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Explore a function graphically. The wave speed \(c\) of water surface waves depends on the length \(\lambda\) of the waves. The following formula relates \(c\) to \(\lambda\) : $$ c(\lambda)=\sqrt{\frac{g \lambda}{2 \pi}\left(1+s \frac{4 \pi^{2}}{\rho g \lambda^{2}}\right) \tanh \left(\frac{2 \pi h}{\lambda}\right)} $$ where \(g\) is the acceleration of gravity, \(s\) is the air-water surface tension \(\left(7.9 \cdot 10^{-4} \mathrm{~N} / \mathrm{cm}\right), \rho\) is the density of water (can be taken as \(\left.1 \mathrm{~kg} / \mathrm{cm}^{3}\right)\), and \(h\) is the water depth. Let us fix \(h\) at \(50 \mathrm{~m}\). First make a plot of \(c(\lambda)\) for small \(\lambda(1 \mathrm{~mm}\) to \(10 \mathrm{~cm})\). Then make a plot \(c(\lambda)\) for larger \(\lambda\) ) (1 m to \(2 \mathrm{~km}\) ). Name of program file: water_wave_velocity.py.

Short Answer

Expert verified
Create a Python script to plot wave speed for small and large wave lengths, utilizing constants and provided formula. Use matplotlib for visualization.

Step by step solution

01

Set Up the Environment

Before solving the exercise, ensure you have a Python environment ready to run the specified code. You will need packages such as matplotlib for plotting, and possibly numpy for handling calculations, which can be installed via pip if not already available.
02

Understand the Function

The given formula is for calculating wave speed, \( c(\lambda) \), based on wave length, \( \lambda \). Each parameter has a defined constant value or relationship to the others, with notable parameters: gravitational acceleration \( g \), surface tension \( s \), water density \( \rho \), and water depth \( h \).
03

Define Constants and Variables

In the script water_wave_velocity.py, define the constants like \( g = 9.81 \text{ m/s}^2 \), \( s = 7.9 \times 10^{-4} \text{ N/cm} \), \( \rho = 1 \text{ kg/cm}^3 \) converted appropriately to be consistent with \( g \) in m/s, and \( h = 50 \text{ m} \). Set \( \lambda \) to range according to the two required plotting scales.
04

Create the Function

Define the function \( c(\lambda) \) as described, utilizing numpy operations for element-wise calculations over the range of \( \lambda \) values. Use \( \tanh \) from numpy for the hyperbolic tangent, ensuring all units are consistent throughout the calculations.
05

Plot for Small Lambda Values

Using matplotlib, plot \( c(\lambda) \) for \( \lambda \) ranging from 1 mm (0.001 m) to 10 cm (0.1 m). Label your axes, and include a title indicating this is the plot for small \( \lambda \). Use logarithmic scale if necessary for better visualization.
06

Plot for Large Lambda Values

Similarly, plot \( c(\lambda) \) for \( \lambda \) ranging from 1 m to 2 km (2000 m), again labeling axes and titling the plot for larger \( \lambda \). This ensures the examining of function behavior over large scales.
07

Save and Test the Script

Save the Python script as water_wave_velocity.py, then run it to check both plots. Verify the output is as expected and adjust scaling or calculations if discrepancies are found in comparison to expected wave velocities.

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Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Function Plotting
In scientific programming with Python, function plotting is a straightforward yet powerful way to visualize mathematical relationships. By plotting the wave speed function, \( c(\lambda) \), you gain insight into how wave speed changes with varying wave length, \( \lambda \).

Utilizing libraries like `matplotlib`, you can create visual representations of functions with ease.
  • Start by defining the wave speed function in Python using `numpy` for managing calculations, a key procedure when working with arrays of \( \lambda \) values.
  • You can choose to visualize different ranges of \( \lambda \) to see how the graph transitions from small to large wave lengths.
  • Functions in Python allow you to dynamically adjust parameters and see immediate visual feedback, helping to reinforce the underlying mathematical principles.
Doing so not only helps in understanding the functions better but also in communicating your findings effectively. Proper labels and titles make graphs more informative, catering to a wider audience.
Numerical Analysis
Numerical analysis is integral in scientific programming, especially when approximating solutions to complex problems. The given formula for wave speed, \( c(\lambda) \), involves variables that can be challenging to compute analytically.

