I have a code that works perfectly well but I wish to speed up the time it takes to converge. A snippet of the code is shown below:
def myfunction(x, i):
y = x + (min(0, target[i] - data[i, :]x))*data[i]/(norm(data[i])**2))
return y
rows, columns = data.shape
start = time.time()
iterate = 0
iterate_count = []
norm_count = []
res = 5
x_not = np.ones(columns)
norm_count.append(norm(x_not))
iterate_count.append(0)
while res > 1e-8:
for row in range(rows):
y = myfunction(x_not, row)
x_not = y
iterate += 1
iterate_count.append(iterate)
norm_count.append(norm(x_not))
res = abs(norm_count[-1] - norm_count[-2])
print('Converge at {} iterations'.format(iterate))
print('Duration: {:.4f} seconds'.format(time.time() - start))
I am relatively new in Python. I will appreciate any hint/assistance.
Ax=b is the problem we wish to solve. Here, 'A' is the 'data' and 'b' is the 'target'
Ugh! After spending a while on this I don't think it can be done the way you've set up your problem. In each iteration over the row, you modify x_not and then pass the updated result to get the solution for the next row. This kind of setup can't be vectorized easily. You can learn the thought process of vectorization from the failed attempt, so I'm including it in the answer. I'm also including a different iterative method to solve linear systems of equations. I've included a vectorized version -- where the solution is updated using matrix multiplication and vector addition, and a loopy version -- where the solution is updated using a for loop to demonstrate what you can expect to gain.
1. The failed attempt
Let's take a look at what you're doing here.
def myfunction(x, i):
y = x + (min(0, target[i] - data[i, :] # x)) * (data[i] / (norm(data[i])**2))
return y
You subtract
the dot product of (the ith row of data and x_not)
from the ith row of target,
limited at zero.
You multiply this result with the ith row of data divided my the norm of that row squared. Let's call this part2
Then you add this to the ith element of x_not
Now let's look at the shapes of the matrices.
data is (M, N).
target is (M, ).
x_not is (N, )
Instead of doing these operations rowwise, you can operate on the entire matrix!
1.1. Simplifying the dot product.
Instead of doing data[i, :] # x, you can do data # x_not and this gives an array with the ith element giving the dot product of the ith row with x_not. So now we have data # x_not with shape (M, )
Then, you can subtract this from the entire target array, so target - (data # x_not) has shape (M, ).
So far, we have
part1 = target - (data # x_not)
Next, if anything is greater than zero, set it to zero.
part1[part1 > 0] = 0
1.2. Finding rowwise norms.
Finally, you want to multiply this by the row of data, and divide by the square of the L2-norm of that row. To get the norm of each row of a matrix, you do
rownorms = np.linalg.norm(data, axis=1)
This is a (M, ) array, so we need to convert it to a (M, 1) array so we can divide each row. rownorms[:, None] does this. Then divide data by this.
part2 = data / (rownorms[:, None]**2)
1.3. Add to x_not
Finally, we're adding each row of part1 * part2 to the original x_not and returning the result
result = x_not + (part1 * part2).sum(axis=0)
Here's where we get stuck. In your approach, each call to myfunction() gives a value of part1 that depends on target[i], which was changed in the last call to myfunction().
2. Why vectorize?
Using numpy's inbuilt methods instead of looping allows it to offload the calculation to its C backend, so it runs faster. If your numpy is linked to a BLAS backend, you can extract even more speed by using your processor's SIMD registers
The conjugate gradient method is a simple iterative method to solve certain systems of equations. There are other more complex algorithms that can solve general systems well, but this should do for the purposes of our demo. Again, the purpose is not to have an iterative algorithm that will perfectly solve any linear system of equations, but to show what kind of speedup you can expect if you vectorize your code.
