Stellar Plasmas

Plasma Physics · Part 7

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Table of Contents

  1. 1.4.1 The Solar Corona
  2. 2.4.2 The Coronal Heating Problem
  3. 3.4.3 Stellar Structure Equations
  4. 4.4.4 Stellar Winds & Mass Loss
  5. 5.4.5 Magnetohydrostatic Equilibria

Key Equations

$$\frac{dp}{dr} = -\rho g = -\frac{n m_p g}{1}$$
$$F_{wave} = \rho \langle \delta v^2 \rangle v_A = \frac{\rho \langle \delta v^2 \rangle B}{\sqrt{\mu_0 \rho}} = \frac{B\langle\delta v^2\rangle\sqrt{\rho}}{\sqrt{\mu_0}}$$
$$F = -\frac{c}{3\kappa\rho}\cdot 4aT^3\frac{dT}{dr} = -\frac{16\sigma_{SB} T^3}{3\kappa\rho}\frac{dT}{dr}$$
$$\boxed{\dot{M}_{CAK} = \frac{\alpha}{1-\alpha}\frac{L}{c^2}\left(\frac{k\Gamma_e}{1-\Gamma_e}\right)^{(1-\alpha)/\alpha}}$$

Equations are rendered with MathJax in the PDF with professional LaTeX typesetting.

Course Context

This PDF is part of the Plasma Physics course on CoursesHub.World. Comprehensive study of the fourth state of matter. Covers single-particle motion, kinetic theory, MHD, waves and instabilities, collisional processes, magnetic and inertial confinement fusion, space a...

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