PREPRINT authorea.com/5263
Main Data History
Export
Show Index Toggle 2 comments
  •  Quick Edit
  • Measurements of Index of Refraction of the Whistler Wave Using Appleton’s Equation

    UCLA Physics 180E

    Introduction

    Radio emission from the ionosphere can produce a whistling sound in the audio frequency that can be heard[1]. The whistling sounds are described as groups of descending tones which are called the whistler mode. When lightning hits the southern hemisphere it produces a range of radio waves, some of which can travel along the earths magnetic field lines from the southern hemisphere to the northern hemisphere[1].These waves are called extraordinary waves .The extraordinary waves emit two solutions to the wave equation named L and R waves.The L and R refer to left and right hand circularly polarized. The waves that describe the whistling sound are R waves and they will be detected in the north and the different frequencies of these waves will travel at different speeds. For \(\omega<\frac{\omega_{ce}}{2}\) the phase and group velocities increase with frequency, where \(\omega_{ce}=\frac{eB}{m}\) is the electron cyclotron frequency[1]. Due to this, the lower frequencies will arrive at the northern hemisphere later than the higher frequencies will, causing the descending tone in the whistler mode. These R waves waves that travel along the magnetic field lines are called whistler waves and these waves can only propagate for \(\omega<\frac{\omega_ce}{2}\). This lab seeks out to measure the dispersion relation of the whistler waves and to find the wave patterns theoretically and experimentally in the inductively coupled plasma device using Appletons equation.

    Theory

    Appleton’s equation is given by

    \[\eta^2=1-\frac{\omega_{pe}^2}{\omega^2\left((1+\frac{i\nu}{\omega})-\frac{\omega_{ce}^2\sin^2\theta}{2\omega^2\left(1-\frac{\omega_{pe}^2}{\omega^2}\right)}\pm\sqrt{\frac{(\omega_{ce}^2\sin^2\theta)^2}{4(1-\frac{\omega_{pe}^2}{\omega^2})}+\frac{\omega_{ce}^2cos^2\theta}{\omega^2}}\right)}\]

    for an infinite plasma[2]. This describes the index of refraction for a whistler wave where \(\eta^2=\left(\frac{kc}{\omega}\right)^2\). \(\omega_{pe}\) is the plasma frequency, \(\omega_{ce}\) is the electron cyclotron frequency, and \(\nu\) is the rate of collisions in the plasma.The angle \(\theta\) refers to the angle the waves make with respect to the background magnetic field \(B_0\).The first assumption made is that the first experiment’s waves are made with \(\theta=0\) for waves parallel to \(B_0\) and that damping is slight so that \(\nu\approx0\) [2].Making these assumptions it is found that Appleton’s equation reduces to \[n^2=1-\frac{\omega_{pe}^2}{\omega(\omega-\omega_{ce})}\].Noting that \(\omega<\omega_{ce}\) then this results in an equation for index of refraction \[n^2\approx\frac{\omega_{pe}^2}{\omega\omega_{ce}}\]. Appleton’s equation can be derived from the plasma force equation,Maxwell’s equations, and using fourier analysis to show pertubations of the magnetic field are in the form \(\vec{B_1}(\vec{r},t)=Be^{i(\vec{k} \cdot \vec{r}-\omega t)}\).The plasma force equation is written assuming that the particles are cold so that there are no pressure gradients and that the quantity \(\vec{v}\cdot\nabla\approx0\) in the convective derivative, then the force equation is \(m\frac{\partial\vec v}{\partial t}=q(\vec{E}+\vec{v}\times\vec{B})-m\nu\vec{v}\) for electrons.The two Maxwell’s equations used are \(\nabla\times\vec{E}=-\frac{\partial\vec{B}}{\partial{t}}\) and \(\nabla\times\vec{B}=\mu_0\vec{J}+\mu_0\epsilon_0\frac{\partial\vec{E}}{\partial t}\).Linearize equations involving \(\vec{B}\) and solve the force equations for \(\frac{kc}{\omega}\).

    Experimental Setup

    The plasma was created by an inductively coupled RF source operating at a power of 120 W with \(4\times 10^{-4}\) Torr Argon as the working gas. A voltage sweep was put across a Langmuir probe 70 cm from the RF source 1.3 ms into the afterglow and over a 101 \(\mu s\) range. A magnetic field was applied to the device through the use of two sets of four coaxial magnets created through the use of 25.4A and 63.0A currents laid out around the device and resulting in a radially symmetric magnetic field through the device, averaging to 60 Gauss along the length. Whistler waves were generated in the plasma using a wave form generating antenna, set to 40 MHz for the experiment with data taken in a plane and set to 9 separate varying frequencies from 40 MHz to 120 MHz, each 10 MHz apart. A B-dot probe was used to measure the oscillations in the magnetic field due to the wave over a range of 70-90cm from the RF source axially and -15 degrees to 15 degrees radially for the set taken in a plane and varying axial lengths for the linear data set such that 10 data points were taken per wavelength of the measured wave. The B-dot probe used in this experiment consists of 3 sets of loops, each with a single wire sheathed by an insulating ceramic exterior. The loops are positioned orthonormal to one another with \(\hat{z}\) along the central axis, and \(\hat{x}\), \(\hat{y}\), representing horizontal and vertical axes respectivily.When the loops detect a change in magnetic flux, will induce a current by Faraday’s law in these conducting loops.The output voltage is recorded electronically and from this a measurement for \(B(t)\) is obtained [3].