I currently have a volume spanned by a few million every unevenly spaced particles and each particle has an attribute (potential, for those who are curious) that I want to calculate the local force (acceleration) for.
np.gradient only works with evenly spaced data and I looked here: Second order gradient in numpy where interpolation is necessary but I could not find a 3D spline implementation in Numpy.
Some code that will produce representative data:
import numpy as np
from scipy.spatial import cKDTreex = np.random.uniform(-10, 10, 10000)
y = np.random.uniform(-10, 10, 10000)
z = np.random.uniform(-10, 10, 10000)
phi = np.random.uniform(-10**9, 0, 10000)kdtree = cKDTree(np.c_[x,y,z])
_, index = kdtree.query([0,0,0], 32) #find 32 nearest particles to the origin
#find the gradient at (0,0,0) by considering the 32 nearest particles?
(My problem is very similar to Function to compute 3D gradient with unevenly spaced sample locations but there seemed to have been no solution there, so I thought I'd ask again.)
Any help would be appreciated.
Here is a Julia implementation that does what you ask
using NearestNeighborsn = 3;
k = 32; # for stability use k > n*(n+3)/2# Take a point near the center of cube
point = 0.5 + rand(n)*1e-3;
data = rand(n, 10^4);
kdtree = KDTree(data);
idxs, dists = knn(kdtree, point, k, true);# Coords of the k-Nearest Neighbors
X = data[:,idxs];# Least-squares recipe for coefficientsC = point * ones(1,k); # central node
dX = X - C; # diffs from central nodeG = dX' * dX;F = G .* G;v = diag(G);N = pinv(G) * G;N = eye(N) - N;a = N * pinv(F*N) * v; # ...these are the coeffs# Use a temperature distribution of T = 25.4 * r^2
# whose analytical gradient is gradT = 25.4 * 2*x
X2 = X .* X;
C2 = C .* C;
T = 25.4 * n * mean(X2, 1)';
Tc = 25.4 * n * mean(C2, 1)'; # central node
dT = T - Tc; # diffs from central nodey = dX * (a .* dT); # Estimated gradient
g = 2 * 25.4 * point; # Analytical# print results
@printf "Estimated Grad = %s\n" string(y')
@printf "Analytical Grad = %s\n" string(g')
@printf "Relative Error = %.8f\n" vecnorm(g-y)/vecnorm(g)
This method has about a 1% relative error. Here are the results from a few runs...
Estimated Grad = [25.51670916224472 25.421038632006926 25.6711949674633]
Analytical Grad = [25.41499027802736 25.44913042322385 25.448202594123806]
Relative Error = 0.00559934Estimated Grad = [25.310574056859014 25.549736360607493 25.368056350800604]
Analytical Grad = [25.43200914200516 25.43243178887198 25.45061497749628]
Relative Error = 0.00426558
Update
I don't know Python very well, but here is a translation that seems to be working
import numpy as np
from scipy.spatial import KDTreen = 3;
k = 32;# fill the cube with random points
data = np.random.rand(10000,n)
kdtree = KDTree(data)# pick a point (at the center of the cube)
point = 0.5 * np.ones((1,n))# Coords of k-Nearest Neighbors
dists, idxs = kdtree.query(point, k)
idxs = idxs[0]
X = data[idxs,:]# Calculate coefficients
C = (np.dot(point.T, np.ones((1,k)))).T # central node
dX= X - C # diffs from central node
G = np.dot(dX, dX.T)
F = np.multiply(G, G)
v = np.diag(G);
N = np.dot(np.linalg.pinv(G), G)
N = np.eye(k) - N;
a = np.dot(np.dot(N, np.linalg.pinv(np.dot(F,N))), v) # these are the coeffs# Temperature distribution is T = 25.4 * r^2
X2 = np.multiply(X, X)
C2 = np.multiply(C, C)
T = 25.4 * n * np.mean(X2, 1).T
Tc = 25.4 * n * np.mean(C2, 1).T # central node
dT = T - Tc; # diffs from central node# Analytical gradient ==> gradT = 2*25.4* x
g = 2 * 25.4 * point;
print( "g[]: %s" % (g) )# Estimated gradient
y = np.dot(dX.T, np.multiply(a, dT))
print( "y[]: %s, Relative Error = %.8f" % (y, np.linalg.norm(g-y)/np.linalg.norm(g)) )
Update #2
I think I can write something comprehensible using formatted ASCII instead of LaTeX...
`Given a set of M vectors in n-dimensions (call them b_k), find a set of
`coeffs (call them a_k) which yields the best estimate of the identity
`matrix and the zero vector
`
` M
` (1) min ||E - I||, where E = sum a_k b_k b_k
` a_k k=1
`
` M
` (2) min ||z - 0||, where z = sum a_k b_k
` a_k k=1
`
`
`Note that the basis vectors {b_k} are not required
`to be normalized, orthogonal, or even linearly independent.
`
`First, define the following quantities:
`
` B ==> matrix whose columns are the b_k
` G = B'.B ==> transpose of B times B
` F = G @ G ==> @ represents the hadamard product
` v = diag(G) ==> vector composed of diag elements of G
`
`The above minimizations are equivalent to this linearly constrained problem
`
` Solve F.a = v
` s.t. G.a = 0
`
`Let {X} denote the Moore-Penrose inverse of X.
`Then the solution of the linear problem can be written:
`
` N = I - {G}.G ==> projector into nullspace of G
` a = N . {F.N} . v
`
`The utility of these coeffs is that they allow you to write
`very simple expressions for the derivatives of a tensor field.
`
`
`Let D be the del (or nabla) operator
`and d be the difference operator wrt the central (aka 0th) node,
`so that, for any scalar/vector/tensor quantity Y, we have:
` dY = Y - Y_0
`
`Let x_k be the position vector of the kth node.
`And for our basis vectors, take
` b_k = dx_k = x_k - x_0.
`
`Assume that each node has a field value associated with it
` (e.g. temperature), and assume a quadratic model [about x = x_0]
` for the field [g=gradient, H=hessian, ":" is the double-dot product]
`
` Y = Y_0 + (x-x_0).g + (x-x_0)(x-x_0):H/2
` dY = dx.g + dxdx:H/2
` D2Y = I:H ==> Laplacian of Y
`
`
`Evaluate the model at the kth node
`
` dY_k = dx_k.g + dx_k dx_k:H/2
`
`Multiply by a_k and sum
`
` M M M
` sum a_k dY_k = sum a_k dx_k.g + sum a_k dx_k dx_k:H/2
` k=1 k=1 k=1
`
` = 0.g + I:H/2
` = D2Y / 2
`
`Thus, we have a second order estimate of the Laplacian
`
` M
` Lap(Y_0) = sum 2 a_k dY_k
` k=1
`
`
`Now play the same game with a linear model
` dY_k = dx_k.g
`
`But this time multiply by (a_k dx_k) and sum
`
` M M
` sum a_k dx_k dY_k = sum a_k dx_k dx_k.g
` k=1 k=1
`
` = I.g
` = g
`
`
`In general, the derivatives at the central node can be estimated as
`
` M
` D#Y = sum a_k dx_k#dY_k
` k=1
`
` M
` D2Y = sum 2 a_k dY_k
` k=1
`
` where
` # stands for the {dot, cross, or tensor} product
` yielding the {div, curl, or grad} of Y
` and
` D2Y stands for the Laplacian of Y
` D2Y = D.DY = Lap(Y)