Given your system
data # x_not = target
Let's define some variables:
A = data.T # data
b = data.T # target
And we'll solve the system A # x = b
x = np.zeros((columns,)) # Initial guess. Can be anything
resid = b - A # x
p = resid
while (np.abs(resid) > tolerance).any():
Ap = A # p
alpha = (resid.T # resid) / (p.T # Ap)
x = x + alpha * p
resid_new = resid - alpha * Ap
beta = (resid_new.T # resid_new) / (resid.T # resid)
p = resid_new + beta * p
resid = resid_new + 0
To contrast the fully vectorized approach with one that uses iterations to update the rows of x and resid_new, let's define another implementation of the CG solver that does this.
def solve_loopy(data, target, itermax = 100, tolerance = 1e-8):
A = data.T # data
b = data.T # target
rows, columns = data.shape
x = np.zeros((columns,)) # Initial guess. Can be anything
resid = b - A # x
resid_new = b - A # x
p = resid
niter = 0
while (np.abs(resid) > tolerance).any() and niter < itermax:
Ap = A # p
alpha = (resid.T # resid) / (p.T # Ap)
for i in range(len(x)):
x[i] = x[i] + alpha * p[i]
resid_new[i] = resid[i] - alpha * Ap[i]
# resid_new = resid - alpha * A # p
beta = (resid_new.T # resid_new) / (resid.T # resid)
p = resid_new + beta * p
resid = resid_new + 0
niter += 1
return x
And our original vector method:
def solve_vect(data, target, itermax = 100, tolerance = 1e-8):
A = data.T # data
b = data.T # target
rows, columns = data.shape
x = np.zeros((columns,)) # Initial guess. Can be anything
resid = b - A # x
resid_new = b - A # x
p = resid
niter = 0
while (np.abs(resid) > tolerance).any() and niter < itermax:
Ap = A # p
alpha = (resid.T # resid) / (p.T # Ap)
x = x + alpha * p
resid_new = resid - alpha * Ap
beta = (resid_new.T # resid_new) / (resid.T # resid)
p = resid_new + beta * p
resid = resid_new + 0
niter += 1
return x
Let's solve a simple system to see if this works first:
2x1 + x2 = -5
−x1 + x2 = -2
should give a solution of [-1, -3]
data = np.array([[ 2, 1],
[-1, 1]])
target = np.array([-5, -2])
print(solve_loopy(data, target))
print(solve_vect(data, target))
Both give the correct solution [-1, -3], yay! Now on to bigger things:
data = np.random.random((100, 100))
target = np.random.random((100, ))
Let's ensure the solution is still correct:
sol1 = solve_loopy(data, target)
np.allclose(data # sol1, target)
# Output: False
sol2 = solve_vect(data, target)
np.allclose(data # sol2, target)
# Output: False
Hmm, looks like the CG method doesn't work for badly conditioned random matrices we created. Well, at least both give the same result.
np.allclose(sol1, sol2)
# Output: True
But let's not get discouraged! We don't really care if it works perfectly, the point of this is to demonstrate how amazing vectorization is. So let's time this:
import timeit
timeit.timeit('solve_loopy(data, target)', number=10, setup='from __main__ import solve_loopy, data, target')
# Output: 0.25586539999994784
timeit.timeit('solve_vect(data, target)', number=10, setup='from __main__ import solve_vect, data, target')
# Output: 0.12008900000000722
Nice! A ~2x speedup simply by avoiding a loop while updating our solution!
For larger systems, this will be even better.
for N in [10, 50, 100, 500, 1000]:
data = np.random.random((N, N))
target = np.random.random((N, ))
t_loopy = timeit.timeit('solve_loopy(data, target)', number=10, setup='from __main__ import solve_loopy, data, target')
t_vect = timeit.timeit('solve_vect(data, target)', number=10, setup='from __main__ import solve_vect, data, target')
print(N, t_loopy, t_vect, t_loopy/t_vect)
This gives us:
N t_loopy t_vect speedup
00010 0.002823 0.002099 1.345390
00050 0.051209 0.014486 3.535048
00100 0.260348 0.114601 2.271773
00500 0.980453 0.240151 4.082644
01000 1.769959 0.508197 3.482822
Related
I would like to solve the above formulation in Scipy and solve it using milp(). For a given graph (V, E), f_ij and x_ij are the decision variables. f_ij is the flow from i to j (it can be continuous). x_ij is the number of vehicles from i to j. p is the price. X is the available number vehicles in a region. c is the capacity.