When you utilize numerical methods:
  • Libraries like `numpy` enable efficient computation with arrays, allowing you to perform element-wise operations over a range of \( \lambda \) values.
  • It is crucial that all units are consistent, particularly when involving constants like gravity \( g \), surface tension \( s \), and density \( \rho \), which can be in differing units.
Numerical analysis helps us approximate the function \( c(\lambda) \) for various conditions, providing practical solutions where analytical methods may be cumbersome or infeasible. This approach is essential in a field where exact solutions are not always easily attainable.
Wave Speed Calculation
Wave speed calculation involves understanding and applying the specific formula provided: \[ c(\lambda)=\sqrt{\frac{g \lambda}{2 \pi}\left(1+s \frac{4 \pi^{2}}{\rho g \lambda^{2}}\right) \tanh \left(\frac{2 \pi h}{\lambda}\right)} \] This equation relates the wave speed \( c \) with the wavelength \( \lambda \), capturing the effects of surface tension and water depth.

Key components that affect wave speed include:
  • Gravitational acceleration \( g \) which drives the natural propagation of waves.
  • Surface tension \( s \), impacting stability and motion between air and water interfaces.
  • Water depth \( h \), influencing how deep-lying wave forces are transmitted.
  • Water density \( \rho \) contributes to mass distribution in the medium.
Proper understanding of these parameters helps in engineering applications such as harbor design, ship construction, and understanding wave patterns for environmental assessments.
Python Environment Setup
Setting up your Python environment effectively is a crucial first step in running any scientific programming task. For plotting the wave speed function, make sure your environment is equipped with the necessary packages:

  • `matplotlib` is a must for plotting, offering capabilities to create detailed figures and graphs.
  • `numpy` will be essential for managing numerical computations, especially when dealing with arrays and trigonometric or hyperbolic operations like `tanh`.
  • Ensure your Python environment is consistent in terms of unit measurement since conversions are frequently necessary in scientific contexts.
Use the package manager `pip` to install any missing libraries. By setting up your environment correctly, you pave the way for efficient coding practices and focus more on analyzing results rather than managing technical setbacks.

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Most popular questions from this chapter

Implement Lagrange's interpolation formula. Imagine we have \(n+1\) measurements of some quantity \(y\) that depends on \(x\) : \(\left(x_{0}, y_{0}\right),\left(x_{1}, y_{1}\right), \ldots,\left(x_{n}, y_{n}\right)\). We may think of \(y\) as a function of \(x\) and ask what \(y\) is at some arbitrary point \(x\) not coinciding with any of the \(x_{0}, \ldots, x_{n}\). This problem is known as interpolation. One way to solve this problem is to fit a continuous function that goes through all the \(n+1\) points and then evaluate this function for any desired \(x\). A candidate for such a function is the polynomial of degree \(n\) that goes through all the points. This polynomial can be written $$ p_{L}(x)=\sum_{k=0}^{n} y_{k} L_{k}(x) $$ where $$ L_{k}(x)=\prod_{i=0, i \neq k}^{n} \frac{x-x_{i}}{x_{k}-x_{j}} $$ The \(\Pi\) notation corresponds to \(\sum\), but the terms are multiplied, e.g., $$ \prod_{i=0, i \neq k}^{n} x_{i}=x_{0} x_{1} \cdots x_{k-1} x_{k+1} \cdots x_{n} $$ The polynomial \(p_{L}(x)\) is known as Lagrange's interpolation formula, and the points \(\left(x_{0}, y_{0}\right), \ldots,\left(x_{n}, y_{n}\right)\) are called interpolation points. Make a function Lagrange \(\left(x\right.\), points) that evaluates \(p_{L}\) at the point x, given \(n+1\) interpolation points as a two-dimensional array points, such that points \([i, 0]\) is the \(x\) coordinate of point number \(i\) and points \([i, 1]\) is the corresponding \(y\) coordinate. To verify the program, we observe that \(L_{k}\left(x_{k}\right)=1\) and that \(L_{k}\left(x_{i}\right)=0\) for \(i \neq k\), implying that \(p_{L}\left(x_{k}\right)=y_{k}\). Write a function verify (points) that computes \(\left|p_{L}\left(x_{k}\right)-y_{k}\right|\) at all the interpolation points and checks that the value is approximately zero. Call verify with 5 equally spaced points along the curve \(y=\sin (x)\) for \(x \in[0, \pi]\). Then evaluate \(p_{L}(x)\) for an \(x\) in the middle of two interpolation points and compare the value of \(p_{L}(x)\) with the exact one: \(\sin (x)\). Name of program file: Lagrange_polynomial1.py.

