**What is SciPy in Python: Learn with an Example**

Letâ€™s start off with this SciPy Tutorial with an example. Scientists and researchers are likely to gather enormous amount of information and data, which are scientific and technical, from their exploration, experimentation, and analysis. Dealing with such huge amount of data becomes a hindrance to them. That is, calculating and computing with large data manually is not an easy task. Hence, they make use of super computers and Data Science for the purpose of faster computing and accurate outcomes.

Another simpler way to deal with scientific and technical computing of data is by making use of one of the Python libraries which is solely built for this purpose. It is referred to as Python SciPy (pronounced as â€˜sigh piâ€™).

Python SciPy is an open-source software; therefore, it can be used free of cost and many new Data Science features are incorporated in it.

Following is the list of all topics covered in this SciPy Tutorial:

- Python Scipy Installation and Setup
- Python Scipy Modules
- Integration
- Python Scipy imread
- Optimize and Minimize Functions in Python SciPy
- Curve fit
- Interpolate function in SciPy in Python
- Statistics
- Sparse matrix
- Fourier Front Transforms

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**Python SciPy Installation and Setup**

The next section of our SciPy Tutorial will deal with SciPy installation. SciPy installation varies with respect to different operating systems. The following content will be useful for us to easily figure out how to install SciPy in Python

in our respective operating systems.

**Installing SciPy with PIP**

Pip is basically a recursive acronym which stands for â€˜Pip Installs Packagesâ€™. It is a standard package manager which can be installed in most of the operating systems.

**Note**: In order to install other packages by using the pip command, we need to make sure that we have installed Python and pip in our system.

Python3 -m pip install â€“user numpy scipy

sudo port install py35-scipy py35-numpy

sudo apt-get installÂ python-scipy python-numpy

**Python SciPy Modules**

Many dedicated software tools are necessary for Python scientific computing, and SciPy is one such tool or library offering many Python modules that we can work with in order to perform complex operations.

The following table shows some of the modules or sub-packages that can be used for computing:

SL No. |
Sub-Package |
Function |

1. | Interpolation |
scipy.interpolate |

2. | Integration |
scipy.integrate |

3. | Optimization |
scipy.optimize |

4. | Signal processing |
scipy.signal |

5. | Statistics |
scipy.stats |

6. | Fast Fourier Transforms |
scipy.fftpack |

7. | Linear algebra |
scipy.linalg |

8. | sparse |
scipy.sparse |

9. | Input/output |
scipy.io |

10. | Special function |
scipy.special |

11. | Multidimensional image processing |
scipy.ndimage |

12. | Spatial data structures and algorithms |
scipy.spatial |

**Python scipy**

Import numpy as np From scipy import signal

This is a basic scipy code where the sub-package signal is being imported. We can import any sub-package in the similar manner. Python Numpy is required for most of the sub-packages. The sub-package signal can be replaced by other modules concerned with scipy.

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**Integration or scipy integrate**

Numerical integration is carried out in scipy by making use of scipy.integrate sub-package. This package provides several integration techniques. Some of the integration functions are listed below.

Sl. No. |
Sub-package |
Function |

1. | Interpolation |
scipy.interpolate |

2. | Integration |
scipy.integrate |

3. | Optimization |
scipy.optimize |

4. | Signal processing |
scipy.signal |

5. | Statistics |
scipy.stats |

6. | Fast Fourier Transforms |
scipy.fftpack |

7. | Linear algebra |
scipy.linalg |

8. | Sparse |
scipy.sparse |

9. | Input/output |
scipy.io |

10. | Special function |
scipy.special |

11. | Multidimensional image processing |
scipy.ndimage |

12. | Spatial data structures and algorithms |
scipy.spatial |

**Single Integrals**

It can also be called as general-purpose integration. When there is only one variable present between two points, then we make use of the function quad.

*a*and

*b*. Let us understand the function with an example.

A researcher is gathering data, and he wants to find out the integrals of the data.

In the above example, 12*x* is the function which lies between the intervals 0 and 1.

Example for single integration:

import scipy.integrate f= lambda x: 12*x i = scipy.integrate.quad(f, 0, 1) print (i) Output: (6.0, 6.661338147750939e-14)

Lambda function is deployed here so that any number of arguments can be used but it can have only one expression. Like here the expression is 12x, and the researcher makes use of the integrate function scipy.integrate.quad(f, 0, 1).

