Cosmical Magnetic Fields - Parker, E N
96,99 €
inkl. MwSt.
Versandkostenfrei*
Versandfertig in über 4 Wochen
payback
48 °P sammeln
  • Broschiertes Buch

This book explores the universal spontaneous generation of magnetic fields in astronomical bodies and the agitation of the bodies by those fields. Properties of magnetic fields, their appearance in the universe, and the havoc they wreak are described in simple physical terms to define the broad scientific problem presented by magnetic fields.

Andere Kunden interessierten sich auch für
Produktbeschreibung
This book explores the universal spontaneous generation of magnetic fields in astronomical bodies and the agitation of the bodies by those fields. Properties of magnetic fields, their appearance in the universe, and the havoc they wreak are described in simple physical terms to define the broad scientific problem presented by magnetic fields.
Hinweis: Dieser Artikel kann nur an eine deutsche Lieferadresse ausgeliefert werden.
Autorenporträt
Eugene N. Parker is S. Chandrasekhar Distinguished Service Professor Emeritus in the Department of Astronomy and Astrophyiscs and the Enrico Fermi Institute at the University of Chicago. He developed the theory on the supersonic solar wind (1958) and predicted the Parker spiral shape of the solar magnetic field in the outer solar system. In 1987, Parker proposed that the solar corona might be heated by myriad tiny "nanoflares", miniature brightenings resembling solar flares that would occur all over the surface of the Sun.