Plot the viscosity of water. The viscosity of water, \(\mu\), varies with the temperature \(T\) (in Kelvin) according to $$ \mu(T)=A \cdot 10^{B /(T-C)} $$ where \(A=2.414 \cdot 10^{-5} \mathrm{~Pa} \mathrm{~s}, B=247.8 \mathrm{~K}\), and \(C=140 \mathrm{~K}\). Plot \(\mu(T)\) for \(T\) between 0 and 100 degrees Celsius. Label the \(x\) axis with 'temperature (C)' and the \(y\) axis with 'viscosity (Pa s)'. Note that \(T\) in the formula for \(\mu\) must be in Kelvin. Name of program file: water_viscosity.py.

Apply a function to a vector. Given a vector \(v=(2,3,-1)\) and a function \(f(x)=x^{3}+x e^{x}+1\), apply \(f\) to each element in \(v .\) Then calculate \(f(v)\) as \(v^{3}+v * e^{v}+1\) using vector computing rules. Show that the two results are equal.

Plot Taylor polynomial approximations to \(\sin x\). The sine function can be approximated by a polynomial according to the following formula: $$ \sin x \approx S(x ; n)=\sum_{j=0}^{n}(-1)^{j} \frac{x^{2 j+1}}{(2 j+1) !} $$ The expression \((2 j+1) !\) is the factorial (see Exercise 3.14). The error in the approximation \(S(x ; n)\) decreases as \(n\) increases and in the limit we have that \(\lim _{n \rightarrow \infty} S(x ; n)=\sin x\). The purpose of this exercise is to visualize the quality of various approximations \(S(x ; n)\) as \(n\) increases. The first part of the exercise is to write a Python function \(\mathrm{S}(\mathrm{x}\), (n) that computes \(S(x ; n)\). Use a straightforward approach where you compute each term as it stands in the formula, i.e., \((-1)^{j} x^{2 j+1}\) divided by the factorial \((2 j+1) !\). (We remark that Exercise A.16 outlines a much more efficient computation of the terms in the series.) The next part of the exercise is to plot \(\sin x\) on \([0,4 \pi]\) together with the approximations \(S(x ; 1), S(x ; 2), S(x ; 3), S(x ; 6)\), and \(S(x ; 12)\) Name of program file: plot_Taylor_sin.py.

Animate a planet's orbit. A planet's orbit around a star has the shape of an ellipse. The purpose of this exercise is to make an animation of the movement along the orbit. One should see a small disk, representing the planet, moving along an elliptic curve. An evolving solid line shows the development of the planet's orbit as the planet moves. The points \((x, y)\) along the ellipse are given by the expressions $$ x=a \cos (\omega t), \quad y=b \sin (\omega t) $$ where \(a\) is the semimajor axis of the ellipse, \(b\) is the semiminor axis, \(\omega\) is an angular velocity of the planet around the star, and \(t\) denotes time. One complete orbit corresponds to \(t \in[0,2 \pi / \omega] .\) Let us discretize time into time points \(t_{k}=k \Delta t\), where \(\Delta t=2 \pi /(\omega n) .\) Each frame in the movie corresponds to \((x, y)\) points along the curve with \(t\) values \(t_{0}, t_{1}, \ldots, t_{i}, i\) representing the frame number \((i=1, \ldots, n)\). Let the plot title of each frame display the planet's instantaneous velocity magnitude. This magnitude is the length of the velocity vector $$ \left(\frac{d x}{d t}, \frac{d y}{d t}\right)=(-\omega a \sin (\omega t), \omega b \cos (\omega t)) $$ which becomes \(\omega \sqrt{a^{2} \sin ^{2}(\omega t)+b^{2} \cos ^{2}(\omega t)}\) Implement the visualization of the planet's orbit using the method above. Run the special case of a circle and verify that the magnitude of the velocity remains constant as the planet moves. Name of program file: planet_orbit.py.

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