**Double Integral**

It is a type of integration where a function consists of at least two variables with *y* being the first argument and *x* being the second.

dblquad(func, a, b, gfun, hfun[, args, â€¦])

The function used above is dblquad, and here the *y* argument lies between the limits *a* and *b*, and the *x* argument lies between the limits *g* and *h*. Hence, two variables are defined.

The researcher now adds another variable to the previous data and makes it into a double integral.

In the above example, the first integral contains one variable denoting the *y* function and the second integral contains the second variable denoting the *x* function.

import scipy.integrate f = lambda x, y : 12*x g = lambda x : 0 h = lambda y : 1 i = scipy.integrate.dblquad(f, 0, 0.5, g, h) print(i) output: (3.0, 6.661338147750939e-14)

Hence, the above code contains the integration function used for double integrals scipy.integrate.dblquad(f, 0, 0.5, g, h), where *f* is the function; 12*x*, 0, and 0.5 are the integrals for the *y* function; and *g* and *h* are the integrals for the *x* function.

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**Triple Integrals**

It is a type of integration where a function consists of at least three variables.

There will be three functions for *x*, *y*, and *z*. Hence, the researcher computes with three integrals.

tplquad(func, a, b, gfun, hfun, qfun, rfun)

The researcher makes use of the tplquad function with three integrals, one with intervals *a* and *b*, the other with intervals *g* and *h*, and the third with intervals *q* and *r*.

The researcher further analyzes to involve with three integrals, so he thinks of combining the two integral values with the third one represented with the *z* function.

The above example denotes three integrals with a new function dz between the intervals 0 and 3.

Example for triple integration:

from scipy import integrate f = lambda z, y, x: 12*x integrate.tplquad(f, 0, 0.5, lambda x: 0, lambda x: 1, lambda x, y: 0, lambda x, y: 3) Output (9.0, 3.988124156968869e-13)

The above code represents the triple integral function integrate.tplquad(f, 0, 1, lambda x: 0, lambda x: 0.5, lambda x, y: 0, lambda x, y: 3), where the researcher has represented three integrals for: the *z* function between 0 and 3 intervals, the *y* function between 0 and 0.5 intervals, and the *x* function between 0 and 1 intervals.

**SciPy in Python imread**

Images can be read from a file as an array by making use of scipy.misc.imread. We will be able to use this Python Function only if we have installed Python imaging library (PIL).

scipy.ndimage.imread('mario.png')

Output

array([[[121, 112, 131], [138, 129, 148], [153, 144, 165], ..., [119, 126, 74], [131, 136, 82], [139, 144, 90]],[[ 89, 82, 100], [110, 103, 121], [130, 122, 143], ..., [118, 125, 71], [134, 141, 87], [146, 153, 99]],[[ 73, 66, 84], [ 94, 87, 105], [115, 108, 126], ..., [117, 126, 71], [133, 142, 87], [144, 153, 98]], ...,[[ 87, 106, 76], [ 94, 110, 81], [107, 124, 92], ..., [120, 158, 97], [119, 157, 96], [119, 158, 95]],[[ 85, 101, 72], [ 95, 111, 82], [112, 127, 96], ..., [121, 157, 96], [120, 156, 94], [120, 156, 94]],[[ 85, 101, 74], [ 97, 113, 84], [111, 126, 97], ..., [120, 156, 95], [119, 155, 93], [118, 154, 92]]], dtype=uint8)

In the above output, we have used an image called mario.png, and this image has been read from its saved file and later converted into an array so that it can be later used for image processing.

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## Optimize and Minimize Functions in Python SciPy

Optimization is the method of selecting the most effectual or best resource or situation for a given problem. The Python syntax of optimization can be given as:

import numpy as np from scipy.optimize import minimize

The minimize function can be used to provide a common interface to constrained and unconstrained algorithms for a multivariate scalar function in scipy.optimize sub-package.

The scipy.optimize package contains various modules:

- Constrained and unconstrained minimization of multivariate scalar functions (minimize ()) using few variety of algorithms (e.g., Nelderâ€“Mead simplex)
- Least-squares minimization (leastsq()) and curve fitting (curve_fit()) algorithms
- Multivariate equation system solvers (root()) using a variety of algorithms (e.g., hybrid Powell)
- Scalar univariate functions minimizers (minimize_scalar()) and root finders (newton())

**Using Nelderâ€“Mead Simplex Algorithm**

It is applied for nonlinear optimization problems for which derivatives will be unknown, and it is a direct search method. We make use of the minimize() routine along with a Nelderâ€“Mead simplex example.

