I have attched some links, which you can use them for your IELTS preparation.
These are some paid courses.
Often you will having a need to connect to your remote servers from home, so I have listed down some of the resources through which you can connect to remote accounts.
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#!/usr/bin/python3.6 | |
# A finite-difference method for the solution of the Cauchy problem for systems of first-order ordinary differential equations: | |
# | |
# dy/dx = f(x, y) | |
# | |
# The method uses the finite-difference formula: | |
# yi - yi-1 = 2hf(xi-1, yi-1). | |
# xi = x0+ih, i = 0,1,2,3,..... | |
# |
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/* | |
A finite-difference method for the solution of the Cauchy problem for systems of first-order ordinary differential equations: | |
dy/dx = f(x, y) | |
The method uses the finite-difference formula: | |
yi - yi-1 = 2hf(xi-1, yi-1). | |
xi = x0+ih, i = 0,1,2,3,..... | |
The predictor-corrector Milne method uses a pair of finite-difference formulas: |
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#!/usr/bin/python3.6 | |
# In numerical analysis, the Runge–Kutta methods are a family of implicit and explicit iterative methods, which include the well-known routine called the Euler Method, used in temporal discretization for the approximate solutions of ordinary differential equations. These methods were developed around 1900 by the German mathematicians Carl Runge and Martin Kutta. | |
# | |
# The most widely known member of the Runge–Kutta family is generally referred to as "RK4", "classical Runge–Kutta method" or simply as "the Runge–Kutta method". | |
# | |
# Let an initial value problem be specified as follows: | |
# y˙ = f(t, y), y(t0) = y0. | |
# | |
# Here y is an unknown function (scalar or vector) of time t, which we would like to approximate; we are told that y˙, the rate at which y changes, is a function of t and of y itself. At the initial time t0 the corresponding y value is y0. The function f and the data t0, y0 are given. |
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/* | |
In numerical analysis, the Runge–Kutta methods are a family of implicit and explicit iterative methods, which include the well-known routine called the Euler Method, used in temporal discretization for the approximate solutions of ordinary differential equations. These methods were developed around 1900 by the German mathematicians Carl Runge and Martin Kutta. | |
The most widely known member of the Runge–Kutta family is generally referred to as "RK4", "classical Runge–Kutta method" or simply as "the Runge–Kutta method". | |
Let an initial value problem be specified as follows: | |
y˙ = f(t, y), y(t0) = y0. | |
Here y is an unknown function (scalar or vector) of time t, which we would like to approximate; we are told that y˙, the rate at which y changes, is a function of t and of y itself. At the initial time t0 the corresponding y value is y0. The function f and the data t0, y0 are given. |
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#!/usr/bin/python3.6 | |
# This method is quite similar to that of the Regula-Falsi method except for the | |
# condition f(x1).f(x2) < 0. Here the graph of the function y = f(x) in the | |
# neighborhood of the root is approximated by a secant line or chords. Further, | |
# the interval at each iteration may not contain the root. | |
# Let the limits of interval initially be x0 and x1. | |
# Then the first approximation is given by: | |
# x2 = x1 – [(x1-x0)/f(x1)-f(x0)]f(x1) |
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/* This method is quite similar to that of the Regula-Falsi method except for the | |
condition f(x1).f(x2) < 0. Here the graph of the function y = f(x) in the | |
neighborhood of the root is approximated by a secant line or chords. Further, | |
the interval at each iteration may not contain the root. | |
Let the limits of interval initially be x0 and x1. | |
Then the first approximation is given by: | |
x2 = x1 – [(x1-x0)/f(x1)-f(x0)]f(x1) | |
Again, the formula for successive approximation in general form is | |
x(n+1) = xn - [xn - x(n-1)/f(xn)-f(x(n-1))]f(xn) */ |
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#!/usr/bin/python3.6 | |
# This method is generally used to improve the result obtained by one of the | |
# previous methods. Let x0 be an approximate root of f(x) = 0 and let x1 = x0 + h be | |
# the correct root so that f(x1) = 0. | |
# Expanding f(x0 + h) by Taylor’s series, we get | |
# f(x0) + hf′(x0) + h2/2! f′′(x0) + ...... = 0 | |
# Since h is small, neglecting h2 and higher powers of h, we get | |
# f(x0) + hf′(x0) = 0 or h = – f(x0)/f'(x0) | |
# A better approximation than x0 is therefore given by x1, where |
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