I have difficulty in translating the formulation to Scipy milp code. I would appreciate it if anyone could give me some pointers.
What I have done:
The code for equation (1):
f_obj = [p[i] for i in Edge]
x_obj = [0]*len(Edge)
obj = f_obj + v_obj
Integrality:
f_cont = [0 for i in Edge] # continous
x_int = [1]*len(Edge) # integer
integrality = f_cont + x_int
Equation (2):
def constraints(self):
b = []
A = []
const = [0]*len(Edge) # for f_ij
for i in v: # for x_ij
for e in Edge:
if e[0] == i:
const.append(1)
else:
const.append(0)
A.append(const)
b.append(self.accInit[i])
const = [0]*len(Edge) # for f_ij
return A, b
Equation (4):
[(0, demand[e]) for e in Edge]
I'm going to do some wild guessing, given how much you've left open to interpretation. Let's assume that
this is a maximisation problem, since the minimisation problem is trivial
Expression (1) is actually the maximisation objective function, though you failed to write it as such
p and d are floating-point vectors
X is an integer vector
c is a floating-point scalar
the graph edges, since you haven't described them at all, do not matter for problem setup
The variable names are not well-chosen and hide what they actually contain. I demonstrate potential replacements.
import numpy as np
from numpy.random._generator import Generator
from scipy.optimize import milp, Bounds, LinearConstraint
import scipy.sparse
from numpy.random import default_rng
rand: Generator = default_rng(seed=0)
N = 20
price = rand.uniform(low=0, high=10, size=N) # p
demand = rand.uniform(low=0, high=10, size=N) # d
availability = rand.integers(low=0, high=10, size=N) # X aka. accInit
capacity = rand.uniform(low=0, high=10) # c
c = np.zeros(2*N) # f and x
c[:N] = -price # (1) f maximized with coefficients of 'p'
# x not optimized
CONTINUOUS = 0
INTEGER = 1
integrality = np.empty_like(c, dtype=int)
integrality[:N] = CONTINUOUS # f
integrality[N:] = INTEGER # x
upper = np.empty_like(c)
upper[:N] = demand # (4) f
upper[N:] = availability # (2) x
eye_N = scipy.sparse.eye(N)
A = scipy.sparse.hstack((-eye_N, capacity*eye_N)) # (3) 0 <= -f + cx
result = milp(
c=c, integrality=integrality,
bounds=Bounds(lb=np.zeros_like(c), ub=upper),
constraints=LinearConstraint(lb=np.zeros(N), A=A),
)
print(result.message)
flow = result.x[:N]
vehicles = result.x[N:].astype(int)
I'm trying to apply the method for baselinining vibrational spectra, which is announced as an improvement over asymmetric and iterative re-weighted least-squares algorithms in the 2015 paper (doi:10.1039/c4an01061b), where the following matlab code was provided:
function z = baseline(y, lambda, ratio)
% Estimate baseline with arPLS in Matlab
N = length(y);
D = diff(speye(N), 2);
H = lambda*D'*D;
w = ones(N, 1);
while true
W = spdiags(w, 0, N, N);
% Cholesky decomposition
C = chol(W + H);
z = C \ (C' \ (w.*y) );
d = y - z;
% make d-, and get w^t with m and s
dn = d(d<0);
m = mean(d);
s = std(d);
wt = 1./ (1 + exp( 2* (d-(2*s-m))/s ) );
% check exit condition and backup
if norm(w-wt)/norm(w) < ratio, break; end
end
that I rewrote into python:
def baseline_arPLS(y, lam, ratio):
# Estimate baseline with arPLS
N = len(y)
k = [numpy.ones(N), -2*numpy.ones(N-1), numpy.ones(N-2)]
offset = [0, 1, 2]
D = diags(k, offset).toarray()
H = lam * numpy.matmul(D.T, D)
w_ = numpy.ones(N)
while True:
W = spdiags(w_, 0, N, N, format='csr')
# Cholesky decomposition
C = cholesky(W + H)
z_ = spsolve(C.T, w_ * y)
z = spsolve(C, z_)
d = y - z
# make d- and get w^t with m and s
dn = d[d<0]
m = numpy.mean(dn)
s = numpy.std(dn)
wt = 1. / (1 + numpy.exp(2 * (d - (2*s-m)) / s))
# check exit condition and backup
norm_wt, norm_w = norm(w_-wt), norm(w_)
