๐”– Scriptorium
โœฆ   LIBER   โœฆ
๐Ÿ“

SOLAR MAGNETOHYDRODYNAMICS

โœ Scribed by E.R. Priest

Publisher
D. Reidel Publishing Company
Year
1982
Tongue
English
Leaves
487
Series
Geophysics and Astrophysics Monographs
Edition
1
Category
Library
โฌ‡  Acquire This Volume

No coin nor oath required. For personal study only.

๐Ÿ“œ SIMILAR VOLUMES

Solar Magnetohydrodynamics
๐Ÿ“ Solar Magnetohydrodynamics
โœ Eric R. Priest (auth.) ๐Ÿ“‚ Library ๐Ÿ“… 1982 ๐Ÿ› Springer Netherlands ๐ŸŒ English

<p>I have felt the need for a book on the theory of solar magnetic fields for some time now. Most books about the Sun are written by observers or by theorists from other branches of solar physics, whereas those on magnetohydrodynamics do not deal extensively with solar applications. I had thought of

Solar Magnetohydrodynamics
๐Ÿ“ Solar Magnetohydrodynamics
โœ Eric R. Priest (auth.) ๐Ÿ“‚ Library ๐Ÿ“… 1982 ๐Ÿ› Springer Netherlands ๐ŸŒ English

<p>I have felt the need for a book on the theory of solar magnetic fields for some time now. Most books about the Sun are written by observers or by theorists from other branches of solar physics, whereas those on magnetohydrodynamics do not deal extensively with solar applications. I had thought of

Advances in solar system magnetohydrodyn
๐Ÿ“ Advances in solar system magnetohydrodynamics
โœ Eric R. Priest, Alan W. Hood ๐Ÿ“‚ Library ๐Ÿ“… 1991 ๐Ÿ› CUP ๐ŸŒ English

Most of the solar system exists in the plasma state (the fourth state of matter). Its subtle nonlinear interaction with the magnetic field can be described by the equations of magnetohydrodynamics (MHD). Over the past few years this important and complex field of research has been actively pursued

Advances in Solar System Magnetohydrodyn
๐Ÿ“ Advances in Solar System Magnetohydrodynamics
โœ Eric R. Priest, Alan W. Hood ๐Ÿ“‚ Library ๐Ÿ“… 1991 ๐Ÿ› Cambridge University Press ๐ŸŒ English

Most of the solar system exists in the plasma state (the fourth state of matter). Its subtle nonlinear interaction with the magnetic field can be described by the equations of magnetohydrodynamics (MHD). Over the past few years this important and complex field of research has been actively pursued