Force Free Magnetic Fields and Solar Activity.

Abstract

This report concerning the prediction of solar flares, centers on devising methods for calculating magnetic field structures in the solar atmosphere. Force-free fields comprise an important class of magnetic-field structures which may be calculated by relaxation techniques. Models of force-free fields with cylindrical symmetry, based on a spherical boundary surface, have been calculated. Evaluation of the energy of such structures provides information about the eruption of closed field patterns to form open current sheets which can then lead to solar flares.

Document Details

Document Type
Technical Report
Publication Date
Aug 01, 1974
Accession Number
ADA013778

Entities

People

  • C. W. Barnes
  • Peter A. Sturrock

Organizations

  • Stanford University

Tags

DTIC Thesaurus Topics

  • Atmospheres
  • Boundaries
  • Free Field
  • Magnetic Fields
  • Solar Activity
  • Solar Atmosphere
  • Solar Flares
  • Sun
  • Symmetry
  • Test And Evaluation

Readers

  • Solar Physics
  • Structural Dynamics.
  • Systems Analysis and Design