The method used in this algorithm is (method = â€˜Nelder-Meadâ€™)

import numpy as np from scipy.optimize import minimize def rosen(x): x0 = np.array([1.3, 0.7, 0.8, 1.9, 1.2]) res = minimize(rosen, x0, method='nelder-mead') print(res.x)

**Least Squares**

We use the optimize function at times to solve the least squares problem with bounds on the variables.

The following example illustrates the use of a rosenbrock function toÂ **implement the least square problem.**

def fun_rosenbrock(x): return np.array([10 * (x[1] - x[0]**2), (1 - x[0])]) from scipy.optimize import least_squares input = np.array([2, 2]) res = least_squares(fun_rosenbrock, input) print (res)

Output:

active_mask: array([0., 0.]) cost: 9.866924291084687e-30 fun: array([4.44089210e-15, 1.11022302e-16]) grad: array([-8.89288649e-14, 4.44089210e-14]) jac: array([[-20.00000015, 10. ], [ -1. , 0. ]]) message: '`gtol` termination condition is satisfied.' nfev: 3 njev: 3 optimality: 8.892886493421953e-14 status: 1 success: True x: array([1., 1.])

**Root Finding**

This is one of the minimization methods that comes under optimization.Â In the following example, we import a root function from the scipy.optimize sub-library in order to use it in further calculation within the cod**e.**

import numpy as np from scipy.optimize import root def func(x): return x*3 + 3 * np.cos(x) sol = root(func, 0.4) print (sol)

**Output**

fjac: array([[-1.]]) fun: array([0.]) message: 'The solution converged.' nfev: 10 qtf: array([-1.26965105e-10]) r: array([-5.02083661]) status: 1 success: True x: array([-0.73908513])

**Curve Fit**

This is part of optimization where we make use of non-linear least squares to fit a function.

The following code illustrates the curve fit:

import numpy as np np.random.seed(0) x_data = np.linspace(-7, 7, num=30) y_data = 2.9 * np.sin(1.5 * x_data) + np.random.normal(size=30) import matplotlib.pyplot as plt plt.figure(figsize=(6, 4)) plt.scatter(x_data, y_data)

from scipy import optimize def test_func(x, a, b): return a * np.sin(b * x) params, params_covariance = optimize.curve_fit(test_func, x_data, y_data, p0=[2, 2]) print(params) plt.figure(figsize=(6, 4)) plt.scatter(x_data, y_data, label='Data') plt.plot(x_data, test_func(x_data, params[0], params[1]), label='Fitted function') plt.legend(loc='best') plt.show()

**Interpolation**

Finding a value between two points in a curve or a line can be termed as interpolation.

import numpy as np from scipy import interpolate import matplotlib.pyplot as plt x = np.linspace(0, 5, 12) y = np.cos(x**2/3+4) print (x,y)

Output:

[0.Â 0.5 1.Â 1.5 2.Â 2.5 3.Â 3.5 4.Â 4.5 5.Â 5.5 6.Â 6.5 7. ] [Â 1.15782128Â Â 1.37425055Â Â 2.51055609 -26.57541423Â -1.39794519 -0.20255593Â Â 0.87144798Â -4.28339592Â -0.09170037Â Â 3.98989845 -0.23734945Â 18.55780867Â Â 0.30063224Â -0.96236589Â 11.46273345]plt.plot(x, y,'o')plt.show()

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## Scipy-stats

This sub-package contains a large number of probability distributions, as well as a growing library of statistical functions.

There are various sub-modules in statistics. They are listed below:

â€¢ rv_continuous

â€¢ rv_discrete

â€¢ rv_histogram

**Sub-module: rv_continuous**

This is a type of a generic continuous random variable class which is mainly meant for sub-classing.

rv_continuous([momtype, a, b, xtol, â€¦])

The continuous random variable is represented as rv_continuous with various parameters within the function.

A simple demonstration of rv_continuous sub-module:

import scipy.stats as st class my_pdf(st.rv_continuous): def _pdf(self,x): return 3*x**2

**rv_discrete**

This is a type of a generic random variable class which is mainly meant for sub-classing.

rv_discrete([a, b, name, badvalue, â€¦])

The discrete random variable is represented as rv_discrete with various parameters within the function.

The following example demonstrates rv_discrete sub-module from scipy import stats under scipy.stats:

import matplotlib.pyplot as plt x = np.arange(7) y = (0.2, 0.3, 0.1, 0.1, 0.1, 0.0, 0.2) custm = stats.rv_discrete(name='custm', values=(x, y)) fig, ax = plt.subplots(1, 1) ax.plot(x, custm.pmf(x), 'ro', ms=12, mec='y') ax.vlines(x, 0, custm.pmf(x), colors='b', lw=4)

In the above generated graph, seven values are plotted at various points specified along the y-axis.

