Book contents
- Frontmatter
- Contents
- Preface
- Acknowledgements
- Introduction
- 1
- Part I Neutral fluids
- Part 2 Plasmas
- Epilogue
- Appendix A Useful vector relations
- Appendix B Integrals in kinetic theory
- Appendix C Formulae and equations in cylindrical and spherical coordinates
- Appendix D Values of various quantities
- Appendix E Basic parameters pertaining to plasmas
- Suggestions for further reading
- References
- Index
1
from Introduction
Published online by Cambridge University Press: 05 June 2012
- Frontmatter
- Contents
- Preface
- Acknowledgements
- Introduction
- 1
- Part I Neutral fluids
- Part 2 Plasmas
- Epilogue
- Appendix A Useful vector relations
- Appendix B Integrals in kinetic theory
- Appendix C Formulae and equations in cylindrical and spherical coordinates
- Appendix D Values of various quantities
- Appendix E Basic parameters pertaining to plasmas
- Suggestions for further reading
- References
- Index
Summary
Fluids and plasmas in the astrophysical context
When a beginning student takes a brief look at an elementary textbook on fluid mechanics and at an elementary textbook on plasma physics, he or she probably forms the impression that these two subjects are very different from each other. Let us begin with some comments why we have decided to treat these two subjects together in this volume and why astrophysics students should learn about them.
We know that all substances are ultimately made up of atoms and molecules. Ordinary fluids like air or water are made up of molecules which are electrically neutral. By heating a gas to very high temperatures or by passing an electric discharge through it, we can break up a large number of molecules into positively charged ions and negatively charged electrons. Such a collection of ions and electrons is called a plasma, provided it satisfies certain conditions which we shall discuss later. Hence a plasma is nothing but a special kind of fluid in which the constituent particles are electrically charged.
When we watch a river flow, we normally do not think of interacting water molecules. Rather we perceive the river water as a continuous substance flowing smoothly as a result of the macroscopic forces acting on it. Engineers and meteorologists almost always deal with fluid flows which can be adequately studied by modelling the fluid as a continuum governed by a set of macroscopic equations.
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- Chapter
- Information
- The Physics of Fluids and PlasmasAn Introduction for Astrophysicists, pp. 3 - 16Publisher: Cambridge University PressPrint publication year: 1998