PREDICTION OF THE CORONAL STRUCTURE FOR THE SOLAR ECLIPSE OF SEPTEMBER 22, 1968.

Abstract

The coronal structure for the solar eclipse of September 22, 1968 has been predicted utilizing a recent model for large-scale structure within the inner corona. Supporting evidence for the model has come from comparisons with interplanetary magnetic field observations, coronal green line emission and comparisons of coronal structures evident in previous eclipses. (Author)

Document Details

Document Type
Technical Report
Publication Date
Sep 30, 1968
Accession Number
AD0676898

Entities

People

  • Kenneth H. Schatten

Organizations

  • University of California, Berkeley

Tags

DTIC Thesaurus Topics

  • Acquisition
  • Eclipses
  • Emission
  • Magnetic Fields
  • Observation
  • Solar Eclipses

Fields of Study

  • Physics

Readers

  • Computational Modeling and Simulation
  • Materials Science and Engineering.
  • Space Exploration and Orbital Mechanics.