比起numpy或scipy，我建议熊猫们更快地做到这一点:

df['data'].rolling(3).mean()

这取列“数据”的3个周期的移动平均值(MA)。你也可以计算移位的版本，例如排除当前单元格的版本(向后移位一个)可以很容易地计算为:

df['data'].shift(periods=1).rolling(3).mean()

虽然这里有这个问题的解决方案，但请看看我的解决方案。这是非常简单和工作良好。

import numpy as np
dataset = np.asarray([1, 2, 3, 4, 5, 6, 7])
ma = list()
window = 3
for t in range(0, len(dataset)):
    if t+window <= len(dataset):
        indices = range(t, t+window)
        ma.append(np.average(np.take(dataset, indices)))
else:
    ma = np.asarray(ma)

上面的一个答案中有一个mab的注释，它有这个方法。瓶颈有move_mean，这是一个简单的移动平均:

import numpy as np
import bottleneck as bn

a = np.arange(10) + np.random.random(10)

mva = bn.move_mean(a, window=2, min_count=1)

Min_count是一个很方便的参数，它可以取数组中该点的移动平均值。如果你不设置min_count，它将等于window，并且直到window points的所有内容都将是nan。

我的解决方案是基于维基百科上的“简单移动平均”。

from numba import jit
@jit
def sma(x, N):
    s = np.zeros_like(x)
    k = 1 / N
    s[0] = x[0] * k
    for i in range(1, N + 1):
        s[i] = s[i - 1] + x[i] * k
    for i in range(N, x.shape[0]):
        s[i] = s[i - 1] + (x[i] - x[i - N]) * k
    s = s[N - 1:]
    return s

与之前建议的解决方案相比，它比scipy最快的解决方案“uniform_filter1d”快两倍，并且具有相同的错误顺序。 速度测试:

import numpy as np    
x = np.random.random(10000000)
N = 1000

from scipy.ndimage.filters import uniform_filter1d
%timeit uniform_filter1d(x, size=N)
95.7 ms ± 9.34 ms per loop (mean ± std. dev. of 7 runs, 10 loops each)
%timeit sma(x, N)
47.3 ms ± 3.42 ms per loop (mean ± std. dev. of 7 runs, 1 loop each)

错误的比较:

np.max(np.abs(np.convolve(x, np.ones((N,))/N, mode='valid') - uniform_filter1d(x, size=N, mode='constant', origin=-(N//2))[:-(N-1)]))
8.604228440844963e-14
np.max(np.abs(np.convolve(x, np.ones((N,))/N, mode='valid') - sma(x, N)))
1.41886502547095e-13

更新:已经提出了更有效的解决方案，scipy的uniform_filter1d可能是“标准”第三方库中最好的，还有一些更新的或专门的库可用。

你可以用np。卷积得到:

np.convolve(x, np.ones(N)/N, mode='valid')

解释

The running mean is a case of the mathematical operation of convolution. For the running mean, you slide a window along the input and compute the mean of the window's contents. For discrete 1D signals, convolution is the same thing, except instead of the mean you compute an arbitrary linear combination, i.e., multiply each element by a corresponding coefficient and add up the results. Those coefficients, one for each position in the window, are sometimes called the convolution kernel. The arithmetic mean of N values is (x_1 + x_2 + ... + x_N) / N, so the corresponding kernel is (1/N, 1/N, ..., 1/N), and that's exactly what we get by using np.ones(N)/N.

边缘

np的模态参数。Convolve指定如何处理边缘。我在这里选择有效模式，因为我认为这是大多数人期望的运行方式，但您可能有其他优先级。下面是一个图表，说明了模式之间的差异:

import numpy as np
import matplotlib.pyplot as plt
modes = ['full', 'same', 'valid']
for m in modes:
    plt.plot(np.convolve(np.ones(200), np.ones(50)/50, mode=m));
plt.axis([-10, 251, -.1, 1.1]);
plt.legend(modes, loc='lower center');
plt.show()

有点晚了，但我已经做了我自己的小函数，它不环绕端点或垫与零，然后用于查找平均值。进一步的处理是，它还在线性间隔点上对信号进行重新采样。随意定制代码以获得其他特性。

该方法是一个简单的矩阵乘法与规范化高斯核。

def running_mean(y_in, x_in, N_out=101, sigma=1):
    '''
    Returns running mean as a Bell-curve weighted average at evenly spaced
    points. Does NOT wrap signal around, or pad with zeros.
    
    Arguments:
    y_in -- y values, the values to be smoothed and re-sampled
    x_in -- x values for array
    
    Keyword arguments:
    N_out -- NoOf elements in resampled array.
    sigma -- 'Width' of Bell-curve in units of param x .
    '''
    import numpy as np
    N_in = len(y_in)

    # Gaussian kernel
    x_out = np.linspace(np.min(x_in), np.max(x_in), N_out)
    x_in_mesh, x_out_mesh = np.meshgrid(x_in, x_out)
    gauss_kernel = np.exp(-np.square(x_in_mesh - x_out_mesh) / (2 * sigma**2))
    # Normalize kernel, such that the sum is one along axis 1
    normalization = np.tile(np.reshape(np.sum(gauss_kernel, axis=1), (N_out, 1)), (1, N_in))
    gauss_kernel_normalized = gauss_kernel / normalization
    # Perform running average as a linear operation
    y_out = gauss_kernel_normalized @ y_in

    return y_out, x_out

正弦信号加正态分布噪声的一个简单用法: