<?xml version="1.0" encoding="utf-8" standalone="yes"?><rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Lecture Notes | James R. Beattie</title><link>https://astro-beattie.com/lecture-notes/</link><atom:link href="https://astro-beattie.com/lecture-notes/index.xml" rel="self" type="application/rss+xml"/><description>Lecture Notes</description><generator>Hugo Blox Builder (https://hugoblox.com)</generator><language>en-us</language><lastBuildDate>Wed, 05 Aug 2026 00:00:00 +0000</lastBuildDate><image><url>https://astro-beattie.com/media/icon_hu58f049e2f3dec21651e29209817604b1_360074_512x512_fill_lanczos_center_3.png</url><title>Lecture Notes</title><link>https://astro-beattie.com/lecture-notes/</link></image><item><title>Fluid Theory, Turbulence, and Dynamos in Magnetized Plasmas</title><link>https://astro-beattie.com/lecture-notes/sceecs-summer-school/</link><pubDate>Wed, 05 Aug 2026 00:00:00 +0000</pubDate><guid>https://astro-beattie.com/lecture-notes/sceecs-summer-school/</guid><description>&lt;p>&lt;strong>Contents&lt;/strong>&lt;/p>
&lt;ul>
&lt;li>Fluid theory, waves, and instabilities.&lt;/li>
&lt;li>Conservation laws for magnetized fluids.&lt;/li>
&lt;li>Ideal-MHD waves and their restoring forces.&lt;/li>
&lt;li>Rayleigh-Taylor instability.&lt;/li>
&lt;li>Hydrodynamic turbulence.&lt;/li>
&lt;li>Kolmogorov phenomenology, exact energy budgets, and intermittency.&lt;/li>
&lt;li>Magnetohydrodynamic turbulence.&lt;/li>
&lt;li>Elsasser variables, weak turbulence, critical balance, and dynamic alignment.&lt;/li>
&lt;li>Fluid dynamos.&lt;/li>
&lt;li>Kinematic and nonlinear small-scale dynamos.&lt;/li>
&lt;li>Mean-field theory and large-scale dynamos.&lt;/li>
&lt;li>Derivations and mathematical details.&lt;/li>
&lt;/ul></description></item><item><title>Magnetic dynamos</title><link>https://astro-beattie.com/lecture-notes/dynamo/</link><pubDate>Mon, 30 Mar 2026 00:00:00 +0000</pubDate><guid>https://astro-beattie.com/lecture-notes/dynamo/</guid><description>&lt;p>&lt;strong>Contents&lt;/strong>&lt;br>
Magnetic dynamos.&lt;br>
Goals for this lecture.&lt;br>
The induction equation.&lt;br>
Small-scale dynamo (kinematic only).&lt;br>
Magnetic energy spectrum evolution.&lt;br>
The Kazantsev (1968) &lt;code>k^(3/2)&lt;/code> model.&lt;br>
Closure of the third-order correlators.&lt;br>
Diffusion-free regime.&lt;br>
Resistively truncated regime.&lt;br>
Comments.&lt;br>
Large-scale dynamo.&lt;br>
Mean-field induction equation and the EMF.&lt;br>
Exact fluctuation equation and the FOSA closure.&lt;br>
Scale expansion and isotropic reduction.&lt;br>
Derivation of &lt;code>alpha&lt;/code> and &lt;code>beta&lt;/code> under FOSA.&lt;br>
Why inhomogeneous mean flows are harder.&lt;br>
Inferring transport coefficients from data.&lt;br>
Some simple large-scale dynamos that may or may not exist.&lt;br>
The &lt;code>alpha^2&lt;/code> dynamo.&lt;br>
The &lt;code>alpha Omega&lt;/code> dynamo.&lt;/p></description></item><item><title>Kinetic to Viscous Fluid Model via First-Order Chapman-Enskog Expansion</title><link>https://astro-beattie.com/lecture-notes/kinetic-viscosity/</link><pubDate>Sun, 08 Feb 2026 00:00:00 +0000</pubDate><guid>https://astro-beattie.com/lecture-notes/kinetic-viscosity/</guid><description>&lt;p>&lt;strong>Contents&lt;/strong>&lt;br>
Boltzmann equation and the BGK collision operator.&lt;br>
Zeroth-moment (mass conservation).&lt;br>
First-moment (momentum conservation).&lt;br>
Second-moment (energy conservation).&lt;br>
Chapman-Enskog expansion.&lt;br>
Zeroth-order: local equilibrium and Euler equations.&lt;br>
Isotropic pressure.&lt;br>
Vanishing heat flux.&lt;br>
First-order expression for f(1).&lt;br>
The zeroth-order material derivatives.&lt;br>
Partial Derivatives of the Maxwellian.&lt;br>
Moments of f(1): heat flux and pressure corrections.&lt;br>
Relevant first-order fluxes.&lt;br>
Decomposition of f(1) by tensorial parity.&lt;br>
First-order heat flux from odd terms of f(1) and Fourier’s law of heat conduction.&lt;br>
Pressure corrections and bulk viscosity from the isotropic, even terms of f(1).&lt;br>
Shear viscosity from the traceless, even terms of f(1).&lt;/p></description></item><item><title>Fluid moments and linear waves in ideal magnetohydrodynamics</title><link>https://astro-beattie.com/lecture-notes/linear-mhd/</link><pubDate>Sat, 07 Feb 2026 00:00:00 +0000</pubDate><guid>https://astro-beattie.com/lecture-notes/linear-mhd/</guid><description>&lt;p>&lt;strong>Contents&lt;/strong>&lt;br>
Lecture goals.&lt;br>
Boltzmann equation for a monoatomic gas.&lt;br>
Zeroth-moment (mass conservation).&lt;br>
First-moment (momentum conservation).&lt;br>
Second-moment (energy conservation).&lt;br>
Isotropic pressure and moment closure.&lt;br>
Boltzmann equation for a non-relativistic, magnetized plasma.&lt;br>
From Boltzmann equation to an ideal MHD fluid.&lt;br>
Moments of the multi-species Boltzmann equation.&lt;br>
Ideal MHD equations.&lt;br>
The repercussions and assumptions of ideal MHD.&lt;br>
Linearization.&lt;br>
Small perturbations about a homogeneous equilibrium.&lt;br>
Linearization of the ideal MHD equations.&lt;br>
Linearized Continuity Equation.&lt;br>
Linearized Induction Equation.&lt;br>
Linearized Momentum Equation.&lt;br>
Plane-wave solutions.&lt;br>
Constructing the linear system.&lt;br>
Constructing the eigenvalue problem for u-hat.&lt;br>
Rearrange u-hat.&lt;br>
Rearrange rho-hat.&lt;br>
Rearrange B-hat.&lt;br>
Rebuilding u-hat in an appropriate form.&lt;br>
Ideal MHD Eigenmodes.&lt;br>
Alfven mode.&lt;br>
Fast and slow magnetosonic modes.&lt;br>
Limiting cases for propagation angle.&lt;br>
High- and low-beta limits.&lt;/p></description></item></channel></rss>