Expanding upon the ideas first proposed in his seminal book Cosmical Magnetic Fields, Eugene N. Parker here offers the first in-depth treatment of the magnetohydrodynamic theory of spontaneous magnetic discontinuities. In detailing his theory of the spontaneous formation of tangential discontinuities (current sheets) in a magnetic field embedded in highly conducting plasma, Parker shows how it can be used to explain the activity of the external magnetic fields of planets, stars, interstellar gas clouds, and galaxies, as well as the magnetic fields in laboratory plasmas. Provocative...

Dynamic Sun presents a comprehensive and authoritative overview of the Sun, from its deep core to the outer corona, and the solar wind. The chapters are written by leading scientists in solar physics and deal with solar models and neutrinos, seismic Sun, rotation of the solar interior, helioseismic tomography, solar dynamo, spectro-polarimetry, solar photosphere and convection, dynamics and heating of the solar chromosphere, and solar transition region. With an introduction by eminent astrophysicist Eugene Parker, the twenty chapters are fully illustrated and have comprehensive reference...

Dynamic Sun presents a comprehensive and authoritative overview of the Sun, from its deep core to the outer corona, and the solar wind. The chapters are written by leading scientists in solar physics and deal with solar models and neutrinos, seismic Sun, rotation of the solar interior, helioseismic tomography, solar dynamo, spectro-polarimetry, solar photosphere and convection, dynamics and heating of the solar chromosphere, and solar transition region. With an introduction by eminent astrophysicist Eugene Parker, the twenty chapters are fully illustrated and have comprehensive reference...