**rv_histogram**

This is a type generates a distribution given by a histogram.

rv_histogram(histogram, *args, **kwargs)

The random variable histogram is represented as rv_histogram with various parameters within the function.

The following example demonstrates the representation of an rv_historgams:

import scipy.stats import numpy as np import matplotlib.pyplot as plt data = scipy.stats.norm.rvs(size=1000, loc=0, scale=1.0, random_state=123) hist = np.histogram(data, bins=100) hist_dist = scipy.stats.rv_histogram(hist) X = np.linspace(-5.0, 5.0, 100) plt.hist(data, density=True, bins=100) plt.plot(X, hist_dist.pdf(X), label='PDF') plt.plot(X, hist_dist.cdf(X), label='CDF')

A gradual increase in and then a stable flow of the wave is represented in the above graph which demonstrates the random variable histogram for the probability density function (PDF) and the cumulative distribution function (CDF).

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**Sparse Matrix**

Arithmetic operations such as addition, subtraction, division, matrix power, and multiplication can make use of sparse matrices. We can implement sparse matrix for following matrix formats:

- Compressed Sparse Row (CSR) format
- Compressed Sparse Column (CSC) format
- Coordinate (COO) Format
- Dictionary of Keys (DOK) format

**Scipy.sparse.csr_matrix**

This enables efficient row slicing.Â Let us see a simple program where we generate an empty 3Ã—3 CSR matrix using scipy.sparse.

import numpy as np from scipy.sparse import csr_matrix csr_matrix((3, 3), dtype=np.int8).toarray()

Output:

array([[0, 0, 0], [0, 0, 0], [0, 0, 0]], dtype=int8)

Representation of a 3Ã—3 CSR matrix upon specifying the rows and columns through inputs:

row = np.array([0, 1, 0, 2, 1, 1]) col = np.array([1, 0, 2, 0, 0, 2]) data = np.array([1, 2, 3, 4, 5, 6]) csr_matrix((data, (row, col)), shape=(3, 3)).toarray()

Output:

array([[0, 1, 3], [7, 0, 6], [4, 0, 0]], dtype=int32)

**Scipy.sparse.csc_matrix**

This enables efficient column slicing.Â Let us see a simple program where we generate an empty 3Ã—3 CSC matrix using scipy.sparse.

import numpy as np from scipy.sparse import csr_matrix csc_matrix((3, 3), dtype=np.int8).toarray()

Output:

array([[0, 0, 0], [0, 0, 0], [0, 0, 0]], dtype=int8)

Representation of a 3Ã—3 CSC matrix upon specifying the rows and columns through inputs:

row = np.array([0, 1, 1, 2, 1, 2]) col = np.array([1, 1, 1, 2, 0, 2]) data = np.array([1, 2, 3, 4, 5, 6]) csc_matrix((data, (row, col)), shape=(3, 3)).toarray()

Output:

array([[ 0, 1, 0], [ 5, 5, 0], [ 0, 0, 10]], dtype=int32)

The Compressed Sparse Column matrix is more efficient at accessing column operations or column vectors as it is stored as arrays of columns and their values are stored at each row.

The Compressed Sparse Row matrix is vice versa. It is stored as arrays of rows and their values are stored at each column and are more efficient at accessing row operations or row vectors.

CSR and CSC are difficult to construct from scratch, while COO and DOK are easier to construct.

**Scipy.sparse.coo_matrix**

This enables efficient row slicing.Â Let us see a simple program where we generate an empty 3Ã—3 COO matrix using scipy.sparse.

from scipy.sparse import coo_matrix coo_matrix((3, 3), dtype=np.int8).toarray()

Output:

array([[0, 0, 0], [0, 0, 0], [0, 0, 0]], dtype=int8)

Representation of a 3Ã—3 COO matrix upon specifying the rows and columns through inputs:

row = np.array([1, 1, 1, 2, 1, 2]) col = np.array([0, 1, 1, 2, 0, 2]) data = np.array([0, 2, 3, 4, 5, 6]) coo_matrix((data, (row, col)), shape=(3, 3)).toarray() array([[ 0,Â 0,Â 0], [ 5,Â 5,Â 0], [ 0,Â 0, 10]])

**Scipy.sparse.dok_matrix**

We can construct sparse matrix incrementally in an efficient manner using this module under the scipy.sparse sub-package.

import numpy as np from scipy.sparse import dok_matrix

The dictionary of keys format allows access for individual values within the matrix.

