Skip to main content Accessibility help
×
Hostname: page-component-5c6d5d7d68-wpx84 Total loading time: 0 Render date: 2024-08-07T04:19:19.825Z Has data issue: false hasContentIssue false

3 - ‘Derivation’ of the macroscopic equations

Published online by Cambridge University Press:  22 February 2010

J. P. Hans Goedbloed
Affiliation:
FOM-Instituut voor Plasmyafysica, Nieuwegein
Stefaan Poedts
Affiliation:
Centre for Plasma Astrophysics, KU Leuven
Get access

Summary

Two approaches

There are basically two ways of introducing the equations of magnetohydrodynamics:

  1. (a) pose them as reasonable postulates for a hypothetical medium called ‘plasma’;

  2. (b) derive them by appropriate averaging of kinetic equations.

Our approach, starting with Chapter 4, is mainly along the lines of the first method, pioneered by Grad [98, 32] in a series of lecture notes, using physical arguments and mathematical criteria to justify the results. In this chapter, the main steps of the second method will be discussed and shown to be somewhat unsatisfactory since they involve a number of approximations that are often difficult to justify. The reason for going through this analysis anyway is that it provides understanding of the domain of validity of the MHD description and that it indicates what kind of modifications are in order when this description fails.

Mathematically inclined readers may skip this digression, where most results from kinetic theory are not derived but simply stated, and continue reading with Chapter 4. Also, the serious student of magnetohydrodynamics is advised to turn to a detailed study of the present chapter only after a first reading of Chapters 4–11 on basic MHD since the level of this chapter is essentially that of the advanced theory, but it has been placed here because this is where it logically belongs.

We give a ‘derivation’ of the MHD equations by averaging the kinetic equations for plasmas.

Type
Chapter
Information
Principles of Magnetohydrodynamics
With Applications to Laboratory and Astrophysical Plasmas
, pp. 83 - 128
Publisher: Cambridge University Press
Print publication year: 2004

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

Save book to Kindle

To save this book to your Kindle, first ensure coreplatform@cambridge.org is added to your Approved Personal Document E-mail List under your Personal Document Settings on the Manage Your Content and Devices page of your Amazon account. Then enter the ‘name’ part of your Kindle email address below. Find out more about saving to your Kindle.

Note you can select to save to either the @free.kindle.com or @kindle.com variations. ‘@free.kindle.com’ emails are free but can only be saved to your device when it is connected to wi-fi. ‘@kindle.com’ emails can be delivered even when you are not connected to wi-fi, but note that service fees apply.

Find out more about the Kindle Personal Document Service.

Available formats
×

Save book to Dropbox

To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Dropbox.

Available formats
×

Save book to Google Drive

To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Google Drive.

Available formats
×