if (norm_wt / norm_w) < ratio:
break
w_ = wt
return(z)
Except for the input vector y the method requires parameters lam and ratio and it runs ok for values lam<1.e+07 and ratio>1.e-01, but outputs poor results. When values are changed outside this range, for example lam=1e+07, ratio=1e-02 the CPU starts heating up and job never finishes (I interrupted it after 1min). Also in both cases the following warning shows up:
/usr/local/lib/python3.9/site-packages/scipy/sparse/linalg/dsolve/linsolve.py: 144: SparseEfficencyWarning: spsolve requires A to be CSC or CSR matrix format warn('spsolve requires A to be CSC or CSR format',
although I added the recommended format='csr' option to the spdiags call.
And here's some synthetic data (similar to one in the paper) for testing purposes. The noise was added along with a 3rd degree polynomial baseline The method works well for parameters bl_1 and fails to converge for bl_2:
import numpy
from matplotlib import pyplot
from scipy.sparse import spdiags, diags, identity
from scipy.sparse.linalg import spsolve
from numpy.linalg import cholesky, norm
import sys
x = numpy.arange(0, 1000)
noise = numpy.random.uniform(low=0, high = 10, size=len(x))
poly_3rd_degree = numpy.poly1d([1.2e-06, -1.23e-03, .36, -4.e-04])
poly_baseline = poly_3rd_degree(x)
y = 100 * numpy.exp(-((x-300)/15)**2)+\
200 * numpy.exp(-((x-750)/30)**2)+ \
100 * numpy.exp(-((x-800)/15)**2) + noise + poly_baseline
bl_1 = baseline_arPLS(y, 1e+07, 1e-01)
bl_2 = baseline_arPLS(y, 1e+07, 1e-02)
pyplot.figure(1)
pyplot.plot(x, y, 'C0')
pyplot.plot(x, poly_baseline, 'C1')
pyplot.plot(x, bl_1, 'k')
pyplot.show()
sys.exit(0)
All this is telling me that I'm doing something very non-optimal in my python implementation. Since I'm not knowledgeable enough about the intricacies of scipy computations I'm kindly asking for suggestions on how to achieve convergence in this calculations.
(I encountered an issue in running the "straight" matlab version of the code because the line D = diff(speye(N), 2); truncates the last two rows of the matrix, creating dimension mismatch later in the function. Following the description of matrix D's appearance I substituted this line by directly creating a tridiagonal matrix using the diags function.)
Guided by the comment #hpaulj made, and suspecting that the loop exit wasn't coded properly, I re-visited the paper and found out that the authors actually implemented an exit condition that was not featured in their matlab script. Changing the while loop condition provides an exit for any set of parameters; my understanding is that algorithm is not guaranteed to converge in all cases, which is why this condition is necessary but was omitted by error. Here's the edited version of my python code:
def baseline_arPLS(y, lam, ratio):
# Estimate baseline with arPLS
N = len(y)
k = [numpy.ones(N), -2*numpy.ones(N-1), numpy.ones(N-2)]
offset = [0, 1, 2]
D = diags(k, offset).toarray()
H = lam * numpy.matmul(D.T, D)
w_ = numpy.ones(N)
i = 0
N_iterations = 100
while i < N_iterations:
W = spdiags(w_, 0, N, N, format='csr')
# Cholesky decomposition
C = cholesky(W + H)
z_ = spsolve(C.T, w_ * y)
z = spsolve(C, z_)
d = y - z
# make d- and get w^t with m and s
dn = d[d<0]
m = numpy.mean(dn)
s = numpy.std(dn)
wt = 1. / (1 + numpy.exp(2 * (d - (2*s-m)) / s))
# check exit condition and backup
norm_wt, norm_w = norm(w_-wt), norm(w_)
if (norm_wt / norm_w) < ratio:
break
w_ = wt
i += 1
return(z)
Say, I have a binary (adjacency) matrix A of dimensions nxn and another matrix U of dimensions nxl. I use the following piece of code to compute a new matrix that I need.