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**Fourier Front Transforms**

The method for expressing any function as a sum of periodic components and recovering the signal from those components can be termed as Fourier analysis. When both Fourier transforms and their respective functions are replaced with some discrete counterparts, then it is termed as discrete Fourier transform.

We make use of the Fourier transform sub-package scipy.fftpack:

from scipy.fftpack import fft, ifft x = np.array([1.0, 2.0, 1.0, -1.0, 1.5]) y = fft(x) print(y)

Output:

[ 4.5 Â Â +0.j Â Â Â Â 2.08155948-1.65109876j Â -1.83155948+1.60822041j Â Â Â Â Â Â Â Â Â Â Â Â Â Â Â Â -1.83155948-1.60822041j Â Â 2.08155948+1.65109876j]

Fourier front transform is performed on a given array of values, and the above output is generated.

**One-dimensional Discrete Fourier Transform**

We can compute 1-dimensional Fourier transforms by making use of the following standard syntax:

fft(a[, n, axis, norm]) ifft(a[, n, axis, norm])

We make use of â€˜fftâ€™ for 1-dimensional discrete Fourier transforms and â€˜ifftâ€™ for 1-dimensional inverse discrete Fourier transforms.

Let us discuss on this sub-package with a simple example of the sum of two cosines for a 1-dimensional discrete Fourier transform.

from scipy.fftpack import fft N = 600 T = 1.0 / 800.0 x = np.linspace(0.0, N*T, N) y = np.cos(70.0 * 2.0*np.pi*x) + 0.5*np.cos(90.0 * 2.0*np.pi*x) yf = fft(y) xf = np.linspace(0.0, 1.0/(2.0*T), N//2) import matplotlib.pyplot as plt plt.plot(xf, 2.0/N * np.abs(yf[0:N//2]))

By making use of two cosine functions, the sum is calculated and plotted in the graph. The waves are plotted at 70 and 90 degrees along the x axis.

**Two-dimensional Discrete Fourier Transform and ***N*-dimensional Discrete Fourier Transform

*N*-dimensional Discrete Fourier Transform

We can compute 2-dimensional Fourier transforms by making use of the following syntax:

fft2(a[, s, axes, norm]) ifft2(a[, s, axes, norm])

We make use of â€˜fftâ€™ for 2-dimensional discrete Fourier transforms and â€˜ifftâ€™ for 2-dimensional inverse discrete Fourier transforms.

fftn(a[, s, axes, norm]) ifftn(a[, s, axes, norm])

We make use of â€˜fftâ€™ for *N*-dimensional discrete Fourier transforms and â€˜ifftâ€™ for *N*-dimensional inverse discrete Fourier transforms.

Let us consider a simple example of time domain signals by making use of 2-dimensional inverse fft:

from scipy.fftpack import ifftn import matplotlib.pyplot as plt import matplotlib.cm as cm N = 30 f, ((ax1, ax2, ax3), (ax4, ax5, ax6)) = plt.subplots(2, 3, sharex='col', sharey='row') xf = np.zeros((N,N)) xf[0, 5] = 10 xf[0, N-5] =10 Z = ifftn(xf) ax1.imshow(xf, cmap=cm.Reds) ax4.imshow(np.real(Z), cmap=cm.gray) xf = np.zeros((N, N)) xf[5, 0] = 10 xf[N-5, N-10] = 10 Z = ifftn(xf) ax2.imshow(xf, cmap=cm.Reds) ax5.imshow(np.real(Z), cmap=cm.gray) xf = np.zeros((N, N)) xf[5, 10] = 10 xf[N-5, N-10] = 10 Z = ifftn(xf) ax3.imshow(xf, cmap=cm.Reds) ax6.imshow(np.real(Z), cmap=cm.gray)

Below graphs are obtained from the time domain signal code generated by illustrating the inverse Fourier front transform.

**Conclusion**

Here, we come to the end of this module in Python Tutorial. I hope that this Tutorial has provided sufficient information about the scientific and technical library of Python, that is, SciPy. There are various computing calculations that are time-consuming and stressful for the human brain. Hence, by making use of such a scientific calculation library in Python programming language to carry out this purpose with ease and incredible speed has proved that this library function plays a vital role in Data Science. Now, if you want to know why Python is the most preferred language for data science, you can go through this blog on Python for Data Science.

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