Astrophysical plasmas
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Astrophysical plasmas codes, models, and observations : Ciudad de México, México, octubre 25-29, 1999 by

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Published by Instituto de Astronomía, Universidad Nacional Autónoma de México in México, D.F .
Written in English

Subjects:

  • Plasma astrophysics -- Congresses.,
  • Space plasmas -- Congresses.

Book details:

Edition Notes

Statementeditores de las memorias, Jane Arthur, Nancy Brickhouse y José Franco.
GenreCongresses.
SeriesRevista mexicana de astronomía y astrofísica., v. 9
ContributionsArthur, Jane, Brickhouse, Nancy., Franco, José.
Classifications
LC ClassificationsQB462.7 .A795 2000
The Physical Object
Paginationxiv, 355 p. :
Number of Pages355
ID Numbers
Open LibraryOL3372971M
LC Control Number2004459149
OCLC/WorldCa44688993

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A plasma is a quasi-neutral gas consisting of positively and negatively charged particles (usually ions and electrons) which are subject to electric, magnetic and other forces, and which exhibit collective. Reset your password. If you have a user account, you will need to reset your password the next time you login. You will only need to do this once. This book is a comprehensive description of hybrid plasma simulation models and will provide a very useful summary and guide to the vast literature on this topic. It addresses researchers and graduate students knowledgeable about computational science and numerical analysis, and can be used in courses on astrophysical and space plasmas. The final part of the book deals with applications in space plasmas, focusing on applications of theoretical and analytical developments in space plasmas from the heliosphere and beyond, in other astrophysical plasmas. Kappa Distributions is ideal for space, plasma, and statistical physicists; geophysicists, especially of the upper atmosphere.

An astrophysical plasma is a plasma (an ionised gas) found in astronomy whose physical properties are studied in the science of astrophysics. The vast majority of the volume of the universe is thought to consist of plasma, a state of matter in which atoms and molecules are so hot, that they have ionized by breaking up into their constituent parts, negatively charged electrons and positively charged ions.   This rigorous explanation of plasmas is relevant to diverse plasma applications such as controlled fusion, astrophysical plasmas, solar physics, magnetospheric plasmas, and plasma thrusters. More thorough than previous texts, it exploits new powerful mathematical techniques to develop deeper insights into plasma behavior. Astrophysical Plasmas. Dr Neil F. Cramer. E-mail address: [email protected] Book Author(s): Dr Neil F. Cramer. E-mail address: [email protected] School of Physics, University of Sydney, Australia. Search for more papers by this author. Cold Pair Plasmas. Relativistic Plasmas. Instabilities. Concluding Remarks. The Physics of. Abstract. Plasmas are generally associated with a hot gas of charged particles which behave classically. However, when the temperature is lowered and/or the density is increased sufficiently, the plasma particles (most importantly, electrons) become quantum degenerate, that is, the extension of their wave functions becomes comparable to the distance between neighboring particles.