import numpy as np
from numpy import linalg as LA
new_U = np.zeros_like(U)
for idx, a in np.ndenumerate(A):
diff = U[idx[0], :] - U[idx[1], :]
if a == 1.0:
new_U[idx[0], :] += 2 * diff
elif a == 0.0:
norm_diff = LA.norm(U[idx[0], :] - U[idx[1], :])
new_U[idx[0], :] += -2 * diff * np.exp(-norm_diff**2)
return new_U
This takes quite a lot of time to run even when n and l are small. Is there a better way to rewrite (vectorize) this code to reduce the runtime?
Edit 1: Sample input and output.
A = np.array([[0,1,0], [1,0,1], [0,1,0]], dtype='float64')
U = np.array([[2,3], [4,5], [6,7]], dtype='float64')
new_U = np.array([[-4.,-4.], [0,0],[4,4]], dtype='float64')
Edit 2: In mathematical notation, I am trying to compute the following:
where u_ik = U[i, k],u_jk = U[j, k], and u_i = U[i, :]. Also, (i,j) \in E corresponds to a == 1.0 in the code.
Leveraging broadcasting and np.einsum for the sum-reductions -
# Get pair-wise differences between rows for all rows in a vectorized manner
Ud = U[:,None,:]-U
# Compute norm L1 values with those differences
L = LA.norm(Ud,axis=2)
# Compute 2 * diff values for all rows and mask it with ==0 condition
# and sum along axis=1 to simulate the accumulating behaviour
p1 = np.einsum('ijk,ij->ik',2*Ud,A==1.0)
# Similarly, compute for ==1 condition and finally sum those two parts
p2 = np.einsum('ijk,ij,ij->ik',-2*Ud,np.exp(-L**2),A==0.0)
out = p1+p2
Alternatively, use einsum for computing squared-norm values and using those to get p2 -
Lsq = np.einsum('ijk,ijk->ij',Ud,Ud)
p2 = np.einsum('ijk,ij,ij->ik',-2*Ud,np.exp(-Lsq),A==0.0)
I have two functions that compute the same metric. One ends up using a list comprehension to cycle through a calculation, the other uses only numpy tensor operations. The functions take in a (N, 3) array, where N is the number of points in 3D space. When N <~ 3000 the tensor function is faster, when N >~ 3000 the list comprehension is faster. Both seem to have linear time complexity in terms of N i.e two time-N lines cross at N=~3000.
