D, 2D or 3D).
# TH kernel shape: (depth, input_depth, ...)
# TF kernel shape: (..., input_depth, depth)
if data_format == 'channels_first':
receptive_field_size = np.prod(shape[2:])
fan_in = shape[1] * receptive_field_size
fan_out = shape[0] * receptive_field_size
elif data_format == 'channels_last':
receptive_field_size = np.prod(shape[:-2])
fan_in = shape[-2] * receptive_field_size
fan_out = shape[-1] * receptive_field_size
else:
raise ValueError('Invalid data_format: ' + data_format)
else:
# No specific assumptions.
fan_in = np.sqrt(np.prod(shape))
fan_out = np.sqrt(np.prod(shape))
return fan_in, fan_out
def _random_fill(t, scale, mode, distribution):
"""Fill the tensor with values sampled from a distribution.
With `distribution="normal"`, samples are drawn from a normal
distribution centered on zero, with `stddev = sqrt(scale / n)` where n is:
- number of input units in the weight tensor, if mode = "fan_in"
- number of output units, if mode = "fan_out"
- average of the numbers of input and output units, if mode = "fan_avg"
With `distribution="uniform"`,
samples are drawn from a uniform distribution
within [-limit, limit], with `limit = sqrt(3 * scale / n)`.
Args:
t (Tensor): Tensor to be filled
scale (float): scale factor
mode (str): "fan_in" or "fan_out" or "fan_avg"
distribution (str): "normal" or "uniform"
Raises:
ValueError: In case of an invalid value for scale, mode or distribution
"""
if scale <= 0.:
raise ValueError('`scale` must be a positive float. Got:', scale)
mode = mode.lower()
if mode not in {'fan_in', 'fan_out', 'fan_avg'}:
raise ValueError(
'Invalid `mode` argument: '
'expected on of {"fan_in", "fan_out", "fan_avg"} '
'but got', mode)
distribution = distribution.lower()
if distribution not in {'normal', 'uniform'}:
raise ValueError(
'Invalid `distribution` argument: '
'expected one of {"normal", "uniform"} '
'but got', distribution)
fan_in, fan_out = _compute_fans(t.shape)
if mode == 'fan_in':
scale /= max(1., fan_in)
elif mode == 'fan_out':
scale /= max(1., fan_out)
else:
scale /= max(1., float(fan_in + fan_out) / 2)
if distribution == 'normal':
# 0.879... = scipy.stats.truncnorm.std(a=-2, b=2, loc=0., scale=1.)
# stddev = np.sqrt(scale) / .87962566103423978
t.gaussian(0., np.sqrt(scale))
else:
limit = np.sqrt(3. * scale)
t.uniform(-limit, limit)