def approximate_area_loop(section, num_area_divisions):
n_a_d = num_area_divisions
interp_vectors = get_section_interp_(section)
a1 = section[:-1]
b1 = section[1:]
a2 = interp_vectors[:-1]
b2 = interp_vectors[1:]
c = lambda u: (1 - u) * a1 + u * a2
d = lambda u: (1 - u) * b1 + u * b2
x = lambda u, v: (1 - v) * c(u) + v * d(u)
area = np.sum([np.linalg.norm(np.cross((x((i + 1)/n_a_d, j/n_a_d) - x(i/n_a_d, j/n_a_d)),\
(x(i/n_a_d, (j +1)/n_a_d) - x(i/n_a_d, j/n_a_d))), axis = 1)\
for i in range(n_a_d) for j in range(n_a_d)])
Dt = section[-1, 0] - section[0, 0]
return area, Dt
def approximate_area_tensor(section, num_area_divisions):
divisors = np.linspace(0, 1, num_area_divisions + 1)
interp_vectors = get_section_interp_(section)
a1 = section[:-1]
b1 = section[1:]
a2 = interp_vectors[:-1]
b2 = interp_vectors[1:]
c = np.multiply.outer(a1, (1 - divisors)) + np.multiply.outer(a2, divisors) # c_areas_vecs_divs
d = np.multiply.outer(b1, (1 - divisors)) + np.multiply.outer(b2, divisors) # d_areas_vecs_divs
x = np.multiply.outer(c, (1 - divisors)) + np.multiply.outer(d, divisors) # x_areas_vecs_Divs_divs
u = x[:, :, 1:, :-1] - x[:, :, :-1, :-1] # u_areas_vecs_Divs_divs
v = x[:, :, :-1, 1:] - x[:, :, :-1, :-1] # v_areas_vecs_Divs_divs
sub_area_norm_vecs = np.cross(u, v, axis = 1) # areas_crosses_Divs_divs
sub_areas = np.linalg.norm(sub_area_norm_vecs, axis = 1) # areas_Divs_divs (values are now sub areas)
area = np.sum(sub_areas)
Dt = section[-1, 0] - section[0, 0]
return area, Dt
Why does the list comprehension version work faster at large N? Surely the tensor version should be faster? I'm wondering if it's something to do with the size of the calculations meaning it's too big to be done in cache? Please ask if I haven't included enough information, I'd really like to get to the bottom of this.
The bottleneck in the fully vectorized function was indeed in the np.linalg.norm as #hpauljs comment suggested.
Norm was used only to get the magnitude of all the vectors contained in axis 1. A much simpler and faster method was to just:
sub_areas = np.sqrt((sub_area_norm_vecs*sub_area_norm_vecs).sum(axis = 1))
This gives exactly the same results and sped up the code by up to 25 times faster than the loop implementation (even when the loop doesn't use linalg.norm either).
Instructions: Compute and store R=1000 random values from 0-1 as x. moving_window_average(x, n_neighbors) is pre-loaded into memory from 3a. Compute the moving window average for x for the range of n_neighbors 1-9. Store x as well as each of these averages as consecutive lists in a list called Y.
My solution:
R = 1000
n_neighbors = 9
x = [random.uniform(0,1) for i in range(R)]
Y = [moving_window_average(x, n_neighbors) for n_neighbors in range(1,n_neighbors)]
where moving_window_average(x, n_neighbors) is a function as follows:
def moving_window_average(x, n_neighbors=1):
n = len(x)
width = n_neighbors*2 + 1
x = [x[0]]*n_neighbors + x + [x[-1]]*n_neighbors
# To complete the function,
# return a list of the mean of values from i to i+width for all values i from 0 to n-1.
mean_values=[]
for i in range(1,n+1):
mean_values.append((x[i-1] + x[i] + x[i+1])/width)
return (mean_values)
This gives me an error, Check your usage of Y again. Even though I've tested for a few values, I did not get yet why there is a problem with this exercise. Did I just misunderstand something?
The instruction tells you to compute moving averages for all neighbors ranging from 1 to 9. So the below code should work:
import random
random.seed(1)
R = 1000
x = []
for i in range(R):
num = random.uniform(0,1)
x.append(num)
Y = []
Y.append(x)
for i in range(1,10):
mov_avg = moving_window_average(x, n_neighbors=i)
Y.append(mov_avg)
Actually your moving_window_average(list, n_neighbors) function is not going to work with a n_neighbors bigger than one, I mean, the interpreter won't say a thing, but you're not delivering correctness on what you have been asked.
I suggest you to use something like:
def moving_window_average(x, n_neighbors=1):
n = len(x)
width = n_neighbors*2 + 1
x = [x[0]]*n_neighbors + x + [x[-1]]*n_neighbors
mean_values = []
for i in range(n):
temp = x[i: i+width]
sum_= 0
for elm in temp:
sum_+= elm
mean_values.append(sum_ / width)
return mean_values
My solution for +100XP
import random
random.seed(1)
R=1000
Y = list()
x = [random.uniform(0, 1) for num in range(R)]
for n_neighbors in range(10):
Y.append(moving_window_average(x, n_neighbors))